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Rotating relativistic stars

John L. Friedman, Nikolaos Stergioulas (Cambridge University Press, 2013)

 Abstrak

Summary:
"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

 Metadata

No. Panggil : 523.887 4 FRI r
Entri utama-Nama orang :
Entri tambahan-Nama orang :
Subjek :
Penerbitan : New York: Cambridge University Press, 2013
Sumber Pengatalogan: LibUI eng rda
ISBN: 9780521872546
Tipe Konten: text
Tipe Media: unmediated
Tipe Carrier: volume
Edisi:
Catatan Seri: Cambridge monographs on matnematical physics
Catatan Umum:
Catatan Versi Asli:
Deskripsi Fisik: xxiv, 409 pages : illustrations ; 26 cm
Lembaga Pemilik: Universitas Indonesia
Lokasi: Perpustakaan UI, Lantai 2.
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No. Panggil No. Barkod Ketersediaan
523.887 4 FRI r 01-18-01137 TERSEDIA
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