Results 61 to 70 of about 199,440 (313)
Nuclear matter calculations with chiral interactions . [PDF]
, 2018 Using two-nucleon and three-nucleon interactions derived in the framework of chiral perturbation theory (ChPT) with and without the explicit Δ isobar contributions, we calculate the energy per particle of symmetric nuclear matter and pure neutron matter ...
Domenico Logoteta +5 more
core +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
AIP Advances, 2020 This paper summarizes the direct observation of tagged hydroxyl within 200 µs after its formation in the temperature range of 294 K–891 K. We estimate the time and temperature frame of the coexistence of chemical reactions and diffusion based on analysis
Jun Shao +7 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
The ubiquitin ligase RNF115 is required for the clearance of damaged lysosomes
FEBS Letters, EarlyView.Upon lysosomal rupture, an E3 ubiquitin ligase RNF115 translocates from the cytosol to the damaged lysosomal membrane. Moreover, RNF115 depletion impairs the clearance of damaged lysosomes, identifying it as a key regulator of lysosomal quality control.
Sae Nakanaga +3 more
wiley +1 more source
The Merger of Two Compact Stars: A Tool for Dense Matter Nuclear Physics
Universe, 2018 We discuss the different signals, in gravitational and electromagnetic waves, emitted during the merger of two compact stars. We will focus in particular on the possible contraints that those signals can provide on the equation of state of dense matter ...
Alessandro Drago +4 more
doaj +1 more source
Implementing Chiral Three-Body Forces in Terms of Medium-Dependent Two-Body Forces
Frontiers in Physics, 2020 Three-nucleon (3N) forces are an indispensable ingredient for accurate few-body and many-body nuclear structure and reaction theory calculations. While the direct implementation of chiral 3N forces can be technically very challenging, a simpler approach ...
Jeremy W. Holt +4 more
doaj +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
FEBS Letters, EarlyView.Septin 9 polybasic domains couple phosphoinositide‐rich membrane binding to centrosome positioning, Golgi organization, and microtubule acetylation to control epithelial polarity. Their loss disrupts this axis, causing centrosome mispositioning, Golgi fragmentation, reduced microtubule acetylation, and polarity inversion via upregulation of the ...
Ting ting Cai +4 more
wiley +1 more source
Periodic structure in nuclear matter [PDF]
Physical Review C, 1992 The properties of nuclear matter are studied in the framework of quantum hadrodynamics. Assuming an {omega}-meson field, periodic in space, a self-consistent set of equations is derived in the mean-field approximation for the description of nucleons interacting via {sigma}-meson and {omega}-meson fields.
Lovas, István +3 more
openaire +2 more sources