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Title: Hyperons and quarks in proto-neutron stars

Authors:
 [1];  [2];  [1];  [1];  [3];  [4]
  1. Department of Physics, Kent State University, Kent, OH 44243, USA
  2. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA
  3. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA, Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
  4. Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA, Department of Physics (Astro), University of Oxford, Keble Road, OX1 3RH Oxford, UK
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1513037
Grant/Contract Number:  
SC0018232
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 486 Journal Issue: 4; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United Kingdom
Language:
English

Citation Formats

Roark, J., Du, X., Constantinou, C., Dexheimer, V., Steiner, A. W., and Stone, J. R. Hyperons and quarks in proto-neutron stars. United Kingdom: N. p., 2019. Web. doi:10.1093/mnras/stz1240.
Roark, J., Du, X., Constantinou, C., Dexheimer, V., Steiner, A. W., & Stone, J. R. Hyperons and quarks in proto-neutron stars. United Kingdom. doi:10.1093/mnras/stz1240.
Roark, J., Du, X., Constantinou, C., Dexheimer, V., Steiner, A. W., and Stone, J. R. Sat . "Hyperons and quarks in proto-neutron stars". United Kingdom. doi:10.1093/mnras/stz1240.
@article{osti_1513037,
title = {Hyperons and quarks in proto-neutron stars},
author = {Roark, J. and Du, X. and Constantinou, C. and Dexheimer, V. and Steiner, A. W. and Stone, J. R.},
abstractNote = {},
doi = {10.1093/mnras/stz1240},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 486,
place = {United Kingdom},
year = {2019},
month = {5}
}

Journal Article:
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This content will become publicly available on May 4, 2020
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