A solution to the baryon-DM coincidence problem in the CMSSM with a 126-GeV Higgs boson
Ayuki Kamada, Masahiro Kawasaki, and Masaki Yamada

TL;DR
This paper proposes a solution to the baryon-dark matter coincidence problem within the CMSSM framework, utilizing late-time decay of Q-balls formed after Affleck-Dine baryogenesis, consistent with a 126-GeV Higgs.
Contribution
It introduces a novel mechanism linking baryon and dark matter production through Q-ball decay in the CMSSM, aligning with Higgs mass observations.
Findings
The baryon-DM coincidence is explained by Q-ball decay in CMSSM.
A specific relation between scalar and gaugino masses is identified.
Results are consistent with the observed 126-GeV Higgs boson.
Abstract
We show that the baryon-dark matter coincidence problem is solved in the CMSSM. The baryons and dark matter are generated simultaneously through the late-time decay of non-topological solitons, Q-balls, which are formed after the Affleck-Dine baryogenesis. A certain relation between the universal scalar mass, , and the universal gaugino mass, , is required to solve the coincidence problem, marginally depending on the other CMSSM parameters, and the result is consistent with the observation of the 126-GeV Higgs boson.
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