Uspekhi Fizicheskikh Nauk
RUS  ENG    JOURNALS   PEOPLE   ORGANISATIONS   CONFERENCES   SEMINARS   VIDEO LIBRARY   PACKAGE AMSBIB  
General information
Latest issue
Forthcoming papers
Archive
Impact factor
Guidelines for authors
Submit a manuscript

Search papers
Search references

RSS
Latest issue
Current issues
Archive issues
What is RSS


UFN:
Year:
Volume:
Issue:
Page:
Find




Personal entry:
Login:
Password:
Save password
Enter
Forgotten password?
Register

Uspekhi Fizicheskikh Nauk, 1991, Volume 161, Number 7, Pages 3–40
DOI: https://doi.org/10.3367/UFNr.0161.199107a.0003 (Mi ufn7416) 		 
This article is cited in 28 scientific papers (total in 28 papers)

REVIEWS OF TOPICAL PROBLEMS

Superfluidity and the magnetic field of pulsars

D. M. Sedrakianab, K. M. Shahabasyanab

a Byurakan Astrophysical Observatory, National Academy of Sciences of Armenia
b Yerevan State University
Full-text PDF (641 kB) Citations (28)
DOI: https://doi.org/10.3367/UFNr.0161.199107a.0003
Abstract: The current state of the theory of superfluidity in pulsars is presented. The superfluidity of hadronic matter in neutron stars is considered. It is shown that strong interaction between the neutron and proton condensates leads to a drag current of superconducting protons and to the generation of a strong time-independent magnetic field (B = 10$^{12}$ G) parallel to the axis of rotation. The strength of this field depends on the microscopic parameters of the superfluid hadrons. Models explaining the origin of glitches and postglitch relaxation are discussed. The coupling time between the neutron superfluid and the rigid crust of the neutron star is calculated.
Received: October 10, 1990
Revised: January 21, 1991
English version:
Physics–Uspekhi, 1991, Volume 34, Issue 7, Pages 555–571
DOI: https://doi.org/10.1070/PU1991v034n07ABEH002446
Document Type: Article
UDC: 532.132 + 524.354.6
PACS: 97.60.Gb, 97.60.Jd, 26.60.+c, 97.10.Ld, 97.10.Cv
Language: Russian
Citation: D. M. Sedrakian, K. M. Shahabasyan, “Superfluidity and the magnetic field of pulsars”, UFN, 161:7 (1991), 3–40; Phys. Usp., 34:7 (1991), 555–571
Citation in format AMSBIB
\Bibitem{SedSha91}
\by D.~M.~Sedrakian, K.~M.~Shahabasyan
\paper Superfluidity and the magnetic field of pulsars
\jour UFN
\yr 1991
\vol 161
\issue 7
\pages 3--40
\mathnet{http://mi.mathnet.ru/ufn7416}
\crossref{https://doi.org/10.3367/UFNr.0161.199107a.0003}
\transl
\jour Phys. Usp.
\yr 1991
\vol 34
\issue 7
\pages 555--571
\crossref{https://doi.org/10.1070/PU1991v034n07ABEH002446}
Linking options:
  • https://www.mathnet.ru/eng/ufn7416
  • https://www.mathnet.ru/eng/ufn/v161/i7/p3
    • This publication is cited in the following 28 articles:
    Citing articles in Google Scholar: Russian citations, English citations
    Related articles in Google Scholar: Russian articles, English articles
    		Успехи физических наук Physics-Uspekhi
    Statistics & downloads:
    Abstract page:42
    Full-text PDF :16
     
      Contact us:
    		  Terms of Use  Registration to the website  Logotypes © Steklov Mathematical Institute RAS, 2024