• Open Access

Revisiting oscillon formation in the Kachru-Kallosh-Linde-Trivedi scenario

Shinta Kasuya, Masahiro Kawasaki, Francis Otani, and Eisuke Sonomoto
Phys. Rev. D 102, 043016 – Published 24 August 2020

Abstract

Kachru-Kallosh-Linde-Trivedi (KKLT) scenario has succeeded in stabilizing the volume modulus and constructing metastable de Sitter (dS) vacua in type IIB string theory. We revisit to investigate the possibility of the oscillon (or I-ball) formation in the KKLT scenario when the volume modulus is initially displaced from the dS minimum. Special attention is paid to physically realistic initial conditions of the volume modulus, which was not taken in the literature. Using lattice simulations, we find that oscillons do not form unless the volume modulus is initially placed at very near the local maximum, which requires severe fine-tuning.

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  • Received 31 January 2020
  • Accepted 4 August 2020

DOI:https://doi.org/10.1103/PhysRevD.102.043016

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 & Fields

Authors & Affiliations

Shinta Kasuya1, Masahiro Kawasaki2,3, Francis Otani2,3, and Eisuke Sonomoto2,3

  • 1Department of Mathematics and Physics, Kanagawa University, Kanagawa 259-1293, Japan
  • 2ICRR, University of Tokyo, Kashiwa 277-8582, Japan
  • 3Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa 277-8583, Japan

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Issue

Vol. 102, Iss. 4 — 15 August 2020

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