Results 131 to 140 of about 42,461 (272)
Purpose Neuromuscular electrical stimulation (NMES) has been increasingly used to preserve or restore neuromuscular function in critically ill patients. However, its effects on inflammatory biomarkers and its safety require to be fully elucidated.
Amanda de Oliveira Santos +8 more
wiley +1 more source
Contraction of cold neutron star due to in the presence a quark core
Motivated by importance of the existence of quark matter on structure of neutron star. For this purpose, we use a suitable equation of state (EoS) which include three different parts: (i) a layer of hadronic matter, (ii) a mixed phase of quarks and ...
B. Eslam Panah +2 more
doaj +1 more source
From an analogy with non-relativistic degenerate QED plasma we make an estimate of the coupling strength of QGP hypothesized to be present in compact star interiors. At densities ranging from 3ρ 0–10ρ 0 (normal nuclear density ρ 0=0.16 fm−3), quark matter is found to be strongly to intermediately coupled.
Sineeba Ramadas, Vishnu M. Bannur
openaire +1 more source
The Spectrum of Low-pTJ/ψ in Heavy-Ion Collisions in a Statistical Two-Body Fractal Model. [PDF]
Ding H +4 more
europepmc +1 more source
Reweighting the quark Sivers function with STAR jet data [PDF]
Carlo Flore +5 more
openalex +1 more source
We investigate binary neutron star (BNS) mergers using general-relativistic numerical simulations with hadronic and hybrid equations of state (EOSs), incorporating the latest observations and theoretical constraints.
Sudipta Hensh +6 more
doaj +1 more source
Instability of quark matter core in a compact newborn neutron star with moderately strong magnetic field [PDF]
Sutapa Ghosh, Somenath Chakrabarty
openalex +1 more source
Gravitational wave signature from phase transition of a combusting neutron star to quark star [PDF]
Ritam Mallick +2 more
openalex +1 more source
Neutron Star masses from the Field Correlator Method Equation of State
We analyse the hadron-quark phase transition in neutron stars by confronting the hadronic Equation of State (EoS) obtained according to the microscopic Brueckner-Hartree-Fock many body theory, with the quark matter EoS derived within the Field Correlator
Zappalà D. +3 more
doaj +1 more source
Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]
Annala E +6 more
europepmc +1 more source

