Stellar Structure (035F3)

in detail...

Key facts

Details for course being taught in current academic year
Level M  -  15 credits  -  autumn term

Resources

Timetable Link
course web pages



Course description

Course outline

* Observed properties of stars.
* Dynamical structure; virial theorem; polytropic models.
* Energy balance; equations of energy transport and energy production. Full equations for star in radiative equilibrium, with boundary conditions.
* Homologous solutions.
* Criterion for the occurrence of convection; changes in structure equations when convection is present. Improved surface boundary condition.
* Physics of stellar interiors: chemical composition; gas and radiation pressure; pressure of degenerate electron gas; nuclear fusion reactions H and He burning, neutrino processes; opacity scattering, bound-bound, bound-free, free-free absorption.
* Outline of stellar evolution: Hayashi track and pre-main-sequence evolution; main sequence structure; chemical inhomogeneity, red giants and post-ms evolution.
* Endpoints of stellar evolution: white dwarf models; neutron stars and black holes.

Pre-requisite

Quantum Mechanics, Thermal & Statistical Physics, Atomic Physics, Nuclear & Particle Physics I

Learning outcomes

By the end of the course, a successful student should be able to
1 outline the principal observed properties of stars;
2 write down the four ordinary differential equations of stellar structure and their boundary conditions;
3. solve quantitative problems on topics in the course.
4. outline the principles of evolution of a star from the main sequence to the final stages.

Library

The Stars: their Structure and Evolution by R J Tayler (CUP 1994)
Other books at a similar level are:
Boehm Vitense, E., Introduction to Stellar Astrophysics (3 volumes; students would need: Vol. 1, Basic Stellar Observations, and Vol. 3, Stellar Structure and Evolution, CUP 1989, 1992).
Prialnik, D., An Introduction to the Theory of Stellar Structure and Evolution (CUP 2000)



Assessments

View old exam papers

Type Timing Weighting
Coursework40.00%
Problem SetsAutumn Week 325.00%
Problem SetsAutumn Week 525.00%
Problem SetsAutumn Week 725.00%
Problem SetsAutumn Week 925.00%
Unseen ExaminationSummer Term  (1 hour 30 minutes)60.00%

Resit mode of assessment

Type Timing Weighting
Unseen ExaminationSummer Vacation   (1 hour 30 minutes)100.00%

Timing

Submission deadlines may vary for different types of assignment/groups of students.

Weighting

Coursework components (if listed) total 100% of the overall coursework weighting value.



Teaching methods

Term Method Duration Week pattern
Autumn Term LECTURE 1 hour 2222222222
Autumn Term CLASS 1 hour 1111111111

How to read the week pattern

The numbers indicate the weeks of the term and how many events take place each week.



Contact details

Dr Robert Smith

Assess convenor
http://www.sussex.ac.uk/physics/profile2477.html



Data maintained by School Administrator (Curriculum) A-Z Index | Help | Contact us