Kinematic parameters in the spherical Rindler frame spacetime

Details Kinematic parameters in the spherical Rindler frame spacetime Kinematic parameters in the spherical Rindler frame spacetime

2008-04-23

arxiv.org/abs/0804.3754v1

Physics

High Energy Physics

High Energy Physics - Theory

5 pages, no figures

Scientific paper

The kinematical quantities derived from the velocity field of a nongeodesic congruence are studied. We found the shear tensor components are finite in time but diverge at the event horizon of the spacetime located at $\rho = 0$, while the vorticity is constant. The surface gravity on the horizon is just the proper acceleration of the uniformly expanding distribution of observers, in spherical Rindler coordinates. The Raychaudhuri equation is fulfilled for the congruence of particles worldlines.

Affiliated with

Also associated with

No associations

Rating

Kinematic parameters in the spherical Rindler frame spacetime 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 Kinematic parameters in the spherical Rindler frame spacetime, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematic parameters in the spherical Rindler frame spacetime will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-105264