Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity

Abstract

We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in N= 1 supergravity with the dilaton–axion chiral superfield T in the presence of an N= 1 vector multiplet with the alternative Fayet–Iliopoulos term. By using the Kähler potential as K= - αlog (T+ T¯) and the superpotential as a sum of a constant and a linear term, we find that viable inflation is possible for 3 ≤ α≤ α_max where α_max≈ 7.235. Observations of the amplitude of primordial scalar perturbations fix the SUSY breaking scale in our models as high as 1013GeV. In the case of α> 3 the axion gets the tree-level (non-tachyonic) mass comparable to the inflaton mass.

Original language	English
Article number	713
Journal	European Physical Journal C
Volume	79
Issue number	8
DOIs	https://doi.org/10.1140/epjc/s10052-019-7225-2
Publication status	Published - 1 Aug 2019

ASJC Scopus subject areas

Engineering (miscellaneous)
Physics and Astronomy (miscellaneous)

Access to Document

10.1140/epjc/s10052-019-7225-2

Fingerprint Dive into the research topics of 'Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity'. Together they form a unique fingerprint.

Cite this

@article{a747858144034860b0f0f4d6261522e4,

title = "Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity",

abstract = "We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in N= 1 supergravity with the dilaton–axion chiral superfield T in the presence of an N= 1 vector multiplet with the alternative Fayet–Iliopoulos term. By using the K{\"a}hler potential as K= - αlog (T+ T¯) and the superpotential as a sum of a constant and a linear term, we find that viable inflation is possible for 3 ≤ α≤ αmax where αmax≈ 7.235. Observations of the amplitude of primordial scalar perturbations fix the SUSY breaking scale in our models as high as 1013GeV. In the case of α> 3 the axion gets the tree-level (non-tachyonic) mass comparable to the inflaton mass.",

author = "Yermek Aldabergenov and Auttakit Chatrabhuti and Ketov, {Sergei V.}",

year = "2019",

month = aug,

day = "1",

doi = "10.1140/epjc/s10052-019-7225-2",

language = "English",

volume = "79",

journal = "European Physical Journal C",

issn = "1434-6044",

publisher = "Springer New York",

number = "8",

}

TY - JOUR

T1 - Generalized dilaton–axion models of inflation, de Sitter vacua and spontaneous SUSY breaking in supergravity

AU - Aldabergenov, Yermek

AU - Chatrabhuti, Auttakit

AU - Ketov, Sergei V.

PY - 2019/8/1

Y1 - 2019/8/1

N2 - We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in N= 1 supergravity with the dilaton–axion chiral superfield T in the presence of an N= 1 vector multiplet with the alternative Fayet–Iliopoulos term. By using the Kähler potential as K= - αlog (T+ T¯) and the superpotential as a sum of a constant and a linear term, we find that viable inflation is possible for 3 ≤ α≤ αmax where αmax≈ 7.235. Observations of the amplitude of primordial scalar perturbations fix the SUSY breaking scale in our models as high as 1013GeV. In the case of α> 3 the axion gets the tree-level (non-tachyonic) mass comparable to the inflaton mass.

AB - We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in N= 1 supergravity with the dilaton–axion chiral superfield T in the presence of an N= 1 vector multiplet with the alternative Fayet–Iliopoulos term. By using the Kähler potential as K= - αlog (T+ T¯) and the superpotential as a sum of a constant and a linear term, we find that viable inflation is possible for 3 ≤ α≤ αmax where αmax≈ 7.235. Observations of the amplitude of primordial scalar perturbations fix the SUSY breaking scale in our models as high as 1013GeV. In the case of α> 3 the axion gets the tree-level (non-tachyonic) mass comparable to the inflaton mass.

UR - http://www.scopus.com/inward/record.url?scp=85071337789&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85071337789&partnerID=8YFLogxK

U2 - 10.1140/epjc/s10052-019-7225-2

DO - 10.1140/epjc/s10052-019-7225-2

M3 - Article

AN - SCOPUS:85071337789

VL - 79

JO - European Physical Journal C

JF - European Physical Journal C

SN - 1434-6044

IS - 8

M1 - 713

ER -