Establishes chi^2-dissipation identities, spectral decomposition of Lyapunov functions, and explicit KL convergence factors for Blahut-Arimoto dynamics.
Sedrakian, Short-Range Correlations and Urca Process in Neutron Stars, Phys
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Elasticity suppresses the magnetorotational instability in neutron-star crusts unless the star spins faster than roughly 300 Hz, so pre-merger magnetic field amplification requires a rapidly rotating binary.
Proton emitting source size is amplified by 24% in neutron-rich versus neutron-deficient tin collisions, revealing a beyond-mean-field short-range n-p correlation effect.
citing papers explorer
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Relaxation Kernel, Spectral Dissipation, and Global Convergence of Blahut--Arimoto Dynamics
Establishes chi^2-dissipation identities, spectral decomposition of Lyapunov functions, and explicit KL convergence factors for Blahut-Arimoto dynamics.
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Magnetorotational instabilities in solids: Application to neutron-star crusts
Elasticity suppresses the magnetorotational instability in neutron-star crusts unless the star spins faster than roughly 300 Hz, so pre-merger magnetic field amplification requires a rapidly rotating binary.
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Large amplification of the isospin-dependence of proton emitting source size in radioactive heavy-ion collisions: a signal of n-p correlation
Proton emitting source size is amplified by 24% in neutron-rich versus neutron-deficient tin collisions, revealing a beyond-mean-field short-range n-p correlation effect.