WIMPless Dark Matter from an AMSB Hidden Sector with No New Mass Parameters

TL;DR

This paper proposes a WIMPless dark matter model within an anomaly-mediated supersymmetry breaking hidden sector, where the relic density is fixed by fundamental parameters, leading to distinctive collider and astrophysical signatures.

Contribution

The model uniquely stabilizes dark matter without new mass parameters and predicts a relic density independent of dark matter mass, aligning with the WIMPless miracle.

Findings

Relic density is ~0.1, independent of dark matter mass and interaction strength.

Dark matter may have a mass around 10 GeV or lighter, relevant for direct detection.

Astrophysical signatures include dark matter self-interactions and additional relativistic degrees of freedom.

Abstract

We present a model with dark matter in an anomaly-mediated supersymmetry breaking hidden sector with a U(1)xU(1) gauge symmetry. The symmetries of the model stabilize the dark matter and forbid the introduction of new mass parameters. As a result, the thermal relic density is completely determined by the gravitino mass and dimensionless couplings. Assuming non-hierarchical couplings, the thermal relic density is ~ 0.1, independent of the dark matter's mass and interaction strength, realizing the WIMPless miracle. The model has several striking features. For particle physics, stability of the dark matter is completely consistent with R-parity violation in the visible sector, with implications for superpartner collider signatures; also the thermal relic's mass may be ~ 10 GeV or lighter, which is of interest given recent direct detection results. Interesting astrophysical signatures are dark matter self-interactions through a long-range force, and massless hidden photons and fermions that contribute to the number of relativistic degrees of freedom at BBN and CMB. The latter are particularly interesting, given current indications for extra degrees of freedom and near future results from the Planck observatory.