Baryogenesis in cosmological models with symmetric and asymmetric quantum bounces
P. C. M. Delgado, M. B. Jesus, N. Pinto-Neto, T. Mour\~ao, G. S., Vicente

TL;DR
This paper explores how baryon asymmetry can be generated in bouncing cosmological models through two proposed mechanisms, showing that realistic models can produce the observed matter-antimatter imbalance within observational constraints.
Contribution
It investigates baryogenesis mechanisms within symmetric and asymmetric quantum bounce scenarios, demonstrating their compatibility with observational data and expanding understanding of matter-antimatter asymmetry origins.
Findings
Baryon asymmetry can be achieved in bouncing models with mild parameter constraints.
Both spontaneous and gravitational baryogenesis mechanisms are viable in these scenarios.
Realistic bouncing models can produce the observed matter-antimatter imbalance.
Abstract
The baryon-antibaryon asymmetry (excess of matter over antimatter in our Universe), indicated by observational data from the Cosmic Microwave Background anisotropies, predictions of primordial Nucleosynthesis, and the absence of intense radiation from matter-antimatter annihilation, constitutes an unsolved puzzle in cosmology. Two mechanisms for baryon asymmetry have been proposed as extensions of the Standard Model of Particle Physics at high energies. They rely on new couplings involving the baryon number current, one with a scalar field, called Spontaneous Baryogenesis, and the other with space-time curvature, named Gravitational Baryogenesis. These two mechanisms are investigated in the context of many bouncing scenarios, either symmetric or asymmetric around the bounce. It is shown that the constraints on the free parameters of these scenarios, imposed to yield the observed…
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