Cosmology

PHYS30392 Cosmology 10 Semester 2 Undergraduate Level 3 Scott Kay Unit coordinator Department of Physics & Astronomy 1 FHEQ level (Framework for Higher Education Qualifications) ' Last part of a Bachelors ' European Credit Transfer & Accumulation System Rating : 5.0 Cosmology Cosmology 1. To provide a broad overview of modern physical cosmology. 2. To make clear the connections between basic physical ideas and modern cosmology. On completion of the course, students should be able to: 1. Explain the concepts of the expansion and curvature of space. 2. Summarize the main evidence in favour of the Big Bang, inflation, dark matter and dark energy. 3. Relate the density of the universe to its rate of expansion and understand how this relation is modified by a cosmological constant. 4. Solve for the scale factor a(t) in different epochs of the Universe’s history. 5. Make quantative calculations of physical processes in the early universe. 6. Relate observed to physical properties of distant objects given the luminosity and angular size distances. 7. Describe the main events of the universe's history and locate them approximately in time and redshift. 1. Basic observations of the Universe                                                                                         (6 lectures) 1.1  What is cosmology? 1.2  Olber’s paradox 1.3  Expansion and acceleration of the Universe 1.4  Cosmic Microwave Background 1.5  Large-scale structure 1.6  Dark matter in galaxies and clusters of galaxies2. FRW Universe Model                                                                                                                 (8 lectures) 2.1  Review of Newtonian gravity 2.2  Geometry of the spacetime 2.3  Dynamical equations 2.4  Solutions for the scale factor 2.5  Distances measures in the FRW Universe 2.6  Cosmological puzzles and inflation3. Thermal History of the Universe                                                                                              (6 lectures) 3.1  Review of statistical mechanics and natural units 3.2  Cosmological freeze-out 3.3  Recombination 3.4  Neutrino decoupling – relativistic freeze-out 3.5  WIMP decoupling – non-relativistic freeze-out 3.6  Nucleosynthesis 3.7  Baryogenesis 3.8  Brief history of time!4. Precision Cosmology                                                                                                                  (2 lectures) 4.1  Standard model of cosmology 4.2  Measurement of parameters using the CMB & P(k) 4.3  Beyond the standard model : curvature, dark energy & massive neutrinos   1 Written exam 100% Feedback will be offered by examples class tutors based on examples sheets, and model answers will be issued. PHYS10071 Mathematics 1 Pre-Requisite Compulsory PHYS10101 Dynamics Pre-Requisite Compulsory PHYS10121 Quantum Physics and Relativity Pre-Requisite Compulsory PHYS10191 Introduction to Astrophysics and Cosmology Pre-Requisite Compulsory PHYS10302 Vibrations & Waves Pre-Requisite Compulsory PHYS10372 Mathematics 2 Pre-Requisite Compulsory PHYS20352 Statistical Mechanics Pre-Requisite Compulsory <div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;">Pre-Requisites:</div><div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;">Mathematics of Waves and Fields PHYS20171 OR MATH24420 PDEs and vector calculus;</div><div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;">Statistical Mechanics PHYS20352;</div><div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;"> </div><div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;">Desirable content:</div><div class="ewa-rteLine" style="-webkit-text-stroke-width:0px;background-color:rgb(255, 255, 255);color:rgb(0, 0, 0);font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;"><span style="-webkit-text-stroke-width:0px;display:inline !important;float:none;font-family:"Aptos Narrow";font-size:16px;font-style:normal;font-variant-caps:normal;font-variant-ligatures:normal;font-weight:400;letter-spacing:normal;orphans:2;text-align:start;text-decoration-color:initial;text-decoration-style:initial;text-decoration-thickness:initial;text-indent:0px;text-transform:none;white-space:pre-wrap;widows:2;word-spacing:0px;">Introduction to Astrophysics and Cosmology PHYS10191</div> N Recommended text: Liddle, A., An Introduction to Modern Cosmology 2nd ed. (Wiley) Ryden, B., Introduction to Cosmology (Addison Wesley)Useful references: Harrison, E., Cosmology: the Science of the Universe, 2nd ed. (CUP) Hawley, J.F and Holcomb, K.A., Foundations of Modern Cosmology (Oxford) Peacock, J.A., Cosmological Physics, (CUP) Serjeant, S., Observational Cosmology (CUP)Supplementary reading:Weinberg, S., The First Three Minutes, Updated ed. (Basic Books)   Assessment written exam 2 Lectures 22 Practical classes & workshops 3 0 73