UFUF012 Selected chapters from physical phenomena in vicinity of black holes

Faculty of Philosophy and Science in Opava
Winter 2013
Extent and Intensity
2/1/0. 4 credit(s). Type of Completion: z (credit).
Teacher(s)
doc. RNDr. Jan Schee, Ph.D. (lecturer)
doc. RNDr. Jan Schee, Ph.D. (seminar tutor)
Guaranteed by
doc. RNDr. Jan Schee, Ph.D.
Centrum interdisciplinárních studií – Faculty of Philosophy and Science in Opava
Prerequisites (in Czech)
Navazuje na UF/TF502, UF/O3381
Course Enrolment Limitations
The course is also offered to the students of the fields other than those the course is directly associated with.
fields of study / plans the course is directly associated with
Course objectives
Discussion of actual developments in the area of physical process in the field of black holes.
Syllabus (in Czech)
  • 1. Testovací toroidální struktury
    1.1. ve statických, sféricky symetrických prostoročasech
    1.2. ve stacionárních, osově symetrických prostoročasech
    2. Self-gravitace
    2.1. v rámci Newtonovy mechaniky
    2.2 v rámci Obecné teorie relativity
    2.3. Rotující hvězdy a toroidální struktury
    3. Řešení systému parciálních diferenciálních rovnic relaxační metodou.
Literature
    recommended literature
  • T. W. Baumgarte and S. L. Shapiro. Numerical Relativity: Solving Einstein's Equations on the Computer. Cambridge University Press, 2010. info
  • P. Slaný. and Z. Stuchlík. Relativistic thick discs in the Kerr de Sitter backgrounds. Classical and Quantum Gravity, 22, p. 3623-3651, 2005. info
  • J. Frank, A. R. King and D. J. Raine. Accretion Power in Astrophysics. Cambridge University Press, 2002. info
  • M. Hashimoto, Y. Eriguchi and E. Muller. Equilibrium structure of self-gravitating Keplerian disks. Astronomy and Astrophysics , 297, p.135-140, 1995. info
  • K. Uryu and Y. Eriguchi. Structures of rapidly rotating baroclinic stars - II. an extended numerical method for realistic stellar models. MNRAS, 277, 1411-1429, 1995. info
  • S. Nishida. and Y. Eriguchi. A general relativistic toroid around a black hole. Astrophysical Journal, 427, p. 429-437, 1994. info
Language of instruction
Czech
Further Comments
The course can also be completed outside the examination period.
Teacher's information
20-40 min presentation or an essay on given topic
Course Content
The discussions will be focused on following topics:
black hole spacetimes,
analysis of test particle motion,
particle acceleration,
particle collisions,
scalar fields,
Penrose process
The course is also listed under the following terms Winter 2014, Winter 2015.
  • Enrolment Statistics (Winter 2013, recent)
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