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| Preprint | PUBDB-2021-03058 |
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2020
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Please use a persistent id in citations: doi:10.3204/PUBDB-2021-03058
Report No.: CERN-TH-2020-185; DESY-20-195; HIP-2020-28/TH; arXiv:2011.12414
Abstract: The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges and gains expected in gravitational wave searches at frequencies above the LIGO/Virgo band, with a particular focus on the MHz and GHz range. The absence of known astrophysical sources in this frequency range provides a unique opportunity to discover physics beyond the Standard Model operating both in the early and late Universe, and we highlight some of the most promising gravitational sources. We review several detector concepts which have been proposed to take up this challenge, and compare their expected sensitivity with the signal strength predicted in various models. This report is the summary of the workshop 'Challenges and opportunities of high-frequency gravitational wave detection' held at ICTP Trieste, Italy in October 2019.
Keyword(s): detector: design ; gravitational radiation ; VIRGO ; LIGO ; gravitation ; detector: sensitivity ; new physics ; gravitational radiation: frequency ; gravitational radiation detector ; gravitational radiation: emission ; neutron star: binary ; black hole: binary ; binary: coalescence ; black hole ; superradiance ; inflation ; critical phenomena ; preheating ; star: compact ; detector: noise ; black hole: evaporation ; laser: interferometer ; electromagnetic field: production ; Neutrino Mediterranean Observatory ; defect: topological
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Journal Article
Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies
Living reviews in relativity 24(1), 4 (2021) [10.1007/s41114-021-00032-5]
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