Supercool composite Dark Matter beyond 100 TeV

被引：45

作者：

Baldes, Iason ^{[1
]}

Gouttenoire, Yann ^{[2
,3
]}

Sala, Filippo ^{[4
,5
]}

Servant, Geraldine ^{[2
,6
]}

机构：

[1] Univ Libre Bruxelles, Serv Phys Theor, Blvd Triomphe,CP225, B-1050 Brussels, Belgium

[2] DESY, Notkestr 85, D-22607 Hamburg, Germany

[3] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel

[4] CNRS, LPTHE, 4 Pl Jussieu, F-75252 Paris, France

[5] Sorbonne Univ, 4 Pl Jussieu, F-75252 Paris, France

[6] Univ Hamburg, Inst Theoret Phys 2, Luruper Chaussee 149, D-22761 Hamburg, Germany

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2022年 / 2022卷 / 07期

关键词：

Beyond Standard Model; Confinement; Cosmology of Theories beyond the SM; Technicolor and Composite Models; ELECTROWEAK PHASE-TRANSITION; FALSE VACUUM; COSMOLOGICAL CONSEQUENCES; HIGGS-BOSON; MODEL; FATE; SUPERSYMMETRY; TEMPERATURE; NUCLEATION; BREAKING;

D O I：

10.1007/JHEP07(2022)084

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

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 10(6) 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.

引用

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