A possible decrease in the equilibrium radius of a neutron star due to the effect of a superstrong magnetic field (Q1762254)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: A possible decrease in the equilibrium radius of a neutron star due to the effect of a superstrong magnetic field |
scientific article; zbMATH DE number 6110126
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | A possible decrease in the equilibrium radius of a neutron star due to the effect of a superstrong magnetic field |
scientific article; zbMATH DE number 6110126 |
Statements
A possible decrease in the equilibrium radius of a neutron star due to the effect of a superstrong magnetic field (English)
0 references
23 November 2012
0 references
The author derived and discusses the necessary condition for achieving an equilibrium state with neutron \(\beta\)-decay in a degenerate magnetized electron gas under conditions of massive neutron stars. It has been shown that the presence of a super-strong magnetic field significantly reduces the radius of the equilibrium neutron star.
0 references
neutron stars
0 references
super-strong magnetic field
0 references
degenerate electron gas
0 references
equilibrium stellar radius
0 references
