• Open Access

4D models of de Sitter uplift

Renata Kallosh, Andrei Linde, Evan McDonough, and Marco Scalisi
Phys. Rev. D 99, 046006 – Published 12 February 2019

Abstract

It was shown in [1] that the modified 4D version of the Kachru, Kallosh, Linde, and Trivedi (KKLT) model proposed in [2] is inconsistent for large values of the parameter c advocated in [2], since there is a point in the moduli space where |DSW|2 vanishes. The authors responded with yet another modification of the 4D KKLT model [3]. However, for large c, this model suffers from an even worse problem: not only is there a point in the moduli space where |DSW|2 vanishes, there is also a region in the moduli space where |DSW|2 is negative. Meanwhile, for small c these models have de Sitter (dS) vacua. We construct improved models, which are fully consistent for all values of parameters, just as the original version of the KKLT model, using a nilpotent superfield. These models have a family of dS vacua for a broad range of parameter values. Thus, the results of the analysis of all presently available consistent generalizations of the 4D KKLT model, in the domain of their validity, confirm the existence of dS vacua in the KKLT scenario.

  • Figure
  • Received 2 October 2018

DOI:https://doi.org/10.1103/PhysRevD.99.046006

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsGravitation, Cosmology & Astrophysics

Authors & Affiliations

Renata Kallosh1,*, Andrei Linde1,†, Evan McDonough2,‡, and Marco Scalisi3,§

  • 1Stanford Institute for Theoretical Physics and Department of Physics, Stanford University, Stanford, California 94305, USA
  • 2Department of Physics, Brown University, Providence, Rhode Island 02903, USA
  • 3Institute for Theoretical Physics, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium

  • *kallosh@stanford.edu
  • alinde@stanford.edu
  • evan_mcdonough@brown.edu
  • §marco.scalisi@kuleuven.be

Article Text

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Issue

Vol. 99, Iss. 4 — 15 February 2019

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