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Автор Simone Calogero
Дата выпуска 2003-05-07
dc.description The kinetic motion of the stars of a galaxy is considered within the framework of a relativistic scalar theory of gravitation. This model, even though unphysical, may represent a good laboratory to study in a rigorous, mathematical way those problems, such as the influence of the gravitational radiation on the dynamics, which are still beyond our present understanding of the physical model represented by the Einstein–Vlasov system. The present paper is devoted to deriving the equations of the model and to proving the existence of spherically symmetric equilibria with finite radius.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Spherically symmetric steady states of galactic dynamics in scalar gravity
Тип paper
DOI 10.1088/0264-9381/20/9/310
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 20
Первая страница 1729
Последняя страница 1741
Аффилиация Simone Calogero; Institut für Mathematik der Universität Wien, Strudlhofgasse 4, 1090 Vienna, Austria
Выпуск 9

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