Cosmological probes of supersymmetric field theory models at superhigh energy scales

Sergei V. Ketov, Maxim Yu Khlopov

Research output: Contribution to journalReview article

1 Citation (Scopus)

Abstract

The lack of positive results in searches for supersymmetric (SUSY) particles at the Large Hadron Collider (LHC) and in direct searches forWeakly 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.

Original languageEnglish
Article number511
JournalSymmetry
Volume11
Issue number4
DOIs
Publication statusPublished - 1 Apr 2019

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Field Theory
Probe
probes
Energy
Inflation
High Energy
Physics
universe
Direct Search
antimatter
physics
Early Universe
weakly interacting massive particles
energy
Colliding beam accelerators
Supergravity
Dark Matter
Baryon
supergravity
Model

Keywords

  • Cosmic antinuclei
  • Inflation
  • Primordial Black Holes
  • Supergravity
  • Superheavy dark matter
  • Supersymmetric models

ASJC Scopus subject areas

  • Computer Science (miscellaneous)
  • Chemistry (miscellaneous)
  • Mathematics(all)
  • Physics and Astronomy (miscellaneous)

Cite this

Cosmological probes of supersymmetric field theory models at superhigh energy scales. / Ketov, Sergei V.; Khlopov, Maxim Yu.

In: Symmetry, Vol. 11, No. 4, 511, 01.04.2019.

Research output: Contribution to journalReview article

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