Abstract
We have applied the numerical method which was developed for Newtonian gravity to general relativistic, differentially rotating bodies including ring-like structures. A number of equilibrium structures are obtained for two different polytropic indices N=1/2 and N=3/2, because the various proposed equations of state for the nuclear density region fall into the range N=1/2 to 3/2 from the viewpoint of its softness. (author).
Komatsu, Hidemi;
[1]
Eriguchi, Yoshiharu;
[2]
Hachisu, Izumi
[3]
- Tokyo Univ. (Japan). Faculty of Science
- Tokyo Univ. (Japan). Dept. of Astronomy
- Kyoto Univ. (Japan). Dept. of Aeronautical Engineering
Citation Formats
Komatsu, Hidemi, Eriguchi, Yoshiharu, and Hachisu, Izumi.
Rapidly rotating general relativistic stars. Pt. 2. Differentially rotating polytropes.
United Kingdom: N. p.,
1989.
Web.
Komatsu, Hidemi, Eriguchi, Yoshiharu, & Hachisu, Izumi.
Rapidly rotating general relativistic stars. Pt. 2. Differentially rotating polytropes.
United Kingdom.
Komatsu, Hidemi, Eriguchi, Yoshiharu, and Hachisu, Izumi.
1989.
"Rapidly rotating general relativistic stars. Pt. 2. Differentially rotating polytropes."
United Kingdom.
@misc{etde_5464038,
title = {Rapidly rotating general relativistic stars. Pt. 2. Differentially rotating polytropes}
author = {Komatsu, Hidemi, Eriguchi, Yoshiharu, and Hachisu, Izumi}
abstractNote = {We have applied the numerical method which was developed for Newtonian gravity to general relativistic, differentially rotating bodies including ring-like structures. A number of equilibrium structures are obtained for two different polytropic indices N=1/2 and N=3/2, because the various proposed equations of state for the nuclear density region fall into the range N=1/2 to 3/2 from the viewpoint of its softness. (author).}
journal = []
volume = {239:1}
journal type = {AC}
place = {United Kingdom}
year = {1989}
month = {Jul}
}
title = {Rapidly rotating general relativistic stars. Pt. 2. Differentially rotating polytropes}
author = {Komatsu, Hidemi, Eriguchi, Yoshiharu, and Hachisu, Izumi}
abstractNote = {We have applied the numerical method which was developed for Newtonian gravity to general relativistic, differentially rotating bodies including ring-like structures. A number of equilibrium structures are obtained for two different polytropic indices N=1/2 and N=3/2, because the various proposed equations of state for the nuclear density region fall into the range N=1/2 to 3/2 from the viewpoint of its softness. (author).}
journal = []
volume = {239:1}
journal type = {AC}
place = {United Kingdom}
year = {1989}
month = {Jul}
}