LRS Bianchi I model with strange quark matter and Λ(t) in f(R,T) gravity

New Astronomy ◽  
2021 ◽  
pp. 101634
Author(s):  
Vijay Singh ◽  
Aroonkumar Beesham
2020 ◽  
Vol 35 (14) ◽  
pp. 2050111
Author(s):  
Onur Özdemir ◽  
Can Aktaş

In this study, we have investigated generalized anisotropic universe models for magnetized strange quark matter (MSQM) distribution in the framework of [Formula: see text] gravitation theory. For this aim, we have used linearly varying deceleration parameter suggested by Akarsu and Dereli (2012) and equation of state for strange quark matter. For LRS Bianchi I universe model, the magnetic field was obtained as zero. But it was found to be different from zero for other universe models. Also, the geometric and physical aspects of the model are discussed in the conclusion.


2019 ◽  
Vol 22 (4) ◽  
pp. 311-317
Author(s):  
Hidezumi Terazawa

New forms of matter such as super-hypernuclei (strange quark matter) and superhypernuclear stars (strange quark stars) as candidates for dark matter are discussed in some detail, based on the so-called "Bodmer–Terazawa–Witten hypothesis" assuming that they are stable absolutely or quasi-stable (decaying only weakly).


1997 ◽  
Vol 56 (1) ◽  
pp. 491-496 ◽  
Author(s):  
G. Peng ◽  
P. Ning ◽  
H. Chiang

1999 ◽  
Vol 59 (4) ◽  
pp. R1829-R1833 ◽  
Author(s):  
T. A. Armstrong ◽  
K. Barish ◽  
S. J. Bennett ◽  
A. Chikanian ◽  
S. D. Coe ◽  
...  

Sign in / Sign up

Export Citation Format

Share Document