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Strange matter

open access: yesInternational Journal of Modern Physics A
Pulsar-like objects are extremely compact, with an average density that exceeds nuclear saturation density, where the fundamental strong interaction plays an essential role, particularly in the low-energy regime. The internal structures and properties of those objects are profoundly connected to phenomena such as supernova explosions, gamma-ray bursts (
Chengjun Xia, Xiaoyu Lai, Renxin Xu
semanticscholar   +4 more sources

Quark Matter May Not Be Strange [PDF]

open access: yesPhysical Review Letters, 2018
If quark matter is energetically favored over nuclear matter at zero temperature and pressure then it has long been expected to take the form of strange quark matter (SQM), with comparable amounts of $u$, $d$, $s$ quarks. The possibility of quark matter with only $u$, $d$ quarks ($ud$QM) is usually dismissed because of the observed stability of ...
Holdom, Bob, Ren, Jing, Zhang, Chen
openaire   +5 more sources

Phase transition toward strange matter [PDF]

open access: yesPhysical Review C, 2012
The phase diagram of a system constituted of neutrons and $ $-hyperons in thermal equilibrium is evaluated in the mean-field approximation. It is shown that this simple system exhibits a complex phase diagram with first and second order phase transitions.
Gulminelli, F.   +2 more
openaire   +6 more sources

Strange hadronic matter [PDF]

open access: yesPhysical Review Letters, 1993
We have studied the composition, stability, and production mechanisms of strange hadronic matter. By applying the RMF model to systems of nucleons, Λ’s, Σ’s, and Ξ’s, stable systems with hyperon lifetimes and charge to mass ratio close to zero are obtained. In this extended model, purely hyperonic matter consisting of lambda’s and cascades is predicted.
Schaffner, Jürgen   +4 more
  +9 more sources

Strange stars within bosonic and fermionic admixed dark matter [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2023
In this work, we study dark matter (DM) admixed strange quark stars exploring the different possibilities about the nature of the DM and their effects on the macroscopic properties of strange stars, such as maximum masses, radii, as well the ...
L. Lopes, H. C. Das
semanticscholar   +1 more source

Strange magnetars admixed with fermionic dark matter [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2022
We discuss strange stars admixed with fermionic dark matter in the presence of a strong magnetic field using the two-fluid Tolman-Oppenheimer-Volkov equations.
O. Ferreira, E. Fraga
semanticscholar   +1 more source

Compact star merger events with stars composed of interacting strange quark matter [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
We investigate the properties of stars participating in double compact star merger events considering interacting model of stable strange quark matter.
Anil Kumar, V. Thapa, M. Sinha
semanticscholar   +1 more source

Vector dark boson mediated feeble interaction between fermionic dark matter and strange quark matter in quark stars [PDF]

open access: yes, 2022
We study the structural properties like the gravitational mass, radius and tidal deformability of dark matter (DM) admixed strange quark stars (SQSs).
Debashree Sen, Atanu Guha
semanticscholar   +1 more source

Moment of inertia, quadrupole moment, Love number of neutron star and their relations with strange-matter equations of state [PDF]

open access: yesEuropean Physical Journal A, 2017
We investigate the impact of strange-matter equations of state involving Λ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek ...
Debades Bandyopadhyay   +3 more
semanticscholar   +1 more source

Hybrid stars with hyperons and strange quark matter [PDF]

open access: yesPROCEEDINGS OF THE 14TH ASIA-PACIFIC PHYSICS CONFERENCE, 2020
We consider the possibility of having hybrid stars with a phase transition from hadrons into strange matter at the core of a neutron star in b equilibrium. For the hadron phase equation of state (EoS) the quark-meson coupling model is used, while the MIT
Wasif Husain, A. Thomas
semanticscholar   +1 more source

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