Rotating relativistic stars:
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 th...
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| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2013
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| Series: | Cambridge monographs on mathematical physics
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| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| 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 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 |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (xxiv, 409 pages) |
| ISBN: | 9780511977596 |
| DOI: | 10.1017/CBO9780511977596 |
Staff View
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| 500 | |a Title from publisher's bibliographic system (viewed on 05 Oct 2015) | ||
| 505 | 8 | |a 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 | |
| 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 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 | ||
| 650 | 4 | |a Neutron stars | |
| 650 | 4 | |a Stellar oscillations | |
| 650 | 4 | |a Gravitational waves | |
| 650 | 4 | |a Stars / Rotation | |
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Record in the Search Index
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| author | Friedman, John L. 1945- |
| author_facet | Friedman, John L. 1945- |
| author_role | aut |
| author_sort | Friedman, John L. 1945- |
| author_variant | j l f jl jlf |
| building | Verbundindex |
| bvnumber | BV043941934 |
| collection | ZDB-20-CBO |
| contents | 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 |
| ctrlnum | (ZDB-20-CBO)CR9780511977596 (OCoLC)967600964 (DE-599)BVBBV043941934 |
| dewey-full | 523.8/874 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.8/874 |
| dewey-search | 523.8/874 |
| dewey-sort | 3523.8 3874 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9780511977596 |
| format | Electronic eBook |
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| id | DE-604.BV043941934 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:16Z |
| institution | BVB |
| isbn | 9780511977596 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029350904 |
| oclc_num | 967600964 |
| open_access_boolean | |
| owner | DE-12 DE-92 |
| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (xxiv, 409 pages) |
| psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
| publishDate | 2013 |
| publishDateSearch | 2013 |
| publishDateSort | 2013 |
| publisher | Cambridge University Press |
| record_format | marc |
| series2 | Cambridge monographs on mathematical physics |
| spelling | Friedman, John L. 1945- Verfasser aut Rotating relativistic stars John L. Friedman, University of Wisconsin, Milwaukee and Nikolaos Stergioulas, Aristotle University of Thessaloniki Cambridge Cambridge University Press 2013 1 online resource (xxiv, 409 pages) txt rdacontent c rdamedia cr rdacarrier Cambridge monographs on mathematical physics 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 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 Neutron stars Stellar oscillations Gravitational waves Stars / Rotation Stergioulas, Nikolaos 1967- Sonstige oth Erscheint auch als Druckausgabe 978-0-521-87254-6 https://doi.org/10.1017/CBO9780511977596 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Friedman, John L. 1945- Rotating relativistic stars 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 Neutron stars Stellar oscillations Gravitational waves Stars / Rotation |
| title | Rotating relativistic stars |
| title_auth | Rotating relativistic stars |
| title_exact_search | Rotating relativistic stars |
| title_full | Rotating relativistic stars John L. Friedman, University of Wisconsin, Milwaukee and Nikolaos Stergioulas, Aristotle University of Thessaloniki |
| title_fullStr | Rotating relativistic stars John L. Friedman, University of Wisconsin, Milwaukee and Nikolaos Stergioulas, Aristotle University of Thessaloniki |
| title_full_unstemmed | Rotating relativistic stars John L. Friedman, University of Wisconsin, Milwaukee and Nikolaos Stergioulas, Aristotle University of Thessaloniki |
| title_short | Rotating relativistic stars |
| title_sort | rotating relativistic stars |
| topic | Neutron stars Stellar oscillations Gravitational waves Stars / Rotation |
| topic_facet | Neutron stars Stellar oscillations Gravitational waves Stars / Rotation |
| url | https://doi.org/10.1017/CBO9780511977596 |
| work_keys_str_mv | AT friedmanjohnl rotatingrelativisticstars AT stergioulasnikolaos rotatingrelativisticstars |