PaperPanorama

Nuclear Theory·nucl-th

Friday·November 12, 2021

6 papers4 primary·2 cross-listed

  1. 05

    Finite volume and magnetic field effects on the two-pion correlation function in relativistic heavy-ion collisions

    Alejandro Ayala🇲🇽 · Santiago Bernal-Langarica🇲🇽 · Cristian Villavicencio🇨🇱

    We study the combined effects of a finite volume and an external magnetic field on the charged two-pion correlation function. For these purposes, we consider a dilute system of pions where the finite volume effects are introduced computing the pion wave functions with rigid boundary conditions in a cylindrical geometry in the presence of a uniform and constant magnetic field. We find that for slow pions, namely, for the case where the average pair momentum is small, the correlation function shows a large distortion, as opposed to the case where the average pair momentum is large. For a finite density system, the intercept of the correlation function is reduced, signaling the increasing importance of the pion ground state contribution. An increasing strength of the magnetic field reduces the importance of the ground state and the intercept becomes closer to 2.

    hep-phnucl-thPRD(2022)·3 citations
  2. 06

    The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter

    Yannick Dengler🇩🇪 · Jürgen Schaffner-Bielich🇩🇪 · Laura Tolos🇪🇸

    We study the mass-radius relation and the second Love number of compact objects made of ordinary matter and non-selfannihilating fermionic dark matter for a wide range of dark matter particle masses, and for the cases of weakly and strongly interacting dark matter. We obtain stable configurations of compact objects with radii smaller than 10 km and masses similar to Earth- or Jupiter-like stellar objects. In certain parameter ranges we find second Love numbers which are markedly different compared to those expected for neutron stars without dark matter. Thus, by obtaining the compactness of these compact objects and measuring their tidal deformability from gravitational wave detections from binary neutron star mergers, the extracted value of second Love number would allow to determine the existence of dark matter inside neutron stars irrespective of the equation of state of ordinary matter.

    astro-ph.HEnucl-thPRD(2022)·77 citations

Affiliations

first authorsco-authorsvia INSPIRE