skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Inflationary scenarios in Starobinsky model with higher order corrections

Abstract

We consider the Starobinsky inflation with a set of higher order corrections parametrised by two real coefficients λ{sub 1} ,λ{sub 2}. In the Einstein frame we have found a potential with the Starobinsky plateau, steep slope and possibly with an additional minimum, local maximum or a saddle point. We have identified three types of inflationary behaviour that may be generated in this model: i) inflation on the plateau, ii) at the local maximum (topological inflation), iii) at the saddle point. We have found limits on parameters λ{sub i} and initial conditions at the Planck scale which enable successful inflation and disable eternal inflation at the plateau. We have checked that the local minimum away from the GR vacuum is stable and that the field cannot leave it neither via quantum tunnelling nor via thermal corrections.

Authors:
 [1];  [2];  [2];  [3]
  1. Institute of Physics, Jagiellonian University,Łojasiewicza 11, 30-348 Kraków (Poland)
  2. Institute of Theoretical Physics, Faculty of Physics, University of Warsaw,ul. Pasteura 5, 02-093 Warsaw (Poland)
  3. (United States)
Publication Date:
Sponsoring Org.:
SCOAP3, CERN, Geneva (Switzerland)
OSTI Identifier:
22454563
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2015; Journal Issue: 06; Other Information: PUBLISHER-ID: JCAP06(2015)032; OAI: oai:repo.scoap3.org:10794; 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; COSMOLOGICAL INFLATION; EINSTEIN FIELD EQUATIONS; GRAVITATION; TOPOLOGY; TUNNEL EFFECT

Citation Formats

Artymowski, Michał, Lalak, Zygmunt, Lewicki, Marek, and Michigan Center for Theoretical Physics, University of Michigan,450 Church Street, Ann Arbor MI 48109. Inflationary scenarios in Starobinsky model with higher order corrections. United States: N. p., 2015. Web. doi:10.1088/1475-7516/2015/06/032.
Artymowski, Michał, Lalak, Zygmunt, Lewicki, Marek, & Michigan Center for Theoretical Physics, University of Michigan,450 Church Street, Ann Arbor MI 48109. Inflationary scenarios in Starobinsky model with higher order corrections. United States. doi:10.1088/1475-7516/2015/06/032.
Artymowski, Michał, Lalak, Zygmunt, Lewicki, Marek, and Michigan Center for Theoretical Physics, University of Michigan,450 Church Street, Ann Arbor MI 48109. Wed . "Inflationary scenarios in Starobinsky model with higher order corrections". United States. doi:10.1088/1475-7516/2015/06/032.
@article{osti_22454563,
title = {Inflationary scenarios in Starobinsky model with higher order corrections},
author = {Artymowski, Michał and Lalak, Zygmunt and Lewicki, Marek and Michigan Center for Theoretical Physics, University of Michigan,450 Church Street, Ann Arbor MI 48109},
abstractNote = {We consider the Starobinsky inflation with a set of higher order corrections parametrised by two real coefficients λ{sub 1} ,λ{sub 2}. In the Einstein frame we have found a potential with the Starobinsky plateau, steep slope and possibly with an additional minimum, local maximum or a saddle point. We have identified three types of inflationary behaviour that may be generated in this model: i) inflation on the plateau, ii) at the local maximum (topological inflation), iii) at the saddle point. We have found limits on parameters λ{sub i} and initial conditions at the Planck scale which enable successful inflation and disable eternal inflation at the plateau. We have checked that the local minimum away from the GR vacuum is stable and that the field cannot leave it neither via quantum tunnelling nor via thermal corrections.},
doi = {10.1088/1475-7516/2015/06/032},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 06,
volume = 2015,
place = {United States},
year = {Wed Jun 17 00:00:00 EDT 2015},
month = {Wed Jun 17 00:00:00 EDT 2015}
}