Kinematic Parameters in the Dimensionally Reduced Witten Bubble Spacetime

Details Kinematic Parameters in the Dimensionally Reduced Witten Bubble Spacetime Kinematic Parameters in the Dimensionally Reduced Witten Bubble Spacetime

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1115..129c&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP Conference Proceedings, Volume

Computer Science

Quantum Gravity, Thermodynamics, Thermodynamic Processes, Conduction, Convection, Equations Of State

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 ρH = 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 our nongeodesic congruence of particles worldlines.

Affiliated with

Also associated with

No associations

Rating

Kinematic Parameters in the Dimensionally Reduced Witten Bubble 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 Dimensionally Reduced Witten Bubble Spacetime, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematic Parameters in the Dimensionally Reduced Witten Bubble Spacetime will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1861012