Neutralino Dark Matter in SUSY-SU(5) with RH neutrinos

TL;DR

This paper explores a SUSY-GUT model with right-handed neutrinos based on SU(5), analyzing its impact on neutralino dark matter relic density and identifying unique phenomenological features and constraints.

Contribution

It introduces a SUSY-SU(5) model with right-handed neutrinos and studies its implications for neutralino dark matter, highlighting modifications to the sparticle spectrum and relic density constraints.

Findings

RG effects alter the sparticle spectrum significantly.

WMAP relic density limits restrict small $ aneta$ regions.

Upper bounds on neutralino mass are identified.

Abstract

In the context of low-energy Supersymmetry, a model of Grand Unification with right-handed neutrinos, based on the group SU(5), is discussed and its implications for neutralino dark matter (DM) are studied and compared with the constrained MSSM. RG effects in this model modify the sparticle spectrum such that the WMAP limit on the DM relic density cannot be satisfied for small values of $\tan\beta$ ($\tan\beta \lesssim 35$) and the region of the parameter space allowed by efficient neutralino-stau coannihilation presents a peculiar phenomenology and an upper bound on the neutralino mass for most of the parameters choices.