Gravitational Radiation from Compact Sources| Gravitational Radiation from Compact Sources |
Single Compact Objects
> s.a. Gravastars; gravitational
radiation [in other theories]; primordial black holes.
* Core collapse supernovae: The strain
is h ≅ ε1/2
M/D, with ε = energy conversion efficiency,
M = mass, D = distance.
@ Reviews: Schutz gq/98;
Jones CQG(02)gq/01 [rotating, strained neutron stars];
Vallisneri gq/02-proc;
Kokkotas & Stergioulas gq/05-proc.
@ Core collapse supernovae:
Dimmelmeier et al a0705-proc;
Ott CQG(09) [gravitational-wave signature];
Yakunin et al CQG(10)-a1005;
Shibata et al PRD(16)-a1606 [radiply rotating, gravitational waveform].
@ Neutron stars / pulsars: Cutler & Jones PRD(01)gq/00 [backreaction on wobble];
Cutler PRD(02) [large toroidal magnetic fields];
Dreyer et al CQG(04)gq/03 [black holes vs neutron stars];
Clark et al PRD(07)gq [ring-downs and glitches];
Benhar et al GRG(07) [quark-matter imprint];
Al Fakir & Unruh a0805;
news sr(08)jun [Crab pulsar, bound];
Horowitz PRD(10) [low-mass];
Haskell et al MNRAS(15)-a1501 [from mountains on neutron stars];
Haskell & Schwenzer a2104-in [rev];
> s.a. neutron stars.
@ Instabilities: Owen et al PRD(98)gq;
Owen & Lindblom CQG(02)gq/01;
Andersson CQG(03);
> s.a. astrophysics.
@ Particle + Schwarzschild black hole: Loustó MPLA(97)gq [model for galactic center];
Cardoso & Lemos PLB(02)gq,
Mitsou PRD(11)-a1012 [radial infall];
Martel PRD(04) [orbiting particle];
Fujita PTP(12)-a1211 [22PN order].
@ Particle + Kerr black hole:
Nakamura et al PTPS(87) [axisymmetric collapse];
Mino et al PRD(96);
Cardoso & Lemos PRD(03)gq/02 [radial infall];
Fujita et al PTP(09)-a0904;
Apostolatos et al PRL(09),
Lukes-Gerakopoulos et al PRD(10) [Kerr vs non-Kerr spacetime];
Han PRD(10)-a1008 [supermassive black hole].
@ Related topics: Date & Hoque PRD(16)-a1510 [in a de Sitter background].
Compact Binaries > s.a. black-hole binaries;
cosmological expansion; phenomenology;
physics teaching [classroom demo].
* Result: In most calculations
and simulations, the eccentricity quickly goes down to ~ 0.1, despite some
contrary claim (& F Ryan); The emission rate depends on the matter
equation of state (through the "chirp mass"
Mchirp:= \(m_{\rm red}^{3/5}\, M_{\rm tot}^{2/5} = (m_1 m_2)^{3/5}/(m_1+m_2)^{1/5}\) .
* Abundance: The estimated number
at any given time is 100/(200 Mpc)3.
@ Overviews: Poisson gq/95-proc;
Thorne gq/95;
Belczynski et al ApJ(02)ap/01;
Blanchet LRR(02)gq,
update LRR(06);
van der Sluys a1108-in;
Blanchet LRR(14) [and post-Newtonian sources];
Antelis & Moreno EPJP(17)-a1610;
Jafari a1908 [pedagogical];
Nitz et al a1910 [open catalog].
@ Close limit: Price & Pullin PRL(94);
Khanna et al PRL(99)gq;
Gleiser et al PRP(00)gq/98;
Baker et al CQG(00)gq [combine methods];
Husa et al PRD(02)gq/01 [retarded wave];
Reisswig et al PRL(09),
Bernuzzi & Nagar PRD(10)-a1003 [black-hole merger].
@ Estimates: Will & Wiseman PRD(96);
Moreschi & Dain PRD(96) [head-on];
Kalogera ap/99-proc;
Schneider et al MNRAS(01)ap/00;
Gualtieri et al PRD(01)gq [particle around neutron star];
Bulik et al MNRAS(04)ap/03;
Centrella AIP(03)ap [rev];
Loustó CQG(05)ap-conf [extreme mass ratio];
Regimbau et al CQG(05)gq [ns-ns coalescence];
issue CQG(05)#15 [perturbative];
Yunes & Sopuerta JPCS(10)-a0909 [extreme mass ratio, Chern-Simons-modified gravity];
Kiuchi et al PRL(10)
+ Spero Phy(10) [ns-ns coalescence, simulations];
Maia IJMPD(10)-a1007;
Schmidt et al PRD(12)-a1207 [precessing binaries, waveforms];
Hannam GRG(14)-a1312;
Macleod et al PRD(16)-a1509 [coalescence, search];
Loutrel & Yunes CQG+(17),
Loutrel a2009 [eccentric binaries].
@ Spinning compact binaries:
Marsat et al a1312-proc [3.5PN];
De Vittori et al PRD(14)-a1410 [in hyperbolic orbits].
@ Neutron stars: Allen et al PRD(99)gq [ns/ns, limit];
Kyutoku et al PRD(10),
Pannarale et al PRD(12)-a1103,
Kyutoku et al PRD(11)-a1108 [bh/ns, and equation of state];
Hannam et al ApJL(13)-a1301 [distinguishing between black holes and neutron stars];
Antoniadis proc(14)-a1407 [binary pulsars];
Baiotti PPNP-a1907 [and the nuclear equation of state].
@ Neutron stars, detection: LSC & Virgo PRL(17)-a1710
+ McLaughlin Phy(17) [GW170817] + many other articles posted the same day.
@ Massive black holes: Hughes gq/99-proc;
Lang & Hughes ApJ(08)-a0710;
Pshirkov et al MNRAS(10)-a0909,
Corbin & Cornish a1008 [and pulsar timing];
news ns(12)dec [and pulsar timing, stronger signal estimates];
Shannon et al Sci(15)sep-a1509 [signal missing in pulsar timing arrays];
> s.a. neutron stars [pulsar timing].
@ Binary supermassive black holes: Sesana CQG(13)-a1307;
Aggarwal et al ApJ(19)-a1812 [NANOGrav 11-year data].
@ Other special systems:
Creighton gq/97-conf [quasinormal ringing];
Ioka et al PRD(99)ap/98 [low f];
Apostolatos et al PRL(09)-a0906 [distinguishing Kerr from non-Kerr background];
Majár et al PRD(10) [unbound orbits];
Ghosh & Nelemans ASSP(14)-a1406 [and optical telescopes];
Tiwari et al PRD(16)-a1511 [coalescence of eccentric binary black holes, search method];
Bonga & Hazboun PRD(17)-a1708 [binary system in de Sitter universe].
@ Kicks: van Meter et al ApJ(10)-a1003 [general formula];
Gerosa & Moore PRL(16)-a1606 [as gravitational-wave observables].
@ Chaotic systems:
Cornish & Levin gq/02 [spinning];
Kiuchi & Maeda PRD(04)gq [spinning particle, Kerr],
et al PRD(07)-a0704 [mass + disk].
@ Quantum-gravity corrections: Abedi et al PRD(17)-a1612 [evidence for Planck-scale structure];
Maselli et al PRL(18)-a1703 [at the horizon scale, with LISA];
Agulló et al PRL(21)-a2007 [from area discretization].
@ Modified gravity: Alexander et al CQG(18)-a1808 [hidden sector modifications];
> s.a. scalar-tensor theories.
@ Other effects:
Price et al PRL(93) [nearby massive body];
Narayan ApJ(00)ap/99 [accretion flow];
Kalogera ApJ(00)ap/99 [spin-orbit misalignment];
Levin et al PRD(00)gq/99 [instabilities];
Loustó CQG(01)gq/00-proc [back-reaction];
Saijo & Nakamura PRL(00)ap,
PRD(01)gq/00 [radius from spectrum];
Ferrari ap/02-proc [information carried];
Klein & Jetzer PRD(10)-a1005 [spin effects on phasing];
Zhao et al PRD(11)-a1009 [luminosity distance, and cosmological model];
Huerta & Gair a1009-proc
[importance of gravitational self-force corrections];
De Martino et al AIP(12)-a1201 [use as standard candles];
Kamble & Kaplan IJMPD(13)-a1602 [electromagnetic counterparts];
Barausse et al JPCS(15)-a1404,
PRD(14)-a1404 [environmental effects];
Ashtekar et al a1910 [angular momentum, supertranslation ambiguities].
> Related topics: see
neutron stars; orbits in gravitation.
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