Results 31 to 40 of about 676,444 (336)
Strange Quark Star (SQS) in Tolman IV potential with density dependent B-parameter and charge
European Physical Journal C: Particles and Fields, 2022 In this paper, the solutions of Einstein–Maxwell Field Equations for relativistic strange quark star in Tolman-IV potential considering MIT bag model EoS $$p=\frac{1}{3}(\rho -4B)$$ p = 1 3 ( ρ - 4 B ) of interior matter in presence of charge in higher ...
K. B. Goswami +3 more
doaj +1 more source
Seeding of Strange Matter with New Physics [PDF]
, 1997 At greater than nuclear densities, matter may convert into a mixture of nucleons, hyperons, dibaryons, and strangelets, thus facilitating the formation of strange matter even before the onset of the quark-matter phase transition.
Ernest Ma +5 more
core +2 more sources
Thermal Evolution and Light Curves of Young Bare Strange Stars [PDF]
, 2002 The cooling of a young bare strange star is studied numerically by solving the equations of energy conservation and heat transport for both normal and superconducting strange quark matter inside the star.
Ch. Schaab +14 more
core +2 more sources
Production of Strange Clusters and Strange Matter in Nucleus-Nucleus Collisions at the AGS [PDF]
, 1994 Production probabilities for strange clusters and strange matter in Au+Au collisions at AGS energy are obtained in the thermal fireball model. The only parameters of the model, the baryon chemical potential and temperature, were determined from a ...
Berger M S +8 more
core +3 more sources
Accretion on to strange-matter pulsars [PDF]
Monthly Notices of the Royal Astronomical Society, 1994 We study the effects of the accretion of normal matter on to strange-matter pulsar models. It is assumed that, because of the high strangeness barrier, normal matter is inert in contact with Q α matter. For this reason, normal matter accretion is able to form a thick outer layer with densities far above neutron drip.
Benvenuto, Omar Gustavo +2 more
openaire +3 more sources
New mass limit of a strange star admitting a colour flavor locked equation of state
European Physical Journal C: Particles and Fields, 2023 A class of strange stars is analysed in the present article in hydrostatic equilibrium, whose state is defined by a CFL phase equation of state. We have compared our results with those obtained from the MIT equation of state for strange quark matter ...
K. B. Goswami +3 more
doaj +1 more source
Hyperon Physics with PANDA at FAIR [PDF]
EPJ Web of Conferences, 2020 Hyperons provide new angles on two of the most challenging problems in contemporary physics: a coherent and quantitative description of the strong interaction, and the matter-antimatter asymmetry of the Universe.
Schönning Karin
doaj +1 more source
Strange Properties of Matter [PDF]
Nature, 1878 THE following are two experiments which will, perhaps interest some of your readers:— Experiment No.
openaire +2 more sources
Strangeness in Astrophysics [PDF]
EPJ Web of ConferencesIn this contribution the role of strangeness in astrophysics is discussed and, more precisely, strange hadronic matter in the interior of neutron stars.
Tolos Laura
doaj +1 more source
Strange Exotic States and Compact Stars [PDF]
, 2006 We discuss the possible appearance of strange exotic multi-quark states in the interior of neutron stars and signals for the existence of strange quark matter in the core of compact stars.
Alford M Blaschke D Drago A Klähn T Pagliara G Schaffner-Bielich J +15 more
core +4 more sources