Literature DB >> 16058160

Superfluid turbulence in neutron stars.

G Greenstein1.   

Abstract

The neutron superfluid in most neutron stars should be in a highly turbulent state. If so, this turbulence drastically alters its rotational properties.

Year:  1970        PMID： 16058160     DOI： 10.1038/227791a0

Source DB:  PubMed          Journal:  Nature        ISSN： 0028-0836            Impact factor:   49.962


  2 in total

1.  Superdiffusion of quantized vortices uncovering scaling laws in quantum turbulence.

Authors:  Yuan Tang; Shiran Bao; Wei Guo
Journal:  Proc Natl Acad Sci U S A       Date:  2021-02-09       Impact factor: 11.205

Review 2.  Physics of Neutron Star Crusts.

Authors:  Nicolas Chamel; Pawel Haensel
Journal:  Living Rev Relativ       Date:  2008-12-12       Impact factor: 40.429
  2 in total

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