Results 71 to 80 of about 42,461 (272)
Quark stars: features and findings [PDF]
Under extreme conditions of temperature and/or density, quarks and gluons are expected to undergo a deconfinement phase transition. While this is an ephemeral phenomenon at the ultra-relativistic heavy-ion collider (BNL-RHIC), quark matter may exist naturally in the dense interior of neutron stars.
openaire +2 more sources
Brain structure as a mediator of the relationship of impaired kidney function and physical function. ABSTRACT Background Older adults with chronic kidney disease (CKD) experience deficits in physical function and cardiorespiratory fitness at higher rates than older adults without impaired renal function.
Julie S. Rekant +7 more
wiley +1 more source
Nonperturbative models of quark stars in f(R) gravity
Quark star models with realistic equation of state in nonperturbative f(R) gravity are considered. The mass-radius relation for f(R)=R+αR2 model is obtained.
Artyom V. Astashenok +2 more
doaj +1 more source
Abstract In patients previously hospitalised for COVID‐19, a 12‐week high‐intensity interval training (HIIT) intervention has previously been shown to increase left ventricular mass (LVM) immediately after the intervention. In the present study, we examined the effects of the same HIIT scheme on LVM, pulmonary diffusing capacity, symptom severity and ...
Iben Elmerdahl Rasmussen +21 more
wiley +1 more source
The spin parameter of uniformly rotating compact stars
We study the dimensionless spin parameter $j (= c J/ (G M^2))$ of uniformly rotating neutron stars and quark stars in general relativity. We show numerically that the maximum value of the spin parameter of a neutron star rotating at the Keplerian ...
Andersson +28 more
core +1 more source
The Equation of State for Dense QCD and Quark Stars [PDF]
We calculate the equation of state for degenerate quark matter to leading order in hard-dense-loop (HDL) perturbation theory. We solve the Tolman-Oppenheimer-Volkov equations to obtain the mass-radius relation for dense quark stars. Both the perturbative
A. Peshier +34 more
core +3 more sources
Early quark deconfinement in compact star astrophysics and heavy-ion collisions [PDF]
O. Ivanytskyi +3 more
openalex +1 more source
Abstract Exercise training reduces tumour growth by increasing tumour‐infiltrating T‐cell density in preclinical models. However, it remains unknown whether exercise training can modify intratumoural T cells in humans.The aim of this study was to compare the effects of an exercise training intervention versus control on human prostate intratumoural T ...
Simon Nørskov Thomsen +13 more
wiley +1 more source
Quark matter nucleation in neutron stars and astrophysical implications [PDF]
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutron stars. We investigate the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matter.
Bombaci, Ignazio +3 more
core +3 more sources
Strange Quark Stars — A Review [PDF]
A pedagogical overview of strange quark matter and strange stars is presented. After a historical notation of the research and an introduction to quark matter, a major part is devoted to the physics and astrophysics of strange stars, with attention being paid to the possible ways by which neutron stars and strange stars can be distinguished in ...
openaire +2 more sources

