Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales

The lack of positive results in searches for supersymmetric (SUSY) particles at the Large Hadron Collider (LHC) and in direct searches for Weakly Interacting Massive Particles (WIMPs) in the underground experiments may hint to a super-high energy scale of SUSY phenomena beyond the reach of direct ex...

Full description

Bibliographic Details
Main Authors: Sergei V. Ketov, Maxim Yu. Khlopov
Format: Article
Language:English
Published: MDPI AG 2019-04-01
Series:Symmetry
Subjects:
Online Access:https://www.mdpi.com/2073-8994/11/4/511
id doaj-293643d1b9194919a8959af9058f691a
record_format Article
spelling doaj-293643d1b9194919a8959af9058f691a2020-11-25T01:21:53ZengMDPI AGSymmetry2073-89942019-04-0111451110.3390/sym11040511sym11040511Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy ScalesSergei V. Ketov0Maxim Yu. Khlopov1Department of Physics, Tokyo Metropolitan University, 1-1 Minami-ohsawa, Hachioji-shi, Tokyo 192-0397, JapanAPC Laboratory 10, Rue Alice Domon et Léonie Duquet, 75205 CEDEX 13 Paris, FranceThe lack of positive results in searches for supersymmetric (SUSY) particles at the Large Hadron Collider (LHC) and in direct searches for Weakly Interacting Massive Particles (WIMPs) in the underground experiments may hint to a super-high energy scale of SUSY phenomena beyond the reach of direct experimental probes. At such scales the supergravity models based on Starobinsky inflation can provide the mechanisms for both inflation and superheavy dark matter. However, it makes the indirect methods the only way of testing the SUSY models, so that cosmological probes acquire the special role in this context. Such probes can rely on the nontrivial effects of SUSY physics in the early Universe, which are all model-dependent and thus can provide discrimination of the models and their parameters. The nonstandard cosmological features like Primordial Black Holes (PBHs) or antimatter domains in a baryon-asymmetric universe are discussed as possible probes for high energy scale SUSY physics.https://www.mdpi.com/2073-8994/11/4/511supersymmetric modelssupergravityinflationsuperheavy dark matterPrimordial Black Holescosmic antinuclei
collection DOAJ
language English
format Article
sources DOAJ
author Sergei V. Ketov
Maxim Yu. Khlopov
spellingShingle Sergei V. Ketov
Maxim Yu. Khlopov
Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
Symmetry
supersymmetric models
supergravity
inflation
superheavy dark matter
Primordial Black Holes
cosmic antinuclei
author_facet Sergei V. Ketov
Maxim Yu. Khlopov
author_sort Sergei V. Ketov
title Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
title_short Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
title_full Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
title_fullStr Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
title_full_unstemmed Cosmological Probes of Supersymmetric Field Theory Models at Superhigh Energy Scales
title_sort cosmological probes of supersymmetric field theory models at superhigh energy scales
publisher MDPI AG
series Symmetry
issn 2073-8994
publishDate 2019-04-01
description The lack of positive results in searches for supersymmetric (SUSY) particles at the Large Hadron Collider (LHC) and in direct searches for Weakly Interacting Massive Particles (WIMPs) in the underground experiments may hint to a super-high energy scale of SUSY phenomena beyond the reach of direct experimental probes. At such scales the supergravity models based on Starobinsky inflation can provide the mechanisms for both inflation and superheavy dark matter. However, it makes the indirect methods the only way of testing the SUSY models, so that cosmological probes acquire the special role in this context. Such probes can rely on the nontrivial effects of SUSY physics in the early Universe, which are all model-dependent and thus can provide discrimination of the models and their parameters. The nonstandard cosmological features like Primordial Black Holes (PBHs) or antimatter domains in a baryon-asymmetric universe are discussed as possible probes for high energy scale SUSY physics.
topic supersymmetric models
supergravity
inflation
superheavy dark matter
Primordial Black Holes
cosmic antinuclei
url https://www.mdpi.com/2073-8994/11/4/511
work_keys_str_mv AT sergeivketov cosmologicalprobesofsupersymmetricfieldtheorymodelsatsuperhighenergyscales
AT maximyukhlopov cosmologicalprobesofsupersymmetricfieldtheorymodelsatsuperhighenergyscales
_version_ 1725128687055011840