Nuclear Matter Theory / by Benhar, Omar, author 642608, Fantoni, S. (Stefano), author 642610

Subjects: “…Nuclear matter…”

Exotic nuclear matter by Lenske H., Dhar M., Tsoneva N., Wilhelm J.

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Nuclear matter and nuclear reactions/ by 283468 Kikuchi, Ken, Kawai, Mitsuji

Properties of Hot Nuclear Matter by Omar Benhar, Alessandro Lovato, Lucas Tonetto

Subjects: “…nuclear matter…”
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Condensates and correlations in nuclear matter by Röpke G.

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Nuclear Matter in 1 + 1 Dimensions by Robert D. Pisarski, Marton Lajer, Alexei M. Tsvelik, Robert M. Konik

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Hydromagnetic Waves in Cold Nuclear Matter by Şerban Mişicu

Subjects: “…nuclear matter…”
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A quark model for nuclear matter by Dagdeviren, Nuri Ruhi

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Incompressibility in finite nuclei and nuclear matter by Stone, JR, Stone, N, Moszkowski, SA

“…The incompressibility (compression modulus) K0 of infinite symmetric nuclear matter at saturation density has become one of the major constraints on mean-field models of nuclear many-body systems as well as of models of high density matter in astrophysical objects and heavy-ion collisions. …”

Skyrme interaction and nuclear matter constraints by Dutra, M, Lourenço, O, Sá Martins, J, Delfino, A, Stone, JR, Stevenson, P

“…Additional, more microscopic, constraints on the density dependence of the neutron and proton effective mass β-equilibrium matter, Landau parameters of symmetric and pure neutron nuclear matter, and observational data on high- and low-mass cold neutron stars further reduce this number to 5, a very small group of recommended Skyrme parametrizations to be used in future applications of the Skyrme interaction of nuclear-matter-related observables. …”

The equation of state of symmetric and asymmetric nuclear matter by S. Shlomo

“…The equation of state (EOS) of nuclear matter is a very important ingredient in the study of nuclear properties, heavy ion collisions, neutron stars and supernova. …”
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The Modification of the Scalar Field in dense Nuclear Matter by Rożynek J.

“…The correction to the Fermi energy from term proportional to the pressure is very important and its inclusion modifies the Equation of State (EoS) for nuclear matter.…”
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Holographic modeling of nuclear matter and neutron stars by Matti Järvinen

“…Abstract I review holographic models for (dense and cold) nuclear matter, neutron stars, and their mergers. I start by a brief general discussion on current knowledge of cold QCD matter and neutron stars, and go on discussing various approaches to model cold nuclear and quark matter by using gauge/gravity duality, pointing out their strengths and weaknesses. …”
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Thermodynamic instabilities in hot and dense nuclear matter by Lavagno A.

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Skyrme Crystals, Nuclear Matter and Compact Stars by Christoph Adam, Alberto García Martín-Caro, Miguel Huidobro, Andrzej Wereszczynski

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Minimal length, nuclear matter, and neutron stars by I. Prasetyo, I. H. Belfaqih, A. B. Wahidin, A. Suroso, A. Sulaksono

“…We have shown that the upper bound for the GUP parameter from nuclear matter properties is $$\beta \le 2\times 10^{-7}$$ β ≤ 2 × 10 - 7 MeV $$^{-2}$$ - 2 . …”
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Experimental Study of Cold Dense Nuclear Matter by Maria Patsyuk, Timur Atovullaev, Goran Johansson, Dmitriy Klimanskiy, Vasilisa Lenivenko, Sergey Nepochatykh, Eli Piasetzky

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The Skyrme interaction in finite nuclei and nuclear matter by Stone, JR, Reinhard, P

The asymmetric nuclear matter correlated states in the LOCV framework by A Tafrihi

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Impact of Fock terms on the isospin properties of nuclear matter by Sun Bao Yuan, Zhao Qian, Long Wen Hui

“…Several topics on the isospin properties of nuclear matter studied within the density-dependent relativistic Hartree-Fock theory are summarized. …”
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