Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model

Details Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model

2005-03-04

arxiv.org/abs/gr-qc/0503015v1

Int.J.Mod.Phys. A20 (2005) 7547-7566

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex file, 13 figures, accepted for publication in Inter. J. Mod. Phys. A

Scientific paper

10.1142/S0217751X05022391

Employing the Quark Mass Denisity- and temperature- dependent model and the Hartle's method, We have studied the slowly rotating strange star with uniform angular velocity. The mass-radius relation, the moment of inertia and the frame dragging for different frequencies are given. We found that we cannot use the strange star to solve the challenges of Stella and Vietri for the horizontal branch oscillations and the moment of inertia $I_{45}/(M/M_ s)>2.3$. Furthermore, we extended the Hartle's method to study the differential rotating strange star and found that the differential rotation is an effective way to get massive strange star.

Affiliated with

Also associated with

No associations

Rating

Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model 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 Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Slowly rotating proto strange stars in Quark mass density- and temperature- dependent model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-200912