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ASTM12: High-energy astrophysics, 7.5 credits

given by the Division of Astrophysics, Department of Physics.

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Contents

After the course you will be able in detail to account for:

The physical processes that occur in all types of supernovae and gamma-ray bursts
How supernovae and gamma-ray bursts are used for cosmological studies
How double stars evolve and how mass transfer between stars takes place

You will have knowledge of:

Snapshot from a simulation of a neutron-star merger

Neutron-star merger. Credit: Daniel Price (U/Exeter) and Stephan Rosswog (Int U/Bremen).

Different types of double star that contain compact objects.
Different types of galactic nuclei.
Those objects that can emit gravitational radiation.
Ongoing research within high-energy astrophysics.

Using the knowledge acquired you will be able to independently take on a complex problem, break it into its essential components, implement a solution and reflect on the results.

General information

Semester: Spring (VT)
Study period: 2
Level: Master
Language: English
Form of teaching: Lectures, group discussion sessions, problem-based learning sessions, and self-study
Note: In 2023 this course is planned to take place in person.
Assessment: Problem-based learning reports (20%), an assessed student lecture (20%), and a written final take-home examination (60%).
Grading scale: U-G-VG
Course plan: in English, in Swedish

Course literature

Introduction to high-energy astrophysics by Stephan Rosswog & Marcus Brüggen

Teachers

Ross Church, ross@astro.lu.se, phone: 046-22 21609
Abbas Askar, askar@astro.lu.se

Schedule

The schedule for the VT 2023 instance of the course is available here. The introductory meeting will start at 13.15 on Monday March 27.

Application

Through antagning.se