Gravitational wave asteroseismology with fast rotating neutron stars
Autor: | Gaertig, Erich, Kokkotas, Kostas D. |
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Rok vydání: | 2010 |
Předmět: | |
Zdroj: | Phys.Rev.D83:064031,2011 |
Druh dokumentu: | Working Paper |
DOI: | 10.1103/PhysRevD.83.064031 |
Popis: | We investigate damping and growth times of the f-mode for rapidly rotating stars and a variety of different polytropic equations of state in the Cowling approximation. We discuss the differences in the eigenfunctions of co- and counterrotating modes and compute the damping times of the f-mode for several EoS and all rotation rates up to the Kepler-limit. This is the first study of the damping/growth time of this type of oscillations for fast rotating neutron stars in a general relativistic framework. We use these frequencies and damping/growth times to create robust empirical formulae which can be used for gravitational wave asteroseismology. The estimation of the damping/growth time is based on the quadrupole formula and our results agree very well with Newtonian ones in the appropriate limit. Comment: 15 pages, 8 figures, version accepted for publication in PhysRevD |
Databáze: | arXiv |
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