Gravitational wave search through electromagnetic telescopes

Fuente: arXiv
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Autores principales: Ito, Asuka, Kohri, Kazunori, Nakayama, Kazunori
Formato: Preprint
Publicado: 2023
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author Ito, Asuka
Kohri, Kazunori
Nakayama, Kazunori
author_facet Ito, Asuka
Kohri, Kazunori
Nakayama, Kazunori
contents We study the graviton-photon conversion in the magnetic fields of the Earth, the Milky Way Galaxy, and intergalactic regions. Requiring that the photon flux converted from gravitons does not exceed the observed photon flux with telescopes, we derive upper limits on the stochastic gravitational waves in frequency ranges from $10^{7}$Hz to $10^{35}$Hz. Remarkably, the upper limits on $h^2 Ω_{\rm GW}$ could be less than unity in the frequency range of $10^{18}$-$10^{23}$ Hz in a specific case. The detection of gravitational waves using telescopes would open up a new avenue for high frequency gravitational wave observations.
format Preprint
id arxiv_https___arxiv_org_abs_2309_14765
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Gravitational wave search through electromagnetic telescopes
Ito, Asuka
Kohri, Kazunori
Nakayama, Kazunori
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
We study the graviton-photon conversion in the magnetic fields of the Earth, the Milky Way Galaxy, and intergalactic regions. Requiring that the photon flux converted from gravitons does not exceed the observed photon flux with telescopes, we derive upper limits on the stochastic gravitational waves in frequency ranges from $10^{7}$Hz to $10^{35}$Hz. Remarkably, the upper limits on $h^2 Ω_{\rm GW}$ could be less than unity in the frequency range of $10^{18}$-$10^{23}$ Hz in a specific case. The detection of gravitational waves using telescopes would open up a new avenue for high frequency gravitational wave observations.
title Gravitational wave search through electromagnetic telescopes
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2309.14765