Relativistic Models for Strange Stars in Massive Brans–Dicke Gravity

2021 ◽  
Vol 65 (10) ◽  
pp. 1048-1053
Author(s):  
M. Sharif ◽  
A. Majid
Pramana ◽  
2007 ◽  
Vol 68 (3) ◽  
pp. 397-406 ◽  
Author(s):  
Ramesh Tikekar ◽  
Kanti Jotania

2006 ◽  
Vol 15 (08) ◽  
pp. 1175-1182 ◽  
Author(s):  
KANTI JOTANIA ◽  
RAMESH TIKEKAR

The objective of this paper is to find out the suitability of an ansatz similar to that suggested by Vaidya–Tikekar, but prescribing paraboloidal geometry for the 3-space of the interior space–time of a relativistic spherical star in describing a family of physically viable models of superdense stars like Her X-1, SAX, and X-ray brust.


2021 ◽  
Vol 103 (4) ◽  
Author(s):  
D. Alvear Terrero ◽  
S. López Pérez ◽  
D. Manreza Paret ◽  
A. Pérez Martínez ◽  
G. Quintero Angulo
Keyword(s):  

2021 ◽  
Vol 342 (1-2) ◽  
pp. 310-314
Author(s):  
Moisés Razeira ◽  
Fabio Köpp ◽  
Guilherme Volkmer ◽  
Magno Machado ◽  
Dimiter Hadjimichef ◽  
...  

2019 ◽  
Vol 19 (2) ◽  
pp. 030 ◽  
Author(s):  
Yu-Bin Wang ◽  
Xia Zhou ◽  
Na Wang ◽  
Xiong-Wei Liu

1991 ◽  
Vol 44 (2) ◽  
pp. 895-898 ◽  
Author(s):  
R. J. Furnstahl ◽  
C. E. Price

2012 ◽  
Vol 8 (S291) ◽  
pp. 536-536
Author(s):  
Martin Urbanec ◽  
John Miller ◽  
Zdenek Stuchlik

AbstractWe present quadrupole moments of rotating neutron and strange stars calculated using standard Hartle Thorne approach. We demonstrate differences between neutron and strange star parameters connected with quadrupole moments and how this parameters could be, in the case of neutron stars, approximated almost independently on neutron star equation of state.


2011 ◽  
Vol 338 (1) ◽  
pp. 157-161 ◽  
Author(s):  
B. J. Ahmedov ◽  
B. B. Ahmedov ◽  
A. A. Abdujabbarov

2009 ◽  
Vol 80 (4) ◽  
Author(s):  
O. Lourenço ◽  
R. L. P. G. Amaral ◽  
M. Dutra ◽  
A. Delfino
Keyword(s):  

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