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Electromagnetic high-frequency gravitational wave detection

Ultra-high frequency gravitational waves in the MHz to THz regime promise a unique possibility to probe the very early universe, particle physics at very high energies and exotic astrophysical objects - but achieving the sensitivity required for detection is an immense challenge. This is a brief sum...

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Autor principal: Domcke, Valerie
Lenguaje:eng
Publicado: 2023
Materias:
Acceso en línea:http://cds.cern.ch/record/2861314
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author Domcke, Valerie
author_facet Domcke, Valerie
author_sort Domcke, Valerie
collection CERN
description Ultra-high frequency gravitational waves in the MHz to THz regime promise a unique possibility to probe the very early universe, particle physics at very high energies and exotic astrophysical objects - but achieving the sensitivity required for detection is an immense challenge. This is a brief summary of recent progress in electromagnetic high-frequency gravitational wave searches, which are based on classical electromagnetism in a space-time perturbed by gravitational waves. A particular focus is given to synergies with axion searches and atomic precision measurements. This article was prepared as proceedings for Moriond EW 2023.
id cern-2861314
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2023
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spelling cern-28613142023-07-11T04:20:03Zhttp://cds.cern.ch/record/2861314engDomcke, ValerieElectromagnetic high-frequency gravitational wave detectionhep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and Astronomygr-qcGeneral Relativity and CosmologyUltra-high frequency gravitational waves in the MHz to THz regime promise a unique possibility to probe the very early universe, particle physics at very high energies and exotic astrophysical objects - but achieving the sensitivity required for detection is an immense challenge. This is a brief summary of recent progress in electromagnetic high-frequency gravitational wave searches, which are based on classical electromagnetism in a space-time perturbed by gravitational waves. A particular focus is given to synergies with axion searches and atomic precision measurements. This article was prepared as proceedings for Moriond EW 2023.arXiv:2306.04496CERN-TH-2023-099oai:cds.cern.ch:28613142023-06-07
spellingShingle hep-ph
Particle Physics - Phenomenology
astro-ph.CO
Astrophysics and Astronomy
gr-qc
General Relativity and Cosmology
Domcke, Valerie
Electromagnetic high-frequency gravitational wave detection
title Electromagnetic high-frequency gravitational wave detection
title_full Electromagnetic high-frequency gravitational wave detection
title_fullStr Electromagnetic high-frequency gravitational wave detection
title_full_unstemmed Electromagnetic high-frequency gravitational wave detection
title_short Electromagnetic high-frequency gravitational wave detection
title_sort electromagnetic high-frequency gravitational wave detection
topic hep-ph
Particle Physics - Phenomenology
astro-ph.CO
Astrophysics and Astronomy
gr-qc
General Relativity and Cosmology
url http://cds.cern.ch/record/2861314
work_keys_str_mv AT domckevalerie electromagnetichighfrequencygravitationalwavedetection