Physics (2013 entry)

MSc, 1 year full time/2 years part time

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Subject overview

Physics and astronomy at Sussex was ranked in the top 5 in the UK in The Times Good University Guide 2013, in the top 10 in the UK in The Sunday Times University Guide 2012, 16th in the UK in The Guardian University Guide 2014 and 21st in the UK in The Complete University Guide 2014.

The Department of Physics and Astronomy was ranked 12th in the UK in the 2008 Research Assessment Exercise, and top in the South East. 95 per cent of our research was rated as internationally recognised or higher, and 60 per cent rated as internationally excellent or higher.

Our research lies at the forefront of fundamental physics, ranging from quantum information processing, quantum optics, and cold atom physics, through a programme of top-rated particle physics experiments, to the theoretical understanding of space, time and matter.

The Department has a truly international character, with collaborations in Europe, North America, South East Asia and Australia.

The Department is a founder member of SEPnet, the South East Physics Network of physics departments, which in 2008 received a joint award of £12.5 million to enhance collaboration in graduate teaching and research.

South East Physics Network logo

Specialist facilities

A wide range of experimental facilities at Sussex, at national centres and at international laboratories is available to graduate students. The Atomic, Molecular and Optical Physics research group at Sussex operates state-of-the-art laboratories for quantum information processing with trapped ions, photons and electrons. Our experimental facilities include a range of high-precision laser systems from infrared to ultraviolet, as well as miniature ion and atom chips for the controlled manipulation of quantum bits. Sussex is one of only two places in the world with the capability to manufacture the optical-fibre cavities needed for quantum networking.

Our postgraduate students have access to a range of computing facilities including the University’s high-performance computing service. Our research groups have dedicated unix-based computing systems, and access to national and international super-computer facilities. The Experimental Particle Physics group is part of a Grid Tier-2 node and benefits from access to the Grid’s distributed high-performance computing resources. We are currently refurbishing all of our research and teaching laboratories.

Academic activities

Both taught and research students are expected to attend research seminars, and to contribute to their group’s discussions of the latest journal papers. PhD students have an opportunity to attend an international conference and give a paper on their specialist subject. Many experimentalist PhD students also have the opportunity to travel to various other sites, such as the Institut Laue-Langevin (ILL) in the French Alps, CERN in Geneva and SNOLAB in Canada. Most PhD students acquire considerable computing skills, which they find an asset in obtaining employment.

Programme outline

This MSc allows you to specialise in any of our faculty's research areas and particularly the fields of atomic, molecular and optical physics, as well as experimental particle physics.

Also refer to Department of Physics and Astronomy: Preparatory study

We continue to develop and update our modules for 2013 entry to ensure you have the best student experience. In addition to the course structure below, you may find it helpful to refer to the 2012 modules tab.

Full-time structure

You take six modules in total from: 

Autumn term: Atom Light Interactions • Cosmology • Data Analysis Techniques • Further Quantum Mechanics • General Relativity • Quantum Field Theory I • Stellar Structure • Symmetry in Particle Physics, or an option from mathematics, chemistry, biology, or engineering. 

Autumn and spring terms: Astronomy Research Skills. 

Spring term: Advanced Particle Physics • Astronomical Detector Technology and Instrumentation • Beyond the Standard Model • Early Universe • Galactic Structure • Particle Physics Detector Technology • Quantum Field Theory II • Quantum Optics and Quantum Computation, or an option from mathematics, chemistry, biology, or engineering. 

Up to two of the six modules may also be chosen from: 

Autumn term: Condensed State Physics • Introduction to C++ • Nuclear and Particle Physics. 

Spring term: Advanced Condensed State Physics • Particle Physics. 

Part-time structure

Distribution of modules over the two years is flexible and will be agreed between you, your supervisor and the module convenor. Most of your project work will naturally fall into the second year. 

Assessment 

Assessment for the taught modules is by coursework and unseen examination. Assessment for the project is by seminar, poster presentation, and a dissertation of not more than 20,000 words. 

Back to module list

Advanced Condensed State Physics

15 credits
Spring teaching, year 1

This module covers the following topics:

  • Electronic Energy bands in Solids. Electrons in periodic potentials; Brillouin Zones; Bloch states. Nearly Free Electron (NFE) model. Tight-Binding Approximation (TBA) model. Band structure of selected metals, insulators and semiconductors. Optical Properties.
  • Electron Dynamics. Electrons and holes. Effective Mass. Mobilities. Magneto-transport.
  • Semiconductors. Classification; Energy Gaps. Donor and Acceptor doping. Equilibrium carrier statistics in intrinsic and doped materials. Temperature dependence of electrical and optical properties.
  • Semiconductor Devices. p-n junctions. Diodes, LEDs, Lasers, Transistors. Superlattices and 2DEG devices. 
  • Lattice Defects. Types of defects. Electronic and optical effects of defects in semiconductors and insulators.

Advanced Particle Physics

15 credits
Spring teaching, year 1

You will acquire an overview of the current status of modern particle physics and current experimental techniques used in an attempt to answer today's fundamental questions in this field. 

The topics discussed will be: 

  • Essential skills for the experimental particle physicist
  • Neutrino physics: Neutrino oscillations and reactor neutrinos
  • Neutrino physics: SuperNova, geo- and solar- neutrinos and direct neutrino mass measurements
  • Cosmic ray physics
  • Dark matter
  • Introduction to QCD (jets, particles distribution functions, etc)
  • Higgs physics
  • BSM (including supersymmetry)
  • Flavour physics & CP violation
  • Electric dipole measurements
  • Future particle physics experiments.

Astronomical Detector Technology & Instrumentation

15 credits
Spring teaching, year 1

This module aims to provide you with: an overview of instrumentation and detectors; awareness of the topical cutting edge questions in the field; an appreciation of how scientific requirements translate to instrument/detector requirements and design.

This module covers:

  • An introduction to astronomy and astrophysics: fluxes, luminosities, magnitudes, etc. Radiation processes, black bodies, spectra. Stars.Galaxies. Planets. Cosmology
  • Telescopes and instruments: optical telescopes. Interferometry. Cameras. Spectroscopy. Astronomy beyond the e/m spectrum
  • Detectors by wavelength: gamma. X-ray. UV. Optical. NIR. Mid-IR. FIR. Sub-mm. Radio
  • Detector selection for a future space mission: scientific motivation and requirements. Detector options. External constraints, financial, risk, etc. Detector selection

 



Astronomy Research Skills

15 credits
Autumn teaching, year 1

Astrophysical Fluid Dynamics

15 credits
Autumn teaching, year 1

This module will introduce you to fluid dynamics with reference primarily to astrophysical flows, but accessible and of interest and value to all physics students. Topics covered include: fluid equations: conservation of mass and momentum; gravitation and the Poisson equation; energy and energy transport; hydrostatic equilibrium: atmospheres; stars as polytropes; Lane-Emden equation; homology relations; sound waves; shocks and blast waves; bernoulli: de Laval nozzle; spherical accretion; winds; instabilities: Rayleigh-Taylor; Kelvin Helmholtz; Jeans; thermal; viscous flows: accretion disks; magnetohydrodynamics.

Atom Light Interactions

15 credits
Autumn teaching, year 1

The module deals with the interaction of atoms with electromagnetic radiation. Starting from the classical Lorentz model, the relevant physical processes are discussed systematically. This includes the interaction of classical radiation with two-level atoms and the full quantum model of atom light interactions. Applications such as light forces on atoms and lasers are explored.

Beyond the Standard Model

15 credits
Spring teaching, year 1

This module covers:

  • Basics of global supersymmetry: motivation and algebra, the Wess-Zumino model, superfields and superspace, construction of supersymmetry-invariant Lagrangians.
  • Weak scale supersymmetry: the gauge hierarchy problem, the Minimal Supersymmetric Standard Model (MSSM).
  • Grand unification: SUS(5), the gauge sector, fermion masses, proton decay.
  • Extra dimensions: Kaluza-Klein reduction for scalars, fermions and gauge fields, generation of hierarchies, warped geometry.

Computational Chemistry

15 credits
Spring teaching, year 1

The aim of the module is to provide a guide to the various levels of theory (with their associated acronyms) appearing in the rapidly expanding field of computational chemistry, with a particular emphasis on quantum chemical methods. The module will start with the concept of a potential energy surface (stationary points, the Born-Oppenheimer approximation, etc), the types of computation normally performed, and the basic quantum mechanics of electrons and nuclei in molecules. The solution of the Schrodinger equation under different approximations will then be explored.

Introduction to Cosmology

15 credits
Autumn teaching, year 1

This module covers:

  • observational overview: In visible light and other wavebands; the cosmological principle; the expansion of the universe; particles in the universe.
  • Newtonian gravity: the Friedmann equation; the fluid equation; the acceleration equation.
  • geometry: flat, spherical and hyperbolic; infinite vs. observable universes; introduction to topology
  • cosmological models: solving equations for matter and radiation dominated expansions and for mixtures (assuming flat geometry and zero cosmological constant); variation of particle number density with scale factor; variation of scale factor with time and geometry.
  • observational parameters: hubble, density, deceleration.
  • cosmological constant: fluid description; models with a cosmological constant.
  • the age of the universe: tests; model dependence; consequences
  • dark matter: observational evidence; properties; potential candidates (including MACHOS, neutrinos and WIMPS)
  • the cosmic microwave background: properties; derivation of photo to baryon ratio; origin of CMB (including decoupling and recombination).
  • the early universe: the epoch of matter-radiation equality; the relation between temperature and time; an overview of physical properties and particle behaviour.
  • nucleosynthesis: basics of light element formation; derivation of percentage, by mass, of helium; introduction to observational tests; contrasting decoupling and nucleosynthesis.
  • inflation: definition; three problems (what they are and how they can be solved); estimation of expansion during inflation; contrasting early time and current inflationary epochs; introduction to cosmological constant problem and quintessence.
  • initial singularity: definition and implications.
  • connection to general relativity: brief introduction to Einstein equations and their relation to Friedmann equation.
  • cosmological distance scales: proper, luminosity, angular distances; connection to observables.
  • structures in the universe: CMB anisotropies; galaxy clustering
  • constraining cosmology: connection to CMB, large scale structure (inc BAO and weak lensing) and supernovae.

Data Analysis Techniques

15 credits
Autumn teaching, year 1

This module introduces you to the mathematical and statistical techniques used to analyse data. The module is fairly rigorous, and is aimed at students who have, or anticipate having, research data to analyse in a thorough and unbiased way.

Topics include: probability distributions; error propagation; maximum likelihood method and linear least squares fitting; chi-squared testing; subjective probability and Bayes' theorem; monte Carlo techniques; and non-linear least squares fitting.

Early Universe

15 credits
Spring teaching, year 1

An advanced module on cosmology.

Topics include:

  • Hot big bang and the FRW model; Redshifts, distances, Hubble law
  • Thermal history, decoupling, recombination, nucleosynthesis
  • Problems with the hot big bang and inflation with a single scalar field
  • Linear cosmological perturbation theory
  • Quantum generation of perturbations in inflation
  • Scalar and tensor power spectrum predictions from inflation
  • Perturbation evolution and growth after reheating; free streaming and Silk damping
  • Matter power spectrum and CMB anisotropies.

Electrons, Cold Atoms & Quantum Circuits

15 credits
Spring teaching, year 1

Topics covered include:

  • Basics of Penning trap technology. Motion and eigenfrequencies of a trapped particle.
  • Electrostatics and design of planar Penning traps. 
  • Electronic detection of a single trapped particle. 
  • The continuous Stern-Gerlach effect. Measurement of the Spin. 
  • Applications 1: Measurement of the electron's g-factor. Test of QED.
  • Applications 2: Measurement of the electron's mass. Mass spectrometry.
  • Trapping of neutral atoms with magnetic fields: Ioffe-Pritchard traps and the atom chip. 
  • Basics of Bose-Einstein condensation. 
  • Matter wave interferometry in atom chips: the adiabatic RF dressing technique.
  • Introduction to circuit-QED. Superconducting microwave resonators and artificial atoms.
  • Coherent quantum wiring of electrons, cold atoms and artificial atoms in a chip.

Experimental Quantum Technologies and Foundations

15 credits
Spring teaching, year 1

The module will introduce you to the practical implementation of quantum technologies. Topics include:

  • general introduction to quantum computers
  • ion trap quantum computers
  • quantum computing with superconducting qubits
  • quantum computing with neutral atoms
  • linear optics quantum computing
  • other quantum computing implementations
  • hybrid quantum technologies
  • quantum simulators
  • quantum cryptography
  • quantum effects in macroscopic systems
  • quantum effects in biological systems
  • foundations of quantum physics
  • quantum physics and philosophy

Fibre Optic Communications

15 credits
Spring teaching, year 1

Topics covered in this module include: analysis of slab wave-guide; analysis of step index fibre; dispersion in the step index fibre; mono-mode fibre; propagation of light rays in multi-mode graded index fibres; dispersion in graded index fibres, light sources and detectors; modulation of semiconductor light sources; transfer characteristic and impulse response of fibre communication systems; power launching and coupling efficiency; receiver principles and signal-to noise ratio in analogue receivers; receivers for digital optical fibre communication systems; system noise; system components and aspects of system design; coherent optical fibre communication; and network systems.

Further Quantum Mechanics

15 credits
Autumn teaching, year 1

Topics covered include:

  • Review of 4-vector notation and Maxwell equations. 
  • Relativistic quantum mechanics: Klein-Gordon equation and antiparticles.
  • Time-dependent perturbation theory. Application to scattering processes and calculation of cross-sections. Feynman diagrams.
  • Spin-1/2 particles and the Dirac equation. Simple fermionic scatterings.

 

Galaxies

15 credits
Spring teaching, year 1

This module covers:

  • Galaxy formation: linear perturbation theory; Growth and collapse of spherical perturbations; derivation of Jeans mass; hierarchical galaxy formation models, large-scale structures.
  • Virial theorem; Stellar dynamics and kinematics: Solutions of Poisson's equation; Oort's analysis; epicyclic motions; two-body relaxation
  • Phase-space distribution function and collisionless Boltzmann equation; Jeans theorems; Solutions of collisionless Boltzmann equation; application of Jeans' equations.
  • Galaxy groups and clusters; galaxy evolution; intergalactic medium.

General Relativity

15 credits
Autumn teaching, year 1

This module provides an introduction to the general theory of relativity, including:

  • Brief review of special relativity
  • Scalars, vectors and tensors
  • Principles of equivalence and covariance
  • Space-time curvature
  • The concept of space-time and its metric
  • Tensors and curved space-time; covariant differentiation
  • The energy-momentum tensor
  • Einstein's equations
  • The Schwarzschild solution and black holes
  • Tests of general relativity
  • Weak field gravity and gravitational waves
  • Relativity in cosmology and astrophysics.

Lasers

15 credits
Spring teaching, year 1

This module covers:

  • Light-matter interaction. 
  • Rate equations of lasers. 
  • Principles of Gaussian optics and optical cavities. 
  • Types of lasers and their applications.

Object Oriented Programming

15 credits
Autumn teaching, year 1

You will be introduced to object-oriented programming, and in particular to understanding, writing, modifying, debugging and assessing the design quality of simple Java applications.

You do not need any previous programming experience to take this module, as it is suitable for absolute beginners.

Particle Physics Detector Technology

15 credits
Spring teaching, year 1

The module explores the technical manner in which some of the scientific questions in the fields of experimental particle physics, including high energy physics, neutrino physics etc, are being addressed. You are introduced to many of the experimental techniques that are used to study the particle phenomena. The focus is on the demands those scientific requirements place on the detector technology and current state-of-the-art technologies.
This module aims to provide you with an introduction to some of the basic concepts of particle physics and an overview of some of the topical cutting edge questions in the field. As well as an understanding of some key types of experiments and a detailed understanding of the underlying detector technologies.

Module topics include:

  • Introduction to particle structure. Particles and forces, masses and lifetimes. Coupling strengths and interactions. Cross sections and decays
  • Accelerators. Principles of acceleration. Kinematics, center of mass. Fixed target experiments, colliders
  • Reactors.Nuclear fission reactors, fission reactions, types of reactors. Neutron sources, absorption and moderation, neutron reactions. Nuclear fusion, solar and fusion reactors
  • Detectors. Gaseous. Liquid (scintillator, cerenkov, bubble chamber). Solid-state. Scintillation. Calorimeters, tracking detectors. Particle identification
  • Monte Carlo modelling. Physics.

Particle Physics

15 credits
Spring teaching, year 1

Programming in C++

15 credits
Autumn teaching, year 1

After a review of the basic concepts of the C++ language, you are introduced to object oriented programming in C++ and its application to scientific computing. This includes writing and using classes and templates, operator overloading, inheritance, exceptions and error handling. In addition, Eigen, a powerful library for linear algebra is introduced. The results of programs are displayed using the graphics interface dislin.

Quantum Field Theory 1

15 credits
Autumn teaching, year 1

This module is an introduction into quantum field theory, covering

  • Action principle and Lagrangean formulation of mechanics
  • Lagrangean formulation of field theory and relativistic invariance
  • Symmetry, invariance and Noether's theorem
  • Canonical quantization of the scalar field
  • Canonical quantization of the electromagnetic field
  • Canonical quantization of the Dirac spinor field
  • Interactions, the S matrix, and perturbative expansions
  • Feynman rules and radiative corrections.

Quantum Field Theory 2

15 credits
Spring teaching, year 1

Module topics include:

  • Path integrals: Path integrals in quantum mechanics; Functionals; Path integral quantisation of scalar field; Gaussian integration; Free particle Green's functions ; Vacuum-vacuum transition function Z[J]. 
  • Interacting field theory in path integral formulation. Generating functional W[J]; Momentum space Greens functions; S-matrix and LSZ reduction formula; Grassmann variables; Fermionic path integral. 
  • Gauge field theory: Internal symmetries; Gauge symmetry 1: Abelian; The electromagnetic field; Gauge symmetry 2: non-Abelian. 
  • Renormalisation of scalar field theory; Quantum gauge theory; Path integral quantisation of non-Abelian gauge theories; Faddeev-Popov procedure, ghosts; Feynman rules in covariant gauge; Renormalisation.

Quantum Optics and Quantum Information

15 credits
Autumn teaching, year 1

The module will introduce you to quantum optics and quantum information, covering:

  • Quantum systems and the qubit
  • Non-locality in quantum mechanics
  • Methods of quantum optics
  • The density matrix
  • The process of measurement
  • Introduction of irreversibility
  • Decoherence and quantum information
  • Quantum and classical communication
  • Measures of entanglement and distance between states
  • Logic operations and quantum algorithms
  • Requirements for quantum computers
  • Physical systems for quantum information processing.

RF Circuit Design

15 credits
Autumn teaching, year 1

This module aims to provide an advanced knowledge of design techniques and current applications in RF Circuit Design. It covers the principles and tools used in the design, construction and testing of radio frequency circuits. Emphasis will be given to practical concepts through demonstrations and example. The module includes; RF transmitters and receivers, two port networks and scattering parameters, the design of impedance matching networks, noise and noise figure matching, low noise amplifiers, power amplifiers, classes and linearity techniques, receiver circuit systems, IF amplifiers, selectivity and RF filters, power combining techniques, wafer probing techniques, RF measuring equipment - spectrum analysers, network analysers.

Symmetry in Particle Physics

15 credits
Autumn teaching, year 1

The module provides an introduction into group theory and aspects of symmetry in particle physics, covering:

  • Groups and representations
  • Lie groups and Lie algebras
  • Space-time symmetries and Poincare group
  • Symmetry and conservation laws
  • Global, local, and discrete symmetry
  • Symmetry breaking and the origin of mass
  • Symmetry of the standard model, CKM matrix, neutrino masses, tree-level interactions.

Back to module list

Entry requirements

UK entrance requirements

A first- or second-class undergraduate honours degree in a physics-based subject (including mathematics and engineering degrees with significant physics content).

Those requesting experimental projects must have laboratory experience, and evidence must be supplied, usually in the form of a reference, of competence in the laboratory.

Overseas entrance requirements

Please refer to column B on the Overseas qualifications.

If you have any questions about your qualifications after consulting our overseas qualifications table, contact the University.
E pg.enquiries@sussex.ac.uk

Visas and immigration

Find out more about Visas and immigration.

English language requirements

IELTS 6.5, with not less than 6.5 in Writing and 6.0 in the other sections. Internet TOEFL with 88 overall, with at least 20 in Listening, 20 in Reading, 22 in Speaking and 24 in Writing.

For more information, refer to English language requirements.

Additional admissions information

We must receive your application by 1 August if you are a non-EEA student because this degree requires clearance by the UK Government Academic Technology Approval Scheme (ATAS).

For more information about the admissions process at Sussex

For pre-application enquiries:

Student Recruitment Services
T +44 (0)1273 876787
E pg.enquiries@sussex.ac.uk

For post-application enquiries:

Postgraduate Admissions,
University of Sussex,
Sussex House, Falmer,
Brighton BN1 9RH, UK
T +44 (0)1273 877773
F +44 (0)1273 678545
E pg.applicants@sussex.ac.uk 

Fees and funding

Fees

Home UK/EU students: £5,5001
Channel Island and Isle of Man students: £5,5002
Overseas students: £16,2003

1 The fee shown is for the academic year 2013.
2 The fee shown is for the academic year 2013.
3 The fee shown is for the academic year 2013.

To find out about your fee status, living expenses and other costs, visit further financial information.

Funding

The funding sources listed below are for the subject area you are viewing and may not apply to all degrees listed within it. Please check the description of the individual funding source to make sure it is relevant to your chosen degree.

To find out more about funding and part-time work, visit further financial information.

Leverhulme Trade Charities Trust for Postgraduate Study (2013)

Region: UK
Level: PG (taught), PG (research)
Application deadline: 1 October 2013

The Leverhulme Trade Charities Trust are offering bursaries to Postgraduate students following any postgraduate degree courses in any subject.

Sussex Graduate Scholarship (2013)

Region: UK, Europe (Non UK), International (Non UK/EU)
Level: PG (taught)
Application deadline: 16 August 2013

Open to final year Sussex students who graduate with a 1st or 2:1 degree and who are offered a F/T place on an eligible Masters course in 2013.

Faculty interests

For more detailed information, visit the Department of Physics and Astronomy. Our four research groups are focused on research into fundamental areas of science: 

Astronomy Centre

Dr Ilian Iliev uses supercomputer simulations to study the formation of large-scale cosmological structures, the cosmic dark ages and reionisation by the first stars.

Dr Antony Lewis works on theoretical and observational cosmology. He is involved with analysing data from the Planck Satellite.

Professor Andrew Liddle works on a range of topics in theoretical cosmology and dark energy. He is involved in the Planck Satellite and the Dark Energy Survey.

Dr Jon Loveday is an astronomer interested in observational cosmology, the nature of dark matter, and in galaxy formation. He participates in several world-leading optical and near-infrared galaxy surveys, including GAMA, SDSS, UKIDSS and VISTA.

Professor Seb Oliver is an astronomer researching the evolution of galaxies since the Big Bang. He undertakes surveys of the distant universe and leads the largest project on the Herschel mission.

Dr Kathy Romer is an observational cosmologist specialising in the detection and study of x-ray clusters of galaxies. She is the principal investigator of the international XMM Cluster Survey project.

Dr David Seery is a theoretical cosmologist working on the physics of the very early universe, and in particular the properties of the primordial density perturbation, which is believed to have seeded later structure formation.

Professor Peter Thomas uses supercomputer simulations to investigate the physics of galaxies and clusters of galaxies.

Atomic, Molecular and Optical Physics

Dr Claudia Eberlein is a theorist working on quantum optics and quantum field theory. 

Dr Barry Garraway heads this group and is a theoretical physicist with a particular research interest in quantum physics and quantum optics. 

Dr Winfried Hensinger researches ion quantum technology and is implementing new quantum technologies using ultracold-trapped ions. 

Dr Matthias Keller studies the interaction between single atomic ions and light to exchange information between quantum computers. 

Dr José Verdú aims to develop novel types of traps for electrons with applications to metrology.

Experimental Particle Physics

Dr Antonella De Santo heads this group and also leads the Sussex effort on ATLAS at CERN. She searches for supersymmetry in ATLAS data in a quest to uncover the nature of dark matter in the universe. 

Dr Elisabeth Falk seeks to find manifestations of new physics in both neutrino experiments and in proton-proton interactions at the Large Hadron Collider. 

Dr Mike Hardiman seeks to uncover the processes that led to the dominance of matter over anti-matter in the universe. 

Professor Philip Harris is spokesperson of the CryoEDM experiment. He makes high-precision measurements of the neutron electric dipole moment, searching for subtle effects from new physics beyond the Standard Model. 

Dr Jeff Hartnell is interested in fundamental properties of neutrinos. He works on the SNO+ experiment, attempting to determine whether the neutrino is its own anti-particle. 

Dr Simon Peeters heads the SNO+ effort at Sussex and is interested in fundamental properties of the neutrino. He is also involved in the DEAP-3600 experiment aimed at direct searches of dark matter. 

Dr Fabrizio Salvatore is involved in the ATLAS experiment at the CERN LHC, working on the experiment’s trigger system and on searches for supersymmetry in tau final states.

Theoretical Particle Physics

Dr Xavier Calmet investigates physics beyond the Standard Model of particle physics and in particular the Higgs sector. 

Professor Mark Hindmarsh is a world expert on the physics of the early universe and looks at the dynamics of strings in cosmology. 

Dr Stephan Huber works on early universe cosmology and particle physics beyond the Standard Model. 

Dr Sebastian Jaeger’s research centres on indirect ways to find new particles via their virtual effects. 

Dr Daniel Litim heads this group and is a world leader of renormalisation group approaches to fundamental interactions in quantum field theory. 

 

 

Careers and profiles

Our graduates go on to take research degrees, or take up employment in a range of industries in roles such as business/data analysis, computer programming, software development, teaching, or research and teaching technical support.

James's student perspective

James Sinclair

‘When I first started my MSc at Sussex I struggled after nearly three years out of education. But the Department of Physics and Astronomy was welcoming, and you quickly build relationships with staff. Lecturers are always willing to answer questions – their doors are always open. The Study Direct website contains a lot of valuable material for further reading, and peer-assisted learning sessions are also useful in providing different perspectives on the subject.

‘As for experimental projects, my supervisor always makes time for me and we normally have several meetings a week. Being part of a research group is a great help, putting you in contact with post-docs, PhD students and professors working in your field of interest who are willing to answer even the most naive of questions. Working within the group also proves quite an incentive, once you can see where, and how, your efforts are being applied. This working environment is the reason I have accepted a PhD within the Department!’

James Sinclair
MSc in Physics

For more information, visit Careers and alumni.

School and contacts

School of Mathematical and Physical Sciences

The School of Mathematical and Physical Sciences brings together two outstanding and progressive departments – Mathematics, and Physics and Astronomy. It capitalises on the synergy between these subjects to deliver new and challenging opportunities for its students and faculty.

Physics and Astronomy, PG Admissions,
University of Sussex, Falmer,
Brighton BN1 9QH, UK
E msc@physics.sussex.ac.uk
Department of Physics and Astronomy

Discover Postgraduate Study information sessions

You’re welcome to attend one of our Discover Postgraduate Study information sessions. These are held in the spring and summer terms and enable you to find out more about postgraduate study and the opportunities Sussex has to offer.

Visit Discover Postgraduate study to book your place.

Other ways to visit Sussex

We run weekly guided campus tours every Wednesday afternoon, year round. Book a place online at Visit us and Open Days.

You are also welcome to visit the University independently without any pre-arrangement.

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