UFDF031 Final Stages of Stellar Evolution

Faculty of Philosophy and Science in Opava
Winter 2019
Extent and Intensity
0/0/0. 0 credit(s). Type of Completion: dzk.
Guaranteed by
Mgr. Martin Urbanec, Ph.D.
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
Course objectives
Equations of state of superdense matter giving structure of white dwarfs and neutron stars are presented. Basic laws of general relativity necessary to determine structure of neutron stars and white dwarfs are discussed. General relativistic polytropes are solved as an example.
Syllabus
  • Creation and evolution of stars. Possible final stages of star evolution - white dwarf, neutron stars, black holes.
    Fermi-Dirac statistics, degenerated Fermi gas.
    Non-relativistic equation of hydrostatic equilibrium. Structure and properties of white dwarfs. Chandrasekhar limiting mass.
    Equation of hydrostatic equilibrium (TOV equation). Its derivation and solution for objects of uniform density, limits for the compactness of neutron stars.
    Equations of state for outer parts of neutron stars.
    Beta equilibrium and its consequences. Equations of state for neutron star core.
    Observations and finding of neutron stars. Pulsars.
    Testing of neutron star equations of state by observed properties of neutron stars.
    Strange and hybrid stars.
Literature
    recommended literature
  • Haensel P., Potekhin A.Y., Yakovlev D. Neutron stars 1: Equation of state and structure. Springer, 2007. ISBN 9780387335438. info
  • Ghosh P. Rotation and accretion powered pulsars. World Scientific, Singapore, 2007. ISBN 9789812708465. info
  • Glendening N.K. Compact stars. Springer, 1997. ISBN 0387947833. info
  • Shapiro S.L., Teukolski S.A. Black Holes, White Dwarfs, and Neutron Stars. The Physics of Compact Objects. A Wiley-Interscience Publication. John Wiley & Sons Inc., 1983. ISBN 978-0-471-87316-7. info
Teaching methods
Lecturing
One-to-One tutorial
Students' self-study
Language of instruction
Czech
Further comments (probably available only in Czech)
The course can also be completed outside the examination period.
Teacher's information
The attendance at lectures is recommended. It can be substituted by
the self-study of recommended literature and individual consultations.
Workout of homework exercises. Written project.
The course is also listed under the following terms Winter 2009, Summer 2010, Winter 2010, Summer 2011, Winter 2011, Summer 2012, Winter 2012, Summer 2013, Winter 2013, Summer 2014, Winter 2014, Summer 2015, Winter 2015, Summer 2016, Winter 2016, Summer 2017, Winter 2017, Summer 2018, Winter 2018, Summer 2019, Summer 2020, Winter 2020, Summer 2021, Winter 2021, Summer 2022.
  • Enrolment Statistics (Winter 2019, recent)
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