scholarly journals Color-flavor locked quark stars in energy–momentum squared gravity

2021 ◽  
Vol 31 ◽  
pp. 100774
Author(s):  
Ksh. Newton Singh ◽  
Ayan Banerjee ◽  
S.K. Maurya ◽  
Farook Rahaman ◽  
Anirudh Pradhan
Keyword(s):  
Quark Stars

Strange Quark Matter as Dark Matter

2019 ◽  
Vol 22 (4) ◽  
pp. 311-317
Author(s):  
Hidezumi Terazawa
Keyword(s):  
Dark Matter ◽  
Quark Matter ◽  
Strange Quark ◽  
Strange Quark Matter ◽  
Quark Stars

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).

Quark stars in the Einstein-Gauss–Bonnet theory: A new branch of stellar configurations

2021 ◽  
pp. 168498
Author(s):  
Takol Tangphati ◽  
Anirudh Pradhan ◽  
Abdelghani Errehymy ◽  
Ayan Banerjee
Keyword(s):  
Quark Stars

scholarly journals Gluon condensates, quark matter equation of state and quark stars

1994 ◽  
Vol 63 (4) ◽  
pp. 681-688 ◽  
Author(s):  
A. Mishra ◽  
H. Mishra ◽  
P. K. Panda ◽  
S. P. Misra
Keyword(s):  
Equation Of State ◽  
Quark Matter ◽  
Quark Stars ◽  
Gluon Condensates

Quark matter in the perturbation QCD model with a rapidly convergent matching-invariant running coupling

2017 ◽  
Vol 26 (06) ◽  
pp. 1750034 ◽  
Author(s):  
Jian-Feng Xu ◽  
Yan-An Luo ◽  
Lei Li ◽  
Guang-Xiong Peng
Keyword(s):  
Perturbation Theory ◽  
Infinite Number ◽  
Quark Matter ◽  
Chemical Potential ◽  
Maximum Mass ◽  
Solar Mass ◽  
Quark Stars ◽  
Dense Quark Matter ◽  
Subtraction Point ◽  
Running Coupling

The properties of dense quark matter are investigated in the perturbation theory with a rapidly convergent matching-invariant running coupling. The fast convergence is mainly due to the resummation of an infinite number of known logarithmic terms in a compact form. The only parameter in this model, the ratio of the renormalization subtraction point to the chemical potential, is restricted to be about 2.64 according to the Witten–Bodmer conjecture, which gives the maximum mass and the biggest radius of quark stars to be, respectively, two times the solar mass and 11.7[Formula: see text]km.

scholarly journals Rotating Quark Stars in General Relativity

Universe ◽  
2018 ◽  
Vol 4 (3) ◽  
pp. 48 ◽  
Author(s):  
Enping Zhou ◽  
Antonios Tsokaros ◽  
Luciano Rezzolla ◽  
Renxin Xu ◽  
Kōji Uryū
Keyword(s):  
General Relativity ◽  
Quark Stars

Population Synthesis of Neutron Stars, Strange (Quark) Stars, and Black Holes

2002 ◽  
Vol 567 (1) ◽  
pp. L63-L66 ◽  
Author(s):  
Krzysztof Belczynski ◽  
Tomasz Bulik ◽  
Włodzimierz Kluźniak
Keyword(s):  
Black Holes ◽  
Neutron Stars ◽  
Strange Quark ◽  
Population Synthesis ◽  
Quark Stars
Sign in / Sign up

Export Citation Format

Share Document