Results 51 to 60 of about 1,046,678 (300)
Hyperonic Interactions in Neutron Stars
Particles, 2023 The matter of neutron stars is characterised by the density of the order of typical nuclear densities; hence, it can be described with methods of nuclear physics.
Semyon Mikheev +3 more
doaj +1 more source
Scalarization of neutron stars with realistic equations of state
, 2017 We consider the effect of scalarization on static and slowly rotating neutron stars for a wide variety of realistic equations of state, including pure nuclear matter, nuclear matter with hyperons, hybrid nuclear and quark matter, and pure quark matter ...
Blázquez-Salcedo, Jose Luis +3 more
core +1 more source
Mapping the evolution of mitochondrial complex I through structural variation
FEBS Letters, EarlyView.Respiratory complex I (CI) is crucial for bioenergetic metabolism in many prokaryotes and eukaryotes. It is composed of a conserved set of core subunits and additional accessory subunits that vary depending on the organism. Here, we categorize CI subunits from available structures to map the evolution of CI across eukaryotes. Respiratory complex I (CI)
Dong‐Woo Shin +2 more
wiley +1 more source
EPJ Web of Conferences, 2014 In this work, we will present beam energy and system size dependence of the higher order moments (skewness and kurtosis) of net-kaon and total proton multiplicity distributions for Au+Au collisions simulated using the UrQMD code.
Ristea Catalin +7 more
doaj +1 more source
Prompt production of the hidden charm pentaquarks in the LHC
European Physical Journal C: Particles and Fields, 2021 Motivated by the observation of the first hidden charm pentaquarks by the LHCb collaboration in 2015 and the updated analysis with an order-of-magnitude larger data set in 2019, we estimate their cross sections for the prompt production as well as their ...
Pan Ling +3 more
doaj +1 more source
Pre/Post-Merger Consistency Test for Gravitational Signals from Binary Neutron Star Mergers
Particles, 2023 Gravitational waves from binary neutron star (BNS) mergers can constrain nuclear models, predicting their equation of state (EOS). Matter effects on the inspiral-merger signal are encoded in the multipolar tidal polarizability parameters, whose leading ...
Matteo Breschi +2 more
doaj +1 more source
Reevaluation of the density dependence of nucleon radius and mass in the global color symmetry model of QCD [PDF]
, 2003 With the global color symmetry model (GCM) at finite chemical potential, the density dependence of the bag constant, the total energy and the radius of a nucleon in nuclear matter is investigated.
Gao, Dong-feng +3 more
core +1 more source
FEBS Letters, EarlyView.Enteropathogenic E. coli (EPEC) infects the human intestinal epithelium, resulting in severe illness and diarrhoea. In this study, we compared the infection of cancer‐derived cell lines with human organoid‐derived models of the small intestine. We observed a delayed in attachment, inflammation and cell death on primary cells, indicating that host ...
Mastura Neyazi +5 more
wiley +1 more source
Low Density Neutron Star Matter with Quantum Molecular Dynamics: The Role of Isovector Interactions
Universe, 2022 The effect of isospin-dependent nuclear forces on the inner crust of neutron stars is modeled within the framework of Quantum Molecular Dynamics (QMD).
Parit Mehta +4 more
doaj +1 more source
Variational Calculation for the Equation of State of Nuclear Matter at Finite Temperatures [PDF]
, 2007 An equation of state (EOS) for uniform nuclear matter is constructed at zero and finite temperatures with the variational method starting from the realistic nuclear Hamiltonian composed of the Argonne V18 and UIX potentials.
Akmal +20 more
core +2 more sources