Dark Matter could be a composite state of a confining sector with an approximate scale symmetry. We consider the case where the associated pseudo-Goldstone boson, the dilaton, mediates its interactions with the Standard Model. When the confining phase transition in the early universe is supercooled, its dynamics allows for Dark Matter masses up to 106 TeV. We derive the precise parameter space compatible with all experimental constraints, finding that this scenario can be tested partly by telescopes and entirely by gravitational waves.

Supercool composite Dark Matter beyond 100 TeV / Baldes I.; Gouttenoire Y.; Sala F.; Servant G.. - In: JOURNAL OF HIGH ENERGY PHYSICS. - ISSN 1029-8479. - ELETTRONICO. - 2022:7(2022), pp. 84.1-84.80. [10.1007/JHEP07(2022)084]

Supercool composite Dark Matter beyond 100 TeV

Sala F.;
2022

Abstract

Dark Matter could be a composite state of a confining sector with an approximate scale symmetry. We consider the case where the associated pseudo-Goldstone boson, the dilaton, mediates its interactions with the Standard Model. When the confining phase transition in the early universe is supercooled, its dynamics allows for Dark Matter masses up to 106 TeV. We derive the precise parameter space compatible with all experimental constraints, finding that this scenario can be tested partly by telescopes and entirely by gravitational waves.
2022
Supercool composite Dark Matter beyond 100 TeV / Baldes I.; Gouttenoire Y.; Sala F.; Servant G.. - In: JOURNAL OF HIGH ENERGY PHYSICS. - ISSN 1029-8479. - ELETTRONICO. - 2022:7(2022), pp. 84.1-84.80. [10.1007/JHEP07(2022)084]
Baldes I.; Gouttenoire Y.; Sala F.; Servant G.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/908101
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