| Автор | S Mukherjee |
| Автор | B C Paul |
| Автор | N Dadhich |
| Дата выпуска | 1997-12-01 |
| dc.description | In a spherically symmetric spacetime we find the general solution for a relativistic star in hydrostatic equilibrium having the spheroidal geometry for the 3-space embedded in 4-Euclidean space. The parameter is the measure of spheroidal character and determines the physical properties of the star. It has a lower bound ; stars with smaller mass to radius ratio can occur for all allowed while ultracompact stars, having ratios between 1/3 and 1/2, will have . It turns out that a wide range of values of can represent objects with the fluid density of a neutron star. The model is shown to possess all the desirable physical features. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | General solution for a relativistic star |
| Тип | paper |
| DOI | 10.1088/0264-9381/14/12/027 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 14 |
| Первая страница | 3475 |
| Последняя страница | 3480 |
| Выпуск | 12 |
