If you are fascinated by the ‘how and why’ of the material world, as well as underlying physical concepts of the stars and galaxies, which make up the Universe, a degree in Physics with Astrophysics is for you. Studying at Kent will equip you with the skills to understand these phenomena and prepare you for a range of career pathways. Our four-year Integrated Masters in Physics also gives you the opportunity to work on a research project, in an area of your choosing, and gain a valuable postgraduate qualification which can help give you the edge in the job market.
The School of Physical Sciences is a dynamic multidisciplinary department, achieving national and international excellence in physics, chemistry, and forensic science. We offer a broad training in physics, and provide an ideal preparation for a wide range of careers in the manufacturing and service industries as well as education, the media and the financial sector.
This programme is fully accredited by Institute of Physics (IOP).
Astrophysics emphasises the underlying physical concepts of the stars and galaxies, which make up the Universe. This provides an understanding of the physical nature of bodies and processes in space and the instruments and techniques used in modern astronomical research.
In your first year, you get to grips with the broad knowledge base on which physical science is built, including electricity and light, mathematics, mechanics, thermodynamics and matter. You also develop your experimental, computational, statistical and analytical skills.
Your second and third years include a broad range of modules such as quantum mechanics, solid state, atomic, nuclear and particle physics, electromagnetism and optics, and mathematical techniques as well as the mulitwavelength universe exoplanets and stars, galaxies and the universe.
The final year of the MPhys programme brings your core knowledge and skills up to an advanced level. This stage concentrates on the in-depth training required for a science-based career, including the practical aspects of the research processes and a major research project in the School's Astrophysics and Planetary Science research group.
The Beacon Observatory provides a fully automised system with both optical telescope and radio telescope capability. It includes a 17" astrograph from Plane Wave Instruments with a 4k x 4k CCD and a BVRIHa filter set, as well as a 90-frames-per-second camera.
You have access to first-class research facilities in new laboratories. These are equipped with state-of-the-art equipment, including a full characterisation suite for materials, including:
The University is a member of the South East Physics Network (SEPnet), which offers a competitive programme of summer internships to Stage 2 and 3 undergraduates.
The School of Physical Sciences is home to an international scientific community of physics and astronomy, chemistry and forensic science students. Numerous formal and informal opportunities for discussion make it easy to participate in the academic life of the School. All students have an academic adviser and we also run a peer mentoring scheme.
You are encouraged to participate in conferences and professional events to build up your knowledge of the science community and enhance your professional development. The School also works collaboratively with business partners, which allows you to see how our research influences current practice.
You can also take part in:
The School of Physical Sciences also has links with:
Institute of Physics
You are more than your grades
At Kent we look at your circumstances as a whole before deciding whether to make you an offer to study here. Find out more about how we offer flexibility and support before and during your degree.
Please contact the School for more information at study-astro@kent.ac.uk.
The University will consider applications from students offering a wide range of qualifications. Some typical requirements are listed below. Students offering alternative qualifications should contact us for further advice. Please also see our general entry requirements.
The University welcomes applications from international students. Our international recruitment team can guide you on entry requirements. See our International Student website for further information about entry requirements for your country.
If you need to increase your level of science/mathematics ready for undergraduate study, we offer a Foundation Year programme which can help boost your previous scientific experience.
For more advice about applying to Kent, you can meet our staff at a range of international events.
ABB including Mathematics and Physics at BB (Use of Mathematics not accepted)
The University will not necessarily make conditional offers to all Access candidates but will continue to assess them on an individual basis.
If we make you an offer, you will need to obtain/pass the overall Access to Higher Education Diploma and may also be required to obtain a proportion of the total level 3 credits and/or credits in particular subjects at merit grade or above.
The University will consider applicants holding/studying BTEC Extended National Diploma Qualifications (QCF; NQF;OCR) in a relevant Science or Engineering subject at 180 credits or more, on a case by case basis. Please contact us via the enquiries tab for further advice on your individual circumstances.
34 points overall or 15 at Higher including Physics and Mathematics 5 at HL or 6 at SL (not Mathematics Studies)
N/A
Please see our English language entry requirements web page.
If you need to improve your English language standard as a condition of your offer, you can attend one of our pre-sessional courses in English for Academic Purposes before starting your degree programme. You attend these courses before starting your degree programme.
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Duration: 4 years full-time
The course structure below gives a flavour of the modules and provides details of the content of this programme. This listing is based on the current curriculum and may change year to year in response to new curriculum developments and innovation
Introduction to Special Relativity:
Inadequacy of Galilean Transformation; Postulates of Relativity; Lorentz transformation; Time dilation, length contraction and simultaneity; Special relativity paradoxes; Invariant intervals; Momentum and energy in special relativity; Equivalence of mass and energy.
Introduction to Astronomy:
Astronomical coordinate systems and conversions; Positions and motions of stars; Timekeeping systems; Introduction to the distance scale.
Introduction to Astrophysics and Cosmology:
Stellar luminosity and magnitudes; Magnitude systems; Colour of stars; Stellar spectral classification; Evolution of stars, Hertzsprung-Russell diagram; Cosmological principle; Redshift; Hubble constant; Space expansion.
Derivatives and Integrals: Derivatives of elementary functions, chain rule, product rule, Integrals of elementary functions, Evaluation by substitution, Integration by parts, Area under the graph of a function.
Vectors: Basic properties, linear dependence, scalar and vector products, triple products, vector identities.
Matrices: Matrix representation, systems of equations, products, inverses, determinants, solution of linear systems, eigenvalues and eigenvectors, transformations.
Elementary Functions: Binomial coefficients, expansions and series, Maclaurin series, Taylor series, Exponential functions, Hyperbolic functions, Inverse functions.
Functions of a single variable: Linear and quadratic functions, polynomials, rational functions, limits, infinite series, approximation of functions.
Complex numbers: Quadratic equations, Argand diagram, modulus, Argument, complex exponential, de Moivre's theorem, roots of polynomials.
Differential Equations: Solving differential equations, separable equations, linearity, homogeneity, first and second order equations, particular integrals. Boundary and initial values, auxiliary equations with complex roots, coefficients and terms, examples from physics.
Partial Derivatives: functions of two variables , partial derivatives, directional derivatives, functions many variables, higher derivatives, function of a function, implicit differentiation, differentiation of an integral w.r.t a parameter, Taylor expansions, stationary points.
Elementary multivariate Calculus: the chain rule, Multiple integrals, integrals over rectangles/irregular areas in the plane, change of order of integration.
Polar Coordinates: Cylindrical polar coordinates in two and three dimensions, integrals, spherical coordinates, solid angle.
Introduction to Vector Calculus : Gradients, Divergence, Gauss's theorem, Curl, Stokes' theorem.
Measurement and motion; Dimensional analysis, Motion in one dimension: velocity, acceleration, motion with constant acceleration, Motion in a plane with constant acceleration, projectile motion, uniform circular motion, and Newton's laws of motion.
Work, Energy and Momentum; Work, kinetic energy, power, potential energy, relation between force and potential energy, conservation of energy, application to gravitation and simple pendulum, momentum, conservation of linear momentum, elastic and inelastic collisions.
Rotational Motion; Rotational motion: angular velocity, angular acceleration, rotation with constant angular acceleration, rotational kinetic energy, moment of inertia, calculation of moment of inertia of a rod, disc or plate, torque, angular momentum, relation between torque and angular momentum, conservation of angular momentum.
Concept of field; 1/r2 fields; Gravitational Field; Kepler's Laws, Newton's law of gravitation, Gravitational potential, the gravitational field of a spherical shell by integration.
Oscillations and Mechanical Waves; Vibrations of an elastic spring, simple harmonic motion, energy in SHM, simple pendulum, physical pendulum, damped and driven oscillations, resonance, mechanical waves, periodic waves, their mathematical representation using wave vectors and wave functions, derivation of a wave equation, transverse and longitudinal waves, elastic waves on a string, principle of superposition, interference and formation of standing waves, normal modes and harmonics, sound waves with examples of interference to form beats, and the Doppler Effect. Phase velocity and group velocity.
Properties of Light and Optical Images; Wave nature of light. Reflection, refraction, Snell’s law, total internal reflection, refractive index and dispersion, polarisation. Huygens' principle, geometrical optics including reflection at plane and spherical surfaces, refraction at thin lenses, image formation, ray diagrams, calculation of linear and angular magnification, magnifying glass, telescopes and the microscope.
Electric Field; Discrete charge distributions, charge, conductors, insulators, Coulomb’s law, electric field, electric fields lines, action of electric field on charges, electric field due to a continuous charge distribution, electric potential, computing the electric field from the potential, calculation of potential for continuous charge distribution.
Magnetic Field; Force on a point charge in a magnetic field, motion of a point charge in a magnetic field, mass spectrometer and cyclotron.
Electric current and Direct current circuits, electric current, resistivity, resistance and Ohm’s Law, electromotive force, ideal voltage and current sources, energy and power in electric circuits, theory of metallic conduction, resistors in series and in parallel, Kirchhoff’s rules and their application to mesh analysis, electrical measuring instruments for potential difference and current, potential divider and Wheatstone’s bridge circuits, power transfer theorem, transient current analysis in RC, RL, LC and LRC circuits using differential equations.
Alternating Current Circuits; Phasor and complex number notation introduced for alternating current circuit analysis, reactance and complex impedance for Capacitance and Inductance, application to LRC series and parallel circuits. Series and parallel resonance, AC potential dividers and filter circuits, Thevenin's theorem, AC bridge circuits to measure inductance and capacitance, mutual inductance, the transformer and its simple applications.
Static Equilibrium, Elasticity and fluids; Elasticity: stress, strain, Hooke's law, Young's modulus, shear modulus, forces between atoms or molecules, intermolecular potential energy curve, equilibrium separation, Morse and 6-12 potentials, microscopic interpretation of elasticity, relation between Young's modulus and parameters of the interatomic potential energy curve, the nature of interatomic forces, the ionic bond, calculation of the energy to separate the ions in an ionic crystal, viscosity of fluids, Poiseuille's law, Stokes' law.
Thermodynamics; Thermal equilibrium, temperature scales, thermal expansion of solids, relation between thermal expansion and the interatomic potential energy curve, the transfer of thermal energy: conduction, convection, radiation, the ideal-gas law, Boltzmann's constant, Avogadro's number, the universal gas constant. The kinetic theory of gases, pressure of a gas, molecular interpretation of temperature, molecular speeds, mean free path, specific heat, molar specific heat. The equipartition theorem, degrees of freedom. Heat capacities of monatomic and diatomic gases and of solids. Internal energy of a thermodynamic system, the first law of thermodynamics, work and the PV diagram of a gas., work done in an isothermal expansion of an ideal gas. Molar heat capacities of gases at constant pressure and at constant volume and the relation between them. Adiabatic processes for an ideal gas. Heat engines and the Kelvin statement of the second law of thermodynamics, efficiency of a heat engine. Refrigerators and the Clausius statement of the second law of thermodynamics. Equivalence of the Kelvin and Clausius statements. The Carnot cycle, the Kelvin temperature scale.
Atoms; The nuclear atom, Rutherford scattering and the nucleus, Bohr model of the atom, energy level calculation and atom spectra, spectral series for H atom. Limitation of Bohr theory. Photoelectric Effect. Blackbody Radiation. Compton scattering. X-ray diffraction. De Broglie hypothesis. Electron diffraction. Introduction to wavefunctions, Heisenberg's Uncertainty Principle.
Standard Lectures:
How Physical Sciences are taught at Kent.
Library use. Bibliographic database searches.
Error analysis and data presentation. Types of errors; combining errors; Normal distribution; Poisson distribution; graphs – linear and logarithmic.
Probability and Statistics. Probability distributions, laws of probability, permutations and combinations, mean and variance.
Academic integrity and report writing skills.
Laboratory experiments:
A number of experiments in weekly sessions; some of the experiments require two consecutive weeks to complete.
Experiments introduce students to test equipment, data processing and interpretation and cover subjects found in the Physics degree program which include the following topics:
Mechanics, Astronomy/Astrophysics, statistical and probability analysis, numerical simulations, electric circuits and Thermodynamics.
Computing Skills:
Introduction to the concept of programming/scripting languages. Introduction to operating systems: including text editors, the directory system, basic utilities and the edit-compile-run cycle.
Introduction to the use of variables, constants, arrays and different data types; iteration and conditional branching.
Modular design: Use of programming subroutines and functions. Simple input/output, such as the use of format statements for reading and writing, File handling, including practical read/write of data files.
Producing graphical representation of data, including histograms. Interpolating data and fitting functions.
Programming to solve physical problems.
Introduction to typesetting formal scientific documents.
SYLLABUS
Most practicing physicists at some point will be required to perform experiments and take measurements. This module, through a series of experiments, seeks to allow students to become familiar with some more complex apparatus and give them the opportunity to learn the art of accurate recording and analysis of data. This data has to be put in the context of the theoretical background and an estimate of the accuracy made. Keeping of an accurate, intelligible laboratory notebook is most important. Each term 3 three week experiments are performed. The additional period is allocated to some further activities to develop experimental and communications skills.
Revision of classical descriptions of matter as particles, and electromagnetic radiation as waves.
Some key experiments in the history of quantum mechanics. The concept of wave-particle duality.
The wavefunction. Probability density. The Schrodinger equation. Stationary states.
Solutions of the Schrodinger equation for simple physical systems with constant potentials: Free particles. Particles in a box. Classically allowed and forbidden regions.
Reflection and transmission of particles incident onto a potential barrier. Probability flux. Tunnelling of particles.
The simple harmonic oscillator as a model for atomic vibrations.
Revision of classical descriptions of rotation. Rotation in three dimensions as a model for molecular rotation.
The Coulomb potential as a model for the hydrogen atom. The quantum numbers l, m and n. The wavefunctions of the hydrogen atom.
Physical observables represented by operators. Eigenfunctions and eigenvalues. Expectation values. Time independent perturbation theory.
Atomic Physics
Review of previous stages in the development of quantum theory with application to atomic physics; Atomic processes and the excitation of atoms; Electric dipole selection rules; atom in magnetic field; normal Zeeman effect; Stern Gerlach experiment; Spin hypothesis; Addition of orbital and spin angular moments; Lande factor; Anomalous Zeeman effect; Complex atoms; Periodic table; General Pauli principle and electron antisymmetry; Alkali atoms; ls and jj coupling; X-rays. Lamb-shift and hyperfinestructure (if time).
Nuclear Physics
Properties of nuclei: Rutherford scattering. Size, mass and binding energy, stability, spin and parity.
Nuclear Forces: properties of the deuteron, magnetic dipole moment, spin-dependent forces.
Nuclear Models: Semi-empirical mass formula M(A, Z), stability, binding energy B(A, Z)/A. Shell model, magic numbers, spin-orbit interaction, shell closure effects.
Alpha and Beta decay: Energetics and stability, the positron, neutrino and anti-neutrino.
Nuclear Reactions: Q-value. Fission and fusion reactions, chain reactions and nuclear reactors, nuclear weapons, solar energy and the helium cycle.
SYLLABUS
Electromagnetism
Vectors: Review of Grad, Div & Curl; and other operations
Electrostatics: Coulomb's Law, electric field and potential, Gauss's Law in integral and differential form; the electric dipole, forces and torques.
Isotropic dielectrics: Polarization; Gauss's Law in dielectrics; electric displacement and susceptibility; capacitors; energy of systems of charges; energy density of an electrostatic field; stresses; boundary conditions on field vectors.
Poisson and Laplace equations.
Electrostatic images: Point charge and plane; point and sphere, line charges.
Magnetic field: Field of current element or moving charge; Div B; magnetic dipole moment, forces and torques; Ampere's circuital law.
Magnetization: Susceptibility and permeability; boundary conditions on field vectors; fields of simple circuits.
Electromagnetic induction: Lenz’s law, inductance, magnetic energy and energy density;
Optics
Field equations: Maxwell's equations; the E.M. wave equation in free space.
Irradiance: E.M. waves in complex notation.
Polarisation: mathematical description of linear, circular and elliptical states; unpolarised and partially polarised light; production of polarised light; the Jones vector.
Interference: Classes of interferometers – wavefront splitting, amplitude splitting. Basic concepts including coherence.
Diffraction: Introduction to scalar diffraction theory: diffraction at a single slit, diffraction grating.
Aims: To provide a basic but rigorous grounding in observational, computational and theoretical aspects of astrophysics to build on the descriptive course in Part I, and to consider evidence for the existence of exoplanets in other Solar Systems.
SYLLABUS:
Observing the Universe
Telescopes and detectors, and their use to make observations across the electromagnetic spectrum. Basic Definitions: Magnitudes, solid angle, intensity, flux density, absolute magnitude, parsec, distance modulus, bolometric magnitude, spectroscopic parallax, Hertzsprung-Russel diagram, Stellar Photometry: Factors affecting signal from a star. Detectors: Examples, Responsive Quantum Efficiency, CCD cameras. Filters, UBV system, Colour Index as temperature diagnostic.
Extra Solar Planets
The evidence for extrasolar planets will be presented and reviewed. The implications for the development and evolution of Solar Systems will be discussed.
Astrophysics
Basic stellar properties, stellar spectra. Formation and Evolution of stars. Stellar structure: description of stellar structure and evolution models, including star and planet formation. Stellar motions: Space velocity, proper motion, radial velocity, Local Standard of Rest, parallax. Degenerate matter: concept of degenerate pressure, properties of white dwarfs, Chandrasekhar limit, neutron stars, pulsars, Synchrotron radiation, Schwarzschild radius, black holes, stellar remnants in binary systems.
The aim of the module in Medical Physics is to provide a primer into this important physics specialisation. The range of subjects covered is intended to give a balanced introduction to Medical Physics, with emphasis on the core principles of medical imaging, radiation therapy and radiation safety. A small number of lectures is also allocated to the growing field of optical techniques. The module involves several contributions from the Department of Medical Physics at the Kent and Canterbury Hospital.
SYLLABUS:
Radiation protection (radiology, generic); Radiation hazards and dosimetry, radiation protection science and standards, doses and risks in radiology; Radiology; (Fundamental radiological science, general radiology, fluoroscopy and special procedures); Mammography (Imaging techniques and applications to health screening); Computed Tomography (Principles, system design and physical assessment); Diagnostic ultrasound (Pulse echo principles, ultrasound imaging, Doppler techniques); Tissue optics (Absorption, scattering of light in the tissue); The eye (The eye as an optical instrument); Confocal Microscopy (Principles and resolutions); Optical Coherence Tomography (OCT) and applications; Nuclear Medicine (Radionuclide production, radiochemistry, imaging techniques, radiation detectors); In vitro techniques (Radiation counting techniques and applications); Positron Emission Tomography (Principles, imaging and clinical applications); Radiation therapies (Fundamentals of beam therapy, brachytherapy, and 131I thyroid therapy); Radiation Protection (unsealed sources); Dose from in-vivo radionuclides, contamination, safety considerations.
Most physically interesting problems are governed by ordinary, or partial differential equations. It is examples of such equations that provide the motivation for the material covered in this module, and there is a strong emphasis on physical applications throughout. The aim of the module is to provide a firm grounding in mathematical methods: both for solving differential equations and, through the study of special functions and asymptotic analysis, to determine the properties of solutions. The following topics will be covered: Ordinary differential equations: method of Frobenius, general linear second order differential equation. Special functions: Bessel, Legendre, Hermite, Laguerre and Chebyshev functions, orthogonal functions, gamma function, applications of special functions. Partial differential equations; linear second order partial differential equations; Laplace equation, diffusion equation, wave equation, Schrödinger’s equation; Method of separation of variables. Fourier series: application to the solution of partial differential equations. Fourier Transforms: Basic properties and Parseval’s theorem.
Aims: After taking the classes students should be more fluent and adept at solving and discussing general problems in Physics (and its related disciplines of mathematics and engineering)
There is no formal curriculum for this course which uses and demands only physical and mathematical concepts with which the students at this level are already familiar. Instruction is given in:
Problems are presented and solutions discussed in topics spanning the entire undergraduate physics curriculum (Mechanics and statics, thermodynamics, electricity and magnetism, optics, wave mechanics, relativity etc)
Problems are also discussed that primarily involve the application of formal logic and reasoning, simple probability, statistics, estimation and linear mathematics.
Special Relativity: Limits of Newtonian Mechanics, Inertial frames of reference, the Galilean and Lorentz transformations, time dilation and length contraction, invariant quantities under Lorentz transformation, energy momentum 4-vector
Maxwell's equations: operators of vector calculus, Gauss law of electrostatics and magnetostatics, Faraday's law and Ampere's law, physical meanings and integral and differential forms, dielectrics, the wave equation and solutions, Poynting vector, the Fresnel relations, transmission and reflection at dielectric boundaries.
Modern Optics: Resonant cavities and the laser, optical modes, Polarisation and Jones vector formulation.
1. Thermodynamics
Review of zeroth, first, second laws. Quasistatic processes. Functions of state. Extensive and intensive properties. Exact and inexact differentials. Concept of entropy. Heat capacities. Thermodynamic potentials: internal energy, enthalpy, Helmholtz and Gibbs functions. The Maxwell relations. Concept of chemical potential. Applications to simple systems. Joule free expansion. Joule-Kelvin effect. Equilibrium conditions. Phase equilibria, Clausius-Clapeyron equation. The third law of thermodynamics and its consequences – inaccessibility of the absolute zero.
2. Statistical Concepts and Statistical Basis of Thermodynamics
Basic statistical concepts. Microscopic and macroscopic descriptions of thermodynamic systems. Statistical basis of Thermodynamics. Boltzmann entropy formula. Temperature and pressure. Statistical properties of molecules in a gas. Basic concepts of probability and probability distributions. Counting the number of ways to place objects in boxes. Distinguishable and indistinguishable objects. Stirling approximation(s). Schottkly defect, Spin 1/2 systems. System of harmonic oscillators. Gibbsian Ensembles. Canonical Ensemble. Gibbs entropy formula. Boltzmann distribution. Partition function. Semi-classical approach. Partition function of a single particle. Partition function of N non-interacting particles. Helmholtz free energy. Pauli paramagnetism. Semi Classical Perfect Gas. Equation of state. Entropy of a monatomic gas, Sackur-Tetrode equation. Density of states. Maxwell velocity distribution. Equipartition of Energy. Heat capacities. Grand Canonical Ensemble.
3. Quantum Statistics
Classical and Quantum Counting of Microstates. Average occupation numbers: Fermi Dirac and Bose Einstein statistics. The Classical Limit. Black Body radiation and perfect photon gas. Planck’s law. Einstein theory of solids. Debye theory of solids.
To provide an introduction to solid state physics. To provide foundations for the further study of materials and condensed matter, and details of solid state electronic and opto-electronic devices.
Structure
Dynamics of Vibrations
Magnetism
Aims: To provide, in combination with PH507, a balanced and rigorous course in Astrophysics for B.Sc. Physics with Astrophysics students, while forming a basis of the more extensive M.Phys. modules.
SYLLABUS
Physics of Stars
Galaxies
Inadequacy of Newton's Laws of Gravitation, principle of Equivalence, non-Euclidian geometry. Curved surfaces. Schwarzschild solution; Gravitational redshift, the bending of light and gravitational lenses; black holes. Brief survey of the universe. Robertson-Walker metric, field equations for cosmological and critical density. Friedmann models. The early universe. Dark Energy.
Minimisation problems and the Euler-Lagrange equation;
Lagrange formulation of classical mechanics;
Link between symmetries and conservation laws (Noether's theorem);
Hamilton formulation of classical mechanics;
Semi-classical mechanics and the link to quantum mechanics;
Continuum mechanics and fluid dynamics;
Dynamical systems and chaos
Aims:
Through two Colloquium Reports, students will learn to write high-impact articles with a critical analysis of research presented by others. They will exercise presentation skills and present critical reviews and referee's reports of the research of others.
SYLLABUS:
The Research Project (60%)
Identification of a research area and the issues to tackle
Investigation of an unresolved issue comparing experiments and models, comparing approaches, assumptions and statistical methods.
Production of a dissertation
Proposal for future novel work as a short Case for Support for a PhD or research outside university environment
Project Management: Scheduling research programmes, Gantt, PERT charts.
Project Management: Costing of research, full economic cost, direct and indirect costs.
Poster presentation of the research
Research Review and Evaluation (40%)
Evaluation of Research: Colloquium attendance/viewing.
Science Communication: Preparation of two colloquium reports as a science magazine article with impact
Referee report on the colloquiums: strengths, weaknesses of both the speaker and the research quality.
Details of the work to be done will be announced by the convenor during the first two weeks of the academic year.
You take all compulsory modules and then choose one from a list of optional modules.
Aims:
Syllabus
All MPhys students undertake a laboratory, theoretical or computationally-based project related to their degree specialism. These projects may also be undertaken by Diploma students. A list of available project areas is made available during Stage 3, but may be augmented/revised at any time up to and including Week 1 of Stage 4. As far as possible, projects will be assigned on the basis of students' preferences – but this is not always possible: however, the project abstracts are regarded as 'flexible' in the sense that significant modification is possible (subject only to mutual consent between student and supervisor). The projects involve a combination of some or all of: literature search and critique, laboratory work, theoretical work, computational physics and data reduction/analysis. The majority of the projects are directly related to the research conducted in the department and are undertaken within the various SPS research teams.
SYLLABUS:
Space Astronomy
Why use space telescopes; other platforms for non-ground-based astronomical observatories (sounding rockets, balloons, satellites); mission case study; what wavelengths benefit by being in space; measurements astronomers make in space using uv, x-ray and infra-red, and examples of some recent scientific missions.
Exploration of the Solar System
Mission types from flybys to sample returns: scientific aims and instrumentation: design requirements for a spacecraft-exploration mission; how to study planetary atmospheres and surfaces: properties of and how to explore minor bodies (e.g. asteroids and comets): current and future missions: mission case study; how space agencies liaise with the scientific community; how to perform calculations related to the orbital transfer of spacecraft.
Solar System Formation and Evolution
The composition of the Sun and planets will be placed in the context of the current understanding of the evolution of the Solar System. Topics include: Solar system formation and evolution; structure of the solar system; physical and orbital evolution of asteroids.
Extra Solar Planets
The evidence for extra Solar planets will be presented and reviewed. The implications for the development and evolution of Solar Systems will be discussed.
Life in Space
Introduction to the issue of what life is, where it may exist in the Solar System and how to look for it.
SYLLABUS:
Interstellar Medium
The major properties of the Interstellar Medium (ISM) are described. The course will discuss the characteristics of the gaseous and dust components of the ISM, including their distributions throughout the Galaxy, physical and chemical properties, and their influence the star formation process. The excitation of this interstellar material will be examined for the various physical processes which occur in the ISM, including radiative, collisional and shock excitation. The way in which the interstellar material can collapse under the effects of self-gravity to form stars, and their subsequent interaction with the remaining material will be examined. Finally the end stages of stellar evolution will be studied to understand how planetary nebulae and supernova remnants interact with the surrounding ISM.
Extragalactic astrophysics
Review of FRW metric; source counts; cosmological distance ladder; standard candles/rods.
High-z galaxies: fundamental plane; Tully-Fisher; low surface brightness galaxies; luminosity functions and high-z evolution; the Cosmic Star Formation History
Galaxy clusters: the Butcher-Oemler effect; the morphology-density relation; the SZ effect
AGN and black holes: Beaming and superluminal motion; Unified schemes; Black hole demographics; high-z galaxy and quasar absorption and emission lines;
This module will give students an overarching introduction to quantum information processing (QIP). At the end of the course the students will have a basic understanding of quantum computation, quantum communication, and quantum cryptography; as well as the implications to other fields such as computation, physics, and cybersecurity.
We will take a multi-disciplinary approach that will encourage and require students to engage in topics outside of their core discipline. The module will cover the most essential mathematical background required to understand QIP. This includes: linear algebra, basic elements of quantum theory (quantum states, evolution of closed quantum systems, Born's rule), and basic theory of computing. The module will introduce students to the following theoretical topics: quantum algorithms, quantum cryptography, quantum communication & information. The module will also address experimental quantum computation & cryptography.
The 2021/22 annual tuition fees for this programme are:
For details of when and how to pay fees and charges, please see our Student Finance Guide.
For students continuing on this programme, fees will increase year on year by no more than RPI + 3% in each academic year of study except where regulated.*
The University will assess your fee status as part of the application process. If you are uncertain about your fee status you may wish to seek advice from UKCISA before applying.
Find out more about accommodation and living costs, plus general additional costs that you may pay when studying at Kent.
Kent offers generous financial support schemes to assist eligible undergraduate students during their studies. See our funding page for more details.
You may be eligible for government finance to help pay for the costs of studying. See the Government's student finance website.
Scholarships are available for excellence in academic performance, sport and music and are awarded on merit. For further information on the range of awards available and to make an application see our scholarships website.
At Kent we recognise, encourage and reward excellence. We have created the Kent Scholarship for Academic Excellence.
The scholarship will be awarded to any applicant who achieves a minimum of A*AA over three A levels, or the equivalent qualifications (including BTEC and IB) as specified on our scholarships pages.
We have a range of subject-specific awards and scholarships for academic, sporting and musical achievement.
Search scholarshipsTeaching is by lectures, practical classes, tutorials and workshops. You have an average of nine one-hour lectures, one or two days of practical or project work and a number of workshops each week. The practical modules include specific study skills in physics and general communication skills. In the MPhys final year, you work with a member of staff on an experimental or computing project.
Assessment is by written examinations at the end of each year and by continuous assessment of practical classes and other written assignments. Your final degree result is made up of a combined mark from the Stage 2/3/4 assessments with a weighting of 20/30/50.
Please note that there are degree thresholds at stages 2 and 3 that you will be required to pass in order to continue onto the next stages.
For a student studying full time, each academic year of the programme will comprise 1200 learning hours which include both direct contact hours and private study hours. The precise breakdown of hours will be subject dependent and will vary according to modules. Please refer to the individual module details under Course Structure.
Methods of assessment will vary according to subject specialism and individual modules. Please refer to the individual module details under Course Structure.
The programme aims to:
MPhys students gain a systematic understanding of most fundamental laws and principles of physics and astrophysics, along with their application to a variety of areas in physics and/or astrophysics, some of which are at the forefront of the discipline.
The areas covered include:
You also gain an understanding of the theory and practice of astrophysics, and of those aspects upon which it depends – a knowledge of key physics, the use of electronic data processing and analysis, and modern day mathematical and computational tools.
You gain intellectual skills in how to:
As an MPhys student, you also develop:
You gain subject-specific skills in:
As an MPhys student, you also gain:
You gain transferable skills in:
All University of Kent courses are regulated by the Office for Students.
Based on the evidence available, the TEF Panel judged that the University of Kent delivers consistently outstanding teaching, learning and outcomes for its students. It is of the highest quality found in the UK.
Please see the University of Kent's Statement of Findings for more information.
Physics and Astronomy at Kent scored 89% overall in The Complete University Guide 2021.
Over 90% of Physics and Astronomy graduates who responded to the most recent national survey of graduate destinations were in work or further study within six months (DLHE, 2017).
Kent Physics graduates have an excellent employment record with recent graduates going on to work for employers:
You graduate with an excellent grounding in scientific knowledge and extensive laboratory experience. In addition, you also develop the key transferable skills sought by employers, such as:
You can also enhance your degree studies by signing up for one of our Kent Extra activities, such as learning a language or volunteering.
The University has a friendly Careers and Employability Service which can give you advice on how to:
The experience you have gained in your placement year will be attractive to employers, putting you in a good position as you look for full-time employment.
Fully accredited by the Institute of Physics
If you are from the UK or Ireland, you must apply for this course through UCAS. If you are not from the UK or Ireland, you can choose to apply through UCAS or directly on our website.
Find out more about how to apply
T: +44 (0)1227 823254
E: internationalstudent@kent.ac.uk
Discover Uni is designed to support prospective students in deciding whether, where and what to study. The site replaces Unistats from September 2019.
Discover Uni is jointly owned by the Office for Students, the Department for the Economy Northern Ireland, the Higher Education Funding Council for Wales and the Scottish Funding Council.
It includes:
Find out more about the Unistats dataset on the Higher Education Statistics Agency website.