2021
DOI: 10.48550/arxiv.2110.05487
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R-Parity Violation Axiogenesis

Raymond T. Co,
Keisuke Harigaya,
Zachary Johnson
et al.

Abstract: We show that the rotation of the QCD axion field, aided by B − L violation from supersymmetric R-parity violating couplings, can yield the observed baryon abundance. Strong sphaleron processes transfer the angular momentum of the axion field into a quark chiral asymmetry, which R-parity violating couplings convert to the baryon asymmetry of the Universe. We focus on the case of dimensionless R-parity violating couplings with textures motivated by grand unified theories and comment on more general scenarios. Th… Show more

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“…The present work also contributes to the larger effort in the community to explore the different possibilities for the cosmological axion evolution which open up once the assumptions of the canonical misalignment picture are relaxed or modified. Indeed, a variety of such scenarios have been proposed in the literature, e. g., large [43][44][45][46] or small [47][48][49][50] misalignment angles, parametric resonance [51][52][53], kinetic misalignment mechanism [39,[54][55][56][57][58][59][60][61][62][63], trapped misalignment [64], axion fragmentation [65][66][67], varying axion decay constant [68], interaction with monopoles [69,70] or modifications in the cosmological history of the Universe [71,72], including entropy injection [12,73,74] or non-standard inflation scenarios [75][76][77][78][79][80].…”
Section: Introductionmentioning
confidence: 99%
“…The present work also contributes to the larger effort in the community to explore the different possibilities for the cosmological axion evolution which open up once the assumptions of the canonical misalignment picture are relaxed or modified. Indeed, a variety of such scenarios have been proposed in the literature, e. g., large [43][44][45][46] or small [47][48][49][50] misalignment angles, parametric resonance [51][52][53], kinetic misalignment mechanism [39,[54][55][56][57][58][59][60][61][62][63], trapped misalignment [64], axion fragmentation [65][66][67], varying axion decay constant [68], interaction with monopoles [69,70] or modifications in the cosmological history of the Universe [71,72], including entropy injection [12,73,74] or non-standard inflation scenarios [75][76][77][78][79][80].…”
Section: Introductionmentioning
confidence: 99%