# Astrophysics MPhys

- Course length: 4 years
- UCAS code: F521
- Year of entry: 2019
- Typical offer: A-level : AAB / IB : 35 / BTEC : Applications considered

## Honours Select

×This programme offers Honours Select combinations.

## Honours Select 100

×This programme is available through Honours Select as a Single Honours (100%).

## Honours Select 75

×This programme is available through Honours Select as a Major (75%).

## Honours Select 50

×This programme is available through Honours Select as a Joint Honours (50%).

## Honours Select 25

×This programme is available through Honours Select as a Minor (25%).

## Study abroad

×This programme offers study abroad opportunities.

## Year in China

×This programme offers the opportunity to spend a Year in China.

## Accredited

×This programme is accredited.

### Module details

### Programme Year One

The first year starts with a one week project to familiarise you with the staff and other students. There will be two Maths modules in each of the first two years, these are designed to provide the Mathematical skills required by Physics students.

#### Year One Compulsory Modules

##### Newtonian Dynamics (PHYS101)

**Level**1 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**60:40 **Aims**- To introduce the fundamental concepts and principles of classical mechanics at an elementary level.
- To provide an introduction to the study of fluids.
- To introduce the use of elementary vector algebra in the context of mechanics.

**Learning Outcomes**Demonstrate a basic knowledge of the laws of classical mechanics, and understand physical quantities with magnitudes, directions (where applicable), units and uncertainties.

- understand physical quantities with magnitudes, directions (where applicable), units and uncertainties.
- apply the laws of mechanics to statics, linear motion, motion in a plane, rotational motion, simple harmonic motion and gravitation.

Apply the laws of mechanics to unseen situations and solve problems.

Develop a knowledge and understanding of the analysis of linear and rotational motion.

Develop a knowledge and understanding of the analysis of orbits, gravity, simple harmonic motion and fluid flow.

##### Thermal Physics (PHYS102)

**Level**1 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**60:40 **Aims**The module aims to make the student familiar with

- The concepts of Thermal Physics
- The zeroth, first and second laws of Thermodynamics
- Heat engines
- The kinetic theory of gasses
- Entropy
- The equation of state
- Van der Waals equation
- States of matter and state changes
- The basis of statistical mechanics

**Learning Outcomes**Construct a temperature scale and understand how to calibrate a thermometer with that scale

Calculate the heat flow into and work done by a system and how that is constrained by the first law of Thermodynamics

Analyse the expected performance of heat engines, heat pumps and refrigerators

Relate the second law of thermodynamics to the operation of heat engines, particularly the Carnot engine

Understand the kinetic theory of gases and calculate properties of gases including the heat capacity and mean free path

Use the theory of equipartition to relate the structure of the molecules to the measured heat capacity

Calculate the linear and volume thermal expansions of materials

Understand the basis of entropy and relate this to the second law of thermodynamics andcalculate entropy changesRelate the equation of state for a material to the macroscopic properties of the material

Understand the PV and PT diagrams for materials and the phase transitions that occur when changing the state variables for materials

Be able to link the microscopic view of a system to its macroscopic state variablesBe able to demonstrate the equivalence of the Clausius and Kelvin-Planck statements of the second law of thermodynamics.

Be able to derive and use Maxwell''s equations

##### Wave Phenomena (PHYS103)

**Level**1 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**60:40 **Aims**- To introduce the fundamental concepts and principles of wave phenomena.
- To highlight the many diverse areas of physics in which an understanding of waves is crucial.
- To introduce the concepts of interference and diffraction.

**Learning Outcomes**Demonstrate an understanding of oscillators.

Understand the fundamental principles underlying wave phenomena.

Apply those principles to diverse phenomena.

Understand wave reflection and transmission, superposition of waves.

Solve problems on the behaviour of electromagnetic waves in vacuo and in dielectric materials.

Understand linear and circular polarisation.

Understand inteference and diffraction effects.

Understand lenses and optical instruments.

Apply Fourier techniques and understand their link to diffraction patterns.

Understand the basic principles of lasers

##### Foundations of Modern Physics (PHYS104)

**Level**1 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**60:40 **Aims**- To introduce the theory of special relativity and its experimental proofs.
- To carry out calculations using relativity and visualise them.
- To introduce the concepts and the experimental foundations of quantum theory.
- To carry out simple calculations related to quantum mechanical problem tasks.
- To show the impact of relativity and quantum theory on contemporary science and society.

**Learning Outcomes**An understanding why classical mechanics must have failed to describe the properties of light, the motion of objects with speeds close to the speed of light and the properties of microspopic systems.

A basic knowledge on the experimental and theoretical concepts which founded modern physics, i.e. that either relativity or quantum theory or both are needed to explain certain phenomena.

A knowledge of the postulates of special relativity.

An understanding of the concept of spacetime, of the relativity of length, time and velocity.

An ability to apply the Lorentz transformation and the concept of Lorentz invariance to simple cases

An ability to apply the equations of relativistic energy, momentum and rest mass.

An understanding of the Doppler effect for light and visualisation of relativistic effects.

An ability to solve problems based on special relativity.

An understanding why quantum theory is the conceptual framework to understand the microscopic properties of the universe.

An understanding of the quantum theory of light and the ability to apply the energy-momentum conservation for light, e.g. photo-electric effect, Compton effect.

An understanding of the structure of atoms and its experimental foundations.

An understanding of Bohr''s theory of the atom and its application to the H-atom including the concept of principal quantum numbers.

An understanding of de Broglie waves and their statistical interpretation.

An ability to explain the experimental evidence of de Broglie waves with scattering experiments of electrons, X-rays and neutrons.

An understanding of the principles of quantum mechanical measurements and Heisenberg''s uncertainty principle.

An understanding of the identity principle of microscopic particles and the basic idea of quantum (Fermi-Dirac and Bose-Einstein) statistics.

A basic knowledge of contemporary applications of quantum theory and relativity, e.g. nuclear reactor and nuclear fissions, and the impact on our society.

##### Introduction to Computational Physics (PHYS105)

**Level**1 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- To develop the ability to break down physical problems into steps amenable to solution using algorithms
- To develop skills in using computers to perform and run algorithms
- To introduce techniques for analysing and presenting data
- To introduce elemenatry Monte Carlo techniques
- To introduce basic computer algebra
- To illustrate the insight into physics which can be obtained using computational methods

**Learning Outcomes**Ability to produce algorithms to solve simple physical problems.

Ability to program and use simple algorithms on a computer

Ability to analyse and present physical data

Ability to produce simple Monte Carlo models

Ability to carry out basic symbolic manipulations using a computer

##### Practical Physics I (PHYS106)

**Level**1 **Credit level**15 **Semester**Whole Session **Exam:Coursework weighting**0:100 **Aims**- To provide a core of essential introductory laboratory methods which overlap and develop from A-Level
- To introduce the basis of experimental techniques in physical measurement, the use of computer techniques in analysis, and to provide experience in doing experiments, keeping records and writing reports.
- To compliment the core physics program with experimental examples of material taught in the lecture courses.

**Learning Outcomes**- Experienced the practical nature of physics.

- Developed an awareness of the importance of accurate experimentation, particularly observation, record keeping.

- Developed the ability to plan, execute and report on the results of an investigation using appropriate analysis of the data and associated uncertainties

- Developed the practical and technical skill required for physics experimentation and an appreciation of the importance of a systematic approach to experimental measurement.

- Developed problem solving skills of a practical nature

- Developed analytical skills in the analysis of the data

- Developed communication skills in the presentation of the investigation in a clear and logical manner

- Developed investgative skills in performing the experiment and extracting information from various sources with which to compare the results

- Developed the ability to organise their time and meet deadlines

- Understand the interaction between theory and experiment, in particular the ties to the material presented in the lecture courses.

##### Mathematics for Physicists I (PHYS107)

**Level**1 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**To ensure all students possess a common level of knowledge and skills irrespective of background.

To provide a foundation for the mathematics required by physical scientists.

To assist students in acquiring the skills necessary to use the mathematics developed in the module.

**Learning Outcomes**- A good working knowledge of differential and integral calculus
- Familiarity with some of the elementary functions common in applied mathematics and science
An introductory knowledge of functions of several variables

Manipulation of complex numbers and use them to solve simple problems involving fractional powers

An introductory knowledge of series

A good rudimentary knowledge of simple problems involving statistics: binomial and Poisson distributions, mean, standard deviation, standard error of mean

- A good working knowledge of differential and integral calculus
##### Mathematics for Physicists II (PHYS108)

**Level**1 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**- To consolidate and extend the understanding of mathematics required for the physical sciences.
- To develop the student’s ability to apply the mathematical techniques developed in the module to the understanding of physical problems.

**Learning Outcomes**Ability to manipulate matrices with confidence and use matrix methods to solve simultaneous linear equations. Familiarity with methods for solving first and second order differential equations in one variable.

A basic knowledge of vector algebra.

A basic understanding of Fourier series and transforms.

A basic understanding of series methods for the solution of differential equations

### Programme Year Two

In year two you will broaden your understanding of Physics, with modules designed to ensure you have mastered the full range of Physics concepts.

#### Year Two Compulsory Modules

##### Electromagnetism (PHYS201)

**Level**2 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To introduce the fundamental concepts and principles of electrostatics, magnetostatics, electromagnetism and Maxwell''s equations, and electromagnetic waves.
- To introduce differential vector analysis in the context of electromagnetism.
- To introduce circuit principles and analysis (EMF, Ohm''s law, Kirchhoff''s rules, RC and RLC circuits)
- To introduce the formulation fo Maxwell''s equations in the presence of dielectric and magnetic materials.
- To develop the ability of students to apply Maxwell''s equations to simple problems involving dielectric and magnetic materials.
- To develop the concepts of field theories in Physics using electromagnetism as an example.
- To introduce light as an electromagnetic wave.

**Learning Outcomes**Demonstrate a good knowledge of the laws of electromagnetism and an understanding of the practical meaning of Maxwell''s equations in integral and differential forms.

Apply differential vector analysis to electromagnetism.

Demonstrate simple knowledge and understanding of how the presence of matter affects electrostatics and magnetostatics, and the ability to solve simple problems in these situations.

Demonstrate knowledge and understanding of how the laws are altered in the case of non-static electric and magnetic fields and the ability to solve simple problems in these situations.

##### Condensed Matter Physics (PHYS202)

**Level**2 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims** The aims of Phys202 are to introduce the most important and basic concepts in condensed matter physics relating to the different materials we commonly see in the world around us. Condensed matter physics is one of the most active areas of research in modern physics, whose scope is extremely broad. The ultimate aim of this course is to introduce its central ideas and methodology to the students.

Condensed matter refers to both liquids and solids and all kinds of other forms of matter in between those two extremes, generally known as “soft matter". While the course will touch on liquids, the emphasis will be on crystalline solids, including some nano-materials. The reason for focusing on crystals is that the periodicity of a crystal is what allows us to make progress in developing a theory for various phenomena in solids based on first principles. Two important concepts are:

• the electronic states of electrons in a solid and

• the vibrations of atoms in the solid.

The description of these ideas basically refer to the theory of electronic band structure and the theory of phonons. These concepts form the basis for understanding a wide range of phenomena including how the atoms bond together to form the crystal, what are some basic statistical properties like specific heat, how electrons move in solids and electronic transport, why are some materials metals and others semiconductors and insulators, and how do solids interact with electromagnetic fields. The course will also introduce optical and magnetic properties in solids, scattering phenomena, thermal conductivity and effect of defects in solids, semiconductors, magnetism and go beyond the free electron model to touch on intriguing effects such as superconductivity.

**Learning Outcomes**On satisfying the requirements of this course, students will have the knowledge and skills to understand the basic concepts of bonding in solids, establish an understanding of electron configuration in atoms and in the condensed matter in terms of bonding, and relating them to band structure description.

Students will be able to understand how solid structures are described mathematically and how material properties can be predicted.

Students will be able to establish a foundation in basic crystallography, using Bragg''s law, and understand the concept of the reciprocal lattice.

Students will understand basic transport properties, both electronic and thermal, in solids.

Students will understand the concept of electron and hole carrier statistics, effective masses and transport in intrinsic and extrinsic semiconductorsStudents will learn the basics of magnetism, the atomic origin and classical treatment of diamagnetism and paramagnetism, quantization of angular momentum and Hund''s rule, and introduced to weak magnetism in solids.

Students will become familiar to the general language of condensed matter physics, key theories and concepts, ultimately enebling them to read and understand research papers.

##### Quantum and Atomic Physics (PHYS203)

**Level**2 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**- To introduce students to the concepts of quantum theory.
- To show how Schrodinger''s equation is applied to bound states (well potentials, harmonic oscillator, hydrogen atoms, multi-electron atoms) and particle flux (scattering).
- To show how quantum ideas provide an understanding of atomic structure.

**Learning Outcomes**At the end of the module the student should have:

- An understanding of the reasons why microscopic systems require quantum description and statistical interpretation.
- Knowledge of the Schrodinger equation and how it is formulated to describe simple physical systems.
- Understanding of the basic technique of using Schrodinger''s equation and ability to determine solutions in simple cases.
- Understanding of how orbital angular momentum is described in quantum mechanics and why there is a need for spin.
- Understanding how the formalism of quantum mechanics describes the structure of atomic hydrogen and, schematically, how more complex atoms are described.

##### Nuclear and Particle Physics (PHYS204)

**Level**2 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**- To introduce Rutherford and related scattering.
- To introduce nuclear size, mass and decay modes
- To provide some applications and examples of nuclear physics
- To introduce particle physics, including interactions, reactions and decay
- To show some recent experimental discoveries
- To introduce relativistic 4-vectors for applications to collision problems

**Learning Outcomes**basic understanding of Rutherford, electron on neutron scattering

understanding of the basic principles that determine nuclear size, mass and decay modes

knowledge of examples and applications of nuclear physics

knowledge of elementary particles and their interactionsbasic understanding of relativistic 4-vectors

##### Working With Physics II (PHYS205)

**Level**2 **Credit level**15 **Semester**Whole Session **Exam:Coursework weighting**0:100 **Aims**- To develop essential research skills
- To use programming techniques to solve problems in Physics, Nuclear Physics, Astrophysics and/or meduical applciations of physics.
- To develop skills in modelling the solution to a problem
- To give students experience iof working in small groups to solve a problem
- To give students further experience of communicating their results using computer packages

**Learning Outcomes**Knowledge of programming techniques in Matlab

The ability to solve problems using a computer programMastered a basic set of research skills

Experience of working in a small group

Improved communication skills written, Oral and Poster

##### Mathematics for Physicists III (PHYS207)

**Level**2 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To re-inforce students'' prior knowledge of mathematical techniques
- To introduce new mathematical techniques for physics modules
- To enhance students'' problem-solving abilities through structured application of these techniques in physics

**Learning Outcomes**At the end of the module the student should be able to:

- Have knowledge of a range of mathematical techniques necessary for physics and astrophysics programmes
- Be able to apply these mathematical techniques in a range of physics and astrophysics programmes

##### Mathematics for Physicists IV (PHYS208)

**Level**2 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**- To re-inforce students'' prior knowledge of mathematical techniques
- To introduce new mathematical techniques for physics modules
- To enhance students'' problem-solving abilities through structured application of these techniques in physics

**Learning Outcomes**At the end of the module the student should be able to:

- Have knowledge of a range of advanced mathematical techniques necessary for physics and astrophysics programmes
- Be able to apply these mathematical techniques in a range of physics and astrophysics programmes

##### Practical Astrophysics I (PHYS216)

**Level**2 **Credit level**15 **Semester**Whole Session **Exam:Coursework weighting**0:100 **Aims**- Setting up and calibrating equipment
- Become familiar with equipment used in later modules
- Taking reliable and reproducible data
- Develop understanding of various techniques of data gathering and analysis in modern astrophysics
- Calculating experimental results and their associated uncertainties
- Using computer software, including specific astrophysical software, to analyse data
- Writing a coherent account of the experimental procedure and conclusions
- Understanding physics in depth by performing specific experiments
- Developing practical, technical and computing skills required for later modules

**Learning Outcomes**Improved practical skills and experience.

A detailed understanding of the fundamental physics and/or astrophysics behind the experiments.

Increased confidence in setting up and calibrating equipment.

Familiarity with IT package for calculating, displaying and presenting results

Familiarity with subject specific astrophysics data analysis software.

Enhanced ability to plan, execute and report the results of an investigation.

Knowledge of the methods employed in the detection and analysis of light at optical wavelengths from astrophysical sources.

A clear understanding of the methods employed in astronomical photometry and spectroscopy.

Experience of the acquisition, reduction and analysis of astronomical data.

##### Quantum Mechanics and Atomic Physics (PHYS361)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the second year module on Quantum and Atomic Physics
- To develop the formalism of quantum mechanics
- To develop an understanding that atoms are quantum systems
- To enable the student to follow elementary quantum mechanical arguments in the literature

**Learning Outcomes**Understanding of the role of wavefunctions, operators, eigenvalue equations, symmetries, compatibility/non-compatibility of observables and perturbation theory in quantum mechanical theory. An ability to solve straightforward problems - different bound states and perturbing interactions.

Developed knowledge and understanding of the quantum mechanical description of atoms - single particle levels, coupled angular momentum, fine structure, transition selection rules.

Developed a working knowledge of interactions, electron configurations and coupling in atoms.

### Programme Year Three

With the core physics modules completed in the first two years there is now considerable scope to choose amongst the optional modules available, mostly based around the research interests of the departmental staff.

#### Year Three Compulsory Modules

##### Stellar Physics (PHYS351)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To provide students with an understanding of the physical processes which determine all aspects of the structure and evolution of stars, from their birth to their death.
- To enable students to determine the basic physical properties of stars via observation (e.g. determination of temperatures, masses and radii etc. using continuum fluxes, broad-band colours, line profiles etc).

**Learning Outcomes**At the end of the module the student should have knowledge of how the basic physical properties of stars can be determined from observation.

At the end of the module the student should have an understanding of how stellar structure can be probed using observable quantities and simple physical principles.

At the end of the module a student should have an understanding of the changes in structure and energy sources for stars throughout their lives.

##### Quantum Mechanics and Atomic Physics (PHYS361)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the second year module on Quantum and Atomic Physics
- To develop the formalism of quantum mechanics
- To develop an understanding that atoms are quantum systems
- To enable the student to follow elementary quantum mechanical arguments in the literature

**Learning Outcomes**Understanding of the role of wavefunctions, operators, eigenvalue equations, symmetries, compatibility/non-compatibility of observables and perturbation theory in quantum mechanical theory. An ability to solve straightforward problems - different bound states and perturbing interactions.

Developed knowledge and understanding of the quantum mechanical description of atoms - single particle levels, coupled angular momentum, fine structure, transition selection rules.

Developed a working knowledge of interactions, electron configurations and coupling in atoms.

##### Advanced Observational Astronomy (PHYS362)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To introduce students to the experimental techniques which enable astrophysicists to use the full range of the electromagnetic spectrum to study the physics of astronomical objects.
- To become familiar with the design of telescopes across the electromagnetic spectrum.
- To understand the physical basis of light detection across the spectrum.
- To understand observing techniques such as photometry, spectroscopy, adaptive optics, interferometry.

**Learning Outcomes**Understand and be able to compare and contrast the basic techniques and problems involved in observing all wavelengths of the electromagnetic spectrum Understand and be able to use and experimental concepts, as applied to observational astrophysics, of signal-to-noise ratio, sampling, resolution.

Be able to determine the observing technique most appropriate for a given scientific goal

Be able to plan observations at a variety of wavelengths

##### Physics of Galaxies (PHYS373)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To provide students with a broad overview of these complex yet fundamental systems which interact at one end with the physics of stars and the interstellar medium and at the other with cosmology and the nature of large-scale structures in the Universe
- To develop in students an understanding of how the various distinct components in galaxies evolve and interact

**Learning Outcomes**Interpret physically the properties of normal galaxies along the Hubble sequenceAccount for the stellar, gas, dust and dark matter content of galaxies Describe the formation and evolution of galaxies in a cosmological context.

Analyze the structure and dynamics of galaxies and clusters of galaxies, using advanced classical mechanics and Newtonian gravity.

Apply fundamental physics to calculate the dynamical state of groups and clusters of galaxies, their intracluster gas, and their dark matter content.

Describe large-scale structure in the Universe, the nature of the first galaxies, and their implications for dark matter and cosmology.

Identify, summarise and present the content of research papers relevant for the field of galactic astronomy

##### Relativity and Cosmology (PHYS374)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**80:20 **Aims**- To introduce the ideas of general relativity and demonstrate its relevance to modern astrophysics
- To provide students with a full and rounded introduction to modern observational cosmology
- To develop the basic theoretical background required to understand and appreciate the significance of recent results from facilities such as the Hubble Space Telescope and the Wilkinson Microwave Anisotropy Probe

**Learning Outcomes**The ability to explain the relationship between Newtonian gravity and Einstein''s General Relativity (GR) Understanding of the concept of curved space time and knowledge of metrics.

A broad and up-to-date knowledge of the basic ideas, most important discoveries and outstanding problems in modern cosmology.

Knowledge of how simple cosmological models of the universe are constructed.

The ability to calculate physical parameters and make observational predictions for a range of such models.##### Nuclear Physics (PHYS375)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the second year module involving Nuclear Physics
- To develop an understanding of the modern view of nuclei, how they are modelled and of nuclear decay processes

**Learning Outcomes**At the end of the module the student should have:

- Knowledge of evidence for the shell model of nuclei, its development and the successes and failures of the model in explaining nuclear properties

Knowledge of the collective vibrational and rotational models of nuclei

Basic knowledge of nuclear decay processes, alpha decay and fission, of gamma-ray transitions and internal conversion

Knowledge of electromagnetic transitions in nuclei

##### Introduction to Particle Physics (PHYS377)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the second year module involving Nuclear and Particle Physics
- To develop an understanding of the modern view of particles, of their interactions and the Standard Model

**Learning Outcomes**At the end of the module the student should have:

Basic understanding of relativistic kinematics (as applied to collisions, decay processes and cross sections)

Descriptive knowledge of the Standard Model using a non rigorous Feynman diagram approach

Knowledge of the fundamental particles of the Standard Model and the experimental evidence for the Standard Model

Knowledge of conservation laws and discrete symmetries

#### Year Three Optional Modules

##### Accelerators and Radioisotopes in Medicine (PHYS246)

**Level**2 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To introduce the students to ionising and non ionising radiation including its origins and production.
- To introduce the various ways in which radiation interacts with materials.
- To introduce the different accelerators and isotopes used in medicine and to give examples of their use.

**Learning Outcomes**- A basic knowledge of the origins of radiation and its properties.

- An understanding of ways in which radiation interacts with materials.

- An understanding of how accelerators operate and how isotopes are produced.

- Knowledge of applications of the use of accelerators and isotopes in medicine.

##### Stellar Atmospheres (PHYS352)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**80:20 **Aims**- To provide students with an understanding of the properties of the light emitted by stars, of the effect of expanding atmospheres and of the relevance for Supernovae.
- To enable students to determine the basic physical properties of stars from observational data (e.g. Temp, Radius, Mass, composition) and the properties of expanding media (stellar winds: velocity, mass-loss rate; Supernovae: velocity, mass, kinetic energy, nucleosynthesis)

**Learning Outcomes**Knowledge of how the physical properties of stars and supernovae can be determined from spectroscopic observations.

An understanding of how the interaction between radiation and matter determines the observable properties of stars.

An understanding of how radiation propagates through a medium (a gas), affecting its properties

##### Planetary Physics (PHYS355)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**To demonstrate the application of basic physical principles to the understanding of planetary sience.

To provide a background in Geophysics and solar system planetary science towards the understanding of exoplanet system research.

To introduce methods of exoplanet detection, and current physical understanding of exoplanet systems

**Learning Outcomes**Understanding of the principles of physics applied to understanding the interior of the Earth.

Understanding of theories of solar system formation and evolution, including orbital evolution.

Understanding of models of the interiors, atmospheres and magnetospheres of planets in the solar system.

Understanding and application of methods of exoplanet detection.

Understanding methods of planetary study of non-solar system bodies.

##### Advanced Condensed Matter Physics (PHYS363)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To develop concepts introduced in Year 1 and Year 2 modules which relate to solids.
- To consolidate concepts related to crystal structure.
- To introduce the concept of reciprocal space and diffraction.
- To enable the students to apply these concepts to the description of crystals,transport properties and the electronic structure of condensed matter.
- To illustrate the use of these concepts in scientific research in condensed matter.
- To introduce various other solids

**Learning Outcomes**Familiarity with the crystalline nature of both perfect and real materials.

An understanding of the fundamental principles of the properties of condensed matter

An appreciation of the relationship between the real space and the reciprocal space view of the properties of crystalline matter

An ability to describe the crystal structure and electronic structure of matter

An awareness of current physics research in condensed matter.

##### Advanced Electromagnetism (PHYS370)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To build on first and second year modules on electricity, magnetism and waves by understanding a range of electromagnetic phenomena in terms of Maxwell''s equations.
- To understand the properties of solutions to the wave equation for electromagnetic fields in free space, in matter (non-dispersive and dispersive dielectrics, and conductors).
- To understand the behaviour of electromagnetic waves at boundaries.
- To understand the behaviour of electromagnetic waves in cavities, waveguides and transmission lines.
- To understand the properties of electric dipole radiation.
- To introduce an explicity covariant formulation of electromagnetism in special relativity.
- To further develop students'' problem-solving and analytic skills.

**Learning Outcomes**Students should have an understanding of the properties of solutions to the wave equation for electromagnetic fields in free space and in matter (non-dispersive and dispersive dielectrics, and conductors).

Students should have an understanding of the behaviour of electromagnetic waves at boundaries.

Students should have an understanding of the behaviour of electromagnetic waves in cavities, waveguides and transmission lines.

Students should have an understanding of the properties of electric dipole radiation.

Students should have the ability to explain an explicity covariant formulation of electromagnetism in special relativity.

##### Surface Physics (PHYS381)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- Develop a syllabus to describe the properties of surfaces
- Convey an understanding of the physical properties of Surfaces
- Provide knowledge of a raneg of surface characterisation techniques
- Illustrate surface processes and their relevance to technologies

**Learning Outcomes**explain how the presence of the surface alters physical properties such as atomic an electronic structure

choose the right characterisation technique to assess different surface properties have gained an appreciation of surface processes and their relevance to the modification of surface propertiesbe able to describe surface alterations and processes using the right terminology

##### Physics of Life (PHYS382)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**To introduce students to the physical principles needed to address important problems such as climate change, the loss of biodiversity, the understanding of ecological systems, the growth of resistance to antibiotics, the challenge of sustainable development and the study of disease. These problems offer excellent opportunities for rewarding careers.

**Learning Outcomes** An understanding of the conditions necessary for life to evolve in a universe.

An understanding of the thermodynamics and organization of living things.

Familiarity with physical techniques used in the study of biological systems. ##### Materials Physics (PHYS387)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To teach the properties and methods of preparation of a range of materials of scientific and technological importance
- To develop an understanding of the experimental techniques of materials characterisation
- To introduce materials such as amorphous solids, liquid crystals and polymers and to develop an understanding of the relationship between structure and physical properties for such materials
- To illustrate the concepts and principles by reference to examples

**Learning Outcomes**At the end of the module the student should have:

- An understanding of the atomic structure in cyrstalline and amorphous materials
- Knowledge of the methods used for preparing single crystals and amorphous materials
- Knowledge of the experimental techniques used in materials characterisation
- Knowledge of the physical properties of superconducting materials
- An appreciation of the factors involved in the design of biomaterials
- The ability to interpret simple phase diagrams of binary systems

##### Physics of Energy Sources (PHYS388)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To develop an ability which allows educated and well informed opinions to be formed by the next generation of physicists on a wide range of issues in the context of the future energy needs of man
- To describe and understand methods of utilising renewable energy sources such as hydropower, tidal power, wave power, wind power and solar power.
- To give knowledge and understanding of the design and operation of nuclear reactors
- To give knowledge and understanding of nuclear fusion as a source of power
- To give knowledge and understanding relevant to overall safety in the nuclear power industry
- To describe the origin of environmental radioactivity and understand the effects of radiation on humans

**Learning Outcomes**At the end of the module the student should have:

- Learned the fundamental physical principles underlying energy production using conventional and renewable energy sources
- Learned the fundamental physical principles underlying nuclear fission and fusion reactors
- Studied the applications of these principles in the design issues power generation
- An appreciation of the role of mathematics in modelling power generation
- Learned the fundamental physical principles concerning the origin and consequences of environmental radioactivity
- Developed an awareness of the safety issues involved in exposure to radiation
- Developed problem solving skills based on the material presented
- Developed an appreciation of the problems of supplying the required future energy needs and the scope and issues associated with the different possible methods

##### Semiconductor Applications (PHYS389)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To develop the physics concepts describing semiconductors in sufficient details for the purpose of understanding the construction and operation of common semiconductor devices

**Learning Outcomes**At the end of the module the student should have:

- Knowledge of the basic theory of p-n junctions
- Knowledge of the structure and function of a variety of semiconductor devices
- An overview of semiconductor device manufacturing processes
- Knowledge of the basic processes involved in the interaction of radiation with matter
- Understanding the application of semiconductors in Nuclear and Particle physics

##### Communicating Science (PHYS391)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- To improve science students'' skills in communicating scientific information in a wide range of contexts
- To develop students'' understanding of some concepts of:

- Science in general
- Their particular area of science
- Other areas of science

**Learning Outcomes** An ability to communicate more confidently

An understanding of some of the key factors in successfulcommunication

An appreciation of the needs of different audiences

Experience of a variety of written and oral media

A broader appreciation of science and particular areas ofscience

##### Statistics for Physics Analysis (PHYS392)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**50:50 **Aims**To give a theoretical and practical understanding of the statistical principles involved in the analysis and interpretation of data.

To give practice in analysing data by computer program.

To show how to write code to solve problems in data analysis.

**Learning Outcomes**Knowledge of experimental errors and probability distributions The ability to use statistical methods in data analysis

The ability to apply statistical analysis to data from a range of sources

Using statistical information to detemine the validity of a hypothesis or experimental measurement

The ability to write code to analyse data sets##### Statistical and Low Temperature Physics (PHYS393)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on material presented in earlier Thermal Physics and Quantum Mechanics courses
- To develop the statistical treatment of quantum systems
- To use theoretical techniques to predict experimental observables
- To introduce the basic principles governing the behaviour of liquid helium and superconductors in cooling techniques

**Learning Outcomes**Understanding of the statistical basis of entropy and temperature

Ability to devise expressions for observables, (heat capacity, magnetisation) from statistical treatment of quantum systems

Understanding of Maxwell Boltzmann, Fermi-Dirac and Bose Einstein gases

Knowledge of cooling techniques

Knowledge and understanding of basic theories of liquid helium behaviour and superconductivity in cooling techniques

##### Practical Astrophysics II (PHYS394)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- To provide practice in the planning and execution of a programme of astronomical observations
- To provide training in the application of astronomical co-ordinate systems
- To provide competence in the handling of a large astronomical telescope
- To gain experience in making, calibrating and analysing astronomical measurements using a CCD camera and spectrometer
- To gain experience in preparing a written report based on the results of astronomical work

**Learning Outcomes**At the end of the module the student should have:

- The ability to plan and execute a simple programme of astronomical observations and measurements
- Familiarity with astronomical coordinate systems and the ability to find astronomical objects in the sky
- Skills in pointing and adjusting a large, manually controlled astronomical telescope
- The ability to take, reduce and analyse astronomical data to produce physically meaningful information.
- Experience of observing at a professional high-altitude observatory
- Experience of preparing a written report based on the results of astronomical work

##### Classical Mechanics (PHYS470)

**Level**M **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To provide students with an awareness of the physical principles that can be applied to understand important features of classical (i.e. non-quantum) mechanical systems.
- To provide students with techniques that can be applied to derive and solve the equations of motion for various types of classical mechanical systems, including systems of particles and fields.
- To develop students'' understanding of the fundamental relationship between symmetries and conserved quantities in physics.
- To reinforce students’ knowledge of quantum mechanics, by developing and exploring the application of closely-related concepts in classical mechanics.

**Learning Outcomes**Students should know the physical principles underlying the Lagrangian and Hamiltonian formulations of classical mechanics, in particular D’Alembert’s principle and Hamilton’s principle, and should be able to explain the significance of these advanced principles in classical and modern physics.

Students should be able to apply the Euler-Lagrange equations and Hamilton’s equations (as appropriate) to derive the equations of motion for specific dynamical systems, including complex nonlinear systems.

Students should be able to use advanced concepts in classical mechanics to describe the connection between symmetries and conservation laws.

Students should be able to apply advanced techniques, including conservation laws, canonical transformations, generating functions, perturbation theory etc. to describe important features of various dynamical systems (including systems of particles and fields) and to solve the equations of motion in specific cases.

##### Elements of Stellar Dynamics (PHYS484)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**75:25 **Aims**To show that there is more to gravity than Newton''s law. This will provide the students with a basic understanding of the dynamics of systems containing millions and billions of point-like gravitating bodies: stars in stellar clusters and galaxies.

**Learning Outcomes**At the end of the module the student should have the ability to

- Show how dynamical processes shape the structure of galaxies and stellar clusters
- Describe the motion of stars in stellar systems
- Apply orbital analysis to stellar systems
- Demonstrate an understanding of the implications of the continuity equation

##### Physics of the Radiative Universe (PHYS485)

**Level**M **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**80:20 **Aims**- To see how physical phenomena can be applied and used to explain the appearance and spectra of celestial objects- To introduce Einstein''s A and B coefficients- To introduce several important radiation mechanisms at work in a variety of astronomical sources- To understand the major physical phenomena at work in non-stellar astronomical sources such as HII regions, giant radio lobes, supernova remnants- To see how important the HI emission line is in astrophysics **Learning Outcomes**At the end of the module the student should have the ability to- Relate observable quantities to physical conditions and mechanism(s) - Describe and calculate the emergent flux and spectrum for several mechanisms (e.g.Bremsstrahlung, synchrotron, Compton effect)

- Apply this knowledge to understand the properties and behaviour of different objects (active galaxies, neutron stars, H II regions, gamma-ray bursts)

- Describe the physics of a few important line ratios in HII regions

- Understand several cooling and heating mechanisms in astrophysical plasmas

- Describe and use the concept of Eddington luminosity in several different situations

- Use measurements of the HI 21cm line to deduce astrophysical information

- Understand the basic physics of gamma-ray bursts

### Programme Year Four

In the final year of the course you will have considerable flexibility to choose between the many optional modules based around various astrophysics and physics research areas. You will also undertake an extended project with a member of staff, normally in their research area in astrophysics.

#### Year Four Compulsory Modules

##### Computational Astrophysics (PHYS494)

**Level**M **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**0:100 **Aims**- To give students an understanding of Programming Basics
- To provide students with practical experience of using computational techniques extensively employed by researchers in the physical sciences

**Learning Outcomes**Obtaining the ability to describe and discuss numerical modelings

Getting familiar with a programming language used by research astronomers and its application in a research context

Obtaining practical experience of numerical used by scientists in analysis of theoretical problems and experimental data

##### The Interstellar Medium (PHYS495)

**Level**M **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To build upon the student''s appreciation of the role which the interstellar medium (ISM) plays in topics as stellar evolution (star-forming regions to supernova remnants) and galaxy evolution
- To provide a firm physical framework for this appreciation by investigating in detail the mechanisms which govern the structure and appearance of the ISM

**Learning Outcomes**At the end of the module the student should have:

- An understanding of the structure and evolution of the ISM and the relationship between its various components
- The ability to list the various types of observable phenomena and relate them to the structure of the various phases of the ISM and the physical process at work
- Knowledge of how observation, specifically spectroscopy, allows astronomers to understand the physical conditions and chemical content of the ISM and thereby construct models of the interstellar medium and its relationship to the formation and evolution of stars and galaxies

##### Astrophysics Research Skills (PHYS496)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- To demonstrate and provide experience of key aspects of professional practice in scientific research-related careers other than the research itself, such as peer review, proposal development, experimental design, and public communication of research results.
- To provide the opportunity for students to deepen their background understanding of specific astrophysics topics, especially those related to their final-year project.
- To develop the ability of the student to think critically about published scientific results, dealing with the objective criticism of existing articles, papers and lecture/seminar presentations, as well as the creation of new material and to communicate results and ideas in astrophysics at a range of technical levels.
- To help students bridge the gap between understanding undergraduate texts and dissecting a journal paper, while at the same time emphasising the importance of being able to communicate ideas concisely and clearly at a simpler level

**Learning Outcomes**The ability to create their own articles, research proposals, discussions, etc., building on the experience gained during the module, and to use this experience beyond the module content. The critical-thinking skills needed to form evidence-based arguments and communicate these persuasively in a wide range of contexts from peer review to formal proposal writing.

The ability to understand and objectively critique current arguments in astrophysics and communicate these appropriately at a range of levels up to to research seminars and proposals.

An understanding of professional practice in science research

A deeper knowledge of current topics in modern astrophysics

##### Project (mphys) (PHYS498)

**Level**M **Credit level**30 **Semester**Whole Session **Exam:Coursework weighting**0:100 **Aims**- To give students experience of working independently on an original problem
- To give students an opportunity to be involved in scientific research
- To encourage learning, understanding and application of a particular physics subject
- To give students an opportunity to display qualities such as initiative and ingenuity
- To improve students ability to keep daily records of the work in hand and its outcomes
- To develop students'' competence in scientific communication, both in oral and written form

**Learning Outcomes**At the end of the module the student should have:

- Experience of participation in planning all aspects of the work
- Experience researching literature and other sources of relevant information
- Experience of the practical nature of physics

The student should have improved practical and technical skills to carrying out physics investigations

The student will gain an appreciation of a selected area of current physics research

The student should have an ability to organise and manage time and to plan, execute and report on the results of an investigation

#### Year Four Optional Modules

##### Condensed Matter Physics (PHYS202)

**Level**2 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims** The aims of Phys202 are to introduce the most important and basic concepts in condensed matter physics relating to the different materials we commonly see in the world around us. Condensed matter physics is one of the most active areas of research in modern physics, whose scope is extremely broad. The ultimate aim of this course is to introduce its central ideas and methodology to the students.

Condensed matter refers to both liquids and solids and all kinds of other forms of matter in between those two extremes, generally known as “soft matter". While the course will touch on liquids, the emphasis will be on crystalline solids, including some nano-materials. The reason for focusing on crystals is that the periodicity of a crystal is what allows us to make progress in developing a theory for various phenomena in solids based on first principles. Two important concepts are:

• the electronic states of electrons in a solid and

• the vibrations of atoms in the solid.

The description of these ideas basically refer to the theory of electronic band structure and the theory of phonons. These concepts form the basis for understanding a wide range of phenomena including how the atoms bond together to form the crystal, what are some basic statistical properties like specific heat, how electrons move in solids and electronic transport, why are some materials metals and others semiconductors and insulators, and how do solids interact with electromagnetic fields. The course will also introduce optical and magnetic properties in solids, scattering phenomena, thermal conductivity and effect of defects in solids, semiconductors, magnetism and go beyond the free electron model to touch on intriguing effects such as superconductivity.

**Learning Outcomes**On satisfying the requirements of this course, students will have the knowledge and skills to understand the basic concepts of bonding in solids, establish an understanding of electron configuration in atoms and in the condensed matter in terms of bonding, and relating them to band structure description.

Students will be able to understand how solid structures are described mathematically and how material properties can be predicted.

Students will be able to establish a foundation in basic crystallography, using Bragg''s law, and understand the concept of the reciprocal lattice.

Students will understand basic transport properties, both electronic and thermal, in solids.

Students will understand the concept of electron and hole carrier statistics, effective masses and transport in intrinsic and extrinsic semiconductorsStudents will learn the basics of magnetism, the atomic origin and classical treatment of diamagnetism and paramagnetism, quantization of angular momentum and Hund''s rule, and introduced to weak magnetism in solids.

Students will become familiar to the general language of condensed matter physics, key theories and concepts, ultimately enebling them to read and understand research papers.

##### Stellar Atmospheres (PHYS352)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**80:20 **Aims**- To provide students with an understanding of the properties of the light emitted by stars, of the effect of expanding atmospheres and of the relevance for Supernovae.
- To enable students to determine the basic physical properties of stars from observational data (e.g. Temp, Radius, Mass, composition) and the properties of expanding media (stellar winds: velocity, mass-loss rate; Supernovae: velocity, mass, kinetic energy, nucleosynthesis)

**Learning Outcomes**Knowledge of how the physical properties of stars and supernovae can be determined from spectroscopic observations.

An understanding of how the interaction between radiation and matter determines the observable properties of stars.

An understanding of how radiation propagates through a medium (a gas), affecting its properties

##### Planetary Physics (PHYS355)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**To demonstrate the application of basic physical principles to the understanding of planetary sience.

To provide a background in Geophysics and solar system planetary science towards the understanding of exoplanet system research.

To introduce methods of exoplanet detection, and current physical understanding of exoplanet systems

**Learning Outcomes**Understanding of the principles of physics applied to understanding the interior of the Earth.

Understanding of theories of solar system formation and evolution, including orbital evolution.

Understanding of models of the interiors, atmospheres and magnetospheres of planets in the solar system.

Understanding and application of methods of exoplanet detection.

Understanding methods of planetary study of non-solar system bodies.

##### Advanced Electromagnetism (PHYS370)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To build on first and second year modules on electricity, magnetism and waves by understanding a range of electromagnetic phenomena in terms of Maxwell''s equations.
- To understand the properties of solutions to the wave equation for electromagnetic fields in free space, in matter (non-dispersive and dispersive dielectrics, and conductors).
- To understand the behaviour of electromagnetic waves at boundaries.
- To understand the behaviour of electromagnetic waves in cavities, waveguides and transmission lines.
- To understand the properties of electric dipole radiation.
- To introduce an explicity covariant formulation of electromagnetism in special relativity.
- To further develop students'' problem-solving and analytic skills.

**Learning Outcomes**Students should have an understanding of the properties of solutions to the wave equation for electromagnetic fields in free space and in matter (non-dispersive and dispersive dielectrics, and conductors).

Students should have an understanding of the behaviour of electromagnetic waves at boundaries.

Students should have an understanding of the behaviour of electromagnetic waves in cavities, waveguides and transmission lines.

Students should have an understanding of the properties of electric dipole radiation.

Students should have the ability to explain an explicity covariant formulation of electromagnetism in special relativity.

##### Surface Physics (PHYS381)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- Develop a syllabus to describe the properties of surfaces
- Convey an understanding of the physical properties of Surfaces
- Provide knowledge of a raneg of surface characterisation techniques
- Illustrate surface processes and their relevance to technologies

**Learning Outcomes**explain how the presence of the surface alters physical properties such as atomic an electronic structure

choose the right characterisation technique to assess different surface properties have gained an appreciation of surface processes and their relevance to the modification of surface propertiesbe able to describe surface alterations and processes using the right terminology

##### Physics of Life (PHYS382)

**Level**3 **Credit level**7.5 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**To introduce students to the physical principles needed to address important problems such as climate change, the loss of biodiversity, the understanding of ecological systems, the growth of resistance to antibiotics, the challenge of sustainable development and the study of disease. These problems offer excellent opportunities for rewarding careers.

**Learning Outcomes** An understanding of the conditions necessary for life to evolve in a universe.

An understanding of the thermodynamics and organization of living things.

Familiarity with physical techniques used in the study of biological systems. ##### Radiation Therapy Applications (PHYS384)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**80:20 **Aims**- To introduce the physics principles of radiation therapy and treatment planning.
- To understand interactions of radiation with biological materials and detectors.
- To understand the need for modelling in radiobiological applications.
- To obtain a knowledge of electron transport.
- To construct a simple model of a radiation therapy application.

**Learning Outcomes**to understand the principles of radiotherapy and treatment planning

to develop a knowledge of radiation transport and the interaction of radiation with biological tissue

to understand the need for Monte Carlo modelling and beam modelling

to have a knowledge of electron transportto have a basic understanding of radiobiology

to have experience developing a simple radiotherapy treatment plan

##### Physics of Medical Imaging (PHYS385)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**80:20 **Aims**- To give students a knowledge of the history of medical imaging.
- To introduce the physics principles underlying imaging techniques.
- To familiarise the students with modern imaging techniques.
- To improve the students communication skills through a poster presentation.

**Learning Outcomes**At the end of the mdoule the students will:

- have a knowledge of the history of medical imaging
- have a knowledge of the physics principles underlying medical imaging
- be familiar with imaging techniques including X-ray, radioisotope, MRI and ultrasound imaging
- have knowledge of the different situations in which the different imaging techniques are used
- be able to describe the instrumentation used in medical imaging
- have improved skills in presenting medical imaging information in the form of a poster

##### Materials Physics (PHYS387)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To teach the properties and methods of preparation of a range of materials of scientific and technological importance
- To develop an understanding of the experimental techniques of materials characterisation
- To introduce materials such as amorphous solids, liquid crystals and polymers and to develop an understanding of the relationship between structure and physical properties for such materials
- To illustrate the concepts and principles by reference to examples

**Learning Outcomes**At the end of the module the student should have:

- An understanding of the atomic structure in cyrstalline and amorphous materials
- Knowledge of the methods used for preparing single crystals and amorphous materials
- Knowledge of the experimental techniques used in materials characterisation
- Knowledge of the physical properties of superconducting materials
- An appreciation of the factors involved in the design of biomaterials
- The ability to interpret simple phase diagrams of binary systems

##### Physics of Energy Sources (PHYS388)

**Level**3 **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To develop an ability which allows educated and well informed opinions to be formed by the next generation of physicists on a wide range of issues in the context of the future energy needs of man
- To describe and understand methods of utilising renewable energy sources such as hydropower, tidal power, wave power, wind power and solar power.
- To give knowledge and understanding of the design and operation of nuclear reactors
- To give knowledge and understanding of nuclear fusion as a source of power
- To give knowledge and understanding relevant to overall safety in the nuclear power industry
- To describe the origin of environmental radioactivity and understand the effects of radiation on humans

**Learning Outcomes**At the end of the module the student should have:

- Learned the fundamental physical principles underlying energy production using conventional and renewable energy sources
- Learned the fundamental physical principles underlying nuclear fission and fusion reactors
- Studied the applications of these principles in the design issues power generation
- An appreciation of the role of mathematics in modelling power generation
- Learned the fundamental physical principles concerning the origin and consequences of environmental radioactivity
- Developed an awareness of the safety issues involved in exposure to radiation
- Developed problem solving skills based on the material presented
- Developed an appreciation of the problems of supplying the required future energy needs and the scope and issues associated with the different possible methods

##### Semiconductor Applications (PHYS389)

**Level**3 **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To develop the physics concepts describing semiconductors in sufficient details for the purpose of understanding the construction and operation of common semiconductor devices

**Learning Outcomes**At the end of the module the student should have:

- Knowledge of the basic theory of p-n junctions
- Knowledge of the structure and function of a variety of semiconductor devices
- An overview of semiconductor device manufacturing processes
- Knowledge of the basic processes involved in the interaction of radiation with matter
- Understanding the application of semiconductors in Nuclear and Particle physics

##### Statistics for Physics Analysis (PHYS392)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**50:50 **Aims**To give a theoretical and practical understanding of the statistical principles involved in the analysis and interpretation of data.

To give practice in analysing data by computer program.

To show how to write code to solve problems in data analysis.

**Learning Outcomes**Knowledge of experimental errors and probability distributions The ability to use statistical methods in data analysis

The ability to apply statistical analysis to data from a range of sources

Using statistical information to detemine the validity of a hypothesis or experimental measurement

The ability to write code to analyse data sets##### Statistical and Low Temperature Physics (PHYS393)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on material presented in earlier Thermal Physics and Quantum Mechanics courses
- To develop the statistical treatment of quantum systems
- To use theoretical techniques to predict experimental observables
- To introduce the basic principles governing the behaviour of liquid helium and superconductors in cooling techniques

**Learning Outcomes**Understanding of the statistical basis of entropy and temperature

Ability to devise expressions for observables, (heat capacity, magnetisation) from statistical treatment of quantum systems

Understanding of Maxwell Boltzmann, Fermi-Dirac and Bose Einstein gases

Knowledge of cooling techniques

Knowledge and understanding of basic theories of liquid helium behaviour and superconductivity in cooling techniques

##### Classical Mechanics (PHYS470)

**Level**M **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To provide students with an awareness of the physical principles that can be applied to understand important features of classical (i.e. non-quantum) mechanical systems.
- To provide students with techniques that can be applied to derive and solve the equations of motion for various types of classical mechanical systems, including systems of particles and fields.
- To develop students'' understanding of the fundamental relationship between symmetries and conserved quantities in physics.
- To reinforce students’ knowledge of quantum mechanics, by developing and exploring the application of closely-related concepts in classical mechanics.

**Learning Outcomes**Students should know the physical principles underlying the Lagrangian and Hamiltonian formulations of classical mechanics, in particular D’Alembert’s principle and Hamilton’s principle, and should be able to explain the significance of these advanced principles in classical and modern physics.

Students should be able to apply the Euler-Lagrange equations and Hamilton’s equations (as appropriate) to derive the equations of motion for specific dynamical systems, including complex nonlinear systems.

Students should be able to use advanced concepts in classical mechanics to describe the connection between symmetries and conservation laws.

Students should be able to apply advanced techniques, including conservation laws, canonical transformations, generating functions, perturbation theory etc. to describe important features of various dynamical systems (including systems of particles and fields) and to solve the equations of motion in specific cases.

##### Advanced Quantum Physics (PHYS480)

**Level**M **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on Y3 module on Quantum Mechanics and Atomic Physics with the intention of providing breadth and depth in the understanding of the commonly used aspects of Quantum mechanics.
- To develop an understanding of the ideas of perturbation theory for complex quantum systems and of Fermi''s Golden Rule.
- To develop an understanding of the techniques used to describe the scattering of particles.
- To demonstrate creation and annihilation operators using the harmonic oscillator as an example.
- To develop skills which enable numerical calculation of real physical quantum problem.
- To encourage enquiry into the philosophy of quantum theory including its explanation of classical mechanics.

**Learning Outcomes**At the end of the module the student should have:

- Understanding of variational techniques.
- Understanding of perturbation techniques.
- Understanding of transition and other matrix elements.
- Understanding of phase space factors.
- Understanding of partial wave techniques.
- Understanding of basic cross section calculations

Understanding of examples of state-of-the art quantum physics experiments.

Understanding of the implications of quantum physics in our daily lifes.

##### Accelerator Physics (PHYS481)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**70:30 **Aims**- To build on modules on electricity, magnetism and waves;
- To study the functional principle of different types of particle accelerators;
- To study the generation of ion and electron beams;
- To study the layout and the design of simple ion and electron optics;
- To study basic concepts in radio frequency engineering and technology.

**Learning Outcomes**At the end of the module the student should have:

- An understanding of the description of the motion of charged particles in complex electromagnetic fields;
- An understanding of different types of accelerators, in which energy range and for which purposes they are utilised;
- An understanding of the generation and technical exploitation of synchrotron radiation;
- An understanding of the concept and the necessity of beam cooling.

##### Stellar Populations (PHYS483)

**Level**M **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**To build upon the students'' knowledge of stellar evolution and describe techniques currently employed to investigate the evolution of stellar populations in the universe.

- To provide the physical background underlying these techniques, and study their application to observations of Galactic and extragalactic stellar systems

**Learning Outcomes**An understanding of the evolution with age and chemical composition of the Colour-Magnitude-Diagrams of resolved stellar populations.

Methods to estimate distances, ages and initial chemical compostions of resolved stellar populations.

An understanding of the evolution with age and chemical composition of the integrated photometric properties of stellar populations.

An understanding of the evolution of integrated spectral features of stellar populations with age and chemical composition.

Knowledge of age and chemical composition diagnostics from integrated photometry and spectroscopy of stellar populations.

##### Elements of Stellar Dynamics (PHYS484)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**75:25 **Aims**To show that there is more to gravity than Newton''s law. This will provide the students with a basic understanding of the dynamics of systems containing millions and billions of point-like gravitating bodies: stars in stellar clusters and galaxies.

**Learning Outcomes**At the end of the module the student should have the ability to

- Show how dynamical processes shape the structure of galaxies and stellar clusters
- Describe the motion of stars in stellar systems
- Apply orbital analysis to stellar systems
- Demonstrate an understanding of the implications of the continuity equation

##### Advanced Nuclear Physics (PHYS490)

**Level**M **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the year 3 modules on Nuclear Physics
- To offer an insight into current ideas about the description of atomic nuclei and nuclear matter

**Learning Outcomes**Knowledge of the basic properties of nuclear forces and the experimental evidence upon which these are based

Knowledge of the factors governing nuclear shapes

Understanding of the origin of pairing forces and the effect of these and rotational forces on nuclear behaviour

An overview of phenomena observed for exotic nuclei far from the line of nuclear stability

Knowledge of astrophysical nucleosynthesis processes

Knowledge of phases of nuclear matter

##### Research Skils (PHYS491)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- Perform literature searches.
- Plan research projects.
- Explain research projects to both expert and non-expert audiences.
- Organise a team of people and work as a group.
- Assess the broader impact of research projects.
- Present a proposal as a written document ans orally.

**Learning Outcomes**Experience in carrying out search of scientific literature. Communicating research to non-expert audience.

Evaluating the possible broader impact of research.Writing a scientific case for an assessment panel. First experience with some project management tools.

##### Advanced Particle Physics (PHYS493)

**Level**M **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the Year 3 module PHYS377 Particle Physics
- To give the student a deeper understanding of the Standard Model of Particle Physics and the basic extensions
- To review the detectors and accelerator technology available to investigate the questions posed by the Standard Model and its extensions

**Learning Outcomes**An understanding of the Standard Model and its extensions. This will be placed in context of the understanding of the origin of the universe, its properties and its physical laws

An understanding of how present and future detector and accelerator technology will be applied to investigate the development of the Standard Model

An understanding of the effects of symmetries on particle properties

Ablity to caclulate decay rates for particles

##### Astrophysics Research Skills (PHYS496)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**0:100 **Aims**- To demonstrate and provide experience of key aspects of professional practice in scientific research-related careers other than the research itself, such as peer review, proposal development, experimental design, and public communication of research results.
- To provide the opportunity for students to deepen their background understanding of specific astrophysics topics, especially those related to their final-year project.
- To develop the ability of the student to think critically about published scientific results, dealing with the objective criticism of existing articles, papers and lecture/seminar presentations, as well as the creation of new material and to communicate results and ideas in astrophysics at a range of technical levels.
- To help students bridge the gap between understanding undergraduate texts and dissecting a journal paper, while at the same time emphasising the importance of being able to communicate ideas concisely and clearly at a simpler level

**Learning Outcomes**The ability to create their own articles, research proposals, discussions, etc., building on the experience gained during the module, and to use this experience beyond the module content. The critical-thinking skills needed to form evidence-based arguments and communicate these persuasively in a wide range of contexts from peer review to formal proposal writing.

The ability to understand and objectively critique current arguments in astrophysics and communicate these appropriately at a range of levels up to to research seminars and proposals.

An understanding of professional practice in science research

A deeper knowledge of current topics in modern astrophysics

##### Magnetic Structure and Function (PHYS497)

**Level**M **Credit level**7.5 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**- To build on the third year module Condensed Matter Physics
- To develop an understanding of the phenomena and fundamental mechanisms of magnetism in condensed matter

**Learning Outcomes**Have a basic understanding of the quantum origin of magnetism and magnetic moments. Understand the concept of magnetic order and the role of exchange interactions.Be able to identify the properties associated with various types of magnetism.

Be able to explain the cause of magnetic phenomena such as hysteresis and domain formation.

##### Nanoscale Physics and Technology (PHYS499)

**Level**M **Credit level**15 **Semester**Second Semester **Exam:Coursework weighting**70:30 **Aims**- Tointroduce the emerging fields of nanoscale physics and nanotechnology
To describe experimental techniques for probing physical properties of nanostructured materials

Todescribe the novel size-dependent electronic, optical, magnetic and chemicalproperties of nanoscale materials

Todescribe several ‘hot topics'' in nanoscience research

Todevelop students'' problem-solving, investigative, communication and analyticskills through appropriate assignments for tutorials and a literature project.

**Learning Outcomes**After the module the students should have the ability to explain how and why nanoscalesystems form.

After the module the students should have the ability to describe how nanoscale systems may be probed experimentally and compare different techniques in terms of strengths and weaknesses.After the module the students should have the ability to explain and apply the fundamental principles that govern nanoscale systems.

After the module the students should have the ability to describe potential applications and to discuss their wider applications.

After the module the students should have enhanced problem-solving, investigative, communication, and analytic skills.

- Tointroduce the emerging fields of nanoscale physics and nanotechnology
##### Chaos and Dynamical Systems (MATH322)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**To develop expertise in dynamical systems in general and study particular systems in detail.

**Learning Outcomes**After completing the module students will be able to understand the possible behaviour of dynamical systems with particular attention to chaotic motion;

After completing the module students will be familiar with techniques for extracting fixed points and exploring the behaviour near such fixed points;

After completing the module students will understand how fractal sets arise and how to characterise them.

##### Relativity (MATH326)

**Level**3 **Credit level**15 **Semester**First Semester **Exam:Coursework weighting**100:0 **Aims**1. To introduce the physical principles behind Special and General Relativity and their main consequences.

2. To develop the competence in the mathematical framework of the subjects: Lorentz transformations and Minkowski space-time, semi-Riemannian geometry and curved space-time, symmetries and conservation laws, variational principles.

3. To develop the understanding of the dynamcis of particles and of the Maxwell field in Minkowski space-time, and of particles in a curved space-time.

4. To develop the knowledge of tests of General Relativity, including the classical tests (perihelion shift, gravitational deflection of light).

5. To understand the basic concepts of black holes, and, time permitting, of relativistic cosmology and gravitational waves.

**Learning Outcomes** To be be proficient in calculations involving Lorentz transformations, the kinematical and dynamical quantities associated to particles in Minkowski space-times, and the application of the conservation law for the four-momentum to scattering processes.

To know the relativistically covariant form of the Maxwell equations.

To know the action principles for relativistic particles, the Maxwell field and the gravitational field.

To be be proficient at calculations in semi-Riemannian geometry as far as needed for General Relativity, including calculations involving general coordinate transformations, tensor fields, covariant derivatives, parallel transport, geodesics and curvature

To understand the arguments leading to Einstein''s field equations and how Newton''s law of gravity arises as a limit.

To be able to calculate the trajectories of bodies in a Schwarzschild space-time.

The programme detail and modules listed are illustrative only and subject to change.

#### Teaching and Learning

Our research-led teaching ensures you are taught the latest advances in cutting-edge physics research. Lectures introduce and provide the details of the various areas of physics and related subjects. You will be working in tutorials and problem-solving workshops, which are another crucial element in the learning process, where you put your knowledge into practice. They help you to develop a working knowledge and understanding of physics. All of the lecturers also perform world class research and use this to enhance their teaching.

Most work takes place in small groups with a tutor or in a larger class where staff provide help as needed. Practical work is an integral part of the programmes, and ranges from training in basic laboratory skills in the first two years to a research project in the third or fourth year. You will undertake an extended project on a research topic with a member of staff who will mentor you. By the end of the degree you will be well prepared to tackle problems in any area and present yourself and your work both in writing and in person. In the first two years students take maths modules which provide the support all students need to understand the physics topics.