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000888023 010__ $$z  2012036771
000888023 020__ $$z9780521872546 
000888023 020__ $$z9781107306165 $$q(electronic book)
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000888023 035__ $$a(Au-PeEL)EBL1113031
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000888023 035__ $$a(OCoLC)829461697
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000888023 050_4 $$aQB843.N4$$bF75 2013
000888023 08204 $$a523.8/874$$223
000888023 1001_ $$aFriedman, John L.,$$d1945-
000888023 24510 $$aRotating relativistic stars$$h[electronic resource] /$$cJohn L. Friedman, Nikolaos Stergioulas.
000888023 260__ $$aCambridge :$$bCambridge University Press,$$c2013.
000888023 300__ $$axxiv, 409 p. :$$bill.
000888023 440_0 $$aCambridge monographs on mathematical physics
000888023 504__ $$aIncludes bibliographical references and index.
000888023 5058_ $$aMachine generated contents note: 1. Stationary, axisymmetric equilibria; 2. 3+1 split, action, Lagrangian and Hamiltonian formalisms; 3. Asymptotics, virial identities and nonaxisymmetric equilibria; 4. Numerical schemes; 5. Equilibrium models; 6. Approximation methods; 7. Perturbation theory of relativistic fluids; 8. Quasinormal modes; 9. Stellar stability; 10. Nonlinear dynamics of rotating relativistic stars; Appendix.
000888023 506__ $$aAccess limited to authorized users.
000888023 520__ $$a"The masses of neutron stars are limited by an instability to gravitational collapse, and an instability driven by gravitational waves limits their spin. Their oscillations are relevant to X-ray observations of accreting binaries and to gravitational wave observations of neutron stars formed during the coalescence of double neutron-star systems. This volume pulls together more than forty years of research to provide graduate students and researchers in astrophysics, gravitational physics, and astronomy with the first self-contained treatment of the structure, stability, and oscillations of rotating neutron stars. This monograph treats the equations of stellar equilibrium; key approximations, including slow rotation and perturbations of spherical and rotating stars; stability theory and its applications, from convective stability to the r-mode instability; and numerical methods for computing equilibrium configurations and the nonlinear evolution of their oscillations. The presentation of fundamental equations, results, and applications is accessible to readers who do not need the detailed derivations"--$$cProvided by publisher.
000888023 650_0 $$aNeutron stars.
000888023 650_0 $$aStellar oscillations.
000888023 650_0 $$aGravitational waves.
000888023 650_0 $$aStars$$xRotation.
000888023 7001_ $$aStergioulas, Nikolaos,$$d1967-
000888023 852__ $$bebk
000888023 85640 $$3ProQuest Ebook Central Academic Complete $$uhttps://univsouthin.idm.oclc.org/login?url=https://ebookcentral.proquest.com/lib/usiricelib-ebooks/detail.action?docID=1113031$$zOnline Access
000888023 909CO $$ooai:library.usi.edu:888023$$pGLOBAL_SET
000888023 980__ $$aEBOOK
000888023 980__ $$aBIB
000888023 982__ $$aEbook
000888023 983__ $$aOnline