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Gravitational Baryogenesis in Energy-Momentum Squared~Gravity

Pereira, David S. et al.
arXiv (OAI Expanded) · Papers
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general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-theory
We demonstrate that the matter sector itself can drive baryogenesis in energy-momentum squared gravity, $f(R,\mathcal T^2)$ with $\mathcal T^2\equiv T_{μν}T^{μν}$. High-density matter corrections provide new time-dependent sources for the baryon asymmetry through derivative couplings to $\mathcal T^
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