2020
DOI: 10.48550/arxiv.2012.12189
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Detecting Planetary-mass Primordial Black Holes with Resonant Electromagnetic Gravitational Wave Detectors

Nicolas Herman,
André Füzfa,
Léonard Lehoucq
et al.

Abstract: The possibility to detect gravitational waves (GW) from planetary-mass primordial black hole (PBH) binaries with electromagnetic (EM) detectors of high-frequency GWs is investigated. We consider two patented experimental designs, based on the inverse Gertsenshtein effect, in which incoming GWs passing through a static magnetic field induce EM excitations inside either a TM cavity or a TEM waveguide. The frequency response of the detectors is computed for post-newtonian GW waveforms. We find that such EM detect… Show more

Help me understand this report
View published versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
18
0

Year Published

2021
2021
2022
2022

Publication Types

Select...
5

Relationship

1
4

Authors

Journals

citations
Cited by 6 publications
(18 citation statements)
references
References 61 publications
(119 reference statements)
0
18
0
Order By: Relevance
“…Finally, as pointed out in [54], the gravitational waves produced by mergers of Earth-mass primordial black holes will be detected by GHz gravitational wave detectors [90][91][92][93][94][95]. Future simultaneous detection of FRBs and high frequency gravitational waves may bring us surprises.…”
Section: Conclusion and Discussionmentioning
confidence: 90%
“…Finally, as pointed out in [54], the gravitational waves produced by mergers of Earth-mass primordial black holes will be detected by GHz gravitational wave detectors [90][91][92][93][94][95]. Future simultaneous detection of FRBs and high frequency gravitational waves may bring us surprises.…”
Section: Conclusion and Discussionmentioning
confidence: 90%
“…Since the discovery of gravitational waves (GWs) by the LIGO collaboration [22], there has been much renewed interest in approaches to their detection (see, for example, the recent proposals [23,24,25,26,27,28,29,30]). Many of these proposals seek to detect low-frequency (sub-10 Hz) GWs, where standard astrophysical sources are expected aplenty.…”
Section: Revisiting Gravitational Wave Detection In An Srf Cavitymentioning
confidence: 99%
“…For example, magnons in cavities are used to obtain the sensitivity at 8 GHz and 14 GHz [5]. Also detectors based on the photon-graviton conversion phenomenon [6] have been proposed to observe gravitational waves from planetarymass primordial black hole binaries(typically 200 MHz) [7]. The photon-graviton conversion is also used as a way to constrain the stochastic background gravitational waves with frequencies above 1 THz [8].…”
Section: Introductionmentioning
confidence: 99%