Torsion-induced one-loop corrections can suppress the stochastic gravitational wave signal from inflaton decay by up to two orders of magnitude relative to tree-level predictions.
Renormalization Group independence of Cosmological Attrac- tors
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An RG-improved EFT matches large-Nc pionless contacts to σ,ρ,ω meson-exchange saturation at scale m_V, normalizes the coupling to the deuteron, and substitutes CD-Bonn couplings to obtain B_ΔΔ ≃ 96 MeV, within 14% of the experimental 84 MeV.
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
citing papers explorer
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Torsion induced one-loop corrections to inflaton decay and the Stochastic gravitational waves
Torsion-induced one-loop corrections can suppress the stochastic gravitational wave signal from inflaton decay by up to two orders of magnitude relative to tree-level predictions.
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Deeply bound dibaryon $d^*(2380)$ from meson-exchange saturation $\Delta\Delta$ effective field theory
An RG-improved EFT matches large-Nc pionless contacts to σ,ρ,ω meson-exchange saturation at scale m_V, normalizes the coupling to the deuteron, and substitutes CD-Bonn couplings to obtain B_ΔΔ ≃ 96 MeV, within 14% of the experimental 84 MeV.
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Dense Matter and Compact Stars in Strong Magnetic Fields
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.