On a mechanism of magnetic field generation in pulsars

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1981 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics, volume 16, pages 417-422 (issn: 0571-7132, eissn: 1573-8191,

Copyright policy )

Authors: D. M. Sedrakyan; K. M. Shakhabasyan;

doi: 10.1007/bf01005525

On a mechanism of magnetic field generation in pulsars

- Summary
- Metrics

Abstract

Consideration is given to a two-component superfluid neutron-proton Fermi liquid in the npe phase of a neutron star. Equations are obtained for the thermal Green functions and the anomalous expectation values of the two-component Fermi liquid. The Green functions are used to obtain an expression for the superconducting proton current and an equation for the magnetic field within the star. It is shown that the rotation leads to the occurrence of proton vortex filaments at the positions of neutron vortex filaments. In addition, rotation leads to the occurrence of a weak homogeneous static magnetic field.

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	5
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average