PaperPanorama

Nuclear Theory·nucl-th

Monday·November 20, 2017

5 papers2 primary·3 cross-listed

  1. 01

    Partial restoration of chiral symmetry in cold nuclear matter: the -meson case

    J.J. Cobos-Martínez🇲🇽 · K Tsushima🇧🇷 · G Krein🇧🇷 · A W Thomas🇦🇺

    The work presented at this workshop is divided into two parts. In the first part, the mass and decay width of the -meson in cold nuclear matter are computed in an effective Lagrangian approach. The medium dependence of these properties are obtained by evaluating kaon-antikaon loop contributions to the -meson self-energy, employing medium-modified kaon masses calculated using the quark-meson coupling model. The loop integral is regularized with a dipole form factor, and the sensitivity of the results to the choice of cutoff mass in the form factor is investigated. At normal nuclear matter density, we find a downward shift of the mass by a few percent, while the decay width is enhanced by an order of magnitude. Our results support the literature which suggest that one should observe a small downward mass shift and a large broadening of the decay width. In the second part, we present -meson--nucleus bound state energies and absorption widths for four selected nuclei, calculated by solving the Klein-Gordon equation with complex optical potentials. The attractive potential for the -meson in the nuclear medium originates from the in-medium enhanced KK loop in the -meson selfenergy. The results suggest that the -meson should form bound states with all the nuclei considered. However, the identification of the signal for these predicted bound states will need careful investigation because of their sizable absorption widths.

    nucl-thhep-phnucl-exJ.Phys.Conf.Ser.(2017)·5 citations
  2. 02

    Neutron skins and neutron stars in the multi-messenger era

    F. J. Fattoyev · J. Piekarewicz · C. J. Horowitz

    The historical first detection of a binary neutron star merger by the LIGO-Virgo collaboration [B. P. Abbott et al. Phys. Rev. Lett. 119, 161101 (2017)] is providing fundamental new insights into the astrophysical site for the -process and on the nature of dense matter. A set of realistic models of the equation of state (EOS) that yield an accurate description of the properties of finite nuclei, support neutron stars of two solar masses, and provide a Lorentz covariant extrapolation to dense matter are used to confront its predictions against tidal polarizabilities extracted from the gravitational-wave data. Given the sensitivity of the gravitational-wave signal to the underlying EOS, limits on the tidal polarizability inferred from the observation translate into constraints on the neutron-star radius. Based on these constraints, models that predict a stiff symmetry energy, and thus large stellar radii, can be ruled out. Indeed, we deduce an upper limit on the radius of a neutron star of . Given the sensitivity of the neutron-skin thickness of Pb to the symmetry energy, albeit at a lower density, we infer a corresponding upper limit of about . However, if the upcoming PREX-II experiment measures a significantly thicker skin, this may be evidence of a softening of the symmetry energy at high densities---likely indicative of a phase transition in the interior of neutron stars.

    nucl-thastro-ph.HEnucl-exPRL(2018)·476 citations
  3. 03

    D-instantons in Real Time Dynamics

    Si-wen Li🇨🇳 · Shu Lin🇨🇳

    Instanton is known to exist in Euclidean spacetime only. Their role in real time dynamics is usually understood as tunneling effect by Wick rotation. We illustrate other effects of instanton in holography by investigating 5d effective gravity theory of the black D3-brane-D-instanton system. The supergravity description of the D3-brane-D-instanton system is dual to the super Yang-Mills theory with topological excitations of the vacuum. We obtain Euclidean correlators in the presence of instantons by analyzing of the fluctuations of the bulk fields in the 5d effective theory. Furthermore, analytic continuation of Euclidean correlators leads to retarded correlators, which characterize real time dynamics. We find interestingly real time fluctuations of topological charge can destroy instantons and the lifetime of instanton is set by temperature. This implies instanton contribution to "real time dynamics" is suppressed at high temperature, which is analogous to classic field theory results that instanton contribution to "thermodynamics" is suppressed at high temperature.

    hep-thhep-phnucl-thPRD(2018)·8 citations
  4. 04

    Scattering of charmed baryons on nucleons

    J. Haidenbauer🇩🇪 · G. Krein🇧🇷

    Chiral effective field theory is utilized for extrapolating results on the interaction, obtained in lattice QCD at unphysical (large) quark masses, to the physical point. The pion-mass dependence of the components that constitute the potential up to next-to-leading order (pion-exchange diagrams and four-baryon contact terms) is fixed by information from lattice QCD simulations. No recourse to SU(3) or SU(4) flavor symmetry is made. It is found that the results of the HAL QCD Collaboration for quark masses corresponding to -- MeV imply a moderately attractive interaction at MeV with scattering lengths of fm for the as well as the partial waves. For such an interaction the existence of a charmed counterpart of the hypertriton is unlikely but four- and/or five-baryons systems with a baryon could be indeed bound.

    hep-phnucl-thEPJA(2018)·33 citations
  5. 05

    Reaction rates and transport in neutron stars

    Andreas Schmitt🇬🇧 · Peter Shternin🇷🇺

    Understanding signals from neutron stars requires knowledge about the transport inside the star. We review the transport properties and the underlying reaction rates of dense hadronic and quark matter in the crust and the core of neutron stars and point out open problems and future directions.

    astro-ph.HEhep-phnucl-thAstrophys.Space Sci.Libr.(2018)·94 citations

Affiliations

first authorsco-authorsvia INSPIRE