PaperPanorama

Nuclear Theory·nucl-th

Monday·February 22, 2016

9 papers7 primary·2 cross-listed

  1. 08

    Precision Electron-Beam Polarimetry using Compton Scattering at 1 GeV

    A. Narayan · D. Jones · J. C. Cornejo · M. M. Dalton · W. Deconinck · D. Dutta · D. Gaskell · J. W. Martin · K.D. Paschke · V. Tvaskis · A. Asaturyan · J. Benesch and 24 other authors

    We report on the highest precision yet achieved in the measurement of the polarization of a low energy, (1 GeV), electron beam, accomplished using a new polarimeter based on electron-photon scattering, in Hall~C at Jefferson Lab. A number of technical innovations were necessary, including a novel method for precise control of the laser polarization in a cavity and a novel diamond micro-strip detector which was able to capture most of the spectrum of scattered electrons. The data analysis technique exploited track finding, the high granularity of the detector and its large acceptance. The polarization of the A, ~GeV electron beam was measured with a statistical precision of ~1\% per hour and a systematic uncertainty of 0.59\%. This exceeds the level of precision required by the \qweak experiment, a measurement of the vector weak charge of the proton. Proposed future low-energy experiments require polarization uncertainty ~0.4\%, and this result represents an important demonstration of that possibility. This measurement is also the first use of diamond detectors for particle tracking in an experiment.

    nucl-exhep-phnucl-thphysics.acc-ph+1PRX(2016)·47 citations
  2. 09

    Numerical models for stationary superfluid neutron stars in general relativity with realistic equations of state

    Aurélien Sourie · Micaela Oertel · Jérôme Novak

    We present a numerical model for uniformly rotating superfluid neutron stars, for the first time with realistic microphysics including entrainment, in a fully general relativistic framework. We compute stationary and axisymmetric configurations of neutron stars composed of two fluids, namely superfluid neutrons and charged particles (protons and electrons), rotating with different rates around a common axis. Both fluids are coupled by entrainment, a non-dissipative interaction which in case of a non-vanishing relative velocity between the fluids, causes the fluid momenta being not aligned with the respective fluid velocities. We extend the formalism by Comer and Joynt (2003) in order to calculate the equation of state (EoS) and entrainment parameters for an arbitrary relative velocity. The resulting entrainment matrix fulfills all necessary sum rules and in the limit of small relative velocity our results agree with Fermi liquid theory ones, derived to lowest order in the velocity. This formalism is applied to two new nuclear equations of state which are implemented in the numerical model. We are able to obtain precise equilibrium configurations. Resulting density profiles and moments of inertia are discussed employing both EoSs, showing the impact of entrainment and the dependence on the EoS.

    astro-ph.HEastro-ph.SRgr-qcnucl-thPRD(2016)·26 citations

Affiliations

first authorsco-authorsvia INSPIRE