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On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field
Author
Source
Advances in High Energy Physics
Issue
Vol. 2012, Issue 2012 (31 Dec. 2012), pp.1-6, 6 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2012-02-26
Country of Publication
Egypt
No. of Pages
6
Main Subjects
Abstract EN
Necessary condition for β-decay suppression of a neutron in degenerate magnetized electron gas is formulated.
Based on this, it is shown that, in superstrong magnetic field, equilibrium radius of a neutron star is approximately several times smaller than without the field influence.
Therefore, we can make a prediction that in short-period pulsars, such fields can be observed.
In fact, possible existence of new class of stellar objects is noted, the objects with superstrong magnetic field and supersmall radius about 1 km which we named minimagnetars.
They can be detected by gravitational red shift of their radiation.
American Psychological Association (APA)
Skobelev, Vladimir V.. 2012. On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field. Advances in High Energy Physics،Vol. 2012, no. 2012, pp.1-6.
https://search.emarefa.net/detail/BIM-462360
Modern Language Association (MLA)
Skobelev, Vladimir V.. On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field. Advances in High Energy Physics No. 2012 (2012), pp.1-6.
https://search.emarefa.net/detail/BIM-462360
American Medical Association (AMA)
Skobelev, Vladimir V.. On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field. Advances in High Energy Physics. 2012. Vol. 2012, no. 2012, pp.1-6.
https://search.emarefa.net/detail/BIM-462360
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-462360