English

Dark matter decay through gravity portals

High Energy Physics - Phenomenology 2017-03-14 v2 Cosmology and Nongalactic Astrophysics

Abstract

Motivated by the fact that, so far, the whole body of evidence for dark matter is of gravitational origin, we study the decays of dark matter into Standard Model particles mediated by gravity portals, i.e., through nonminimal gravitational interactions of dark matter. We investigate the decays in several widely studied frameworks of scalar and fermionic dark matter where the dark matter is stabilized in flat spacetime via global symmetries. We find that the constraints on the scalar singlet dark matter candidate are remarkably strong and exclude large regions of the parameter space, suggesting that an additional stabilizing symmetry should be in place. In contrast, the scalar doublet and the fermionic singlet candidates are naturally protected against too fast decays by gauge and Lorentz symmetry, respectively. For a nonminimal coupling parameter ξO(1)\xi\sim {\cal{O}}(1), decays through the gravity portal are consistent with observations if the dark matter mass is smaller than 105\sim 10^5 GeV, for the scalar doublet, and 106\sim 10^6 GeV, for the fermionic singlet.

Keywords

Cite

@article{arxiv.1611.00725,
  title  = {Dark matter decay through gravity portals},
  author = {Oscar Catà and Alejandro Ibarra and Sebastian Ingenhütt},
  journal= {arXiv preprint arXiv:1611.00725},
  year   = {2017}
}

Comments

30 pages, 4 figures. Minor modifications to match the published version

R2 v1 2026-06-22T16:40:04.377Z