Results 191 to 200 of about 1,078 (229)

HHH whitepaper. [PDF]

open access: yesEur Phys J C Part Fields
Abouabid H   +33 more
europepmc   +1 more source

Modulational instability and associated multiple dark solitons in relativistically degenerate electron-positron-ion plasmas. [PDF]

open access: yesSci Rep
Jahangir R   +7 more
europepmc   +1 more source

Synthesis and characterization of γ-acyloxyl-ε-caprolactones. [PDF]

open access: yesiScience
Greischar G   +12 more
europepmc   +1 more source

On the uncertainty principle of neural networks. [PDF]

open access: yesiScience
Zhang JJ   +4 more
europepmc   +1 more source
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Quark Matter in Neutron Stars

2020
Fil: Spinella, William M..
Spinella, William M.   +3 more
openaire   +2 more sources

Stability of Quark Star Models

Communications in Theoretical Physics, 2016
Summary: In this paper, we investigate the stability of quark stars with four different types of inner matter configurations; isotropic, charged isotropic, anisotropic and charged anisotropic by using the concept of cracking. For this purpose, we have applied local density perturbations technique to the hydrostatic equilibrium equation as well as on ...
Azam, M., Mardan, S. A., Rehman, M. A.
openaire   +2 more sources

Quarks in stars

Soviet Physics Journal, 1974
The basic parameters — mass and radius — of the quark configurations having central densities from 1019 to 1032 g/cm3 are obtained. It is shown that similar objects should have large gravitational mass defects. The curve of the stable configurations is extended to the region of densities substantially exceeding those of the nucleus.
openaire   +1 more source

STABILITY OF QUARK MATTER AND QUARK STARS

New Worlds in Astroparticle Physics, 2003
We use the confining chromodielectric model to study quark matter. In the version of the model with a quartic potential for the confining field we obtain two solutions for the mean-field equations. The resulting equations of state for strange quark matter are degenerate at large densities with a small energy barrier between them.
M. FIOLHAIS, M. MALHEIRO, A. R. TAURINES
openaire   +1 more source

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