Gravitational production of spectator massless vector particles in quasi-de Sitter inflation generates superhorizon entanglement, favors sub-Hubble highly energetic collinear pairs, and sets a lower bound on reheating temperature.
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Derives recurrence relations for all-loop leading log quantum corrections and RG equations for the effective potential in SO(N) scalar theories in curved spacetime, applied to power-like potentials in the Jordan frame for inflation.
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Entanglement generation from gravitationally produced massless vector particles during inflation
Gravitational production of spectator massless vector particles in quasi-de Sitter inflation generates superhorizon entanglement, favors sub-Hubble highly energetic collinear pairs, and sets a lower bound on reheating temperature.
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Effective potential in $SO(N)$ symmetric scalar field theories in curved spacetime
Derives recurrence relations for all-loop leading log quantum corrections and RG equations for the effective potential in SO(N) scalar theories in curved spacetime, applied to power-like potentials in the Jordan frame for inflation.