Statistics – Computation
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sssmp..28..422w&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 28, April 1985, p
Statistics
Computation
3
Magnetic Moments, Neutron Stars, Stellar Gravitation, Stellar Magnetic Fields, Computational Astrophysics, Einstein Equations, Magnetic Dipoles, Maxwell Equation, Space-Time Functions
Scientific paper
In this paper, taking the magnetic R-N metric as a space-time background, a static magnetic field in this curved space-time is derived. Substituting the derived static magnetic field as a source of gravitational field into the right-hand side of Einstein-Maxwell equation, the Einstein-Maxwell equation is solved with a step-by-step approximation method by the first degree, and a new metric is derived. This metric describes the external field of a neutron star with magnetic charge and magnetic dipole moment. A discussion is presented of various kinds of celestial bodies with a characteristic parameter that satisfies chi less than 1, chi = 1 and chi greater than 1, and some properties which some electric charged celestial bodies do not possess are obtained.
Peng Qian
Wang Yadong
No associations
LandOfFree
Gravitational properties of the neutron star with magnetic charge and magnetic moment does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Gravitational properties of the neutron star with magnetic charge and magnetic moment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational properties of the neutron star with magnetic charge and magnetic moment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1291084