Results 91 to 100 of about 1,287 (235)
QCD Equations of State in Hadron–Quark Continuity
The properties of dense matter in quantum chromodynamics (QCD) are delineated through equations of state constrained by the neutron star observations. The two solar mass constraint, the radius constraint of ≃11–13 km, and the causality constraint on the ...
Toru Kojo
doaj +1 more source
Effects of quark-matter symmetry energy on hadron-quark coexistence in neutron-star matter [PDF]
Xuhao Wu, Akira Ohnishi, Hong Shen
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The application of the Quark-Hadron Chiral Parity-Doublet model to neutron star matter [PDF]
A. Mukherjee +3 more
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Quark Matter and Quark Stars [PDF]
Guangxiong Peng +2 more
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Computation of the structure of a magnetized strange quark star [PDF]
G. H. Bordbar, Ali Reza Peivand
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Stars and quark stars in bumblebee gravity
In this work, the interior spacetime of stars is built in a Lorentz symmetry breaking model called bumblebee gravity. Firstly, we calculated the modified Tolman-Oppenheimer-Volkoff equation in this context of modified gravity. Then we show that the bumblebee field, responsible for the symmetry breaking, increases the star mass-radius relation when it ...
Juliano C.S. Neves, Fernando G. Gardim
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The puzzles of RX J1856.5-3754: neutron star or quark star? [PDF]
J. E. Trumper +3 more
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On the conversion of neutron stars into quark stars
The possible existence of two families of compact stars, neutron stars and quark stars, naturally leads to a scenario in which a conversion process between the two stellar objects occurs with a consequent release of energy of the order of $10^{53}$ erg.
openaire +3 more sources
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
We investigate binary neutron star (BNS) mergers using general-relativistic numerical simulations with hadronic and hybrid equations of state (EOSs), incorporating the latest observations and theoretical constraints.
Sudipta Hensh +6 more
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