COSMOLOGY AND GALAXY FORMATION - 2018/9
Module code: PHY3055
In this module, students will learn about the observational evidence and theoretical framework of our standard model of cosmology. Using this framework, they will go on to learn about the growth of structure in the Universe and the formation and evolution of galaxies.
COLLINS ML Dr (Physics)
Number of Credits: 15
ECTS Credits: 7.5
Framework: FHEQ Level 6
JACs code: F510
Module cap (Maximum number of students): N/A
Prerequisites / Co-requisites
Introduction to Astronomy (BSc Physics Year 2 equivalent)
- General overview and introduction -
Historical background, observational cosmology and extragalactic astronomy, Big Bang and the early Universe, the cosmic microwave background, contents of the Universe: baryons, radiation, dark matter and dark energy. The cosmological principle, isotropy and homogeneity, standard candles and cosmic distances, the distance ladder, Hubble's law.
- Cosmological models -
The Friedmann equations, cosmological parameters, observational tests of the Friedman model, redshift and various distance measures in cosmology, matter and radiation dominated expansion, the flatness and the horizon problem, inflation, the thermal history of the Universe, recombination, the surface of last scattering, synthesis of the light elements. Observational constraints of our cosmological models (CMB, clustering, Lyman alpha alpha forest, reionisation of H and He).
- Formation of structure -
Growth of perturbations: gravitational instabilities in an expanding space-time, formation of large scale structure, the cosmic web, statistical properties of cosmological density fields: correlation functions and power spectra from theory and observations, Press-Schecter theory, Non-linear collapse, virialisation and the formation of dark matter haloes, the dark matter halo mass function, the halo model, halo bias.
- Galaxy Formation -
Dissipative collapse, cooling and heating processes, origin of angular momentum: tidal torque theory, disk formation, the role of galaxy mergers, modes of accretion: hot vs. cold inflow, the inter-galactic medium, the galaxy luminosity function, the galaxy-dark matter halo connection.
- Galaxy Evolution -
Galactic scaling relations: the Tully-Fisher and Faber-Jackson relation and the fundamental plane. The Hubble sequence and the blue and red sequence of galaxies. The high redshift Universe: the cosmic star formation history, gas rich high redshift galaxies, results from numerical simulations. Star formation and feedback processes. Puzzles in galaxy formation theory: the missing satellite problem, missing baryon problem, overcooling.
|Assessment type||Unit of assessment||Weighting|
|Examination||END OF SEMESTER 1.5HR EXAMINATION||70|
The assessment strategy is designed to provide students with the opportunity to demonstrate core competencies in astrophysics materials, through examination.
Thus, the summative assessment for this module consists of:
- a written examination of 1.5 hrs duration, with two questions from three to be attempted
- a midterm coursework assignment consisting of three questions of the type discussed during the weekly tutorials.
Formative assessment and feedback
Formative assessment is provided by verbal feedback in tutorials and lecture classes
- To provide the students with a coherent picture of our cosmological world view and the formation and evolution of galaxies and large scale structures. The module will provide the necessary theoretical framework to describe the evolution of the Universe and the principles structure formation.
|1||Describe modern cosmological models, the basic structure and contents of the Universe and how cosmic structures arise||KC|
|2||Demonstrate understanding of how to derive and solve the Friedmann equations, and explain the role of baryons, radiation, as well as the role of exotic concepts such as dark ¿matter and dark energy, in the standard model of cosmology||KC|
|3||Understand the thermodynamic evolution of the Universe, and should be able to describe the growth of density perturbations leading to the formation of structure||KC|
|4||Characterise the large scale distribution of matter in the Universe, and describe how modern observations can be used to constrain cosmological model||KC|
|5||Understand the processes relevant for dissipative collapse leading to disk galaxy formation, and how star formation and “feedback” operate in galaxies||K|
|6||Characterise galactic morphologies and how these follow observed galactic scaling relations||C|
|7||Discuss our current understanding of how high redshift galaxies relate to locally observed systems||KCT|
|8||Appreciate the evolving nature of galaxy formation theory and insight into ongoing puzzles, like the “missing satellite” and “missing baryons” problems||K|
C - Cognitive/analytical
K - Subject knowledge
T - Transferable skills
P - Professional/Practical skills
Overall student workload
Lecture Hours: 22
Tutorial Hours: 11
Methods of Teaching / Learning
The learning and teaching strategy is designed to increase students’ critical understanding of physics and astrophysics, and through this module to provide students with the opportunity to explore both the theoretical and experimental concepts of Cosmology and Galaxy Formation.
The learning and teaching methods include:
lectures (2hrs per week x 11 weeks) ‘
tutorials (1hr per week x 11 weeks)
Indicated Lecture Hours (which may also include seminars, tutorials, workshops and other contact time) are approximate and may include in-class tests where one or more of these are an assessment on the module. In-class tests are scheduled/organised separately to taught content and will be published on to student personal timetables, where they apply to taken modules, as soon as they are finalised by central administration. This will usually be after the initial publication of the teaching timetable for the relevant semester.
Reading list for COSMOLOGY AND GALAXY FORMATION : http://aspire.surrey.ac.uk/modules/phy3055
Programmes this module appears in
|Physics MSc||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics BSc (Hons)||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Nuclear Astrophysics BSc (Hons)||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Astronomy BSc (Hons)||1||Compulsory||A weighted aggregate mark of 40% is required to pass the module|
|Mathematics and Physics MPhys||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Mathematics and Physics BSc (Hons)||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Mathematics and Physics MMath||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics MPhys||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Quantum Technologies BSc (Hons)||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Quantum Technologies MPhys||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Nuclear Astrophysics MPhys||1||Optional||A weighted aggregate mark of 40% is required to pass the module|
|Physics with Astronomy MPhys||1||Compulsory||A weighted aggregate mark of 40% is required to pass the module|
Please note that the information detailed within this record is accurate at the time of publishing and may be subject to change. This record contains information for the most up to date version of the programme / module for the 2018/9 academic year.