Gravitational Collapse of a Rotating Star ---Formulation I---

Details Gravitational Collapse of a Rotating Star ---Formulation I--- Gravitational Collapse of a Rotating Star ---Formulation I---

Jul 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972pthph..48...78t&link_type=abstract

Progress of Theoretical Physics, Vol. 48, No. 1, pp. 78-103

Physics

4

Scientific paper

First, a system of general relativistic hydrodynamical and gravitational field equations is generally formulated under Bondi-Sachs's coordinate condition, and then it is applied to an approximate description of dynamical motions of a slowly rotating axisymmetric star. Our approximation comes from putting attention on the quantities of the first and second orders of magnitude with respect to small angular velocity. Moreover, the deviation of event horizon appearing in the strong field from the Schwarzschild surface and the behavior of the asymptotically flat field are examined, and, in order to see the dragging of local inertial frame by the strong field of that star, equations of motion for that frame are also considered.

Affiliated with

Also associated with

No associations

Rating

Gravitational Collapse of a Rotating Star ---Formulation I--- 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 Collapse of a Rotating Star ---Formulation I---, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational Collapse of a Rotating Star ---Formulation I--- will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1647154