Testing high scale supersymmetry via second order gravitational waves
Testing high scale supersymmetry via second order gravitational waves
Supersymmetry predicts multiple flat directions, some of which carry a net baryon or lepton number. Condensates in such directions form during inflation and later fragment into Q-balls, which can become the building blocks of primordial black holes. Thus supersymmetry can create conditions for an intermediate matter-dominated era with black holes dominating the energy density of the universe. Unlike particle matter, black holes decay suddenly enough to result in an observable gravitational wave signal via the poltergeist mechanism. We investigate the gravitational waves signatures of supersymmetry realized at energy scales that might not be accessible to present-day colliders.
hep-ph, astro-ph.CO
Flores, Marcos M.
4e4e80b9-645e-4b0b-85bd-52f265249fe6
Kusenko, Alexander
947377e3-3001-4a91-8c9f-08b608167d20
Pearce, Lauren
d4bc45df-b75d-428b-82cc-bdfd3aad78ac
Perez-Gonzalez, Yuber F.
b1310ba3-94e4-4abe-b5b1-c72ce5a1a046
White, Graham
652445c5-e1e5-4ff7-84e1-a3bca45e75d0
29 August 2023
Flores, Marcos M.
4e4e80b9-645e-4b0b-85bd-52f265249fe6
Kusenko, Alexander
947377e3-3001-4a91-8c9f-08b608167d20
Pearce, Lauren
d4bc45df-b75d-428b-82cc-bdfd3aad78ac
Perez-Gonzalez, Yuber F.
b1310ba3-94e4-4abe-b5b1-c72ce5a1a046
White, Graham
652445c5-e1e5-4ff7-84e1-a3bca45e75d0
[Unknown type: UNSPECIFIED]
Abstract
Supersymmetry predicts multiple flat directions, some of which carry a net baryon or lepton number. Condensates in such directions form during inflation and later fragment into Q-balls, which can become the building blocks of primordial black holes. Thus supersymmetry can create conditions for an intermediate matter-dominated era with black holes dominating the energy density of the universe. Unlike particle matter, black holes decay suddenly enough to result in an observable gravitational wave signal via the poltergeist mechanism. We investigate the gravitational waves signatures of supersymmetry realized at energy scales that might not be accessible to present-day colliders.
Text
2308.15522v1
- Author's Original
More information
Published date: 29 August 2023
Additional Information:
9 pages, 3 figures
Keywords:
hep-ph, astro-ph.CO
Identifiers
Local EPrints ID: 481576
URI: http://eprints.soton.ac.uk/id/eprint/481576
PURE UUID: 035d425c-e227-4d1d-9328-36b1b67dfb22
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Date deposited: 04 Sep 2023 16:37
Last modified: 17 Mar 2024 04:25
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Contributors
Author:
Marcos M. Flores
Author:
Alexander Kusenko
Author:
Lauren Pearce
Author:
Yuber F. Perez-Gonzalez
Author:
Graham White
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