Hmotové a nábojové proudy v obecné relativitě a astrofyzice

Název projektu anglicky
Mass and charge currents in general relativity and astrophysics
Anotace anglicky
Quasi-stationary rotating compact configurations of matter drive such compelling astrophysical systems as X-ray binaries or active galactic nuclei. As an outcome of gravitational and centrifugal effects, they include discs, rings, toroids, and black holes or neutron stars encircled by this type of structures. In many cases, matter includes electric currents, and thus magnetic fields are important as well. We plan to deepen the understanding of such systems, using primarily analytical methods within general relativistic framework. Despite an enormous recent progress in numerical methods, analytical treatment keeps its fundamental relevance, although it can usually be pursued in idealized situations only. We will study the theoretical background of these problems and consider possible implications for astrophysics. The project is submitted by a Prague team from the Faculty of Mathematics and Physics, Charles University, and from the Astronomical Institute, Czech Academy of Sciences. The members of the team have already achieved a number of results in the given area.

Kategorie VaV
ZV - Základní výzkum
OECD FORD - hlavní obor
10308 - Astronomy (including astrophysics,space science)
OECD FORD - vedlejší obor
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OECD FORD - další vedlejší obor
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CEP - odpovídající obory <br>(dle <a href="http://www.vyzkum.cz/storage/att/E6EF7938F0E854BAE520AC119FB22E8D/Prevodnik_oboru_Frascati.pdf">převodníku</a>)
BN - Astronomie a nebeská mechanika, astrofyzika

Důvěrnost údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Systémové označení dodávky dat
CEP24-GA0-GA-R
Datum dodání záznamu
21. 5. 2024

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