SH2403 Astrophysics, Advanced Course 6.0 credits

Astrofysik, fortsättningskurs

This is an advanced course in Astrophysics.

  • Education cycle

    Second cycle
  • Main field of study

    Physics
  • Grading scale

    A, B, C, D, E, FX, F

Course offerings

Autumn 19 for programme students

Autumn 19 for Study Abroad Programme (SAP)

  • Periods

    Autumn 19 P2 (6.0 credits)

  • Application code

    10058

  • Start date

    28/10/2019

  • End date

    14/01/2020

  • Language of instruction

    English

  • Campus

    AlbaNova

  • Tutoring time

    Daytime

  • Form of study

    Normal

  • Number of places

    No limitation

  • Course responsible

    Josefin Larsson <josla@kth.se>

  • Teacher

    Felix Ryde <fryde@kth.se>

    Josefin Larsson <josla@kth.se>

  • Target group

    Only SAP-students. Students from UCAS only.

    Physics Background

  • Application

    Apply for this course at antagning.se through this application link.
    Please note that you need to log in at antagning.se to finalize your application.

Autumn 18 for programme students

Intended learning outcomes

After completing the course the student should be able to:

  • Describe the most important radiation processes in the Universe.
  • Apply the theories for the production of continuum spectra to calculate the most important properties of the emitting object/medium from observed spectra.
  • Explain the main points of accretion theory and use the theory to solve problems for relevant astrophysical phenomena.
  • Describe Compact objects (black holes and neutron stars) and phenomena related to these objects (e.g., active galactic nuclei, pulsars and gamma-ray bursts).
  • Apply the learning outcomes above to critically evaluate different ways of using high-energy observations to study the properties of compact objects.

Course main content

The course gives a solid foundation in astrophysics, with particular emphasis on high-energy astrophysics. The following topics are covered:

  • Continuum spectra: Compton emission, Synchrotron emission and Brehmsstrahlung.
  • Accretion onto neutron stars and black holes
  • Astrophysical applications of the theory of relativity
  • Compact objects (black holes and neutron stars) and phenomena related to these objects (e.g., active galactic nuclei, pulsars and gamma-ray bursts), with particular focus on relevant radiation processes.

Eligibility

Recommended prerequisites: Astrophysics equivalent to SH2204 and Mathematical methods in physics.

Literature

Lecture notes and hand outs.

Examination

  • INL1 - Exercises, 2.0, grading scale: P, F
  • PRO1 - Project Work, 4.0, grading scale: A, B, C, D, E, FX, F

Requirements for final grade

Hand-in exercises (2hp)

Project work (4 hp)

Offered by

SCI/Undergraduate Physics

Contact

Josefin Larsson, jlarsson@particle.kth.se

Examiner

Josefin Larsson <josla@kth.se>

Version

Course syllabus valid from: Autumn 2015.
Examination information valid from: Autumn 2013.