English

Light Higgsinos in Pure Gravity Mediation

High Energy Physics - Phenomenology 2015-06-23 v1

Abstract

Pure gravity mediation (PGM), with two free parameters, is a minimalistic approach to supergravity models, yet is capable of incorporating radiative electroweak symmetry breaking, a Higgs mass in agreement with the experimental measurement, without violating any phenomenological constraints. The model may also contain a viable dark matter candidate in the form of a wino. Here, we extend the minimal model by allowing the μ\mu-term to be a free parameter (equivalent to allowing the two Higgs soft masses, m1m_1 and m2m_2, to differ from other scalar masses) which are set by the gravitino mass. In particular, we examine the region of parameter space where μm3/2\mu \ll m_{3/2} in which case, the Higgsino becomes the lightest supersymmetric particle (LSP) and a dark matter candidate. We also consider a generalization of PGM which incorporates a Peccei-Quinn symmetry which determines the μ\mu-term dynamically. In this case, we show that the dark matter may either be in the form of an axion and/or a neutralino, and that the LSP may be either a wino, bino, or Higgsino.

Keywords

Cite

@article{arxiv.1412.3403,
  title  = {Light Higgsinos in Pure Gravity Mediation},
  author = {Jason L. Evans and Masahiro Ibe and Keith A. Olive and Tsutomu T. Yanagida},
  journal= {arXiv preprint arXiv:1412.3403},
  year   = {2015}
}

Comments

24 pages, 13 Figures

R2 v1 2026-06-22T07:26:51.828Z