Results 121 to 130 of about 282,852 (262)

Modified F(R,T)-Gravity Model Coupled with Magnetized Strange Quark Matter Fluid

Mathematics
This research note presents the properties of the F(R,T)-gravity model in combination with magnetized strange quark matter. We obtain the equation of state for the magnetized strange quark matter in the F(R,T)-gravity model endowed with the Lagrangian ...
Mohd Danish Siddiqi, Meraj Ali Khan, Ibrahim Al-Dayel   +2 more
doaj   +1 more source

Probing QCD critical fluctuations from the yield ratio of strange hadrons in relativistic heavy-ion collisions

Physics Letters B, 2020
By analyzing the available data on strange hadrons in central Pb+Pb collisions from the NA49 Collaboration at the Super Proton Synchrotron (SPS) and in central Au+Au collisions from the STAR Collaboration at the Relativistic Heavy-Ion Collider (RHIC) in ...
Tianhao Shao, Jinhui Chen, Che Ming Ko, Kai-Jia Sun   +3 more
doaj   +1 more source

QCD in neutron stars and strange stars

, 2011
This paper provides an overview of the possible role of Quantum Chromo Dynamics (QDC) for neutron stars and strange stars. The fundamental degrees of freedom of QCD are quarks, which may exist as unconfined (color superconducting) particles in the cores ...
Negreiros, R., Weber, F.
core   +1 more source

Strange matter and strange stars in a thermodynamically self-consistent perturbation model with running coupling and running strange quark mass [PDF]

, 2015
A quark model with running coupling and running strange quark mass, which is thermodynamically self-consistent at both high and lower densities, is presented and applied to study properties of strange quark matter and structure of compact stars.
Jia Xu, G. Peng, F. Liu, De-fu Hou, Lie-Wen Chen   +4 more
semanticscholar   +1 more source

Cylindrically Symmetric Diffusion Model for Relativistic Heavy‐Ion Collisions

Annalen der Physik, Volume 536, Issue 5, May 2024.
To account for particle production in relativistic heavy‐ion collisions at the Large Hadron Collider, a relativistic diffusion model with cylindrical symmetry is derived from nonequilibrium–statistical considerations. It propagates an initial state based on quantum chromodynamics in time toward a thermal equilibrium limit.
Johannes Hoelck, Georg Wolschin
wiley   +1 more source

Stellar model with non-zero strange quark mass ( $$m_s\ne 0$$ m s ≠ 0 ) and Mak–Harko density profile admitting observational results

European Physical Journal C: Particles and Fields
This article describes the configuration of strange quark stars composed of three flavour quarks in hydrostatic equilibrium considering the energy density profile of Mak and Harko and non-zero strange quark mass ( $$m_s\ne {0}$$ m s ≠ 0 ).
R. Roy, K. B. Goswami, A. Saha, A. Hakim, P. K. Chattopadhyay   +4 more
doaj   +1 more source

String breaking by light and strange quarks in QCD

Physics Letters B, 2019
The energy spectrum of a system containing a static quark anti-quark pair is computed for a wide range of source separations using lattice QCD with Nf=2+1 dynamical flavours.
John Bulava, Ben Hörz, Francesco Knechtli, Vanessa Koch, Graham Moir, Colin Morningstar, Mike Peardon   +6 more
doaj   +1 more source

Quark-Antiquark Condensates in the Hadronic Phase

, 2005
We use a hadron resonance gas model to calculate the quark-antiquark condensates for light (up and down) and strange quark flavors at finite temperatures and chemical potentials.
A. Tawfik, Allton, Allton, Allton, Aoki, Azcoiti, Barducci, Barducci, Barducci, Bernard, Bernard, Braun-Munzinger, Cleymans, D'Elia, D'Elia, D. Toublan, de Forcrand, de Forcrand, de Forcrand, Fodor, Fodor, Fodor, Frank, Gasser, Gavai, Gavai, Gerber, Göckler, Jamin, Karsch, Karsch, Karsch, Karsch, Klein, Leutwyler, Leutwyler, Narison, Pelaez, Rajagopal, Redlich, Sainio, Tawfik, Tawfik, Toublan, Toublan, Toublan, Zanotti   +46 more
core   +1 more source

COALESCENCE OF STRANGE-QUARK PLANETS WITH STRANGE STARS: A NEW KIND OF SOURCE FOR GRAVITATIONAL WAVE BURSTS [PDF]

, 2015
Strange-quark matter (SQM) may be the true ground state of hadronic matter, indicating that the observed pulsars may actually be strange stars (SSs), but not neutron stars.
J. Geng, Yong-feng Huang, T. Lu, T. Lu
semanticscholar   +1 more source

Consumer acceptance of microalgae as a novel food ‐ Where are we now? And how to get further

Physiologia Plantarum, Volume 176, Issue 3, May/June 2024.
Abstract Microalgae provide a potential new food resource for sustainable human nutrition. Many microalgae species can produce a high content of total protein with a balanced composition of essential amino acids, healthy oils rich in polyunsaturated fatty acids, carotenoids, fibers, and vitamins.
Malene Lihme Olsen, Karsten Olsen, Poul Erik Jensen   +2 more
wiley   +1 more source