scholarly journals A neutron star with a strange quark star-like mass-radius relation

2020 ◽  
Vol 28 ◽  
pp. 100488
Author(s):  
A. Savaş Arapoğlu ◽  
A. Emrah Yükselci
Keyword(s):  
Neutron Star ◽  
Strange Quark ◽  
Quark Star

scholarly journals Combustion of a neutron star into a strange quark star: The neutrino signal

2013 ◽  
Vol 87 (10) ◽  
Author(s):  
Giuseppe Pagliara ◽  
Matthias Herzog ◽  
Friedrich K. Röpke
Keyword(s):  
Neutron Star ◽  
Strange Quark ◽  
Quark Star

scholarly journals DISTINGUISHING BARE QUARK STARS FROM NEUTRON STARS

2004 ◽  
Vol 19 (31) ◽  
pp. 5335-5342 ◽  
Author(s):  
P. JAIKUMAR ◽  
C. GALE ◽  
D. PAGE ◽  
M. PRAKASH
Keyword(s):  
Neutron Star ◽  
Neutron Stars ◽  
Strange Quark ◽  
Spectral Characteristics ◽  
Extended Period ◽  
Complete Characterization ◽  
Quark Star ◽  
Quark Stars ◽  
Shed Light

Observations to date cannot distinguish neutron stars from self-bound bare quark stars on the basis of their gross physical properties such as their masses and radii alone. However, their surface luminosity and spectral characteristics can be significantly different. Unlike a normal neutron star, a bare quark star can emit photons from its surface at super-Eddington luminosities for an extended period of time. We present a calculation of the photon bremsstrahlung rate from the bare quark star's surface, and indicate improvements that are required for a complete characterization of the spectrum. The observation of this distinctive photon spectrum would constitute an unmistakable signature of a strange quark star and shed light on color superconductivity at stellar densities.

scholarly journals Was GW190814 a Black Hole–Strange Quark Star System?

2021 ◽  
Vol 126 (16) ◽  
Author(s):  
I. Bombaci ◽  
A. Drago ◽  
D. Logoteta ◽  
G. Pagliara ◽  
I. Vidaña
Keyword(s):  
Black Hole ◽  
Strange Quark ◽  
Quark Star ◽  
Star System

scholarly journals Strange quark star in dilaton gravity

2019 ◽  
Vol 19 (6) ◽  
pp. 078
Author(s):  
Alireza Peivand ◽  
Kazem Naficy ◽  
Gholam Hossein Bordbar
Keyword(s):  
Strange Quark ◽  
Quark Star ◽  
Dilaton Gravity

Is RXJ1856.5-3754 a strange quark star?

2003 ◽  
Vol 718 ◽  
pp. 351-358 ◽  
Author(s):  
Jeremy J. Drake ◽  
Herman L. Marshall
Keyword(s):  
Strange Quark ◽  
Quark Star

scholarly journals QUARK STARS ADMITTING A ONE-PARAMETER GROUP OF CONFORMAL MOTIONS

2004 ◽  
Vol 13 (01) ◽  
pp. 149-156 ◽  
Author(s):  
M. K. MAK ◽  
T. HARKO
Keyword(s):  
Analytical Solution ◽  
Quark Matter ◽  
Spherical Symmetry ◽  
Total Mass ◽  
Strange Quark ◽  
Exact Analytical Solution ◽  
Quark Star ◽  
Parameter Group ◽  
Quark Stars

An exact analytical solution describing the interior of a charged strange quark star is found under the assumption of spherical symmetry and the existence of a one-parameter group of conformal motions. The solution describes a unique static charged configuration of quark matter with radius R=9.46 km and total mass M=2.86M⊙.

scholarly journals Does Submillisecond Pulsar XTE J1739−285 Contain a Weak Magnetic Neutron Star or Quark Star?

2007 ◽  
Vol 119 (860) ◽  
pp. 1108-1113 ◽  
Author(s):  
C. M. Zhang ◽  
H. X. Yin ◽  
Y. H. Zhao ◽  
Y. C. Wei ◽  
X. D. Li
Keyword(s):  
Neutron Star ◽  
Quark Star

Magnetostatics of a superconducting quark star

1993 ◽  
Vol 71 (9-10) ◽  
pp. 488-492 ◽  
Author(s):  
Somenath Chakrabarty
Keyword(s):  
Relativistic Theory ◽  
Quark Mass ◽  
Strange Quark ◽  
Quark Star ◽  
Fermion System ◽  
Superconducting Properties ◽  
Mass Model ◽  
Density Dependent ◽  
System A ◽  
Theory Of Superconductivity

The superconducting properties of a strange quark star are investigated using the relativistic theory of superconductivity for a fermion system. A dynamical density-dependent quark mass model is used for confinement. The type of superconductivity and the magnetostatic properties for the material of the star are also studied.

scholarly journals Neutron Stars, Strange Pulsars and Strange Dwarfs

1996 ◽  
Vol 160 ◽  
pp. 135-136
Author(s):  
Fridolin Weber ◽  
Norman K. Glendenning
Keyword(s):  
Neutron Star ◽  
Neutron Stars ◽  
Strong Interaction ◽  
Ground State ◽  
Strange Quark ◽  
Complete Sequence ◽  
Strange Quark Matter ◽  
Compact Stars ◽  
Strange Dwarfs ◽  
Separate Class

The hypothesis that strange quark matter may be the absolute ground state of the strong interaction (not56Fe) has been raised independently by Boder and Witten. If the hypothesis is true, then a separate class of compact stars could exist, which are calledstrange matter stars. The properties of the complete sequence of such stars, which range from compact neutron-star-like strange stars to strange dwarfs to strange planets. The latter two constitute the strange counterparts of ordinary white dwarfs and planets, respectively. The properties of these objects are discussed in this paper.

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