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Автор Kjell Rosquist
Дата выпуска 1995-05-01
dc.description An ADM-like Hamiltonian approach is proposed for static spherically symmetric relativistic star configurations. For a given equation of state the entire information about the model can be encoded in a certain two-dimensional minisuperspace geometry. We derive exact solutions which arise from symmetries corresponding to linear and quadratic geodesic invariants in minisuperspace by exploiting the relation to minisuperspace Killing tensors. A classification of exact solutions having the full number of integration constants is given according to their minisuperspace symmetry properties. In particular it is shown that Schwarzschild's exterior solution and Buchdahl's n=1 polytrope solution correspond to minisuperspaces with a Killing vector symmetry, while Schwarzschild's interior solution, Whittaker's solution and Buchdahl's n=5 polytrope solution correspond to minisuperspaces with a second rank Killing tensor. New solutions filling in empty slots in this classification scheme are also given. One of these new solutions has a physically reasonable equation of state and is a generalization of Buchdahl's n=1 polytrope model.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Hamiltonian approach to relativistic star models
Тип paper
DOI 10.1088/0264-9381/12/5/019
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 12
Первая страница 1305
Последняя страница 1326
Аффилиация Kjell Rosquist; Department of Physics, Stockholm University, Box 6730, 113 85 Stockholm, Sweden; RGGR Group, Chimie-Physique, CP231, ULB Campus Plaine, Brussels, Belgium
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