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Title: Constraints on Inflation in MSSM from Baryon Asymmetry

Abstract

Finite density effects can change the inflationary reheating temperature of a large class of inflationary scenarios in the context of supersymmetry by a multiplicative factor of 1012. This gives the flat direction HuHd in MSSM a unique advantage over all other flat directions for being a participant in inflationary dynamics. More details concerning the content of this talk can be found in [1].

Authors:
 [1]
  1. Department of Physics, University of Wisconsin, 1150 University Ave., Madison, WI 53706 (United States)
Publication Date:
OSTI Identifier:
20729155
Resource Type:
Journal Article
Resource Relation:
Journal Name: AIP Conference Proceedings; Journal Volume: 805; Journal Issue: 1; Conference: PASCOS 2005: 11. international symposium on particles, strings, and cosmology, Gyeongju (Korea, Republic of), 30 May - 4 Jun 2005; Other Information: DOI: 10.1063/1.2149669; (c) 2005 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ASYMMETRY; BARYONS; COSMOLOGY; DENSITY; INFLATIONARY UNIVERSE; STANDARD MODEL; SUPERSYMMETRY

Citation Formats

Chung, Daniel J.H. Constraints on Inflation in MSSM from Baryon Asymmetry. United States: N. p., 2005. Web. doi:10.1063/1.2149669.
Chung, Daniel J.H. Constraints on Inflation in MSSM from Baryon Asymmetry. United States. doi:10.1063/1.2149669.
Chung, Daniel J.H. Fri . "Constraints on Inflation in MSSM from Baryon Asymmetry". United States. doi:10.1063/1.2149669.
@article{osti_20729155,
title = {Constraints on Inflation in MSSM from Baryon Asymmetry},
author = {Chung, Daniel J.H.},
abstractNote = {Finite density effects can change the inflationary reheating temperature of a large class of inflationary scenarios in the context of supersymmetry by a multiplicative factor of 1012. This gives the flat direction HuHd in MSSM a unique advantage over all other flat directions for being a participant in inflationary dynamics. More details concerning the content of this talk can be found in [1].},
doi = {10.1063/1.2149669},
journal = {AIP Conference Proceedings},
number = 1,
volume = 805,
place = {United States},
year = {Fri Dec 02 00:00:00 EST 2005},
month = {Fri Dec 02 00:00:00 EST 2005}
}