Superradiant Bounds on Ultralight Fields
(see Brito, Cardoso and Pani, Superradiance, Lectures Notes in Physics 906 (2015); arXiv:1501.0657)
| Excluded Region (in eV) | Source |
References |
|---|---|---|
|
* 5.2x10-13< mS <6.5x10-12 * 1.1x10-13< mV <8.2x10-12 * 2.9x10-13< mT <9.8x10-12
|
Direct bounds from absence of spin in Cyg X-1 |
|
|
6×10−13< mS <2×10−11 7×10−20< mS <1×10−16 * 2×10−14< mV <1×10−11 * 1×10−20< mV <9×10−17 * 6×10−14< mT <1×10−11 * 3×10−20< mT <9×10−17
|
Indirect bounds from BHmass-spin measurements |
|
|
1.2×10−13< mS <1.8×10−13 mV: NA mT: NA
|
Null results from blind all-sky searches for continuous GW signals |
[1] |
|
5.8×10−13< mS <8.6×10−13 mV: NA mT: NA
|
Null results from searches for continuous GW signals from Cygnus X-1 |
[1], [2] |
|
2.0×10−13< mS <3.8×10−13 mV: NA mT: NA
|
Negative searches for a GW background | [1], [2], [3] |
|
5×10−13< mS <3×10−12 mV ~ 10−12 mT: NA
|
Bounds from pulsar timing | [1], [2] |
|
2.9×10−21< mS <4.6×10−21 8.5×10−22< mV <4.6×10−21 * 1.0×10−21< mT <8.2×10−21
|
Bounds from mass and spin measurement of M87 with EHT |
[1] |
* Brito, Cardoso and Pani, Superradiance, Lectures Notes in Physics 906 (2015)
Direct bounds from absence of spin down in Cyg X-1
[1] V. Cardoso, O. J. C. Dias, G. S. Hartnett,M. Middleton,P. Pani, and J. E. Santos, “Constraining the mass of dark photons and axion-like particles through black holesuperradiance,”JCAP1803(2018) no. 03, 043,arXiv:1801.01420 [gr-qc]
[2] R. Brito, S. Grillo, and P. Pani, “Black hole superradiant instability from ultralightspin-2 fields,”arXiv:2002.04055 [gr-qc]
Indirect bounds from BH mass-spin measurements
[1] A. Arvanitaki, M. Baryakhtar, and X. Huang, “Discovering the QCD Axion withBlack Holes and Gravitational Waves,”Phys. Rev.D91(2015) no. 8, 084011,arXiv:1411.2263 [hep-ph]
[2] P. Pani, V. Cardoso, L. Gualtieri, E. Berti, and A. Ishibashi, “Black hole bombs andphoton mass bounds,”Phys.Rev.Lett.109(2012) 131102,arXiv:1209.0465 [gr-qc]
[3] R. Brito, V. Cardoso, and P. Pani, “Massive spin-2 fields on black hole spacetimes:Instability of the Schwarzschild and Kerr solutions and bounds on the graviton mass,”Phys. Rev.D88(2013) 023514,arXiv:1304.6725 [gr-qc]
[4] M. Baryakhtar, R. Lasenby, and M. Teo, “Black Hole Superradiance Signatures of Ul-tralight Vectors,”Phys. Rev.D96(2017) no. 3, 035019, arXiv:1704.05081 [hep-ph]
[5] R. Brito, S. Ghosh, E. Barausse, E. Berti, V. Cardoso, I. Dvorkin, A. Klein, and P. Pani,“Gravitational wave searches for ultralight bosons with LIGO and LISA,”Phys. Rev.D96(2017) no. 6, 064050,arXiv:1706.06311 [gr-qc]
[6] M. J. Stott and D. J. E. Marsh, “Black hole spin constraints on the mass spectrum andnumber of axionlike fields,”Phys. Rev.D98(2018) no. 8, 083006,arXiv:1805.02016[hep-ph]
[7] V. Cardoso, O. J. C. Dias, G. S. Hartnett, M. Middleton, P. Pani, and J. E. Santos,“Constraining the mass of dark photons and axion-like particles through black-holesuperradiance,”JCAP1803(2018) no. 03, 043, arXiv:1801.01420 [gr-qc]
[8] R. Brito, S. Grillo, and P. Pani, “Black hole superradiant instability from ultralightspin-2 fields,”arXiv:2002.04055 [gr-qc]
Null results from blind all-sky searches for continuous GW signals
[1] C. Palombaet al., “Direct constraints on ultra-light boson mass from searches for con-tinuous gravitational waves,”Phys. Rev. Lett.123(2019) 171101, arXiv:1909.08854[astro-ph.HE]
Null results from searches for continuous GW signals from Cygnus X-1
[1] L. Sun, R. Brito, and M. Isi, “Search for ultralight bosons in Cygnus X-1 with AdvancedLIGO,”arXiv:1909.11267 [gr-qc]
[2] H. Yoshino and H. Kodama, “Probing the string axiverse by gravitational waves fromCygnus X-1,”PTEP2015(2015) no. 6, 061E01, arXiv:1407.2030 [gr-qc]
Negative searches for a GW background
[1] R. Brito, S. Ghosh, E. Barausse, E. Berti, V. Cardoso, I. Dvorkin, A. Klein, and P. Pani,“Stochastic and resolvable gravitational waves from ultralight bosons,”Phys. Rev. Lett.119(2017) no. 13, 131101, arXiv:1706.05097 [gr-qc]
[2] R. Brito, S. Ghosh, E. Barausse, E. Berti, V. Cardoso, I. Dvorkin, A. Klein, and P. Pani,“Gravitational wave searches for ultralight bosons with LIGO and LISA,”Phys. Rev.D96(2017) no. 6, 064050, arXiv:1706.06311 [gr-qc]
[3] L. Tsukada, T. Callister, A. Matas, and P. Meyers, “First search for a stochasticgravitational-wave background from ultralight bosons,”Phys. Rev.D99(2019) no. 10,103015, arXiv:1812.09622 [astro-ph.HE]
Bounds from pulsar timing
[1] V. Cardoso, P. Pani, and T.-T. Yu, “Superradiance in rotating stars and pulsar-timing constraints on dark photons,”Phys. Rev.D95(2017) no. 12, 124056, arXiv:1704.06151 [gr-qc]
[2] D. E. Kaplan, S. Rajendran, and P. Riggins, “Particle Probes with Superradiant Pul-sars,”arXiv:1908.10440 [hep-ph]
Bounds from mass and spin measurement of M87 with EHT
[1] H. Davoudiasl and P. B. Denton, “Ultralight Boson Dark Matter and Event Hori-zon Telescope Observations of M87*,”Phys. Rev. Lett.123(2019) no. 2, 021102, arXiv:1904.09242 [astro-ph.CO]