Collective excitations of a quantized vortex in P23 superfluids in neutron stars

Chandrasekhar Chatterjee, Mareike Haberichter, and Muneto Nitta
Phys. Rev. C 96, 055807 – Published 21 November 2017

Abstract

We discuss collective excitations (both fundamental and solitonic excitations) of quantized superfluid vortices in neutron P23 superfluids, which likely exist in high density neutron matter such as neutron stars. Besides the well-known Kelvin modes (translational zero modes), we find a gapful mode whose low-energy description takes the simple form of a double sine-Gordon model. The associated kink solution and its effects on spontaneous magnetization inside the vortex core are analyzed in detail.

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  • Received 11 January 2017
  • Revised 29 July 2017

DOI:https://doi.org/10.1103/PhysRevC.96.055807

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Chandrasekhar Chatterjee1,*, Mareike Haberichter1,2,3,†, and Muneto Nitta1,‡

  • 1Department of Physics, and Research and Education Center for Natural Sciences, Keio University, Hiyoshi 4-1-1, Yokohama, Kanagawa 223-8521, Japan
  • 2Institut für Physik, Universität Oldenburg, Postfach 2503, D-26111 Oldenburg, Germany
  • 3Department of Mathematics and Statistics, University of Massachusetts, Amherst, Massachusetts 01003-4515, USA

  • *chandra@phys-h.keio.ac.jp
  • mareike@math.umass.edu
  • nitta@phys-h.keio.ac.jp

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Issue

Vol. 96, Iss. 5 — November 2017

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