Home > Research > Publications & Outputs > Inflation in string theory

Electronic data

  • E063527

    Rights statement: © 2011 American Physical Society

    Final published version, 107 KB, PDF document

Links

Text available via DOI:

View graph of relations

Inflation in string theory: a graceful exit to the real world

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Inflation in string theory: a graceful exit to the real world. / Cicoli, Michele; Mazumdar, Anupam.
In: Physical Review D – Particles and Fields, Vol. 83, No. 6, 063527, 05.10.2010.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Cicoli, M & Mazumdar, A 2010, 'Inflation in string theory: a graceful exit to the real world', Physical Review D – Particles and Fields, vol. 83, no. 6, 063527. https://doi.org/10.1103/PhysRevD.83.063527

APA

Cicoli, M., & Mazumdar, A. (2010). Inflation in string theory: a graceful exit to the real world. Physical Review D – Particles and Fields, 83(6), Article 063527. https://doi.org/10.1103/PhysRevD.83.063527

Vancouver

Cicoli M, Mazumdar A. Inflation in string theory: a graceful exit to the real world. Physical Review D – Particles and Fields. 2010 Oct 5;83(6):063527. doi: 10.1103/PhysRevD.83.063527

Author

Cicoli, Michele ; Mazumdar, Anupam. / Inflation in string theory : a graceful exit to the real world. In: Physical Review D – Particles and Fields. 2010 ; Vol. 83, No. 6.

Bibtex

@article{53fb0a00ffdd4ab089e8aa72a63e2aab,
title = "Inflation in string theory: a graceful exit to the real world",
abstract = "The most important criteria for a successful inflation are to explain the observed temperature anisotropy in the cosmic microwave background radiation, and exiting inflation in a vacuum where it can excite the Standard Model quarks and leptons required for the success of Big Bang Nucleosynthesis. In this paper we provide the first ever closed string model of inflation where the inflaton couplings to hidden sector, moduli sector, and visible sector fields can be computed, showing that inflation can lead to reheating the Standard Model degrees of freedom before the electro-weak scale.",
author = "Michele Cicoli and Anupam Mazumdar",
note = "5 pages, 1 table; added a discussion on the interplay between global and local issues of string compactifications {\textcopyright} 2011 American Physical Society",
year = "2010",
month = oct,
day = "5",
doi = "10.1103/PhysRevD.83.063527",
language = "English",
volume = "83",
journal = "Physical Review D – Particles and Fields",
issn = "1550-2368",
publisher = "American Physical Society",
number = "6",

}

RIS

TY - JOUR

T1 - Inflation in string theory

T2 - a graceful exit to the real world

AU - Cicoli, Michele

AU - Mazumdar, Anupam

N1 - 5 pages, 1 table; added a discussion on the interplay between global and local issues of string compactifications © 2011 American Physical Society

PY - 2010/10/5

Y1 - 2010/10/5

N2 - The most important criteria for a successful inflation are to explain the observed temperature anisotropy in the cosmic microwave background radiation, and exiting inflation in a vacuum where it can excite the Standard Model quarks and leptons required for the success of Big Bang Nucleosynthesis. In this paper we provide the first ever closed string model of inflation where the inflaton couplings to hidden sector, moduli sector, and visible sector fields can be computed, showing that inflation can lead to reheating the Standard Model degrees of freedom before the electro-weak scale.

AB - The most important criteria for a successful inflation are to explain the observed temperature anisotropy in the cosmic microwave background radiation, and exiting inflation in a vacuum where it can excite the Standard Model quarks and leptons required for the success of Big Bang Nucleosynthesis. In this paper we provide the first ever closed string model of inflation where the inflaton couplings to hidden sector, moduli sector, and visible sector fields can be computed, showing that inflation can lead to reheating the Standard Model degrees of freedom before the electro-weak scale.

U2 - 10.1103/PhysRevD.83.063527

DO - 10.1103/PhysRevD.83.063527

M3 - Journal article

VL - 83

JO - Physical Review D – Particles and Fields

JF - Physical Review D – Particles and Fields

SN - 1550-2368

IS - 6

M1 - 063527

ER -