Litcius/Paper detail

Detailed examination of astrophysical constraints on the symmetry energy and the neutron skin of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Pb</mml:mi><mml:mprescripts/><mml:none/><mml:mn>208</mml:mn></mml:mmultiscripts></mml:math> with minimal modeling assumptions

R. C. Essick, Philippe Landry, A. Schwenk, Ingo Tews

2021Physical review. C90 citationsDOIOpen Access PDF

Abstract

The symmetry energy and its density dependence are pivotal for many nuclear physics and astrophysics applications, as they determine properties ranging from the neutron-skin thickness of nuclei to the crust thickness and the radius of neutron stars. Recently, PREX-II reported a value of $0.283\ifmmode\pm\else\textpm\fi{}0.071$ fm for the neutron-skin thickness of $^{208}\mathrm{Pb}$, ${R}_{\mathrm{skin}}^{^{208}\mathrm{Pb}}$, implying a symmetry-energy slope parameter $L$ of $106\ifmmode\pm\else\textpm\fi{}37$ MeV, larger than most ranges obtained from microscopic calculations and other nuclear experiments. We use a nonparametric equation of state representation based on Gaussian processes to constrain the symmetry energy ${S}_{0}$, $L$, and ${R}_{\mathrm{skin}}^{^{208}\mathrm{Pb}}$ directly from observations of neutron stars with minimal modeling assumptions. The resulting astrophysical constraints from heavy pulsar masses, LIGO/Virgo, and NICER favor smaller values of the neutron skin and $L$, as well as negative symmetry incompressibilities. Combining astrophysical data with chiral effective field theory ($\ensuremath{\chi}\mathrm{EFT}$) and PREX-II constraints yields ${S}_{0}=33.{0}_{\ensuremath{-}1.8}^{+2.0}$ MeV, $L={53}_{\ensuremath{-}15}^{+14}$ MeV, and ${R}_{\mathrm{skin}}^{^{208}\mathrm{Pb}}=0.{17}_{\ensuremath{-}0.04}^{+0.04}$ fm. We also examine the consistency of several individual $\ensuremath{\chi}\mathrm{EFT}$ calculations with astrophysical observations and terrestrial experiments. We find that there is only mild tension between $\ensuremath{\chi}\mathrm{EFT}$, astrophysical data, and PREX-II's ${R}_{\mathrm{skin}}^{^{208}\mathrm{Pb}}$ measurement ($p$ value $=12.3%$) and that there is excellent agreement between $\ensuremath{\chi}\mathrm{EFT}$, astrophysical data, and other nuclear experiments.

Topics & Concepts

NeutronPhysicsComputer scienceNuclear physicsPulsars and Gravitational Waves ResearchNuclear physics research studiesCosmology and Gravitation Theories