FPF:UFTF008 Relativistic Physics and Astro - Course Information

UFTF008 Relativistic Physics and Astrophysics II

Extent and Intensity

4/2/0. 8 credit(s). Type of Completion: zk (examination).

Teacher(s)

doc. RNDr. Petr Slaný, Ph.D. (lecturer)
doc. RNDr. Petr Slaný, Ph.D. (seminar tutor)
doc. RNDr. Jan Schee, Ph.D. (lecturer)
Mgr. Dmitriy Ovchinnikov (seminar tutor)
doc. RNDr. Jan Schee, Ph.D. (seminar tutor)

Guaranteed by

prof. RNDr. Zdeněk Stuchlík, CSc.
Centrum interdisciplinárních studií – Faculty of Philosophy and Science in Opava

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

• Theoretical Physics (programme FPF, N1701 Fyz)

Course objectives

This course represents a continuation of F 1U 301 and brings an extension of mathematical methods of general relativity and it further expanses the astrophysical and cosmological applications of general relativity.

Syllabus

• Selected problems of relativistic physics. Introduction to differential forms formalism, dual tensors, integration in spacetimes; integral form of conservation laws of energy and momentum, angular momentum tensor and spin; Fermi-Walker transfer and local reference frames; Lie derivation and Killing vectors; integration in curved spacetimes, Stokes rule, energy, momentum and angular momentum of gravitational field.
  Charged and rotating black holes. Reissner-Nordstrom geometry, inner and outer horizont, analytic continuation, complete Penrose diagram; Kerr geometry, naked singularities, Kerr-Schild and Boyer-Lindquist coordinates, event horizont and static limit surface, dragging of inertial frames; Kerr-Newman geometry, dipole electromagnetic field, mass, angular momentum and magnetic moment; Carter equations of motion, extraction of energy from ergosphere, superradiation, reversible and irreversible transformations, Penrose diagram of Kerr-Newman metrics, instability of the inner horizont.
  Properties of black holes. Wheeler's no hair theorem, uniqueness theorems, cosmic censorship hypothesis, singularity theorems.
  Black hole thermodynamics. Connection of geometrical and thermodynamical characteristics of black holes, four laws of black hole thermodynamics, Hawking quantum evaporation of black holes, black holes as thermodynamical systems.
  Standard cosmological model. Friedman equation and age of the Universe, equilibrium thermodynamics, entropy, thermal history of the Universe, causal horizont.
  Nuclear synthesis. Nuclear statistical equilibrium, initial conditions, creation of light elements, primordial nuclear synthesis as a test.
  Baryogenesis. Baryon asymmetry of the Universe, breaking of baryon symmetry, simple Boltzmann equation, vanishing of primordial asymmetries, lepton numbers in the Universe, non-equilibrium decay.
  

Literature

recommended literature
• Straumann, N. General Relativity. Springer, 2004. ISBN 3540219242. info
• Börner G. The Early Universe. Springer, 2003. ISBN 3540441972. info
• Wald R.M. General Relativity. The University of Chicago Press, 1984. ISBN 0226870324. info
• Chandrasekhar S. The Mathematical Theory of Black Holes. Clarendon Press, 1983. ISBN 0-226-10100-2. info
• Hawking S.W., Ellis, G. F. R. The Large Scale Structure of Space-Time. Cambridge Univ. Press, 1975. ISBN 0521200164. info
• ] Misner C.W., Thorne K.S., Wheeler J.A. Gravitation. Freeman and Co., San Francisco, 1973. info

Language of instruction

Czech

Further comments (probably available only in Czech)

Study Materials
The course can also be completed outside the examination period.

Teacher's information

60% attendance at lectures

• Enrolment Statistics (recent)
  
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