| タイトル | Determining the nuclear equation of state from neutron-star masses and radii |
| 著者（英） | Lindblom, Lee |
| 著者所属（英） | NASA Headquarters |
| 発行日 | 1992-10-20 |
| 言語 | eng |
| 内容記述 | A method is developed for determining the nuclear equation of state directly from a knowledge of the masses and radii of neutron stars. This analysis assumes only that equilibrium neutron-star matter has the stress-energy tensor of an isotropic fluid with a barotropic equation of state, and that general relativity describes a neutron star's internal gravitational field. We present numerical examples which illustrate how well this method will determine the equation of state when the appropriate observational data become available. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 93A11893 |
| 権利 | Copyright |
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