Implications of a supercooled universe

Pietro Baratella; Alex Pomarol; Fabrizio Rompineve

doi:10.1016/j.nuclphysbps.2019.03.016

Implications of a supercooled universe

Pietro Baratella, Alex Pomarol, Fabrizio Rompineve

Department of Physics

Research output: Contribution to journal › Article › Research

Abstract

© 2019 Elsevier B.V. We argue that strongly-interacting theories at the TeV scale can naturally lead to a long period of supercooling in the early universe. We analyze the implications for the relic abundance of axions, dark matter and baryons.

Original language	English
Pages (from-to)	80-85
Journal	Nuclear and Particle Physics Proceedings
Volume	303-305
DOIs	https://doi.org/10.1016/j.nuclphysbps.2019.03.016
Publication status	Published - 1 Oct 2018

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title = "Implications of a supercooled universe",

abstract = "{\textcopyright} 2019 Elsevier B.V. We argue that strongly-interacting theories at the TeV scale can naturally lead to a long period of supercooling in the early universe. We analyze the implications for the relic abundance of axions, dark matter and baryons.",

author = "Pietro Baratella and Alex Pomarol and Fabrizio Rompineve",

year = "2018",

month = oct,

day = "1",

doi = "10.1016/j.nuclphysbps.2019.03.016",

language = "English",

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pages = "80--85",

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TY - JOUR

T1 - Implications of a supercooled universe

AU - Baratella, Pietro

AU - Pomarol, Alex

AU - Rompineve, Fabrizio

PY - 2018/10/1

Y1 - 2018/10/1

N2 - © 2019 Elsevier B.V. We argue that strongly-interacting theories at the TeV scale can naturally lead to a long period of supercooling in the early universe. We analyze the implications for the relic abundance of axions, dark matter and baryons.

AB - © 2019 Elsevier B.V. We argue that strongly-interacting theories at the TeV scale can naturally lead to a long period of supercooling in the early universe. We analyze the implications for the relic abundance of axions, dark matter and baryons.

U2 - 10.1016/j.nuclphysbps.2019.03.016

DO - 10.1016/j.nuclphysbps.2019.03.016

M3 - Article

VL - 303-305

SP - 80

EP - 85

ER -

Implications of a supercooled universe

Abstract

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