用户名: 密码: 验证码:
A hybrid space–time of Schwarzschild interior and Vaidya–Tikekar solution as an embedding class I
详细信息    查看全文
文摘
A new type of embedding class-I metric representing anisotropic fluid distribution is presented in this paper. The new solution satisfies TOV equation and does represent a static stellar configuration. This new solution is an interesting hybrid solution where gtt is of Schwarzschild interior and grr is of Vaidya–Tikekar. The new solution satisfies all the physical criteria like positive finite central pressure, density, causality condition etc. It also satisfies all the energy conditions such as SEC, WEC, NEC and DEC. Using this new solution, we have presented some compact star models for Her X-1, RX J1856.5-3754, Cyg X-2 and PSR J1614-2230 by optimizing their masses and radii.

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700