PaperPanorama

Nuclear Theory·nucl-th

Thursday·March 5, 2020

5 papers3 primary·2 cross-listed

  1. 04

    Thermo-magnetic spectral properties of neutral mesons in vector and axial-vector channels using NJL model

    Snigdha Ghosh🇮🇳 · Arghya Mukherjee🇮🇳 · Nilanjan Chaudhuri🇮🇳 · Pradip Roy🇮🇳 · Sourav Sarkar🇮🇳

    In this work the neutral meson properties have been investigated in the presence of thermo-magnetic background using two-flavor Nambu--Jona-Lasinio model. Mass, spectral function and dispersion relations are obtained in the scalar () and pseudo-scalar () channels as well as in the vector () and axial vector () channels. The general Lorentz structures for the vector and axial-vector meson polarization functions have been considered in detail. The ultra-violet divergences appearing in this work have been regularized using a mixed regularization technique where the gamma functions arising in dimensional regularization are replaced with incomplete gamma functions as usually done in the proper time regularization procedure. The meson spectral functions obtained in the presence of a magnetic field possess nontrivial oscillatory structure. Similar to the scalar and pseudo-scalar channel, the spectral functions for each of the modes of are observed to overlap with the corresponding modes of its chiral partner mesons in the chiral symmetry restored phase. We observe discontinuities in the masses of all the mesonic excitations for a non-zero external magnetic field.

    hep-phnucl-thPRD(2020)·30 citations
  2. 05

    Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations

    Micaela Oertel (LUTH (UMR\_8102))🇫🇷 · Aurélien Pascal (LUTH (UMR\_8102))🇫🇷 · Marco Mancini (LUTH (UMR\_8102))🇫🇷 · Jerome Novak (LUTH (UMR\_8102))🇫🇷

    Neutrinos play an important role in compact star astrophysics: neutrino-heating is one of the main ingredients in core-collapse supernovae, neutrino-matter interactions determine the composition of matter in binary neutron star mergers and have among others a strong impact on conditions for heavy element nucleosynthesis and neutron star cooling is dominated by neutrino emission except for very old stars. Many works in the last decades have shown that in dense matter medium effects considerably change the neutrino-matter interaction rates, whereas many astrophysical simulations use analytic approximations which are often far from reproducing more complete calculations. In this work we present a scheme which allows to incorporate improved rates, for charged current interactions, into simulations and show as an example some results for core-collapse supernovae, where a noticeable difference is found in the location of the neutrinospheres of the low-energy neutrinos in the early post-bounce phase.

    astro-ph.HEnucl-thPRC(2020)·28 citations

Affiliations

first authorsco-authorsvia INSPIRE