Results 61 to 70 of about 4,373,503 (314)
Asymmetric nuclear matter based on chiral two- and three-nucleon interactions [PDF]
, 2015 We calculate the properties of isospin-asymmetric nuclear matter based on chiral nucleon-nucleon (NN) and three-nucleon (3N) interactions. To this end, we develop an improved normal-ordering framework that allows to include general 3N interactions ...
C. Drischler, K. Hebeler, A. Schwenk
semanticscholar +1 more source
ELECTRODYNAMICS FOR NUCLEAR MATTER IN BULK [PDF]
International Journal of Modern Physics D, 2007 We present an approach to analyze the electrodynamics of nuclear matter in bulk using the relativistic Thomas–Fermi equation. We generalize to the case of N ≃ (m Planck /m n )3 nucleons of mass m n an approach well tested in very heavy nuclei (Z ≃ 106).
RUFFINI, Remo +2 more
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From holography towards real-world nuclear matter [PDF]
, 2015 Quantum chromodynamics is notoriously difficult to solve at nonzero baryon density, and most models or effective theories of dense quark or nuclear matter are restricted to a particular density regime and/or a particular form of matter.
Si-wen Li, A. Schmitt, Qun Wang
semanticscholar +1 more source
Neutrino Emissivity of Dense Stars [PDF]
, 1995 The neutrino emissivity of compact stars is investigated in this work. We consider stars consisting of nuclear as well as quark matter for this purpose.
Ghosh, Sanjay K. +2 more
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Frontiers in PhysicsA compact and stable diagnostic system is established using Raman scattering to measure parameters such as major species concentration and temperature in the combustion flow field. Despite an engine’s huge vibration, the prototype works stably and has an
Ke Wang +8 more
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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
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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
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Universe, 2022 Neutron star is an important object for us to verify the equation of state of hadronic matter. For a specific choice of equations of state, mass and radius of a neutron star are determined, for which there are constraints from observations.
Chinatsu Watanabe +2 more
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, 1992 The goal in this thesis is thus twofold: The first is to investigate the feasibility of using heavy ion collisions to create conditions in the laboratory which are ripe for the formation of a quark-gluon plasma. The second is to develop a technique for studying some of the many non-perturbative features of this novel phase of matter.
openaire +4 more sources
Saturation properties of nuclear matter in the presence of strong magnetic field
, 2016 Different saturation properties of cold symmetric nuclear matter in the strong magnetic field have been considered. We have seen that for magnetic fields about $B> 3 \times 10 ^ {17}\ G$, {for both cases with and without nucleon anomalous magnetic ...
Bordbar, G. H., Rezaei, Z.
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