AS5523 Gravitational Dynamics and Accretion Physics
Academic year
2025 to 2026 Semester 2
Curricular information may be subject to change
Further information on which modules are specific to your programme.
Key module information
SCOTCAT credits
15
SCQF level
SCQF level 11
Availability restrictions
Available only to students on MSc Astrophysics.
Module description
This theoretical module explores the basics of gravitational dynamics and accretion physics and their application to systems such as circumstellar discs, stellar clusters to galaxies and clusters of galaxies. The module will provide students with the techniques to determine physical properties from observable quantities and to model the dynamics and evolutionary pathways of these systems. Starting from two-body motion and orbits under a central-force law, the module describes the calculation of extended potentials and their associated orbits. The use of the virial theorem and the statistical treatment of large numbers of self-gravitating bodies is then developed with application to stellar systems. Accretion as a source of energy and mass growth will be explored with particular emphasis on models of viscous accretion discs. Applications of these methods are made to several different astrophysical objects including accretion discs in stellar systems, collisions in globular clusters, the growth of super-massive black holes, to the presence of dark matter in the universe.
Relationship to other modules
Pre-requisites
STUDENTS MUST BE REGISTERED FOR MSC ASTROPHYSICS.
Co-requisites
YOU MUST ALSO TAKE AS5500
Assessment pattern
2-hour Written Examination = 75%, Coursework = 25%
Re-assessment
Oral re-assessment = 100%, capped at grade 7
Learning and teaching methods and delivery
Weekly contact
3 lectures occasionally replaced by whole-group tutorials.
Scheduled learning hours
31
Guided independent study hours
119