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@ARTICLE{Aggarwal:646132,
author = {Aggarwal, Nancy and Aguiar, Odylio D. and Blas, Diego and
Bauswein, Andreas and Cella, Giancarlo and Clesse, Sebastian
and Cruise, Adrian Michael and Domcke, Valerie and Ellis,
Sebastian and Figueroa, Daniel G. and Franciolini, Gabriele
and Garcia-Cely, Camilo and Geraci, Andrew and Goryachev,
Maxim and Grote, Hartmut and Hindmarsh, Mark and Ito, Asuka
and Lee, Sung Yun and Martineau, Killian and McDonald, Jamie
and Muia, Francesco and Mukund, Nikhil and Ottaway, David
and Peloso, Marco and Peters, Krisztian and Quevedo,
Fernando and Ricciardone, Angelo and Ringwald, Andreas and
Steinlechner, Jessica and Steinlechner, Sebastian and Sun,
Sichun and Tamarit, Carlos and Tobar, Michael E. and
Torrenti, Francisco and Ünal, Caner and White, Graham},
collaboration = {Kopp, Joachim},
title = {{C}hallenges and opportunities of gravitational-wave
searches above 10 k{H}z},
journal = {Living reviews in relativity},
volume = {28},
number = {1},
issn = {1433-8351},
address = {Potsdam},
publisher = {Inst.},
reportid = {PUBDB-2026-00732, arXiv:2501.11723. CERN-TH-2025-014.
DESY-25-007},
pages = {10},
year = {2025},
note = {Living Rev Relativ 28, 10 (2025). 138 pages, 13 figures.
Update and extension of Living Rev$.$Rel. 24 (2021) 1, 4 on
high frequency gravitational waves (arxiv: 2011.12414).
Matches published version},
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. The scarcity of
possible astrophysical sources in most of 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
of these sources. We review several detector concepts that
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 a
series of workshops on the topic of high-frequency
gravitational wave detection, held in 2019 (ICTP, Trieste,
Italy), 2021 (online) and 2023 (CERN, Geneva, Switzerland).},
keywords = {Gravitational waves (autogen) / Early universe (autogen) /
Compact objects (autogen) / Quantum sensing (autogen) /
Axion searches (autogen) / Microwave cavities (autogen)},
cin = {ATLAS / T},
ddc = {530},
cid = {I:(DE-H253)ATLAS-20120731 / I:(DE-H253)T-20120731},
pnm = {611 - Fundamental Particles and Forces (POF4-611) /
GreatMoves - General Relativistic Moving-Mesh Simulations of
Neutron-Star Mergers (759253) / DFG project 279384907 - SFB
1245: Atomkerne: Von fundamentalen Wechselwirkungen zu
Struktur und Sternen (279384907) / DFG project
G:(GEPRIS)138713538 - SFB 881: Das Milchstraßensystem
(138713538) / DFG project G:(GEPRIS)390831469 - EXC 2118:
Precision Physics, Fundamental Interactions and Structure of
Matter (PRISMA+) (390831469) / DFG project
G:(GEPRIS)390833306 - EXC 2121: Das Quantisierte Universum
II (390833306)},
pid = {G:(DE-HGF)POF4-611 / G:(EU-Grant)759253 /
G:(GEPRIS)279384907 / G:(GEPRIS)138713538 /
G:(GEPRIS)390831469 / G:(GEPRIS)390833306},
experiment = {EXP:(DE-H253)LHC-Exp-ATLAS-20150101},
typ = {PUB:(DE-HGF)16},
eprint = {2501.11723},
howpublished = {arXiv:2501.11723},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2501.11723;\%\%$},
doi = {10.1007/s41114-025-00060-5},
url = {https://bib-pubdb1.desy.de/record/646132},
}