External magnetic field of a static spherically symmetric star in Rosen's bimetric theory of gravitation

Journal Article · Sat May 15 00:00:00 EDT 1982 · Phys. Rev. D; (United States)

DOI:https://doi.org/10.1103/PhysRevD.25.2701· OSTI ID:5385418

Prasanna, A R

In this brief paper we present a complete exact solution for the external magnetic field (dipolar at infinity) of a static magnetic star on the spherically symmetric background metric solution of Rosen's bimetric theory of gravity. Unlike in general relativity the field is well behaved throughout the manifold except at r = 0, and thus allows one to consider the field for stars collapsed beyond 2m.

• Research Organization: Physical Research Laboratory, Navrangpura, Ahmedabad, India
• OSTI ID: 5385418
• Journal Information: Phys. Rev. D; (United States), Vol. 25:10
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
MAGNETIC STARS
MAGNETIC FIELDS
GENERAL RELATIVITY THEORY
MAXWELL EQUATIONS
METRICS
SPACE-TIME
DIFFERENTIAL EQUATIONS
EQUATIONS
FIELD THEORIES
PARTIAL DIFFERENTIAL EQUATIONS
STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources
657003 - Theoretical & Mathematical Physics- Relativity & Gravitation