UFUF011 Selected chapters from physical processes in the field of black holes

Faculty of Philosophy and Science in Opava
Summer 2016
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 kurz UF/O3380.
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
In this course the compact object are described as a particle accelerators, particle collisions will be studied and efficiency in these collisions. In addition, students will become familiar with methods of determining stability criteria stationary spacetimes.
Syllabus
  • 1.0 Stationary spacetimes
    1.1 Precipitation in the field of black holes
    1.2 Precipitation in the naked singularities
    2.0 Stability of stationary spacetimes
    1.2 incident gravitational wave
    2.2 incident electromagnetic wave
    3.2 Numerical methods for finding stability criteria
Literature
    recommended literature
  • Z. Stuchlik ans J. Schee. Ultra-high energy collisions in the superspinning Kerr geometry,. CQG, 2013. info
  • M. Patil, P. S. Joshi; M. Kimura and K. Nakao. Acceleration of particles and shells by Reissner-Nordström naked singularities. Phys. Rev. D, 86, 8, 2012. info
  • T. W. Baumgarte and S. L. Shapiro. Numerical Relativity: Solving Einstein's Equations on the Computer. Cambridge University Press, 2010. info
  • M. Ba?ados, J. Silk and S. M. West,. Kerr Black Holes as Particle Accelerators to Arbitrarily High Energy. Phys. Rev. Lett.,103, 11, 2009. info
  • S Chandrasekhar. The Mathematical Theory of Black Holes. Oxford University Press, 1998. info
  • S. A. Teukolsky a W. H. Press. Perturbations of a rotating black hole. III - Interaction of the hole with gravitational and electromagnetic radiation. Astrophys. J., 193, 443-461, 1974. info
  • S. A. Teukolsky. Perturbations of a Rotating Black Hole. I. Fundamental Equations for Gravitational, Electromagnetic, and Neutrino-Field Perturbations. Astrophys. J., 185, p. 635-648, 1973. info
Language of instruction
Czech
Further comments (probably available only in Czech)
The course can also be completed outside the examination period.
Teacher's information
20-40 min presentation or an essay on given topic
The course is also listed under the following terms Summer 2014, Summer 2015.
  • Enrolment Statistics (recent)
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