Equilibrium configuration of magnetar in general relativity

Details Equilibrium configuration of magnetar in general relativity Equilibrium configuration of magnetar in general relativity

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasb.conf..193i&link_type=abstract

"Pulsars, AXPs and SGRs observed with BeppoSAX and Other Observatories, Proceedings of the International Workshop held in Marsal

Other

Scientific paper

It is well known that basic equations for the axisymmetric stationary ideal magnetohydrodynamic (MHD) system are reduced to a single second-order, nonlinear partial differential equation, so called the Grad-Shafranov (GS) equation. However, the GS equation for the most general case, when the stress-energy tensor is not circular so that one cannot make the usual foliation of spacetime into two orthogonal families of two-surfaces, has not been given explicitly in the framework of the general relativity. We derive the GS equation for the noncircular (the most general) axisymmetric stationary spacetimes. Such a study is needed to solve the equilibrium configuration of relativistic stars with strong toroidal magnetic field or convection such as magnetars.

Affiliated with

Also associated with

No associations

Rating

Equilibrium configuration of magnetar in general relativity 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 Equilibrium configuration of magnetar in general relativity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Equilibrium configuration of magnetar in general relativity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885062