PaperPanorama

Nuclear Theory·nucl-th

Wednesday·January 9, 2019

4 papers2 primary·2 cross-listed

  1. 03

    General structure of the neutral meson self-energy and its spectral properties in a hot and dense magnetized medium

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

    The one loop self energy of the neutral meson is obtained for the effective and interaction at finite temperature and density in the presence of a constant background magnetic field of arbitrary strength. In our approach, the eB-dependent vacuum part of the self energy is extracted by means of dimensional regularization where the ultraviolet divergences corresponding to the pure vacuum self energy manifest as the pole singularities of gamma as well as Hurwitz zeta functions. This improved regularization procedure consistently reproduces the expected results in the vanishing magnetic field limit and can be used quite generally in other self energy calculations dealing with arbitrary magnetic field strength. In presence of the external magnetic field, the general Lorentz structure for the in-medium vector boson self energy is derived which can also be implemented in case of the gauge bosons such as photons and gluons. It has been shown that with vanishing perpendicular momentum of the external particle, essentially two form factors are sufficient to describe the self energy completely. Consequently, two distinct modes are observed in the study of the effective mass, dispersion relations and the spectral function of where one of the modes possesses two fold degeneracy. For large baryonic chemical potential, it is observed that the critical magnetic field required to block the decay channel increases significantly with temperature. However, in case of smaller values reaching down to vanishing chemical potential, the critical field follows the opposite trend.

    hep-phnucl-thPRD(2019)·28 citations
  2. 04

    Solar neutrino problem as evidence of new interaction

    L.M. Slad🇷🇺

    A new concept is proposed to solve the solar neutrino problem, that is based on a hypothesis about the existence of a new interaction of electron neutrinos with nucleons mediated by massless pseudoscalar bosons. At every collision of a neutrino with nucleons of the Sun, its handedness changes from left to right and vice versa, and its energy decreases. The postulated hypothesis, having only one free parameter, provides a good agreement between the calculated and experimental characteristics of all five observed processes with solar neutrinos.

    hep-phastro-ph.SRnucl-thJ.Exp.Theor.Phys.(2020)·9 citations

Affiliations

first authorsco-authorsvia INSPIRE