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Title: Microscopic origin of volume modulus inflation

Abstract

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large values during inflation to smaller values today. We describe a possible microscopic origin of the scalar potential of volume modulus inflation by exploiting non-perturbative effects, string loop and higher derivative perturbative corrections to the supergravity effective action together with contributions from anti-branes and charged hidden matter fields. We also analyse the relation between the size of the flux superpotential and the position of the late-time minimum and the inflection point around which inflation takes place. We perform a detailed study of the inflationary dynamics for a single modulus and a two moduli case where we also analyse the sensitivity of the cosmological observables on the choice of initial conditions.

Authors:
 [1];  [2];  [2];  [3];  [2];  [4]
  1. ICTP, Strada Costiera 11, Trieste 34014 (Italy)
  2. (Italy)
  3. Dipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126 Bologna (Italy)
  4. Departamento de Fisica Teórica UAM and Instituto de Fisica Teórica UAM/CSIC, Universidad Autónoma de Madrid, Cantoblanco, 28049 Madrid (Spain)
Publication Date:
Sponsoring Org.:
SCOAP3, CERN, Geneva (Switzerland)
OSTI Identifier:
22458416
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2015; Journal Issue: 12; Other Information: PUBLISHER-ID: JCAP12(2015)040; OAI: oai:repo.scoap3.org:13129; Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ACTION INTEGRAL; BRANES; CORRECTIONS; COSMOLOGICAL INFLATION; GRAVITINOS; POTENTIALS; SENSITIVITY; STRING MODELS; STRING THEORY; SUPERGRAVITY; SUPERSYMMETRY

Citation Formats

Cicoli, Michele, Dipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126 Bologna, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, Muia, Francesco, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, and Pedro, Francisco Gil. Microscopic origin of volume modulus inflation. United States: N. p., 2015. Web. doi:10.1088/1475-7516/2015/12/040.
Cicoli, Michele, Dipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126 Bologna, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, Muia, Francesco, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, & Pedro, Francisco Gil. Microscopic origin of volume modulus inflation. United States. doi:10.1088/1475-7516/2015/12/040.
Cicoli, Michele, Dipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126 Bologna, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, Muia, Francesco, INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna, and Pedro, Francisco Gil. Mon . "Microscopic origin of volume modulus inflation". United States. doi:10.1088/1475-7516/2015/12/040.
@article{osti_22458416,
title = {Microscopic origin of volume modulus inflation},
author = {Cicoli, Michele and Dipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126 Bologna and INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna and Muia, Francesco and INFN, Sezione di Bologna, via Irnerio 46, 40126 Bologna and Pedro, Francisco Gil},
abstractNote = {High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large values during inflation to smaller values today. We describe a possible microscopic origin of the scalar potential of volume modulus inflation by exploiting non-perturbative effects, string loop and higher derivative perturbative corrections to the supergravity effective action together with contributions from anti-branes and charged hidden matter fields. We also analyse the relation between the size of the flux superpotential and the position of the late-time minimum and the inflection point around which inflation takes place. We perform a detailed study of the inflationary dynamics for a single modulus and a two moduli case where we also analyse the sensitivity of the cosmological observables on the choice of initial conditions.},
doi = {10.1088/1475-7516/2015/12/040},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 12,
volume = 2015,
place = {United States},
year = {Mon Dec 21 00:00:00 EST 2015},
month = {Mon Dec 21 00:00:00 EST 2015}
}