Results 91 to 100 of about 1,345 (236)
Rotating Quark Stars in General Relativity
We have built quasi-equilibrium models for uniformly rotating quark stars in general relativity. The conformal flatness approximation is employed and the Compact Object CALculator (cocal) code is extended to treat rotating stars with surface density ...
Enping Zhou +4 more
doaj +1 more source
Abstract We examined the impact of moderate hypoxia (HYPO) on muscle activation during incremental exercise matched for both absolute and equivalent relative intensity. Fifteen active subjects (10 males, 5 females) completed two ramp incremental test and two step tests in normoxia (NORM; FiO2${F_{{\mathrm{i}}{{\mathrm{O}}_2}}}$ = 0.209) and HYPO (FiO2${
Dania Ibrahim +2 more
wiley +1 more source
We introduce the theoretical basis for modeling the cooling evolution of compact stars starting from Boltzmann equations in curved space-time. We open a discussion on observational verification of different neutron star models by consistent statistics ...
Grigorian H.
doaj +1 more source
Impact of the Nuclear Equation of State on the Stability of Hybrid Neutron Stars
We construct a set of equations of state (EoS) of dense and hot matter with a 1st order phase transition from a hadronic system to a deconfined quark matter state. In this two-phase approach, hadrons are described using the relativistic mean field theory
Mateusz Cierniak +4 more
doaj +1 more source
Abstract figure legend Intrathoracic pressure (ITP) manipulation during submaximal exercise reveals load‐ and sex‐specific cardiac volume responses. Inspiratory loading increased oesophageal pressure swings and the work of breathing (Wb) but did not alter stroke volume (SV) or ventricular volumes in males or females.
Sarah A. Angus +6 more
wiley +1 more source
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
Hybrid Quark Stars with Quark-Quark Phase Transitions
13 pages, 7 figures; updated version with possible signatures of gravitational wave ...
Yang, Zongcan +5 more
openaire +2 more sources
Reweighting the quark Sivers function with STAR jet data [PDF]
Carlo Flore +5 more
openalex +1 more source
Strongly interacting quark matter in massive quark stars
Abstract This paper investigates the properties of strongly coupled matter at high baryon densities (ρ B) in quark stars (QSs). The QS model is based on the density-dependent quark mass (DDQM) framework, modified DDQM (MDDQM) by enhancing the single-gluon interaction to generate higher repulsive pressure.
Adamu Issifu +4 more
openaire +2 more sources
Effects of quark-matter symmetry energy on hadron-quark coexistence in neutron-star matter [PDF]
Xuhao Wu, Akira Ohnishi, Hong Shen
openalex +1 more source

