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  3. Rotating Relativistic Stars
  • Cited by 193
Publisher:
Cambridge University Press
Online publication date:
July 2013
Print publication year:
2013
Online ISBN:
9780511977596
DOI:
https://doi.org/10.1017/CBO9780511977596
Subjects:
Physics and Astronomy, Theoretical Physics and Mathematical Physics, Astrophysics
Series:
Cambridge Monographs on Mathematical Physics
Information

Book description

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.

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