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Advanced Physical Cosmology (PHAS0067)

Key information

Faculty
Faculty of Mathematical and Physical Sciences
Teaching department
Physics and Astronomy
Credit value
15
Restrictions
This module requires knowledge of material covered in PHAS0037 Physical Cosmology, or a similar intermediate-level cosmology course. Necessary aspects of GR are introduced in lectures, but students may find it helpful to take MATH0025 Mathematics for General Relativity, or to study the recommended text 'An Introduction to General Relativity, Space-time and Geometry' (Sean Carroll).
Timetable

Alternative credit options

There are no alternative credit options available for this module.

Description

Outline:

The aim of this module is to provide an advanced level exposition of modern theoretical and observational cosmology, building upon the foundations provided by the third year module PHAS0037 Physical Cosmology. The emphasis will be on developing physical understanding rather than on mathematical principles. Over the past two decades, cosmology has made dramatic advances. A flood of data has transformed our understanding of the basic parameters of the universe -- the expansion rate, the densities of various types of energy and the nature of the primordial density variations. The basic Big Bang picture, underpinned by General Relativity, continues to hold good, explaining the expansion of the universe, the cosmic microwave background radiation, the synthesis of light chemical elements and the formation of stars, galaxies and large-scale structures. However, there are important gaps in our understanding including the nature of the dark matter, the cause of the observed late-time acceleration of the universe and the classic puzzles of the initial singularity and what caused the Big Bang.

Aims:

This module will develop the standard Big Bang cosmology and review its major successes and some of the challenges now faced at the cutting-edge of the field. After the completion of this module, students will have an appreciation of the basic theoretical foundations of physical cosmology, as well as an advanced understanding of the physics of several observational results critical to our current picture of the Universe.

Teaching and Learning Methodology:

This module is delivered via weekly lectures supplemented by a series of workshops and additional discussion. In addition to timetabled lecture hours, it is expected that students engage in self-study in order to master the material. This can take the form, for example, of practicing example questions and further reading in textbooks and online.

Module deliveries for 2024/25 academic year

Intended teaching term: Term 2 ÌýÌýÌý Undergraduate (FHEQ Level 7)

Teaching and assessment

Mode of study
In person
Methods of assessment
90% Exam
10% Coursework
Mark scheme
Numeric Marks

Other information

Number of students on module in previous year
9
Module leader
Professor Andrew Pontzen
Who to contact for more information
a.pontzen@ucl.ac.uk

Intended teaching term: Term 2 ÌýÌýÌý Postgraduate (FHEQ Level 7)

Teaching and assessment

Mode of study
In person
Methods of assessment
90% Exam
10% Coursework
Mark scheme
Numeric Marks

Other information

Number of students on module in previous year
10
Module leader
Professor Andrew Pontzen
Who to contact for more information
a.pontzen@ucl.ac.uk

Last updated

This module description was last updated on 8th April 2024.

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