Quasi-radial modes of rotating stars in general relativity

Citation
S. Yoshida et Y. Eriguchi, Quasi-radial modes of rotating stars in general relativity, M NOT R AST, 322(2), 2001, pp. 389-396
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
322
Issue
2
Year of publication
2001
Pages
389 - 396
Database
ISI
SICI code
0035-8711(20010401)322:2<389:QMORSI>2.0.ZU;2-D
Abstract
By using the Cowling approximation, quasi-radial modes of rotating general relativistic stars are computed along equilibrium sequences from non-rotati ng to maximally rotating models. The eigenfrequencies of these modes are de creasing functions of the rotational frequency. The eigenfrequency curve of each mode as a function of the rotational frequency has discontinuities, w hich arise from the avoided crossing with other curves of axisymmetric mode s.