QMUL_PHYSICS and ASTRONOMY_UG

Queen Mary, University of LondonSchool of Physics and AstronomyUndergraduate Studies

www.ph.qmul.ac.uk

The east LondonadvantageBarts and The London serves ahuge population of unrivalleddiversity in the east of London,but is also next door to the City ofLondon, one of the UK’s richestneighbourhoods. This means thatour medical and dental studentsencounter a huge range ofmedical conditions while buildingthe patient contact hours theyneed to become confident andcompetent professionals.

“East London and the widerThames Gateway offer ourmedical students the opportunityto observe a wide range ofdiseases – from diabetes,hypertension, heart disease,cancer, obesity, TB and evenmalnutrition. This is a uniquelearning environment for theirmedical training.”Cathy Baker, Head of GraduateEntry Programme in Medicine

2012 Olympics onour doorstepThe 2012 Olympics are takingplace very close to Queen Mary’sMile End campus, and ourWhitechapel and West Smithfieldcampuses are also not far away.Barts Hospital, the new RoyalLondon Hospital and ourassociated Trusts will providehealthcare for the Olympicathletes and the general publicduring the summer games. Thiswill be an exciting time to be inLondon.

Campus-basedBarts and The London is part ofQueen Mary, the only College ofthe University of London to offerextensive campus-based facilities.This promotes a sense ofcommunity and encourages anactive student life. All our firstyear medical and dental studentswho live a certain distance fromthe School are allocated places inresidences at the Whitechapel,Charterhouse Square and MileEnd campuses. East London alsooffers affordable privately-ownedaccommodation at a walkingdistance from our campuses. Seepage XX for more details aboutaccommodation.

State-of-the-artclinical facilitiesWe have modern state-of-the artbuildings alongside moretraditional teaching facilities suchas our fantastic library. The DentalSchool now contains a clinicalskills laboratory which closelysimulates the real clinical

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Contents

Introduction 2

Degree programmes 6

Module descriptions 10

Career opportunities 20Student life, Students’ Union, student support and health services 24

Accommodation 26School of Physics and AstronomyEntry requirements 28

Living in London 30

Frequently asked questions 34

Next steps 38

Campus map 40

Introduction

School of Physics and Astronomy 3

School of Physics and Astronomy at Queen Mary, University of London

Welcome to theSchool of Physicsand Astronomy at Queen Mary,University of LondonThe School maintains a longtradition of excellence in ground-breaking research combined witha commitment to maintaining thehighest standards of studenteducation, giving our graduatesthe best possible preparation fortheir chosen careers. In fact over91% were in a graduate level jobsix months after leaving (source:Destination of Leavers fromHigher Education survey).

Research in the School isorganised into four centres: high-energy particle physics,condensed matter physics,theoretical physics andastrophysics. All of these groupscontribute to the teaching on ourdegree programmes. These coverthe key areas of Physics, ParticlePhysics, Astrophysics andTheoretical Physics, all at BSc orMSci level.

Queen Mary's record in this areahas been acknowledged by aninvitation to join the Russell Groupof research-intensive universities.This group is committed tomaintaining the very bestresearch, an outstanding teachingand learning experience, excellentgraduate employability andunrivalled links with business andthe public sector.

We have dedicated support staff,covering all academic and pastoralareas, to help and advise youduring your time at university.Studying at university is anopportunity and a challenge, andcan be a very rewarding experienceboth intellectually and personally.We are committed to helping you tobenefit as much as possible duringyour time with us.

By the end of your degree you willhave attained a thoroughknowledge of modern physicsalong with high level analytical,problem-solving and researchskills. These will open up careeropportunities across a spectrumfrom postgraduate research todiverse careers in business. Wealso provide opportunities for paidsummer research internshipswithin our research centres, aswell as those in other universities,plus a wide variety of paidsummer employer placements inindustry. Visit: www.ph.qmul.ac.uk/undergraduate/internships

Our reputation is built on thequality of our graduates. Whatevertheir choice of degree programme,career aims, or other interests, ourstudents have reported high levelsof satisfaction with our teachingand support, and have gone on tobuild successful careers in manyprofessions. Should you enrol atQueen Mary I have everyconfidence that you would jointhem.

Professor William J Spence, Head of School of Physics and Astronomy and Professor of Theoretical Physics

What is physics?Physics is fundamental in helpingus understand how our worldworks: from the behaviour ofprotons and electrons to themovement of the stars andplanets. Theory and experimentare vital to developing answers toquestions about the universe andhow things work. Technologicaladvances and benefits to our dailylives often come as a result of thepursuit of new knowledge, oneexample being the development ofthe language of the Internet. Thiswas developed as a way to sharehuge amounts of informationrapidly and easily by a researchteam at the particle physicslaboratory, CERN. The new LargeHadron Collider (LHC) experimentat CERN is developing a new formof cloud computing called GridPP.

Within the discipline of physicsyou will find subsections coveringthe full spectrum of scales:particle physics for the smallestparticles; nano-science forcreating new small structures; andgeneral relativity forunderstanding large scalebehaviour of the universe. Onetheory that physics is lacking,however, is the Grand UnifiedTheory, and many physicists areworking to find the one theory thatapplies to all scales, so there’splenty of work still to be done.

Why study physics?As a physicist you have agrounding in both theoretical andexperimental principles. Thisresults in a way of thinking that

School of Physics and Astronomy4

School of Physics and Astronomy at Queen Mary, University of London

can be applied not only within thefield of physics, but to other real-world situations, for example thestock market.

The nature of physics means thatyou need to continue yourmathematical studies, so youshould either enjoy the applicationof mathematics or be comfortableusing mathematical tools.

A physics degree provides youwith:

• a practical approach to problemsolving

• high level research skills

• the ability to reason andcommunicate complex ideas

• excellent IT skills through theuse of word processing andspreadsheets with additionalknowledge of computerprogramming

• the ability to manage your timeeffectively

• experience of working withothers

• confidence in reporting/presenting the work to others inthe form of projects, essays orseminars.

Why study physicsat Queen Mary?Our degree programmes aresupported by our researchstrengths. Students directlybenefit from the high qualityresearch carried out by ouracademic staff – the researchwork they do informs theirteaching.

The School of Physics andAstronomy is located in the GOJones building on our Mile Endcampus. While lectures and

tutorials may be held in otherbuildings around campus, thereare many facilities within the GOJones building for your use. Theseinclude: the Physics Museumwhere undergraduates worktogether on material covered inlectures, the Hive study area, theundergraduate teachinglaboratories, and the centraladministration area where you canhand in your coursework and talkto support staff such as theStudent Support Administrator.

Our academic and support staffare on hand to advise you fromthe first day of term. You areassigned an academic adviserwho will help you make yourmodule choices. Someprogrammes are more flexiblethan others. See the informationon programme structure on p5.

We have a full-time StudentSupport Administrator who isthere to help with any queries orproblems during the academicyear. They are the first point ofcontact for any student concerns,be they academic or pastoral.They are available to provideadvice and guidance on matterssuch as student funding,bursaries and financial support,accommodation and welfareconcerns, help with special examarrangements for those studentsin need of additional support andoffers advice on careers andfurther study.

Our undergraduate society PsiStarorganises regular social events forundergraduates and encourages

first year students to participate inthe Peer Assisted Study Support(PASS) scheme for academichelp. PASS mentors are second orthird year students who work withfirst year students to help themwith any parts of their academicmodules that they have notunderstood. These mentors alsohelp to ease first year students’transition from school or college to university. They clearlyunderstand what first years aregoing through having recently had the same experience.

ProgrammestructureYour studying is arranged so thatyou take eight different modules

in each academic year for allprogrammes. You are required totake four in each semester.Semester A runs from Septemberto December and Semester Bruns from January until April.

Generally for each module you willhave three or four hours oflectures per week and one or twohours of tutorials or exerciseclasses. If you are taking apractical module, such asScientific Measurement in the firstyear, you will spend twoafternoons a week in ourundergraduate laboratory.

Our degrees are structured so thatyou take a number of compulsorymodules. In the first year, thecompulsory modules are common

across all degree programmes.From the second year onwards,you have a number of optionsavailable. The exact number ofoptions will depend on yourchoice of degree programme. Forexample, if you are studyingastrophysics you will have feweroptional module choices thansomeone studying physics. Youwill find a detailed outline of eachprogramme further on in thisbrochure.

All of our degree programmes areaccredited by the Institute ofPhysics: www.iop.org

Once in employment you canwork towards Chartered Physiciststatus which shows you have anaccredited degree and havereached high professionalstandards in your job.


Degree programmes


Degree programmes

Physics F300 BSc/Phy (three years) F303 MSci/Phy (four years)

Programme description The range of research in ourdepartment reflects the breadth ofthis subject: from understandingthe most basic building blocks inour universe through particlephysics, to building structures andmanipulating matter on amolecular scale with condensedmatter physics to understandingthe formation of stars andgalaxies. A degree in physicsgives you knowledge of theories,techniques and mathematicalapproaches which can be appliedin many different careers (seepage 16 for information on whatour graduates go on to do).

Programme outline Year 1 Electric and MagneticFields • From Newton to Einstein• Mathematical Techniques 1 •Mathematical Techniques 2 •Quantum Physics • ScientificMeasurement • Waves andOscillations • Options include:Introduction to C++ • OurUniverse

Year 2 Condensed Matter A •Electromagnetic Waves and Optics• Nuclear Physics andAstrophysics • Physics Laboratory• Quantum Mechanics A •Thermal and Kinetic Physics •Options include: MathematicalTechniques 3 (core for MSci) •Physics of Energy and theEnvironment • Planetary Systems •Physics of Galaxies • PhysicalDynamics

Year 3 Extended IndependentProject (MSci: Physics ReviewProject) • Elementary ParticlePhysics • Statistical Physics •Synoptic Physics • Optionsinclude: Advanced C++ •Communicating and TeachingPhysics • Condensed Matter B •Fluid Dynamics • Group Project •Mathematical Techniques 4 •Quantum Mechanics B (Core forMSci) • Quantum Mechanics andSymmetry (Core for MSci) •Physical Cosmology • RadiationDetectors • Solid State Physics(Core for MSci) • Space Time and Gravity • Stars

Year 4 Physics InvestigativeProject or Physics ResearchProject • Options include:Advanced Cosmology • AdvancedQuantum Field Theory •Astrophysical Plasmas • Atomand Photon Physics • CondensedMatter • ElectromagneticRadiation in Astrophysics •

Electromagnetic Theory •Electrons in Solids • ElectronicStructure Methods • ExtrasolarPlanets and Astrophysical Discs •The Galaxy • Low TemperaturePhysics and Nanotechnology •Molecular Physics • ParticlePhysics • Plasma Physics •Relativistic Waves and QuantumFields • Relativity and Gravitation• Solar System • Stellar Structureand Evolution

Astrophysics F526 BSc/Asph (three years)F523 MSci/Asph (four years)

Programme description There are lots of questions aboutthe origin and evolution of theuniverse that we do not haveanswers to yet. However,astrophysics can help usinvestigate our surroundings by applying our knowledge ofphysics and mathematics to the


Degree programmes

observations of stars, galaxies and planets. This allows us toinvestigate how old we think theuniverse is, how and why it isexpanding, how the planetsformed and if there is potential for life on other planets.

Programme outline Year 1 Electric and MagneticFields • From Newton to Einstein• Mathematical Techniques 1 •Mathematical Techniques 2 •Our Universe • Quantum Physics• Scientific Measurement •Waves and Oscillations

Year 2 Condensed Matter A •Electromagnetic Waves andOptics • Nuclear Physics andAstrophysics • Planetary Systems• Quantum Mechanics A • Stars •Thermal and Kinetic Physics

Options include: PhysicsLaboratory • Physics of Energyand the Environment •Introduction to C++

Year 3 Extended IndependentProject (MSci: Physics ReviewProject) • Physical Cosmology •Physics of Galaxies • Space Timeand Gravity • Statistical Physics •Synoptic Physics

Options include: Advanced C++ •Condensed Matter B •Communicating and TeachingPhysics • Elementary ParticlePhysics • Fluid Dynamics • GroupProject • Quantum Mechanics B• Mathematical Techniques 4 •Radiation Detectors

Year 4 Physics InvestigativeProject or Physics ResearchProject. Choose at least two from:Advanced Cosmology • ExtrasolarPlanets and Astrophysical Discs •Planetary Atmospheres • SolarPhysics • Stellar Structure andEvolution • Options include:Advanced Quantum Field Theory• Astrophysical Plasmas • Atomand Photon Physics • CondensedMatter • ElectromagneticRadiation in Astrophysics •Electromagnetic Theory •Electrons in Solids • ElectronicStructure Methods • The Galaxy •Low Temperature Physics andNanotechnology • MolecularPhysics • Particle Physics •Plasma Physics • RelativisticWaves and Quantum Fields •Relativity and Gravitation • SolarSystem

Physics with ParticlePhysics F392 BSc/PWPP (three years)F393 MSci/PWPP (four years)

Programme description Understanding what the universeis made from and how particlesinteract is the goal of particlephysics research. We can design,build and analyse data fromleading experiments worldwide to help achieve this. Specialistmodules have been designedspecifically for this degreeprogramme and your researchproject will be with an academicmember of staff from the ParticlePhysics Research Centre, so youcould find yourself working onexperimental results from the

ATLAS experiment in CERN or theT2K experiment sited in Japan.

Programme outline Year 1 Electric and MagneticFields • From Newton to Einstein• Mathematical Techniques 1 •Mathematical Techniques 2 •Quantum Physics • ScientificMeasurement • Waves andOscillations • Introduction to C++

Year 2 Condensed Matter A •Electromagnetic Waves andOptics • Nuclear Physics andAstrophysics • Physics Laboratory• Quantum Mechanics A •Thermal and Kinetic Physics •Options include: Our Universe •Physics of Energy and theEnvironment • Physical Dynamics• Stars

Year 3 Extended IndependentProject (MSci: Physics ReviewProject) • Elementary ParticlePhysics • Statistical Data Analysis• Statistical Physics • SynopticPhysics • Options include:Advanced C++ • CommunicatingPhysics • Condensed Matter B •Fluid Dynamics • Group Project •Mathematical Techniques 4 •Quantum Mechanics B •Quantum Mechanics andSymmetry • Physical Cosmology• Radiation Detectors • SolidState Physics • Space Time andGravity • Stars

Year 4 Physics InvestigativeProject or Physics ResearchProject • Particle AcceleratorPhysics • Particle Physics •Relativistic Waves and QuantumFields • Options include:


Advanced Cosmology • AdvancedQuantum Field Theory •Astrophysical Plasmas • Atomand Photon Physics • CondensedMatter • ElectromagneticRadiation in Astrophysics •Electromagnetic Theory •Electrons in Solids • ElectronicStructure Methods • ExtrasolarPlanets and Astrophysical Discs •The Galaxy • Low TemperaturePhysics and Nanotechnology •Molecular Physics • ParticlePhysics • Plasma Physics •Relativity and Gravitation • SolarSystem • Stellar Structure andEvolution

Theoretical Physics F340 BSc/ThPhy (three years)F323 MSci/ThPhy (four years)

Programme description The most fundamental questionsabout the universe are examinedusing the tools of theoreticalphysics. What is the origin ofmass? What is dark matter? Domore than four dimensions exist?These kinds of questions can be

considered by examining currenttheories, identifying theirweaknesses and proposing newsolutions. Investigations bymembers of the Centre forResearch in String Theory arehaving an impact on areas suchas particle physics: Twistor StringTheory is giving us a newsimplified understanding ofparticle scattering in the LargeHadron Collider.

Programme outline Year 1 Electric and MagneticFields • From Newton to Einstein• Mathematical Techniques 1 •Mathematical Techniques 2 •Quantum Physics • ScientificMeasurement • Waves andOscillations • Options include:Introduction to C++ • OurUniverse

Year 2 Condensed Matter A •Electromagnetic Waves andOptics • Mathematical Techniques3 • Nuclear Physics andAstrophysics • Physical Dynamics• Quantum Mechanics A •Thermal and Kinetic Physics •

Options include: PhysicsLaboratory • Physics of Energyand the Environment • PlanetarySystems • Physics of Galaxies

Year 3 Extended IndependentProject (MSci: Physics ReviewProject) • Elementary ParticlePhysics • Quantum Mechanics B• Solid State Physics • StatisticalPhysics • Synoptic Physics •Options include: Advanced C++ •Communicating and TeachingPhysics • Condensed Matter B •Fluid Dynamics • Group Project •Mathematical Techniques 4 •Quantum Mechanics andSymmetry • Physical Cosmology •Radiation Detectors • Space Timeand Gravity • Stars

Year 4 Physics InvestigativeProject or Physics ResearchProject • Advanced QuantumField Theory • ElectromagneticTheory • Relativistic Waves andQuantum Fields • StatisticalMechanics • Options include:Advanced Cosmology •Astrophysical Plasmas • Atomand Photon Physics • CondensedMatter • ElectromagneticRadiation in Astrophysics •Electrons in Solids • ElectronicStructure Methods • ExtrasolarPlanets and Astrophysical Discs •The Galaxy • Low TemperaturePhysics and Nanotechnology •Molecular Physics • ParticlePhysics • Plasma Physics •Relativity and Gravitation • SolarSystem • Stellar Structure andEvolution

Moduledescriptions


Module descriptions

This section contains a selectionof our modules and includes coremodules for the different degreeprogrammes, however please notethat there are more optionalmodules available to choose from.The list is organised by year withthe core modules being listedbefore optional modules. Fulldetails can be found on ourwebsite: www.ph.qmul.ac.uk/

Year 1Electric and Magnetic FieldsThis is an introduction to thebasic laws of electricity andmagnetism, including Maxwell’sequations. By the end of themodule you will be able tomathematically state the laws,whilst also be able to explain andapply the laws to solve a variety ofproblems.

From Newton to EinsteinThis module reviews thedevelopments in ourunderstanding of the laws ofspace, time and motion, from theseventeenth century to thepresent day. Topics from classicalmechanics include kinematicsand dynamics, gravity andplanetary orbits. Special relativity,length contraction and timedilation, general relativity andblack holes are covered inrelativistic mechanics.

Mathematical Techniques 1An understanding ofmathematics, calculus in themain, is required in the study ofthe physical sciences. Complexnumbers, differentiation, partial

differentiation, series, integration,polar coordinates and multipleintegration are particular areascovered by this module.

Mathematical Techniques 2Following from MathematicalTechniques 1, this modulecontinues work on some topicsand extends into others. You willstudy: complex numbers andhyperbolic functions; polar andspherical coordinates andcoordinate transformations;multiple integrals; line and surfaceintegrals; vector algebra; vectorcalculus; the theorems of Gauss,Green and Stokes; matrices;determinants; eigenvalues andeigenvectors; Fourier series andtransforms including theconvolution theorem; anddifferential equations.

Quantum PhysicsHere you will study the evidencefor particle-like properties ofwaves and wave-like properties ofparticles. This is followed by astudy of their consequences andtheir formal expression in physicallaw: topics include Heisenberg’sUncertainty Principle andSchroedinger’s equation.

Scientific MeasurementIn this module you will learnvaluable laboratory techniquesand skills: from measurementtechniques to data analysis andreporting; you will find all of theseskills necessary to carry outexperimental investigations intoconcepts in physics.

Waves and OscillationsThis module provides anintroduction to oscillatoryphenomena and wave motion.The concepts covered in thiscourse can be found throughoutnature, from biology to quantummechanics.

Some examples of areas coveredinclude: free, damped, forced andcoupled oscillations (illustrated byexamining the simple pendulum,an LC circuit and Helmholtzresonator); resonance and simpleharmonic motion are explored;with regards to waves, they areexamined in linear media and the1D wave equation is calculatedunder various conditions and thebehaviour of waves in gases andsolids is looked at along withsound and electromagnetic waves.

Introduction to C++ ProgrammingDeveloping your computerprogramming skills is animportant part of yourundergraduate studies. In thisintroductory course no priorprogramming knowledge isassumed. You are taught thebasics of writing and compilingC++ code within a robusttheoretical framework ofincreasing complexity.

Our UniverseThis module is intended to makeyou familiar with the componentswhich make up our universe: fromstars and planets to solar systemsand galaxies. The role of theknown laws of physics inunderstanding observations isinvestigated.


Module descriptions

Year 2Electromagnetic Waves and OpticsA triumph of Nineteenth Centuryphysics was the unification of thetheories of electricity andmagnetism. This module will giveyou an understanding ofMaxwell’s equations, theelectromagnetic wave equation,diffraction, interference effectsand polarisation.

Nuclear Physics and AstrophysicsYou will be introduced to theconcept of the atomic nucleusalong with the various forms ofradioactivity and their properties.We explore the possible decaymodes (radioactive decay andfission) of the nuclei and learnhow these properties help explainthe cosmological abundances ofnuclides via the big bang andstellar nucleo-synthesis.

Physics LaboratoryThis module covers theapplications of the principles ofphysics explained in other areasand aims to demonstrate theimportance of experimentalphysics to the understanding ofthe subject. This module ismarked by continuousassessment of laboratorynotebooks. You will learn how towrite up experiments as aresearch paper from your labbook. There are eight experimentsto be completed and each take 6hours. Examples of experimentsinclude: building a helium laser,

observation of nuclear magneticresonance and X-ray diffractionspectroscopy.

Quantum Mechanics AThis module aims to introduce thefundamental concepts ofquantum mechanics from thebeginning. By studyingapplications of the principles ofquantum mechanics to simpleone-dimensional systems, themodule will provide a foundationfor understanding concepts suchas energy quantisation, theuncertainty principle andquantum tunnelling, illustratingthese with experimentaldemonstrations and otherphenomena found in nature.

Thermal and Kinetic PhysicsThis module is an introduction tostatistical physics. The aim of thisarea of physics is to establish lawsand descriptions of matter on a

macroscopic scale and to relatethese macroscopic concepts tothe microscopic laws whichgovern the behaviour of morefundamental building blocks ofmatter. We will concentrate on thenotion of energy and itstransformations using mainlyclassical ideas. Key ideas in thesecond year course will includethe concept of equilibrium,temperature and entropy, and anintroduction to the kineticdescription of gases in equilibriumand of phenomena such asdiffusion and heat conduction.

Mathematical Techniques 3The aim is to explain the use ofmathematics as a tool forformulating and solving problemsin physics. This module will coverthe area of matrices, vectors andaspects of calculus. You willdevelop the use of index notationas a powerful tool formanipulating matrices andvectors. You will solve a variety of


1st and 2nd order differentialequations both ordinary andpartial for physical problems usingvarious methods, includingseparation of variables and Greenfunction techniques.

Physics of Energy and theEnvironmentThis module examines conceptsand equations of physics(including mechanics,thermodynamics, waves, quantumphysics) with respect to energytransfer processes in naturalenergy sources, and in energytechnologies. Analysis ofefficiencies of energy transfer willbe included. The emphasis will beon useful quantitative results fromphysics rather than detailedderivations. Examples will bedrawn from wind, wave, solar andnuclear energies. The relevance ofPhysics in understanding andimproving energy technologies aswell as assessing theirenvironmental impact will beemphasised. Specific topics willinclude; first and second laws ofthermodynamics, wind energy,Betz limit on efficiency of windturbines, solar energy,semiconductor physics relevant tosolar cells, radioactivity, nuclearreactors and nuclear wastedisposal.

Planetary SystemsHuman beings have charted thepaths of the planets across thenight sky and speculated abouttheir nature for thousands ofyears. Indeed the word planet has

its origin in the ancient Greekterm ‘planete’ – meaningwanderer. Used in its modernscientific context the word planetrefers to an object which orbitsabout a star, but which itself is nota star. Planets have a specialphilosophical significance sincethey are the bodies on which lifeitself is expected to come intoexistence. This module providesan in depth description of ourcurrent knowledge andunderstanding of the planets inour Solar System, and of theplanetary systems now known toorbit around stars other than theSun – the extra-solar planets. Theproperties of individual planetsand their satellites will bedescribed and contrasted, andbasic physical principles will beused to explain their orbits andphysical features. Ourunderstanding of how planetarysystems form will be explored,and current scientific ideas aboutthe origin of life will be discussed.

Physics of GalaxiesThere are a variety of differenttypes of galaxies and you willlearn their categories and how toestimate properties such as massand luminosity. As well asexploring the properties ofgalaxies, you will also learn aboutthe evolution of structure in theuniverse.

Physical DynamicsThis module is a more specialised- and at the same time a broader- study of mechanical ideas thanthe first year module From

Newton To Einstein. The basicphysics is mainly Newtonian, butthe module will cover a number ofmore technical ways of expressingthose ideas which enable you tounderstand better the role ofsymmetry and the role ofgeometrical ideas in mechanics.In addition you will learn how toset up and solve in an efficientway a number of "harder''mechanics problems.

Year 3Extended Independent ProjectThis project runs throughout thefinal two semesters of your degreeprogramme. You will be expectedto study a problem in physics anddevelop your design,experimental, computational andanalytical skills throughindependent study. You willproduce a final written report onyour project which could involvethings such as simulating aphysical process, carrying outexperiments to test a currenthypothesis or building a piece ofequipment.

Physics Review ProjectYou will use scientific researchliterature to examine a specialisedarea of physics. This will be acombination of directed readingand independent study. By theend of this project you will haveinvestigated an area of physics ofinterest to you to a deeper degreethan is normally possible inconventional modules.

Module descriptions

Elementary Particle PhysicsThis module covers anonmathematical introduction tothe standard model of particlephysics – the strong andelectroweak interactions betweenthe basic constituents of theworld, quarks and leptons, via theexchange of gluons, photons andW and Z particles. You will alsocover the following topics: 'Particleastrophysics – the relationshipbetween particle physics andcosmology'; 'Beyond the standardmodel – Grand unified theoriesand supersymmetry'.

Statistical PhysicsWe use this subject to help us tobridge the gap betweenmicroscopic quantum mechanicsand the behaviour of matter as weobserve it daily on a macroscopicscale. This module will teach youthe theoretical basis of statisticalphysics. You will also develop thevaluable skill of usingspreadsheets to calculate andvisualise complex algorithmicexpressions.

Synoptic PhysicsA study only module providinghighly structured professorialtutorials aimed at bringingtogether and summarising themain elements of physics. At theend of the module, you should beable to answer oral questionsaddressed to the generality of anytopic within the area of studyknown as physics and especiallywithin the subjects of gravitationaland rotational forces,electromagnetism and Lorentzforces, optics and interference,

thermodynamics and nuclear andastrophysics. In addition, youshould be able to respond to moredetailed questions on the subjectof any project you are completing.In all cases, you should be able todemonstrate an intimateknowledge of the help provided bydimensional analysis, symmetryand conservation rules.

Communicating and TeachingPhysicsThis module gives you theopportunity to contribute toteaching physics at secondaryschool level. Being able toeffectively communicate physicsto others is an important skill todevelop. In this module you willobserve teaching in a local school,act as a classroom assistant andprogress onto whole classteaching for part of a lesson. Themodule is assessed based on thecompletion of a project, in

conjunction with your teachingmentor. Previous examples ofprojects have included setting upan after school or lunchtime clubfor pupils or participating inmentoring sessions for gifted andtalented students.

Mathematical Techniques 4You will develop your knowledgeand skill in using advancedtechniques in mathematicalphysics. Taught in three parts, thefirst will look at the area ofanalysis covering Fouriertransforms, differential equations,special functions, asymptoticseries and complex analysis. Thesecond will cover groups, algebraand representations. The thirdand final section will covergeometry, including differentialforms, homology and topologicalinvariants.



Quantum Mechanics BThis module has an extendedexposition of the basic principlesand applications of quantummechanics. Topics include:Operators and the generalstructure of quantum mechanics,observables, orthonormality ofeigenstates, expansion theorem,commuting operators, theory ofmeasurement; The harmonicoscillator; Angular momentumtheory, the rigid rotator andapplications to rotation-vibrationspectra of diatomic molecules;Spin in quantum mechanicsillustrated with spin1/2: matrixrepresentations, Stern-Gerlachexperiments and measurementtheory exemplified;Indistinguishable particles inquantum mechanics: bosons andfermions; Spherically symmetricpotentials and the Hydrogenatom.

Quantum Mechanics and SymmetryThis module will give students agrounding in a more formal way toquantum mechanics andintroduce you to the application ofthese tools in the quantummechanical description ofsymmetries in particle physics.Specifically, you will be given ageneral description of non-relativistic quantum mechanics interms of Hilbert spaces and theconcept of spin and its relation tothe representations of the rotationgroup will be introduced.

Physical CosmologyCosmology is the study of theuniverse, its present constituentsand its evolution. It thereforeendeavours to answerfundamental questions that havefascinated humans since theearliest days of civilisation: wheredo we come from, why is the

universe the way it is, what is itsbeginning and is there an end toit? This module covers theessential concepts of moderncosmology, and in particularintroduces you to what hasbecome known as the"cosmological standard model". Itdiscusses the structure andproperties of the universe as weobserve it today, its evolution andthe underlying physical concepts,and the observations that formedour understanding of the universe.

Solid State PhysicsThis module aims to provide adescription of the physicalproperties of macroscopic solidsthat follow from elementaryquantum physics. The courseaims to convey the role thatconcepts such as scale,dimensionality, and order play inthe behaviour of solids. The keyexperimental tools for probing

Module descriptions

solid structures and the controlledfabrication of solids with tailoredproperties will be outlined. Themodule is intended to providefinal-year students with theessential knowledge of the solidstate that is key to many branchesof physics, materials science, andengineering.

Space Time and GravityThis module presents theessential concepts of both specialand general relativity. Theemphasis is on the physicalunderstanding of the theory andthe mathematical development iskept simple, although moredetailed treatments are includedfor those who wish to follow them;space-time diagrams are usedextensively. The module includesdiscussion of the big bang andblack holes.

StarsStars are a vital building block inthe Universe: forming out ofinterstellar gas and dust, andthemselves being a majorcomponent of galaxies. They arealso vital for providing the nuclearreactions that create the elementsfrom which planets and evenourselves are formed. Thismodule describes how thefundamental properties of starsare related to observations.Temperatures and densities in thecentre of stars reach values thatare unattainable in the laboratory.Yet the application of basicphysical principles can help usdetermine much about theinternal structure and evolution ofstars, from their formation to their

ultimate end states in such exoticand spectacular objects as whitedwarfs, neutron stars and blackholes.

Statistical Data AnalysisThis module will review basicmetrics and techniques used todescribe ensembles of data suchas averages, variances, standarddeviation, errors and errorpropagation. These will beextended to treatmultidimensional problems andcircumstances where observablesare correlated with one another.The Binomial, Poisson, andGaussian distributions will bediscussed, with emphasis onphysical interpretation in terms ofevents. Concepts of probability,confidence intervals, limits, andhypothesis testing will bedeveloped. Optimizationtechniques will be introducedincluding chi2 minimisation andmaximum-likelihood techniques.A number of multivariateanalysers will be discussed in thecontext of data mining. These willinclude Fisher discriminants,multi-layer perceptron basedartificial neural networks, decisiontrees and genetic algorithms.

Year 4Physics Research ProjectIn this module you will examine aspecific area of physics viadirected reading and independentstudy. You will use scientificliterature and databases. Thetopic will be an area of physicswhich has undergone recentdevelopment or is topical. A list of

projects will be provided, but youcan propose one of your own. Bythe end of this project you willhave written a review that criticallysummarises your chosen area.

Advanced CosmologyCosmology is a rapidly developingsubject that is the focus of aconsiderable research effortworldwide. It is the attempt tounderstand the present state ofthe universe as a whole andthereby shed light on its originand ultimate fate. Why is theuniverse structured today in theway that it is, how did it developinto its current form and what willhappen to it in the future? Theaim of this module is to addressthese and related questions fromboth the observational andtheoretical perspectives.

Advanced Quantum Field TheoryPhysicists aim to unify differenttheories into one. This modulegives a broad exposition of themodern framework for theunification of special relativity andquantum theory, called relativisticquantum field theory (QFT). Inconjunction with the moduleRelativistic Waves and QuantumFields, this module will prepareyou for studies at PhD level intheoretical physics and particlephysics/phenomenology.

Astrophysical PlasmasPlasmas are present in almostevery astrophysical environment,from the surface of pulsars to theEarth's ionosphere. A plasma isan ionized gas where themagnetic and electric field play a



key role in binding the materialtogether. This module explores theunique properties of plasmas andthe emphasis is on plasmas foundin the Solar System. The modulehighlights the links between theplasmas we can observe withspacecraft and the plasmas inmore distant and extremeastrophysical objects.

Electromagnetic Radiation in AstrophysicsThis module is an introduction tounderstanding the origin,propagation, detection andinterpretation of electromagnetic(EM) radiation from astronomicalobjects. In this module you willlearn: how to describe EMradiation and its propagationthrough a medium to an observer;the main processes responsiblefor line and continuum emissionand how they depend on thenature and state the emittingmaterial; the effects of the Earth’satmosphere and the operation ofthe detection process at variouswavelengths. The material will beillustrated by examples fromoptical, infrared and radio portionsof the EM spectrum.

Electromagnetic TheoryIn this module you will beintroduced to classicalelectromagnetism, in particularMaxwell’s equations. Building onthe mathematical skills developedin earlier modules, you will usethese to explore Maxwell’sequations under differentcircumstances and finally extendyour investigations to Lorentztransformations of Special

Module descriptions

Relativity. You will find that theknowledge gained through thismodule can be applied in manydifferent circumstances.

Extrasolar Planets andAstrophysical DiscsEver since the dawn of civilisation,human beings have speculatedabout the existence of planetsoutside of the Solar Systemorbiting other stars. The first bonafide extrasolar planet orbiting anordinary main sequence star wasdiscovered in 1995, andsubsequent planet searches haveuncovered the existence of manyhundreds of planetary systems inthe Solar neighbourhood of ourgalaxy. These discoveries havereignited speculation andscientific study concerning thepossibility of life existing outside ofthe Solar System. This moduleprovides an in-depth descriptionof our current knowledge andunderstanding of these extrasolarplanets. Their statistical andphysical properties are describedand contrasted with the planets inour Solar System. Ourunderstanding of how planetarysystems form in the discs of gasand dust observed to exist aroundyoung stars will be explored, andcurrent scientific ideas about theorigin of life will be discussed.Rotationally supported discs ofgas (and dust) are not onlyimportant for explaining theformation of planetary systems,but also play an important role ina large number of astrophysicalphenomena such as cataclysmicvariables, X-ray binary systems,and active galactic nuclei. These

so-called accretion discs providethe engine for some of the mostenergetic phenomena in theuniverse. The second half of thismodule will describe theobservational evidence foraccretion discs and currenttheories for accretion discevolution.

The GalaxyThe module considers in detailthe basic physical processes thatoperate in galaxies, using our own

Galaxy as a detailed example.This includes the dynamics andinteractions of stars, and howtheir motions can be describedmathematically. The interstellarmedium is described and modelsare used to represent how theabundances of chemical elementshave changed during the lifetimeof the Galaxy. Dark matter can bestudied using rotation curves ofgalaxies, and through the way thatgravitational lensing by darkmatter affects light. The various



topics are then put together toprovide an understanding of howthe galaxies formed.

Relativistic Waves and QuantumFieldsHere you will be given anintroduction into the unification ofquantum mechanics and specialrelativity. You will review both ofthese topics before going on toinvestigate the relativistic waveequations and quantum fieldtheory.

Relativity and GravitationIn this module you will explore thefundamental principles of GeneralRelativity. Analysis of the motionof particles and the propagation ofelectromagnetic waves in agravitational field will beundertaken. Various derivationswill be completed, includingEinstein’s field equations. TheSchwarzschild solution andanalysis of the Kerr solution willfacilitate discussion of thephysical aspects of stronggravitation fields around black

holes. The generation,propagation and detection ofgravitational waves ismathematically analysed. Finally,weak general relativistic effects inthe Solar System and binarypulsars are included along with adiscussion of the experimentaltests of General Relativity.

Solar SystemAs the planetary system mostfamiliar to us, the Solar Systempresents the best opportunity tostudy questions about the originof life and how enormouscomplexity arise from simplephysical systems in general. Thismodule surveys the physical anddynamical properties of the SolarSystem. It focuses on theformation, evolution, structure,and interaction of the Sun,planets, satellites, rings, asteroids,and comets. The module appliesbasic physical and mathematicalprinciples needed for the study,such as fluid dynamics,electrodynamics, orbitaldynamics, solid mechanics, and

elementary differential equations.However, prior knowledge in thesetopics is not needed, as they willbe introduced as required. Themodule will also includediscussions of very recent,exciting developments in theformation of planetary and satellitesystems and extrasolar planets(planetary migration, giantimpacts, and exoplanetaryatmospheres).

Stellar Structure and EvolutionStars are important constituents ofthe universe. By considering well-known physical phenomena, youcan deduce stellar properties thatcan be observed and comparedwith the theoretical prediction.These properties includeluminosity, temperature,magnitude and colour. You willdevelop an understanding of pre-main sequence and dwarf stagesof evolution of stars, as well as thehelium flash and supernovastages.

Career opportunities



Based on the most recent results,91% of our graduates were in agraduate-level job six months afterleaving. In recent years over 20per cent of our graduates havegone on to some form of furtherstudy, this can be a one yearMasters degree or PhD. Theremaining students go on intoemployment in a wide range offields, including roles such as aMarket Research Analyst,Accountant and AdvertisingExecutive in the Business andFinance field and ComputerAnalyst, Programmer and ICTManager in IT. They have alsotaken on technical physics rolesin engineering firms and medicaland non-medical laboratories.

Your potential earnings also reflectthe contribution you can make:according to a report byPriceWaterhouseCoopers, physics

graduates earn around £187,000more during their career than non-graduates.

The reason for these increasedpotential earnings is down to theparticular skills and abilities youhave as a physics graduate. Theway in which you approachproblem solving and yourmathematical skills make you avaluable employee.

The Queen Mary Careers Service isavailable to help you with anycareer-related issue throughoutyour time at university. If you arenot sure what you want to do, adiscussion with a careers adviserwill help you to be clearer aboutyour options for work or furtherstudy, and our resources will helpyou to begin investigating thecareers open to graduates.

Tejpal SinghPhysics

“I havealways beenpassionateabout physicsever since Iwas a child. I have always

been interested in how and why thingswork. Therefore, the best thing aboutthe subject for me is that it requires more than justknowledge to solve problems; creativethinking is also necessary.

“The best thing about the College isdefinitely the staff; they are verywelcoming. Outside of lectures thephysics professors are always willing tohelp when I have any questions. They doan excellent job of explaining clearly.

“Queen Mary has excellent facilities,and they are always improving. ThePhysics laboratory was recently fullyrenovated to provide each student withthe use of computing facilities. It is agreat place to study.

I would also rate the social, leisure and recreational facilities as excellent.There is always something to do andmany social clubs and societiesavailable.

“My favourite memory so far has to bewhen a few of the physics postgraduatesstarted gathering people in front of thePhysics building and created ‘ice cream’using liquid nitrogen. It was fun towatch, and then we started to freezesome other things… mostly fruit. It wasso interesting to see what happens tothings when they are frozen in that way.”

Student profile

Students and mentors at the SEPnet Student Expo – Undegraduate studentspresented summer placment projects



Queen Mary students have accessto a wide range of eventsorganised locally by the QueenMary Careers Service and London-wide by The Careers Group givingyou a chance to talk to employersand take part in interactiveactivities, enabling you to get abetter taste of what the jobs arereally like. There are also a numberof talks and events offered by theCareers Service and the School ofPhysics and Astronomy.

Recent events have included aPhysics Careers Forum where our students had the chance toquestion employers from a rangeof fields: from IT and computing to engineering and academicresearch. Alumni also contribute to careers sessions, giving currentundergraduate students the benefitof their experiences.

Graduate profile: Marcus ChownStudied: Physics, graduated 1980

Currently: Science writer and journalist. I write about space and physics but I’m alsothe cosmology consultant on the New Scientist.

Why did you choose Queen Mary? I had never heard of Queen Mary but it did astrophysics, which I was interested in, so Iapplied. The department was very clever. They made sure Patrick Moore had tea with uswhen we came for an interview. At the time he lectured an introductory astronomycourse with Heather Couper. It was immediately obvious it was a small, friendly placewhere you would know your lecturers well.

What are the best things about your job?I get to talk to the most interesting people in the world and ask them really stupid questions!I really enjoy writing and the physics element is also really important. I think I’m reasonablygood at communicating complicated things. Some students have told me they only studiedphysics because they read my book. So as a writer you can really make a difference.

How did you get into science journalism?When I graduated, there were no real career paths for science journalists. I wrote tonewspapers and magazines asking for a job. They all told me to get lost – you need to bereally persistent! Then finally I got a job on Nature magazine. That really helped, becauseeditors always ask if you have any experience. Nowadays it’s easier perhaps, because youcan write a blog or use Twitter to get your words and ideas out there.

Tell us about some of the high-points in your career I was sent to the 2009 Sydney Writers Festival by my publisher. I have also spoken at theCheltenham, Oxford and Bath Literature Festivals and the Edinburgh Science Festival. AndI’ve worked on a comedy TV series with Andy Hamilton and Reginald D Hunter. But ofcourse there are also bread and butter things that I have to do to pay the gas bill.

At The Serpentine, London - by Jorn Tomter

Student life – Students’ Union,student support and health services


Student life – Students’ Union, student support and health services

Students’ Union All Queen Mary studentsautomatically become members ofQMSU, an active and flourishingStudents’ Union run by studentsfor students. Best known for itsclubs and societies, there areliterally hundreds to choose from,whether your interests lie infootball or philately. And if youhave a passion that isn’trepresented, you can always startyour own club. Clubs and societiesprovide a great opportunity formeeting people, especially thosewho are studying a differentsubject to you. One of the aims ofQMSU is to ensure that your timeat university is not just about work,but also includes socialising andpersonal development.

QMotion QMotion is Queen Mary’s recentlyrefurbished Health and Fitnesscentre. Equipped with a greatrange of exercise machines andweights, there’s also a women onlyarea and loads of classes includingyoga, spinning and Pilates. There’sa squash court and sports hall oncampus, and a swimming pool ashort distance away.

Sports Playing sports is a good way torelax after a day spent studying.Queen Mary teams regularlycompete against other collegeteams, and there’s a great socialscene with after-match drinks anda regular social night, Hail Mary,hosted by one of the SU’s sportsteams. There’s even a team ofcheerleaders, the Queen MaryAngels!

QM Provide: Volunteering Volunteering with charities andnon-profit organisations is abrilliant way to explore whatLondon has to offer, make adifference and really get involvedin your local area.

You can volunteer on a regularbasis in a placement with a localcharity or organisation, doinganything from mentoring localschool kids, to volunteering inlocal hospitals, to becoming ahelpline volunteer and managinga local sports team. See: www.providevolunteering.org

Student support You will be assigned an academicadviser when you start at QueenMary, and the same adviser willstay with you throughout yourstudies. Your adviser will help youchoose which modules to take(some programmes offer greaterflexibility when it comes to modulechoices), sign any forms you needand help you with any academic orpersonal problems that you have.

Many students find it extremelyhelpful to have one adviser onhand throughout their time atQueen Mary.

Health services All the services are provided for all students and staff living in the London Borough of TowerHamlets. In order to access theseservices and other availableservices under the NHS, you needto register with the Globe Townsurgery at the Student HealthCentre at the beginning of term.Students living outside TowerHamlets can be treated oncampus in the event of an urgentmedical situation.

For more information see:www.globetown.org/qmu/

Advice and counselling Our advice service offers in-depthand specialist advice on a rangeof financial, practical and legalissues, such as student finance,housing rights, immigration lawand international student issues.Counselling is also available –from cognitive behaviouraltherapy, ongoing weekly therapygroups and support groups onspecific issues such as anxiety,academic performance. Ouradvice and counseling service is acompletely free and confidentialservice.

For more information see:www.welfare.qmul.ac.uk

Accommodation

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Accommodation

Queen Mary’s Student Villageincorporates 2,000 rooms oncampus, all provided in self-catered houses, flats andmaisonettes. All rooms in theVillage have a bathroom en-suite,and you’ll share a kitchen.

If you are a single full-time first-year undergraduate, apply duringthe normal admissions cycle, andhave not lived in Queen Mary’shousing before, you may beeligible for accommodation oncampus. Priority is given to thoseapplying by the deadline of 30June of the year of entry, andthose who live furthest away. Thisoffer does not extend to studentswho join through the Clearingprocess or those holding insuranceoffers with Queen Mary, althoughevery attempt is made toaccommodate them, subject toavailability.

If you live close enough to theCollege to commute, you willnormally be expected to live athome until rooms becomeavailable after term begins, onceall those students who cannotcommute are housed. Once youhave firmly accepted your offer tostudy at Queen Mary, full details onhow to apply for College housingwill be sent to you by theAdmissions Office.

Queen Mary students also haveaccess to places in the fully-catered Intercollegiate Halls incentral London, which are ownedcentrally by the University ofLondon.

Another option is a house share.There are a number of privately let houses in the area suitable forgroups of students to share. Theresidences office can put you intouch with local landlords, as wellas groups of students who arelooking for extra people to makeup numbers.

For more information, see:www.residences.qmul.ac.uk

‘‘You feel like you belong a bit more, living on campus. The place ispacked with people all doing the same thing, unloading their cars at the beginning of term. It’s really sociable.Jen Holton

‘‘

‘‘I had a beautiful canal view frommy room. I just can’t believe this is student accommodation – it’svery airy, bright, fresh and clean.Fariah Khan

School of Physics and AstronomyEntry requirements


School of Physics and AstronomyEntry requirements

A/AS-levels

Vocational orapplied A-levels

Acceptability: Acceptable only when combined with other A2-equivalent physics andmathematics qualifications.

BTEC NationalCertificate (12 units)


Subjects and grades required: Overall in Double Award DD. Must have high physics andmathematics content.

BTEC NationalDiploma (18 units)


Subjects and grades required: Overall DMM. Must have high physics and mathematicscontent.

InternationalBaccalaureate

Acceptability: Acceptable on its own and combined with other qualifications.

Subjects and grades required: BSc programmes: 30 points overall with 6 in both HigherLevel physics and Higher Level mathematics.

MSci programmes: 34 points overall with 6 in both HL physics and HL mathematics.

EuropeanBaccalaureate

Acceptability: Acceptable on its own and combined with other qualifications.

Subjects and grades required: BSc entry: 75 per cent overall 7/6 in maths/physics in anyorder.

MSci entry: 80 per cent overall with 7 in maths and physics

Access to HEDiploma

Credits required: A total of 60 credits, out of which 45 at level 3 and 18 level 3 credits inmaths units and 18 level 3 credits in physics units for BSc entry.Grade required: Distinction.Additional information: Must be physics and mathematics based.

Recognised by the Quality Assurance Agency for HE

European andinternationalqualifications

Otherqualifications

The university accepts a wide range of EU and international qualifications, includingselected international foundation programmes. For further information please contact the Admissions Office, or visit: www.qmul.ac.uk/international/countries

The College welcomes applications from those holding qualifications not listed above. Staff in the Admissions and Recruitment Office will be happy to advise you as to theacceptability of your qualification.

Tariff/Grades requirement: BSc programmes: a total of 320 tariff points. Applicants shouldaim to achieve grades A and B at A-level in physics and mathematics.

MSci programmes: a total of 340 tariff points. Applicants should aim to achieve grade A atA-level in physics and mathematics. If you do not perform as well in one subject and dobetter in others, then that is acceptable, providing you gain the minimum number of pointsrequired for the degree programme.

Additional information: General studies should not be included in the points tariff.

Living in London


A world-famous cityand the nation’scapital, London is an exciting place tolive. If you’re new to the city, you’re in for a treat; and if you’ve lived herebefore, then you’llknow there’s alwaysmore to explore.Either way, student life inLondon promises to be an adventure.

With eight million residents,London is up there with Tokyoand NYC in terms of sheer size.Yet rather than a single city,London is actually a patchwork ofdifferent areas – many of themformer villages in their own right.Many retain their own centres,with a parade of shops, bars andrestaurants that reflects its ownparticular and historic character.

Depending on your mood, theoccasion and the kind of placeyou are looking for, you can make this diversity work to youradvantage – there’s alwayssomewhere that will suit yourmood, budget, and the kind ofoccasion you are looking for.

Queen Mary’s main campus is atMile End, well connected to therest of the city by tube. Mile End(Central line) and Stepney Green(Hammersmith and City, andDistrict lines) are both a shortwalk away.

Living in London

‘‘‘‘Why, Sir, you find no man, at allintellectual, who is willing to leaveLondon. No, Sir, when a man istired of London, he is tired of life;for there is in London all that lifecan afford.Samuel Johnson


Living in London

1 Old Street, and surrounding EAT… Yelo, on Hoxton Square(Thai food) Shish, an upmarketkebab restaurant.VISIT… White Cube2 Gallery. This area is the epicentre of theEast End’s artistic community. SHOP… The Hoxton Boutique. The Sunday Flower Market atColumbia Road is legendaryamongst Londoners.

2 Shoreditch, and Brick LaneEAT… Brick Lane is London’s‘Curry Capital’– an entire streetlined with Indian and Bangladeshirestaurants. Brick Lane Beigel Bake, open 24-hours (greatfor bagel emergencies).VISIT… The Old Truman Brewery,a converted brewery and home tonumerous fashion designers,artists and DJs.

3 Bow WharfThe complex includes: The FatCat Café Bar; The Thai Room;and Jongleurs Comedy Club,which, as well as the comedy, has a bar and restaurant pluspost-comedy disco on Friday and Saturday nights.

4 Docklands, and Canary WharfEAT… Ubon by Nobu (the sisterrestaurant to the West Endfavourite of the stars), or Carluccio’s, an Italian chainserving exceptional food.Wagamama in the Jubilee PlaceMall. Bene Bene, which offers ahuge selection of seriously cheapsandwiches, salads, bagels anddesserts.VISIT… The Museum inDocklands, which explores thestory of the docks from Romansettlement through to recentregeneration.


5 Bethnal Green,and Victoria ParkEAT… E Pellici, on Bethnal GreenRoad, an Italian greasy spooncafé which has been aroundsince 1900. Nando’s, HackneyVillage for a range of otherrestaurants and cafes, includingFrocks, Mojo’s and Déjà Vu.VISIT… Modern Art and VilmaGold galleries on Vyner Street, just north of Bethnal Green.

6 Mile End, andsurrounding areaEAT… with Mile End’s big range ofeating places, our students nevergo hungry, whatever their culinaryskills. Wetherspoon's pub, offeringthe ‘cheap and cheerful’ deals.The Morgan Arms, a bit more ofan up-market pub. The GoldenBird (Chinese), The Pride of Asia(Indian), Matsu (Japanese)restaurants, if you like to eat yourway around the world. Roastarscoffee shop, for a small caffeinebuzz at the start of the day.

VISIT… Mile End Park, 90 acresof greenery in the heart of theEast End where you’ll find anecology park; an arts park; and a terraced garden and a sportspark. The Mile End Stadium,includes an eight lane athleticstrack, artificial hockey/footballpitches and grass football pitches.The Genesis Cinema, go onWednesday night for a studentdiscount. The WhitechapelGallery: famous for exhibitions by big name artists.

Tower Hill

Monument

Blackfriars

Mansion House

St Paul’s

Bank

Holborn

Chancery Lane

Temple

BarbicanLiverpool

Street

Shoreditch

Whitechapel

Aldgate

Stepney Green

Bethnal Green

London Bridge

Waterloo

Mile End

Charing Cross

Canary Wharf

Wapping

Limehouse

Tower of London

Mile EndPark

EAST LONDONTo Olympic

Stadium

TOWER HAMLETS

CITY OFLONDONHOLBORN

St James’Park

1

2

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Leicester Square

Clerkenwell

IslingtonBloomsbury

ULU: Students’ Union

Kings CrossBritish Library

Euston

To O2 Arena

Frequently asked questions



Should I take theBSc or MSci?We offer two different types ofqualification: BSc or MSci. TheBSc takes three years tocomplete, and the MSci fouryears. An MSci will provide youwith more advanced training andproject experience which couldlead to a PhD or provide you withan advantage if you wish to entera career at a higher level. TheBSc and MSci courses havecommon programmes andmodule options over the first twoyears and transfer between theprogrammes is possible duringthis time, subject to satisfactoryperformance.

In the final year of the MSci youwill have the opportunity to take

modules selected from a largerange of current research topicsin physics. This year is taught asan intercollegiate year and you willbe able to take modules taught bylecturers from Colleges throughoutthe University of London.

Can I study abroad?Queen Mary students can takepart in an international exchangeprogramme spending either theautumn semester or full academicyear at one of our partnerinstitutions. The academic workcompleted abroad is creditedtowards your Queen Mary degree.Tuition fees will still be paid toQueen Mary for your periodabroad and you do not have topay tuition fees at the hostinstitution but you are still

responsible for all travel,accommodation and livingexpenses. You will find fulleligibility details and otherconditions for participation in thisprogramme on our website:www.qmul.ac.uk/qmlearning/exchangesOur partner universities withphysics specialities are:• Hunter College (City Universityof New York)

• University of Miami• University of Richmond• University of California (withseveral campuses and differentspecialities)

It is also possible to study inEurope within the Erasmusprogramme. Queen Mary enjoysclose links with Europe through itsparticipation in the SOCRATESERASMUS programme andbelieves this presents a greatopportunity for students toimmerse themselves in thelanguage, lifestyle and culture ofanother country. Students areselected by their academic schoolat Queen Mary and the criteria forselection include academic ability,proficiency in the language of thehost country and the desire toparticipate in an exchange. TheLanguage Learning Unit providescourses to give students practicalskills in a foreign language andhelp prepare them for theexchange. Students are givencredit for courses passed at thehost institution. You can find outmore on the British Councilwebsite: www.britishcouncil.org/erasmus.htm



What does studyingPhysics at Universityinvolve?You will be expected to devoteyourself full-time to your studies.With regards to your timetabledhours, in the first semester of yourfirst year you should expect tospend on average each week:• 3 or 4 hours in lectures for eachmodule (4 modules per semester)

• 3-6 hours in the laboratory• 3 hours in exercise classes ortutorials

However, overall you should bedevoting around 40 hours a weekto your degree. This will includeyour timetabled lessons, studyingand preparation for laboratorysessions and exercise classes.

How will I be taught?The teaching in the School ofPhysics and Astronomy is carriedout through lectures and exerciseclasses backed up by a practicalelement. Lectures take place invarious locations around thecampus and will not always beheld in the School of Physics andAstronomy. This will give you achance to get to know thedifferent areas of the College.

Tutorials and exercise classes areused to support the lectures.These classes will be taken by thelecturer and postgraduatestudents They are an opportunityfor you to ask questions and workthrough any problems you havewith the material.

We have laboratories which arereserved solely for the use of ourundergraduate students. In thefirst year you are required to take the module ScientificMeasurement, (see page 11 for a description) which will illustratethe basic concepts in physics: you will carry out experiments and interpret results. This givesyou valuable knowledge on howcertain laboratory instrumentswork and it will also give you theopportunity to develop your timemanagement and reporting skills.You are supported in theselaboratory sessions by dedicatedtechnicians, academic staff andpostgraduate students.

How is theacademic yearstructured?You will take four modules in eachof the two semesters in every yearof study. The academic year runsfrom September to June. Thereare typically three or four lecturesper week for each module. Youwill also have one or two hoursscheduled for tutorial work foreach module. You are expected todo some independent studyoutside of your timetabled hours.Modules often have an element ofcoursework to them therefore youwill be expected to spend timepreparing your hand-ins andthese count towards your finalmark. Some modules have a classtest and most have an end of yearexamination which makes up thebulk of your mark for that module.

Can I take modulesfrom outside of theSchool of Physicsand Astronomy?You will have a number of optionsavailable to you each year, but theexact number will depend onwhich degree programme you areregistered on. Our modularsystem allows you take a subjectfrom another academic schoolwhich will still count towards yourdegree. For example, you maychoose to study a language withchoices from beginner toadvanced level in a variety oflanguages. Visit the Language andLearning Unit website for moredetails: www.languageandlearning.qmul.ac.uk

Who can I go to foradvice and help?When you start at Queen Mary,you will be allocated an AcademicAdviser. This person will talk toyou about your module optionsand will discuss with you what isbest for your needs beforeregistering you on the appropriatemodules. If you need support oradvice on personal or academicmatters, then your Adviser is thereto help you.

We have a full-time StudentSupport Administrator (SSA) whoacts as the first point of contactfor any student concerns, be theyacademic or pastoral. The SSA isavailable to provide advice andguidance on matters such asStudent Funding, Bursaries and

Financial Support,Accommodation and Welfareconcerns, help with special examarrangements for those studentsin need of additional support andoffers advice on careers andfurther study.

If you wish to you will be able totake part in a supplemental studyprogram in your first year of study.The Peer Assisted Study Support(PASS) scheme supports newstudents through weekly one hoursessions led by second and thirdyear students.

Is there any financialsupport available?There is a comprehensivepackage of support available tostudents. For the latest details onwhat is available and for eligibility,please visit our website.

Are there anyScholarshipsavailable?If you are a home/UK student andachieve higher than AAA (orequivalent) you may be awardedan Excellence Scholarship of£3,000 per year of study. Fulldetails are available online. Enterthe term “ExcellenceScholarships” into our search:www.qmul.ac.uk

For international students, thereare Excellence Awards available ofa £1,500 fee reduction if youmeet the entry requirements or ifyou exceed AAA (or equivalent)you could be awarded a £4,000deduction. Full details areavailable on our website:www.qmul.ac.uk/international/scholarships/

What teachingfacilities are availablefor experimentalmodules?Our undergraduate teachinglaboratories have recently beenrefurbished and contain a mainlab with 46 spacious work stations,two optics rooms providing afurther 11 work stations and fourspecialist vibration free surfacesfor sensitive experiments. Thelaboratories are open access andwe have two members of staffoffering technical support for allphysics students during normalworking hours. Each work stationhas a PC with internet access andhas an adjustable height function.It is a well-funded resource with amix of traditional and modernequipment. The modules ScientificMeasurement and PhysicsLaboratory are taught here.


Next steps


Next steps

Visit usThe School of Physics andAstronomy runs numerous eventsfor students thinking of studyingphysics at university. From oneday taster courses to week-longsummer schools. For moreinformation on when theseactivities are taking place, please visit our website:www.ph.qmul.ac.uk

In addition to the School activities,the College has two open dayseach year: one in June and asecond in September. If you areunable to visit us at any of thesetimes then you can book acampus tour. Information can befound online at: www.qmul.ac.uk/visitus

Applying to Queen Mary For all full-time higher educationprogrammes at universities andcolleges in the UK, students mustapply online at: www.ucas.comYou’ll find full instructions to helpyou fill in your online application,plus help text where appropriate.UCAS also has a comprehensiveguide called Applying Online,which can be downloaded fromthe website (www.ucas.com).

You can also visit our QM:Insightpages which offers guidance onapplying to university.www.qmul.ac.uk/qminsight

There are three types of applicant:

1 Students at a school or collegeregistered with UCASAll UK schools and colleges (andmany establishments overseas)are registered with UCAS tomanage their students’applications. Advice is availablefrom your teacher or a careersadviser at your school or college.You fill in an online applicationand submit it to a member ofstaff.

After checking your details, andhaving added the academicreference, your school or collegesubmits the completed applicationonline to UCAS. You pay onlineusing a credit card or debit card.You may also be able to paythrough your school or college.

2 Independent applicants in the UKOther UK applicants, who are notat school or college, apply onlineindependently. It is likely that youare a mature applicant, who,unlike school and collegestudents, cannot readily seekadvice from your teacher, but caninstead consult with variouscareers organisations (such asConnexions).

You are responsible for paying thecorrect application fee, forobtaining and attaching theacademic reference and forsubmitting the completedapplication online to UCAS.

3 International applicants outsidethe UK (EU and worldwide)Except for those whose school orcollege is registered with UCAS,individuals from the EU (excludingthe UK), and worldwide, applyonline independently. Advice isavailable from British Counciloffices and other centresoverseas, such as your school orcollege or one of our overseasrepresentatives.You will find a step-by-step guideto applying at: www.qmul.ac.uk/international/ howtoapply/index.htm

Contact usSchool of Physics and AstronomyQueen Mary, University of LondonMile End RoadLondonE1 4NSTel: 0207 882 6958Fax: 0208 981 9465email: [email protected]

For latest news, see:Facebook:www.facebook.com/PhysicsatQMTwitter:www.twitter.com/PhysicsatQM

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‘‘One of the best things you can dois visit a university and find outfrom the students this what theythink about studying thereAsmi Barot Physics student


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10

6 857

5

4

3

2

21

13

31

32

11

17

19

26

54

18

34

23

25

28

59

52

33

35

36

37

38

39

40

44

45

55

49

4647

43

42

50

41

53

41

48

45

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Arts One 29

Arts Two 27

Arts Research Centre 31

Bancroft Road Teaching Rooms 60

Computer Science 6

Engineering Building 7

Environmental Health and Safety 10

Fogg Building 11

Francis Bancroft Building 26

G.O. Jones Building 20

Geography 19

IRC 13

Informatics Teaching Laboratories 5

Joseph Priestley Building 34

Library 25

Law 28

Lock-keeper’s Graduate Centre 33

Mathematical Sciences 4

The People’s Palace / Great Hall 15

Queens’ Building / Octagon 16

Mile End Campus Map IndexEducational / Research

Albert Stern Cottages 3

Albert Stern House 1

Beaumont Court 43

Chapman House 35

Chesney House 37

Creed Court 46

France House 45

Feilden House 41

Hatton House 32

Ifor Evans Place 2

Lodge House 38

Lindop House 23

Lynden House 48

Maynard House 36

Maurice Court 47

Pooley House 49

Selincourt House 40

Varey House 39

Residential FacilitiesAdvice and Counselling Service 17

Bookshop 51

Clock Tower 62

Curve 53

Drapers’ Bar 58

Ground Café 52

Occupational Health Service and Student Health Service 18

Hive 21

Hub 24

Infusion 59

Mucci’s 54

Police Box 30

Post Room 14

QMotion Fitness Centre 57

Residences Reception 44

Security 61

St Benet’s Chapel 22

Students’ Union 8

Students’ Union Offices / Blomeley Centre 50

The Copy Shop 63

Village Shop 42

Westfield Nursery 9

World Marché 55

Bicycle parking 3

Cash machine 3

Staff car park )

No Smoking policy on campusCCTV operates on this campus

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School of Physics and AstronomyQueen Mary, University of LondonMile End RoadLondonE1 4NSTel: 0207 882 6958Fax: 0208 981 9465email: [email protected]

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Documents

QMUL_PHYSICS and ASTRONOMY_UG