arXiv · astro-ph/9804264
Many-Body Corrections to Charged-Current Neutrino Absorption Rates in Nuclear Matter
Abstract
Including nucleon--nucleon correlations due to both Fermi statistics and nuclear forces, we have developed a general formalism for calculating the charged--current neutrino--nucleon absorption rates in nuclear matter. We find that at one half nuclear density many--body effects alone suppress the rates by a factor of two and that the suppression factors increase to $\sim$5 at $4\times10^{14}$ g cm$^{-3}$. The associated increase in the neutrino--matter mean--free--paths parallels that found for neutral--current interactions and opens up interesting possibilities in the context of the delayed supernova mechanism and protoneutron star cooling.
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Adam Burrows, R. F. Sawyer. 1998-04-24. Many-Body Corrections to Charged-Current Neutrino Absorption Rates in Nuclear Matter. https://doi.org/10.1103/physrevc.59.510
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