Nuclear pasta (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Nuclear pasta" in English language version.

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aps.org

link.aps.org

journals.aps.org

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.

arxiv.org

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.
  • Pons, José A.; Viganò, Daniele; Rea, Nanda (2013). "Too much "pasta" for pulsars to spin down". Nature Physics. 9 (7): 431–434. arXiv:1304.6546. Bibcode:2013NatPh...9..431P. doi:10.1038/nphys2640. S2CID 119253979.
  • Schneider, A. S.; Horowitz, C. J.; Hughto, J.; Berry, D. K. (2013-12-20). "Nuclear Pasta Formation". Physical Review C. 88 (6): 065807. arXiv:1307.1678. Bibcode:2013PhRvC..88f5807S. doi:10.1103/PhysRevC.88.065807. ISSN 0556-2813.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Yakovlev, D. G. (2015). "Electron transport through nuclear pasta in magnetized neutron stars". Monthly Notices of the Royal Astronomical Society. 453 (1): 581–590. arXiv:1508.02603. Bibcode:2015MNRAS.453..581Y. doi:10.1093/mnras/stv1642.

books.google.com

doi.org

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.
  • Pons, José A.; Viganò, Daniele; Rea, Nanda (2013). "Too much "pasta" for pulsars to spin down". Nature Physics. 9 (7): 431–434. arXiv:1304.6546. Bibcode:2013NatPh...9..431P. doi:10.1038/nphys2640. S2CID 119253979.
  • Beskin, Vasilii S. (1999). "Radio pulsars". Physics-Uspekhi. 42 (11): 1173–1174. Bibcode:1999PhyU...42.1071B. doi:10.1070/pu1999v042n11ABEH000665. S2CID 250831196.
  • Schneider, A. S.; Horowitz, C. J.; Hughto, J.; Berry, D. K. (2013-12-20). "Nuclear Pasta Formation". Physical Review C. 88 (6): 065807. arXiv:1307.1678. Bibcode:2013PhRvC..88f5807S. doi:10.1103/PhysRevC.88.065807. ISSN 0556-2813.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Yakovlev, D. G. (2015). "Electron transport through nuclear pasta in magnetized neutron stars". Monthly Notices of the Royal Astronomical Society. 453 (1): 581–590. arXiv:1508.02603. Bibcode:2015MNRAS.453..581Y. doi:10.1093/mnras/stv1642.

harvard.edu

ui.adsabs.harvard.edu

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.
  • Pons, José A.; Viganò, Daniele; Rea, Nanda (2013). "Too much "pasta" for pulsars to spin down". Nature Physics. 9 (7): 431–434. arXiv:1304.6546. Bibcode:2013NatPh...9..431P. doi:10.1038/nphys2640. S2CID 119253979.
  • Beskin, Vasilii S. (1999). "Radio pulsars". Physics-Uspekhi. 42 (11): 1173–1174. Bibcode:1999PhyU...42.1071B. doi:10.1070/pu1999v042n11ABEH000665. S2CID 250831196.
  • Schneider, A. S.; Horowitz, C. J.; Hughto, J.; Berry, D. K. (2013-12-20). "Nuclear Pasta Formation". Physical Review C. 88 (6): 065807. arXiv:1307.1678. Bibcode:2013PhRvC..88f5807S. doi:10.1103/PhysRevC.88.065807. ISSN 0556-2813.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Yakovlev, D. G. (2015). "Electron transport through nuclear pasta in magnetized neutron stars". Monthly Notices of the Royal Astronomical Society. 453 (1): 581–590. arXiv:1508.02603. Bibcode:2015MNRAS.453..581Y. doi:10.1093/mnras/stv1642.

indiana.edu

racinfo.indiana.edu

nih.gov

pubmed.ncbi.nlm.nih.gov

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.

semanticscholar.org

api.semanticscholar.org

  • Caplan, M. E.; Schneider, A. S.; Horowitz, C. J. (24 September 2018). "Elasticity of Nuclear Pasta". Physical Review Letters. 121 (13): 132701. arXiv:1807.02557. Bibcode:2018PhRvL.121m2701C. doi:10.1103/PhysRevLett.121.132701. PMID 30312063. S2CID 206317364. Retrieved 26 August 2021.
  • Pons, José A.; Viganò, Daniele; Rea, Nanda (2013). "Too much "pasta" for pulsars to spin down". Nature Physics. 9 (7): 431–434. arXiv:1304.6546. Bibcode:2013NatPh...9..431P. doi:10.1038/nphys2640. S2CID 119253979.
  • Beskin, Vasilii S. (1999). "Radio pulsars". Physics-Uspekhi. 42 (11): 1173–1174. Bibcode:1999PhyU...42.1071B. doi:10.1070/pu1999v042n11ABEH000665. S2CID 250831196.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.
  • Kycia, Radosław A.; Kubis, Sebastian; Wójcik, Włodzimierz (2017-08-14). "Topological analysis of nuclear pasta phases". Physical Review C. 96 (2): 025803. arXiv:1709.07521. Bibcode:2017PhRvC..96b5803K. doi:10.1103/PhysRevC.96.025803. ISSN 2469-9985. S2CID 119352018.

web.archive.org

worldcat.org