PH40112: Relativistic cosmology
[Page last updated: 21 April 2022]
Academic Year: | 2022/3 |
Owning Department/School: | Department of Physics |
Credits: | 6 [equivalent to 12 CATS credits] |
Notional Study Hours: | 120 |
Level: | Masters UG & PG (FHEQ level 7) |
Period: |
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Assessment Summary: | EX 100% |
Assessment Detail: |
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Supplementary Assessment: |
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Requisites: | Before taking this module you must take PH30043 OR take PH30101 |
Learning Outcomes: | After taking this unit the student should be able to:
* show proficiency in calculations involving tensors (inner and outer products, contraction, parallel transport); * understand the basics of geometric/coordinate-free vector and tensor analysis; * perform covariant differentiation of tensor quantities in curved space; * provide a physical explanation of the Einstein field equations; * show how the Friedmann-Robertson-Walker metric is an exact solution to the Einstein equations; * describe the key ideas behind cosmology and the expanding universe; * describe the observations and techniques used to establish the accelerating expansion of the universe, including systematics and sources of uncertainty; * describe the observation and analysis of the Cosmic Microwave Background Radiation, including systematics and sources of uncertainty; * describe current state of the art cosmology experiments, how their results compare to each other, and current open questions that they address. |
Aims: | This unit aims to develop a mathematically rigorous description of general relativity and cosmology, including derivation of the Einstein field equations and the exploration of the Friedmann-Robertson-Walker solution, which forms the basis for modern cosmological models. The unit also aims to provide an overview of observational cosmology, and the techniques and observations that have constrained current cosmological models. |
Skills: | Numeracy T/F A, Problem Solving T/F A. |
Content: | Vectors, one-forms and tensors. Vector spaces, manifolds and tangent spaces. Einstein summation convention. Curvilinear coordinates. Tensor operations, covariant differentiation. Review of special relativity, spacetime metric and geodesics. Local coordinates. Locally inertial frames.
The Riemann tensor. The Bianchi identity, The Ricci tensor. Curvature scale. The Stress-energy tensor. Energy as the source of gravity. The dynamics of a pressureless dust. Conservation laws. Perfect fluids. The Einstein field equations. The Einstein tensor. The cosmological constant. Interpreting the field equations. The Friedmann-Robertson-Walker metric. Cosmological dynamics. Inflationary cosmology. Observations of the Cosmic Microwave Background Radiation. Observations and analysis of the extragalactic distance ladder. Sources of systematic and measurement uncertainty in cosmology. Comparison of results from different cosmological experiments. Current state of the art experiments. Open questions in the field and potential implications. |
Programme availability: |
PH40112 is Compulsory on the following programmes:Department of Physics
PH40112 is Optional on the following programmes:Department of Physics
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Notes:
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