Pairing gaps in neutron stars

Xian-Rong Zhou, H.-J. Schulze, En-Guang Zhao, Feng Pan, and J. P. Draayer
Phys. Rev. C 70, 048802 – Published 28 October 2004

Abstract

Nucleonic S01 and PF23 pairing gaps in neutron stars are determined and their sensitivity to medium effects realized through nucleonic three-body forces, and the presence of hyperons is explored.

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  • Received 8 June 2004

DOI:https://doi.org/10.1103/PhysRevC.70.048802

©2004 American Physical Society

Authors & Affiliations

Xian-Rong Zhou1,2,3, H.-J. Schulze4, En-Guang Zhao5, Feng Pan1,2, and J. P. Draayer2

  • 1Department of Physics, Liaoning Normal University, Dalian 116029, China
  • 2Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA
  • 3Department of Physics, Tsinghua University, Beijing 100084, China
  • 4Dipartimento di Fisica, Università di Catania, Via Santa Sofia 64, I-95123 Catania, Italy
  • 5Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100080, China

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Issue

Vol. 70, Iss. 4 — October 2004

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