Results 91 to 100 of about 203,600 (192)
Magnetic field inhibits the conversion of neutron stars to quark stars [PDF]
Neutron stars provide a natural laboratory to test some unique implications of Quantum Chromodynamics (QCD)- the underlying theory of strong interactions- at extreme conditions of very high baryon density. It has been suggested that the true ground state of QCD is strange quark matter, and, consequently, neutron stars should convert to strange quark ...
arxiv
Heavy flavor quarks, owing to their large masses, are predominantly produced through initial hard parton scatterings in heavy-ion collisions, and thus are excellent probes to study properties of the strongly coupled Quark Gluon Plasma (sQGP) medium ...
Radhakrishnan Sooraj
doaj +1 more source
Magnetic field of a neutron star with color superconducting quark matter core [PDF]
Д. М. Седракян, D. Blaschke
openalex +1 more source
Nonperturbative models of quark stars in f(R) gravity
Quark star models with realistic equation of state in nonperturbative f(R) gravity are considered. The mass-radius relation for f(R)=R+αR2 model is obtained.
Artyom V. Astashenok+2 more
doaj
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E+6 more
europepmc +1 more source
Dense and hot matter in compact stars and heavy-ion collisions
We discuss the effect of exotic particles in neutron star matter and the corresponding impact on gross properties of neutron stars within effective models for the strong interaction.
Schramm Stefan+3 more
doaj +1 more source
The Spectrum of Low-pTJ/ψ in Heavy-Ion Collisions in a Statistical Two-Body Fractal Model. [PDF]
Ding H+4 more
europepmc +1 more source
Upper Limit on the Mass of RX J1856.5-3754 as a Possible Quark Star [PDF]
Kazunori Kohri, Kei Iida, K. Satô
openalex +1 more source
Instability of quark matter core in a compact newborn neutron star with moderately strong magnetic field [PDF]
Sutapa Ghosh, Somenath Chakrabarty
openalex +1 more source