PaperPanorama

Nuclear Theory·nucl-th

Friday·February 24, 2017

12 papers2 primary·10 cross-listed

  1. 01

    Electromagnetic characteristics of physical and lattice nuclei

    Johannes Kirscher🇺🇸 · Ehoud Pazy🇮🇱 · Jonathan Drachman🇮🇱 · Nir Barnea🇮🇱

    We analyze the quark-mass dependence of electromagnetic properties of two and three-nucleon states. To that end, we apply the pionless effective field theory to experimental data and numerical lattice calculations which simulate QCD at pion masses of 450~MeV and 806~MeV. At the physical pion mass, we postdict the magnetic moment of helium-3, nNM, and the magnetic polarizability of deuterium, fm. Magnetic polarizabilities of helium-3, fm, and the triton, fm, are predictions. Postdictions of the effective theory for the magnetic moments are found consistent with QCD simulations at 806~MeV pion mass while our EFT result fm was not extracted from the lattice. The deuteron would thus be relatively pliable compared to a three-nucleon state for which we postdict fm. At MeV, the magnetic moment of the triton is predicted, nNM, based on a conjecture of its binding energy, ~MeV. For all three pion masses, we compare the point-charge radii of the two and three-nucleon bound states. The sensitivity of the electromagnetic properties to the Coulomb interaction between protons is studied in anticipation of lattice calculations with dynamical QED.

    nucl-thhep-latPRC(2017)·28 citations
  2. 02

    Taming instability of magnetic field in chiral medium

    Kirill Tuchin🇺🇸

    Magnetic field is unstable in a medium with time-independent chiral conductivity. Owing to the chiral anomaly, the electromagnetic field and the medium exchange helicity which results in time-evolution of the chiral conductivity. Using the fastest growing momentum and helicity state of the vector potential as an ansatz, the time-evolution of the chiral conductivity and magnetic field is solved analytically. The solution for the hot and cold equations of state shows that the magnetic field does not develop an instability due to he helicity conservation. Moreover, it develops a peak only if a significant part of the \emph{initial} helicity is stored in the medium. The initial helicity determines the height and position of the peak.

    nucl-thhep-phhep-thNPA(2018)·17 citations

Affiliations

first authorsco-authorsvia INSPIRE