Sources of Gravitational Radiation| Sources of Gravitational Radiation |
In General
> s.a. gravitational radiation [including modified gravity
theories]; astronomy [multimessenger astronomy].
* Strongest sources: 2005, The
strongest predicted one is the tight white dwarf binary RX J0806.3+1527 in Cancer,
with P = 5.36 min (the shortest known for a binary) and a = 80,000 km
(S&T).
@ Reviews: Damour gq/96-GR14;
Blanchet gq/96-ln;
Marck & Lasota ed-97;
Flanagan gq/98-GR15;
Ferrari AdP(00)gq/99;
Finn gq/99-ln;
Cutler & Thorne gq/02-GR16;
Goldberger hp/07-ln [uses of effective field theory];
Cattani a1001-ln,
a1003-ln;
Buonanno & Sathyaprakash ch-a1410;
Colpi & Sesana in(17)-a1610 [multi-frequency gravitational wave astronomy];
Cai et al NSR(17)-a1703.
@ Radiation reaction: Galley et al PRD(16)-a1511 [tail effect];
> s.a. radiation from compact sources.
> Related topics: see models
in numerical general relativity; Quadrupole Formula.
Specific Types of Sources
> s.a. compact sources [black holes, neutron stars including
binaries]; radiation [gravitational Cerenkov radiation].
* Isolated objects: Oscillating stars;
X-ray binaries; Soliton stars (there is a whole zoo of them, some can be very massive
and emit very high-frequency gravitational waves, simulating black holes –
& T D Lee); Cosmic strings and other topological defects.
@ Isolated systems: Blanchet PTPS(99)gq/01-proc [PN expansion];
Kokkotas CQG(04)gq/03 [high-frequency];
Ashtekar et al PRL(16)-a1510 [with a positive cosmological constant];
Kozameh & Quiroga PRD-a1311 [center of mass and spin];
Mastrogiovanni et al a2103 [source population models].
@ Cosmic strings:
Hawking PLB(90);
Allen & Casper PRD(94)gq,
et al PRD(94)gq,
PRD(95)gq/94;
Casper & Allen PRD(95)gq;
Damour & Vilenkin PRL(00)gq,
PRD(01)gq [bursts from cusps and kinks];
Allen & Ottewill PRD(01) [waveforms];
Siemens & Olum NPB(01);
Canfora & Vilasi PLB(04)gq/03 [and GRBs];
Siemens et al PRD(06)gq;
Hogan PRD(06)ap;
Polchinski a0707-MGXI;
Brandenberger et al JCAP(09)-a0810 [junctions];
Key & Cornish PRD(09)-a0812 [cusps];
Depies PhD(09)-a0908;
Kawasaki et al PRD(10)-a1002 [from kinks];
O'Callaghan et al PRL(10)-a1003,
JCAP(10)-a1005 [with extra dimensions];
Kuroyanagi et al PRD(12)-a1202 [determining cosmic-string parameters];
Aasi et al PRL(14) [constraints];
> s.a. gravitational-wave background [anisotropy].
@ Other topological defects:
Hiramatsu et al JCAP(10) [collapsing domain walls];
Kawasaki & Saikawa JCAP(11) [domain walls];
Figueroa et al PRL(13)-a1212 [scale-invariant spectrum];
Saikawa Univ(17)-a1703 [rev].
@ Naked singularities: Iguchi et al PTP(99)gq,
PTP(00)gq/99;
Nakao & Morisawa PRD(05)gq [cylindrical].
@ Triple systems: Montanari et al IJMPA(99)gq,
Dmitrašinović et al PRL(14) [waveforms and luminosities];
Meiron et al ApJ(17)-a1604 [prospects];
Bonetti et al CQG(17)-a1707.
@ Core-collapse supernovae: Fuller et al MNRAS(15)-a1501 [rapidly rotating];
Hayama et al PRL(16)-a1606 [rotation and gravitational-wave polarization];
Radice et al ApJL(19)-a1812;
Astone et al PRD(18)-a1812 [analysis method];
Srivastava et al PRD(19)-a1906.
@ Stellar systems: Dionysiou IJTP(79) [N bodies, in terms of multipole moments];
Cutler & Lindblom PRD(96) [the Sun];
Andersson et al MNRAS(02)ap/01 [strange stars];
New LRR(03)gq/02,
revised Fryer & New LRR(03),
LRR(11) [collapse];
Biotti et al PRL(05) [rotating stars];
Hartwig et al MNRAS(16)-a1603 [the first stars].
@ GRBs: Piran ap/01-ln;
van Putten PRP(01),
NCC(05)ap-proc;
Corsi et LSC IAU-a1204;
van Putten a1301-conf [and supernovae];
> s.a. detection; interferometers.
@ Galactic sources:
Quilis et al A&A-ap/99 [galaxy clusters];
Inagaki et al PRD(10)-a1011 [galaxy mergers].
@ Other sources: Ferrari et al IJMPD(00)ap [planets];
Mapelli et al ApJ(10)-a1006 [intermediate-mass black holes in star clusters];
Herrera et al PRD-a1506
[geodesic dissipative dust does not produce gravitational radiation];
Ain et al PRD(15)-a1504 [exoplanets, background];
Jackson & Benford a1806 [transmitters];
Gourgoulhon et al A&A(19)-a1903 [bodies around the galactic center];
Toubiana et al a2011 [exotic compact objects].
Early-Universe Sources > s.a. gravitational-wave
background [inflation]; space-based detectors.
* Phase transitions: In first-order phase
transitions, such as the QCD phase transition from a quark-gluon plasma to hadrons, bubbles
of the new phase form inside the plasma, expand and collide generating gravitational waves.
@ Cosmic bubble collisions: Caprini et al PRD(08)-a0711;
Salem et al JCAP(13)-a1210;
Kim et al EPJC(15)-a1410;
García et al PLB(18)-a1607 [and string theory].
@ Phase transitions:
Kamionkowski et al PRD(94) + refs;
Schwarz MPLA(98) [QCD transition];
Jones-Smith et al PRL(08)-a0712 [global];
Kahniashvili et al PRD(08)-a0806 [detectability],
PRD(10)-a0905 [from magnetic fields];
Caprini et al PRD(09)-a0901 [spectrum],
JCAP(09)-a0909 [from turbulence and magnetic fields];
Durrer JPCS(10)-a1002;
Krauss et al PRD(10)-a1003;
Chung & Zhou PRD(10)-a1003 [electroweak];
Chialva PRD(11)-a1004 [during inflation];
Caprini a1005-proc [first-order, during inflation];
Caprini et al PRD(10)-a1007,
Schettler et al PRD(11)-a1010,
proc(12)-a1105 [QCD transition];
Wainwright et al PRD(11)-a1104 [gauge artifacts];
Giblin et al JCAP(12)-a1111 [global second-order phase transitions];
Leitao et al JCAP(12) [electroweak];
Hindmarsh et al PRL(14)-a1304,
a1511-conf;
Addazi & Marcianò ChPC(18)-a1703 [and dark photons];
Jinno et al JCAP(17)-a1703;
Capozziello et al PLB(19)-a1808 [QCD, and stochastic background];
Jinno et al a1905;
Alanne et al a1909.
@ Primordial gravitational waves:
Mureika & Stojković PRL(11)-a1102
+ news prf(11)mar
+ comment Sotiriou et al PRL(11)-a1104 [and small-scale spacetime dimensionality];
Smith et al PRL(14)-a1404 [tension between BICEP2 and Planck];
Franciolini et al JCAP(19)-a1811 [and the standard model of particle physics].
@ Other early universe: Mielczarek JCAP(08)-a0807,
et al PRD(10)-a1003 [big bounce in lqc];
Müller et al a1103
[Bianchi I isotropization process in higher-order theories];
Andersen SA(13)oct;
Figueroa a1402 [decay of the Higgs boson after inflation].
@ Related topics: Caprini et al PRD(06)ap [source wavenumber spectrum];
Mitra PRD(06) [collapse, and Newtonian];
Maluf et al IJMPD(07)gq/06 [linearly accelerated];
Berchtold & Scharf GRG(07) [gravitational bremsstrahlung];
Linder JCAP(08)-a0711 [standard sirens and expansion history].
> Other types:
see higher-dimensional gravity;
string phenomenology.
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send feedback and suggestions to bombelli at olemiss.edu – modified 3 apr 2021