Undergraduate MPhys
Physics with Astrophysics
Excited by discovery? Passionate about exploring the cosmos? This is the degree for you.
Physics gives you the tools to understand our world at a fundamental level, from the smallest sub-atomic particles to the large-scale structure of the universe. By combining your study with astrophysics, you’ll use the principles of physics, our dedicated astrophysics lab module and fantastic facilities such as the Beacon Observatory, to explore the cosmos – from our own solar system to galaxies and cosmology.
Our four-year integrated Master's programme (MPhys) allows you to hone the skills needed for research and technical roles in industry, or as a preparation for a PhD. Deepen your knowledge with specialised taught modules and work with an academic to carry out a real, open-ended research project.
Our focus is on helping you follow your passion as well as giving you the best possible start to your future. You'll gain a wide range of skills that will open up career pathways in the growing space industry, finance, manufacturing and technology.
If you don’t have a science background or don’t meet our entry requirements, you can take our foundation year.
You might also be interested in our Physics MPhys or Astronomy, Space Science and Astrophysics MPhys degrees.
This course is fully accredited by the Institute of Physics.
Spend a year studying abroad at one of our partner universities. We currently have links with institutions in the US, Canada, Hong Kong and Switzerland.
You'll be able to move between our courses in the earlier years, ensuring you are studying the best course for you.
Exploring all areas of physics was important to Lucy Abbott, which is why she chose to study at Kent – that and Kent's friendly atmosphere.
You'll discover the latest developments in areas such as quantum materials and medical imaging from innovative teachers who are also active researchers.
You'll use newly-refurbished physics and astronomy labs, a photonics centre and the Beacon Observatory with optical telescope.
Our typical offer levels are listed below and include indicative contextual offers. If you hold alternative qualifications just get in touch and we'll be glad to discuss these with you.
ABB including Mathematics at B (Use of Mathematics not accepted)
The University will consider applicants holding/studying BTEC Extended National Diploma Qualifications (QCF; NQF;OCR) in Engineering. A typical offer would be to achieve Distinction, Distinction, Merit.
128 tariff points - typically H5, H6, H6 at HL including HL Maths/Maths Method or HL Mathematics: Analysis and Approaches at 5 or SL Maths/Maths Methods at 6 (not Maths Studies/SL Maths: Applications & Interpretations).
N/A
The University will consider applicants holding T level qualifications in subjects closely aligned to the course.
The University welcomes applications from Access to Higher Education Diploma candidates for consideration. A typical offer would be to obtain Access to HE Diploma with 45 Credits at level 3 with 30 credits at Distinction and 15 credits at Merit. A Science Access programme including Maths and Physics credits at Level 3 would be required.
The following modules are offered to our current students. This listing is based on the current curriculum and may change year to year in response to new curriculum developments and innovation:
You’ll get to grips with the broad knowledge base on which physics is built and develop your, experimental, computational, statistical and analytical skills.
This module provides an introduction to astronomy, beginning with our own solar system and extending to objects at the limits of the universe. Straightforward mathematics is used to develop a geometrical optics model for imaging with lenses and mirrors, and this is then used to explore the principles of astronomical telescopes.
This module builds on prior knowledge of arithmetic, algebra, and trigonometry. It will cover key areas of mathematics which are widely used throughout undergraduate university physics. In the first part it will look at functions, series, derivatives and integrals. In the second part it will look at vectors, matrices and complex numbers.
This module builds on the Mathematics I module to develop key mathematical techniques involving multiple independent variables. These include the topics of differential equations, multivariate calculus, non-Cartesian coordinates, and vector calculus that are needed for Physics modules in Stages 2 and 3.
In this module the mathematics of vectors and calculus are used to describe motion, the effects of forces in accordance with Newton's laws, and the relation to momentum and energy. This description is extended to rotational motion, and the force of gravity. In addition, the modern topic of special relativity is introduced.
This module examines key physical phenomena of waves and fields which extend over time and space. The first part presents a mathematical description of oscillations and develops this to a description of wave phenomena. The second part is an introduction to electromagnetism which includes electric and magnetic fields before providing an introduction to the topic of electrical circuits.
This module develops the principles of mechanics to describe mechanical properties of liquids and solids. It also introduces the principles of thermodynamics and uses them to describe properties of gases. The module also introduces the modern description of atoms and molecules based on quantum mechanics.
This module guides students through a series of experiments giving them experience in using laboratory apparatus and equipment. Students will also learn how to accurately record and analyse data in laboratory notebooks and write scientific laboratory reports. The experiments cover subjects found in the Physics degree program and are run parallel with Computing Skills workshops in which students are introduced to the concept of using programming/scripting languages to analyse and report data from their experiments.
One-on-one meetings and small group tutorials focused on academic progression and the development of key skills to support the core curriculum and future study or employment. Students meet with their Academic Advisor individually or in small groups at intervals during the academic year. Individual meetings review academic progress, support career planning etc. Themed tutorials develop transferable skills; indicative topics are essay and report writing, presentation skills, sourcing information, critical analysis etc. The tutorials are informal involving student activity and discussion. Year group events deliver general information e.g. on University resources, 4-year programmes, module selection etc.
You’ll deepen your understanding of physics and astrophysics, carry out in-depth laboratory experiments and work on group projects.
One-on-one meetings and small group tutorials focused on academic progression and the development of key skills to support the core curriculum and future study or employment. Students meet with their Academic Advisor individually or in small groups at intervals during the academic year. Individual meetings review academic progress, support career planning etc. Themed tutorials develop transferable skills; indicative topics are essay and report writing, presentation skills, sourcing information, critical analysis etc. The tutorials are informal involving student activity and discussion. Year group events deliver general information e.g. on University resources, 4-year programmes, module selection etc.
This module provides an introduction to quantum mechanics, developing knowledge of wave-functions, the Schrodinger equation, solutions and quantum numbers for important physical properties. Topics include: 2-state systems. Bras and kets. Eigenstates and Eigenvalues; Superposition Principle; Probability Amplitudes; Change of Basis; Operators. The Schrodinger equation. Stationary states. Completeness. Expectation values. Collapse of the wave function. Probability density. 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. Atomic vibrations.
This module will build on the general principles of quantum mechanics introduced earlier in the degree and applied them to the description of atoms, starting by the description of the hydrogen atom and covering other topics such as the effect of magnetic fields on an atom or X-ray spectra.
This module looks to introduce a range of important laws and principles relating to the physics of electromagnetism and optics. Students will also learn mathematical techniques to enable the modelling of physical behaviour and apply important theory to a range of electromagnetism and optics scenarios.
This module builds on the brief introduction to astronomy previously taught in earlier stages. Students enhance their knowledge of astrophysics through the study of the theory, formalism and fundamental principles developing a rigorous grounding in observational, computational and theoretical aspects of astrophysics. In particular they study topics such as properties of galaxies and stars and the detection of planets outside the solar system.
In this module students develop their experience of the practical nature of physics, including developing their ability to execute an experiment, and to use programming scripts to process data. Students also develop their skill in analysis of uncertainties, and comparison with theory. The module strengthens students' communication skills and knowledge of, and ability to write, all components of laboratory reports.
This module gives students experience of group work in the context of a physics investigation in an unfamiliar area. The module includes workshops for advice about successful group project work, and culminates in each group producing a report and presentation.
This module introduces and develops a knowledge of numerical approximations to solve problems in physics, building on the programming skills gained in earlier stages. In addition, it complements the analytical methods students are trained to use and extends the range of tools that they can use in later stages of the degree. This module covers for example how to solve linear equations, how to find eigenvalues and numerical integration and differentiation.
The module will 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.
You’ll take more advanced and specialised modules and conduct open-ended laboratory investigations.
One-on-one meetings and small group tutorials focused on academic progression and the development of key skills to support the core curriculum and future study or employment. Students meet with their Academic Advisor individually or in small groups at intervals during the academic year. Individual meetings review academic progress, support career planning etc. Themed tutorials develop transferable skills; indicative topics are essay and report writing, presentation skills, sourcing information, critical analysis etc. The tutorials are informal involving student activity and discussion. Year group events deliver general information e.g. on University resources, 4-year programmes, module selection etc.
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.
Problems are presented and solutions discussed in topics spanning several topics in the undergraduate physics curriculum (Mechanics and statics, thermodynamics, and optics, 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.
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.
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.
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:
Interaction potential for atoms and ions. Definitions, crystal types. Miller indices. Reciprocal lattice. Diffraction methods.
Dynamics of Vibrations.
Lattice dynamics, phonon dispersion curves, experimental techniques.
Electrons in k-space: metals.
Free electron theory of metals. Density of states. Fermi-Dirac distribution. Band theory of solids - Bloch's theorem. Distinction between metals and insulators. Electrical conductivity according to classical and quantum theory. Hall effect.
Semiconductors.
Band structure of ideal semiconductor. Density of states and electronic/hole densities in conduction/valence band. Intrinsic carrier density. Doped semiconductors.
Magnetism.
Definitions of dia, para, ferromagnetism. Magnetic moments. General treatment of paramagnetism, Curie's law. Introduction to ferromagnetism.
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.
Physics of Stars
equations of state for an ideal multiple chemical component star; degenerated stars, Nuclear reactions: PPI, PPII, PPIII chains; CNO cycle, Triple-alpha process; elemental abundances; energy transportation inside a star; derivation of the approximate opacity and energy generation models as function of density, temperature and chemical components; Solar neutrino problem; polytropic models applied to the equations of stars; Lane-Emden equation; Chandrasekhar mass; the Eddington Luminosity and the upper limit of mass; detailed stellar models; Post main sequence evolution of solar mass stars; Red Giants; White Dwarfs; Neutron Stars; Degenerate matter; properties of white dwarfs; Chandrasekhar limit; neutron stars; pulsars; Supernovae
General Relativity and Cosmology
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; Einstein Rings, black holes, gravitational waves; Brief survey of the universe; Olbers paradox, Cosmology, principles, FRW Metric, Laws of Motion & Distances, Friedmann equation, Scale Factor, Fluid equation, The Hubble Parameter, Critical Density parameter, Cosmological Constant parameter, Radiation-Matter-Dark Energy phases; The CMB, Temperature Horizons. Monopoles. Flatness problem. Hubble sphere, Inflation, Anisotropies, Polarisation Baryon Acoustic Oscillations, Secondary anisotropies; Baryosynthesis, Nucleosynthesis, Dark Matter observations, Lensing, Bullet Cluster, Dark Matter candidates, Cosmic Distance Ladder, Redshifts Galaxy surveys; Acceleration equation, Deceleration equation, Supernova as standard candles, Dark Energy, Einstein Field equations, Coincidence problem, The Cosmic Dark Ages & AGN Reionisation, High-z galaxies
This module is an introduction to the developments in classical mechanics since the time of Newton. In it, students will learn a variety of methods to formulate complex problems in classical systems and classify different types of dynamics that may occur.
This module will introduce students to basic concepts in nuclear and particle physics, and will provide an understanding of how the principles of quantum mechanics are used to describe matter at sub-atomic length scales. The following concepts will be covered:
* 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.
* Experimental methods in Nuclear and Particle Physics (Accelerators, detectors, analysis methods, case studies will be given).
* Discovery of elementary particles and the standard model of particles
* Leptons, quarks and vector bosons
* The concept of four different forces and fields in classical and quantum physics; mediation of forces via virtual particles, Feynman Diagrams
* Relativistic Kinematics
* Relativistic Quantum Mechanics and Prediction of Antiparticles
* Symmetries and Conservation Laws
* Hadron flavours, isospin, strangeness and the quark model
* Weak Interactions, W and Z bosons
Students will develop a number of skills related to the investigation and planning of research such as analytical skills, critical thinking and ability to understand and communicate scientific information in graphically. Students will learn how to search and retrieve information from a variety of locations (colloquia, websites, journals, proceedings etc). They will learn how to compile professionally-produced scientific documents such as colloquia reports, posters and applications for funding of future research activities/research job applications. The Group research investigation strengthens these skills, adding experience of working in a team.
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.
Aims:
To provide an experience of open-ended research work.
To begin to prepare students for postgraduate work towards degrees by research or for careers in R&D in industrial or government/national laboratories.
To deepen knowledge in a specialised field and be able to communicate that knowledge orally and in writing.
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.
One-on-one meetings and small group tutorials focused on academic progression and the development of key skills to support the core curriculum and future study or employment. Students meet with their Academic Advisor individually or in small groups at intervals during the academic year. Individual meetings review academic progress, support career planning etc. Themed tutorials develop transferable skills; indicative topics are essay and report writing, presentation skills, sourcing information, critical analysis etc. The tutorials are informal involving student activity and discussion. Year group events deliver general information e.g. on University resources, 4-year programmes, module selection etc.
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.
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.
In this module you learn what is meant by neural networks and how to explain the mathematical equations that underlie them. You also familiarise yourself with cognitive neural networks using state of the art simulation technology and apply these networks to the solution of problems. In addition, the module discusses examples of computation applied to neurobiology and cognitive psychology. The module also introduces artificial neural networks from the machine learning perspective. You will study the existing machine learning implementations of neural networks, and you will also engage in implementation of algorithms and procedures relevant to neural networks.
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.
Introduction. Magnetism, magnetometry and measuring techniques, Localised magnetic moments, spin and orbital moments, magnetic moments in solids. Paramagnetism. Exchange interactions, direct, indirect and superexchange, Magnetic structures, ferro, ferri, antiferromagnetism. Neutron and X-ray scattering. Spin waves, magnons. Magnetic phase transitions. Superconductivity: Introduction to properties of superconductors, Thermodynamics and electrodynamics of superconductors, Type I and Type II superconductors, the flux lattice Superconducting phase transitions. Microscopic superconductivity, correlations lengths, isotope effect, Cooper pairs, Froehlich Interaction, BCS theory. High Tc superconductors, superfluids, liquid helium.
Quantum mechanics is the theoretical basis of much of modern physics. Building on the introductory quantum theory studied in earlier stages, this module will review some key foundational ideas before developing more advanced topics of quantum mechanics and quantum field theory.
Teaching 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.
For programme aims and learning outcomes please see the programme specification.
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: excellent communication and analytical skills; problem-solving and the ability to work independently or as part of a team. This means you’re well equipped for careers in a range of fields.
Our graduates have gone on to work for companies such as:
Read some of their stories and find out about the range of support and extra opportunities available to further your career potential.
The course pushes you to try your hardest in the core aspects and pushes you to broaden your horizons in terms of your skills.
The 2024/25 annual tuition fees for this course 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.
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.
Join the student-led Physics Society and Space Soc. They organise talks, practical demonstrations and social events. A great way to meet students across year groups.
Next steps
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 apply through UCAS or directly on our website if you have never used UCAS and you do not intend to use UCAS in the future.
We welcome applications from students all around the world with a wide range of international qualifications.
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