Universität Wien

280497 VU PM-Astr Cosmological structure formation: theoretical foundations and modern applications (PI) (2018W)

Continuous assessment of course work

Registration/Deregistration

Note: The time of your registration within the registration period has no effect on the allocation of places (no first come, first served).

Details

max. 15 participants
Language: German, English

Lecturers

Classes (iCal) - next class is marked with N

First class on Thu, 4.10. 2018 at 9:45 in Seminarraum 2 in the Univ.-Observatory

as of November some units in the computer lab (PC-Labor) of the Observatory

Thursday 04.10. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 11.10. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 18.10. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 25.10. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 08.11. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 15.11. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 22.11. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 29.11. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 06.12. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 13.12. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 10.01. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 17.01. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 24.01. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday 31.01. 09:45 - 11:15 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17

Information

Aims, contents and method of the course

Content:

Intro/Recap to the cosmological standard model and cosmic inventory; Gravitational instabilities in an expanding Universe; Linear perturbations of structure growth and information gathered from the cosmic microwave background radiation (transfer functions and power spectra); Simple/approximate models of nonlinear structure growth; Postcollapse equilibrium structure of galaxies and galaxy clusters; Halo mass functions and abundances (Press-Schechter theory); Theoretical and practical foundations of N-body and hydrodynamical cosmological simulations; Galaxy correlation functions in real space and redshift space; Inhomogeneities in the IGM; Constraints from structure growth for models of dark matter and dark energy

Methods:

analytical and numerical calculations; Application of scientific software for cosmological structure formation simulations ( Practicum in computer lab)

Assessment and permitted materials

This course requires presence in class. Course grade will be based upon homework/problem sets, prakticum protocols and presence in class.
No exams !

Minimum requirements and assessment criteria

Details in the first class (Thu, Oct 4th, 2018)

Prerequisite: Knowledge of astrophysics and theoretical physics as acquired through a Bachelor study of Astronomy or Physics; Knowledge in computer science is useful, but not required.

Examination topics

Content of Lecture Course

Reading list

Details to be discussed in the first class

Association in the course directory

Last modified: Mo 07.09.2020 15:42