Unified model for inflation and dark energy with Planck-scale pseudo-Goldstone bosons

Eduard Massó; Gabriel Zsembinszki

doi:10.1088/1475-7516/2006/02/012

Unified model for inflation and dark energy with Planck-scale pseudo-Goldstone bosons

Eduard Massó, Gabriel Zsembinszki

Departament de Física

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Resum

We present a model with a complex and a real scalar field and a potential with a symmetry which is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe. © 2006 IOP Publishing Ltd.

Idioma original	Anglès
Número d’article	012
Revista	Journal of Cosmology and Astroparticle Physics
Número	2
DOIs	https://doi.org/10.1088/1475-7516/2006/02/012
Estat de la publicació	Publicada - 1 de febr. 2006

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10.1088/1475-7516/2006/02/012

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https://www.scopus.com/pages/publications/33644640131

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title = "Unified model for inflation and dark energy with Planck-scale pseudo-Goldstone bosons",

abstract = "We present a model with a complex and a real scalar field and a potential with a symmetry which is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe. {\textcopyright} 2006 IOP Publishing Ltd.",

keywords = "Cosmological phase transitions, Cosmology of theories beyond the SM, Inflation",

author = "Eduard Mass{\'o} and Gabriel Zsembinszki",

year = "2006",

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day = "1",

doi = "10.1088/1475-7516/2006/02/012",

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journal = "Journal of Cosmology and Astroparticle Physics",

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T1 - Unified model for inflation and dark energy with Planck-scale pseudo-Goldstone bosons

AU - Massó, Eduard

AU - Zsembinszki, Gabriel

PY - 2006/2/1

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N2 - We present a model with a complex and a real scalar field and a potential with a symmetry which is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe. © 2006 IOP Publishing Ltd.

AB - We present a model with a complex and a real scalar field and a potential with a symmetry which is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe and for the period of acceleration of the late universe. © 2006 IOP Publishing Ltd.

KW - Cosmological phase transitions

KW - Cosmology of theories beyond the SM

KW - Inflation

UR - https://www.scopus.com/pages/publications/33644640131

U2 - 10.1088/1475-7516/2006/02/012

DO - 10.1088/1475-7516/2006/02/012

M3 - Article

SN - 1475-7516

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 2

M1 - 012

ER -

Unified model for inflation and dark energy with Planck-scale pseudo-Goldstone bosons

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