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Title: Nuclear pasta in hot dense matter and its implications for neutrino scattering

Abstract

The abundance of large clusters of nucleons in neutron-rich matter at subnuclear density is found to be greatly reduced by finite-temperature effects when matter is close to β equilibrium, compared to the case where the electron fraction is fixed at Y e > 0.1 , as often considered in the literature. Large nuclei and exotic nonspherical nuclear configurations called pasta, favored in the vicinity of the transition to uniform matter at T = 0 , dissolve at a relatively low temperature T u as protons leak out of nuclei and pasta. For matter at β-equilibrium with a negligible neutrino chemical potential we find that T$$β\atop{u}$$ ≃ 4 ± 1 MeV for realistic equations of state. This is lower than the maximum temperature T$$β\atop{max}$$ ≃ 9 ± 1 MeV at which nuclei can coexist with a gas of nucleons and can be explained by a change in the nature of the transition to uniform matter called retrograde condensation. An important new finding is that coherent neutrino scattering from nuclei and pasta makes a modest contribution to the opacity under the conditions encountered in supernovas and neutron star mergers. This is because large nuclear clusters dissolve at most relevant temperatures, and at lower temperatures, when clusters are present, Coulomb correlations between them suppress coherent neutrino scattering off individual clusters. Lastly, implications for neutrino signals from galactic supernovas are briefly discussed.

Authors:
 [1];  [2];  [3];  [4]
  1. Univ. of Washington, Seattle, WA (United States). Inst. for Nuclear Theory; Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  2. Univ. of Washington, Seattle, WA (United States). Inst. for Nuclear Theory; Univ. de Lyon, Villeurbanne (France); Univ. Claude Bernard Lyon, Villeurbanne (France). Inst. de Physique Nucleaire de Lyon
  3. Michigan State Univ., East Lansing, MI (United States). National Superconducting Lab. and Dept. of Physics and Astronomy
  4. Univ. of Washington, Seattle, WA (United States). Inst. for Nuclear Theory
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE Office of Science (SC). Nuclear Physics (NP) (SC-26); USDOE
OSTI Identifier:
1438361
Alternate Identifier(s):
OSTI ID: 1433276
Report Number(s):
LA-UR-17-29841
Journal ID: ISSN 2469-9985; PRVCAN
Grant/Contract Number:
AC52-06NA25396; FG02-00ER41132; SC0017955
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Physical Review C
Additional Journal Information:
Journal Volume: 97; Journal Issue: 4; Journal ID: ISSN 2469-9985
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; Atomic and Nuclear Physics

Citation Formats

Roggero, Alessandro, Margueron, Jerome, Roberts, Luke F., and Reddy, Sanjay. Nuclear pasta in hot dense matter and its implications for neutrino scattering. United States: N. p., 2018. Web. doi:10.1103/PhysRevC.97.045804.
Roggero, Alessandro, Margueron, Jerome, Roberts, Luke F., & Reddy, Sanjay. Nuclear pasta in hot dense matter and its implications for neutrino scattering. United States. doi:10.1103/PhysRevC.97.045804.
Roggero, Alessandro, Margueron, Jerome, Roberts, Luke F., and Reddy, Sanjay. Mon . "Nuclear pasta in hot dense matter and its implications for neutrino scattering". United States. doi:10.1103/PhysRevC.97.045804.
@article{osti_1438361,
title = {Nuclear pasta in hot dense matter and its implications for neutrino scattering},
author = {Roggero, Alessandro and Margueron, Jerome and Roberts, Luke F. and Reddy, Sanjay},
abstractNote = {The abundance of large clusters of nucleons in neutron-rich matter at subnuclear density is found to be greatly reduced by finite-temperature effects when matter is close to β equilibrium, compared to the case where the electron fraction is fixed at Ye > 0.1 , as often considered in the literature. Large nuclei and exotic nonspherical nuclear configurations called pasta, favored in the vicinity of the transition to uniform matter at T = 0 , dissolve at a relatively low temperature Tu as protons leak out of nuclei and pasta. For matter at β-equilibrium with a negligible neutrino chemical potential we find that T$β\atop{u}$ ≃ 4 ± 1 MeV for realistic equations of state. This is lower than the maximum temperature T$β\atop{max}$ ≃ 9 ± 1 MeV at which nuclei can coexist with a gas of nucleons and can be explained by a change in the nature of the transition to uniform matter called retrograde condensation. An important new finding is that coherent neutrino scattering from nuclei and pasta makes a modest contribution to the opacity under the conditions encountered in supernovas and neutron star mergers. This is because large nuclear clusters dissolve at most relevant temperatures, and at lower temperatures, when clusters are present, Coulomb correlations between them suppress coherent neutrino scattering off individual clusters. Lastly, implications for neutrino signals from galactic supernovas are briefly discussed.},
doi = {10.1103/PhysRevC.97.045804},
journal = {Physical Review C},
number = 4,
volume = 97,
place = {United States},
year = {Mon Apr 16 00:00:00 EDT 2018},
month = {Mon Apr 16 00:00:00 EDT 2018}
}

Journal Article:
Free Publicly Available Full Text
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