Pith. sign in

New Q-ball Solutions in Gauge-Mediation, Affleck-Dine Baryogenesis and Gravitino Dark Matter

1 Pith paper cite this work, alongside 12 external citations. Polarity classification is still indexing.

1 Pith paper citing it
12 external citations · Pith
abstract

Affleck-Dine (AD) baryogenesis along a d=6 flat direction in gauge-mediated supersymmetry-breaking (GMSB) models can produce unstable Q-balls which naturally have field strength similar to the messenger scale. In this case a new kind of Q-ball is formed, intermediate between gravity-mediated and gauge-mediated type. We study in detail these new Q-ball solutions, showing how their properties interpolate between standard gravity-mediated and gauge-mediated Q-balls as the AD field becomes larger than the messenger scale. It is shown that E/Q for the Q-balls can be greater than the nucleon mass but less than the MSSM-LSP mass, leading to Q-ball decay directly to Standard Model fermions with no MSSM-LSP production. More significantly, if E/Q is greater than the MSSM-LSP mass, decaying Q-balls can provide a natural source of non-thermal MSSM-LSPs, which can subsequently decay to gravitino dark matter without violating nucleosynthesis constraints. The model therefore provides a minimal scenario for baryogenesis and gravitino dark matter in the gauge-mediated MSSM, requiring no new fields.

fields

gr-qc 1

years

2012 1

verdicts

UNVERDICTED 1

representative citing papers

Dynamical Boson Stars

gr-qc · 2012-02-27 · unverdicted · novelty 2.0

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

citing papers explorer

Showing 1 of 1 citing paper.

  • Dynamical Boson Stars gr-qc · 2012-02-27 · unverdicted · none · ref 172 · internal anchor

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.