TY  - BOOK
AU  - Friedman,John L.
AU  - Stergioulas,Nikolaos
TI  - Rotating relativistic stars
T2  - Cambridge monographs on mathematical physics
SN  - 9780511977596 (ebook)
AV  - QB843.N4 F75 2013
U1  - 523.8/874 23
PY  - 2013///
CY  - Cambridge
PB  - Cambridge University Press
KW  - Neutron stars
KW  - Stellar oscillations
KW  - Gravitational waves
KW  - Stars
KW  - Rotation
N1  - Title from publisher's bibliographic system (viewed on 05 Oct 2015); 1. Stationary, axisymmetric equilibria -- 2. 3+1 split, action, Lagrangian and Hamiltonian formalisms -- 3. Asymptotics, virial identities and nonaxisymmetric equilibria -- 4. Numerical schemes -- 5. Equilibrium models -- 6. Approximation methods for equilibria -- 7. Perturbation theory of relativistic fluids -- 8. Quasinormal modes -- 9. Stellar stability -- 10. Nonlinear dynamics of rotating relativistic stars -- Appendix A: Lie derivatives, forms, densities, and integration -- Appendix B: The Newtonian limit of the two-potential
N2  - 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
UR  - https://doi.org/10.1017/CBO9780511977596
ER  -