Rotating Relativistic Stars (Hardcover, New)

The masses of neutron stars are limited by an instability to gravitational collapse and an instability driven by gravitational waves limits their spin. Their oscillations are relevant to x-ray observations of accreting binaries and to gravitational wave observations of neutron stars formed during the coalescence of double neutron-star systems. This volume includes more than forty years of research to provide graduate students and researchers in astrophysics, gravitational physics and astronomy with the first self-contained treatment of the structure, stability and oscillations of rotating neutron stars. This monograph treats the equations of stellar equilibrium; key approximations, including slow rotation and perturbations of spherical and rotating stars; stability theory and its applications, from convective stability to the r-mode instability; and numerical methods for computing equilibrium configurations and the nonlinear evolution of their oscillations. The presentation of fundamental equations, results and applications is accessible to readers who do not need the detailed derivations.

General

Imprint:	Cambridge UniversityPress
Country of origin:	United Kingdom
Series:	Cambridge Monographs on Mathematical Physics
Release date:	February 2013
First published:	February 2013
Authors:	John L. Friedman • Nikolaos Stergioulas
Dimensions:	262 x 186 x 33mm (L x W x T)
Format:	Hardcover
Pages:	429
Edition:	New
ISBN-13:	978-0-521-87254-6
Categories:	Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter > General Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics Promotions
LSN:	0-521-87254-5
Barcode:	9780521872546

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