Results 1 to 10 of about 1,230,906 (339)

Nuclear Matter and Nuclear Dynamics [PDF]

Journal of Physics: Conference Series, 2009
Highlights on the recent research activity, carried out by the Italian Community involved in the "Nuclear Matter and Nuclear Dynamics" field, will be presented.
, Baldo M, De Filippo E, Di Toro M, Famiano, Fantoni S, Fuchs C, Giordano V, Landau LD, Li BA, Li ZH, M Colonna, Serot BD   +12 more
arxiv   +6 more sources

Equation of state for nuclear matter based on density dependent effective interaction [PDF]

Int.J.Mod.Phys. E14 (2005) 739-749, 2003
An interesting method of obtaining equation of state for nuclear matter, from a density dependent M3Y interaction, by minimizing the energy per nucleon is described. The density dependence parameters of the interaction are obtained by reproducing the saturation energy per nucleon and the saturation density of spin and isospin symmetric cold infinite ...
Audi G., Bandyopadhyay D., Basu D. N., Bertsch G., Blaizot J. P., Brockmann R., D. N. BASU, Friedman B., Khoa D. T., Khoa D. T., Kobos A. M., Myers W. D., Schutz Y., Sharma M. M., Srivastava D. K.   +14 more
arxiv   +3 more sources

Quark Condensates in Nuclear Matter in the Global Color Symmetry Model of QCD [PDF]

Phys.Rev. C68 (2003) 035204, 2003
With the global color symmetry model being extended to finite chemical potential, we study the density dependence of the local and nonlocal scalar quark condensates in nuclear matter. The calculated results indicate that the quark condensates increase smoothly with the increasing of nuclear matter density before the critical value (about 12$\rho_0$) is
Gao, Dong-feng, Guo, Hua, Liu, Yu-xin
arxiv   +3 more sources

Hollow nuclear matter [PDF]

Phys. Rev. C 93, 014602 (2016), 2015
It is generally considered that an atomic nucleus is always compact. Based on the isospin-dependent Boltzmann nuclear transport model, here I show that large block nuclear matter or excited nuclear matter may both be hollow. And the size of inner bubble in these matter is affected by the charge number of nuclear matter.
arxiv   +4 more sources

Vlasov Description Of Dense Quark Matter [PDF]

Phys.Rev. C60 (1999) 065212, 1999
We discuss properties of quark matter at finite baryon densities and zero temperature in a Vlasov approach. We use a screened interquark Richardson's potential consistent with the indications of Lattice QCD calculations. We analyze the choices of the quark masses and the parameters entering the potential which reproduce the binding energy (B.E.) of ...
A. Bonasera, A. Bonasera, B. Povh, C. Y. Wong, E. M. Lifshitz, G. Bertsch, G. E. Brown, H. W. Crater, J. Kapusta, J. L. Richardson, L. P. Csernai, M. Dey, R. M. Barnett, S. E. Koonin, S. Loh, S. Loh, S. Loh, T. Vetter, V. Baluni   +18 more
arxiv   +7 more sources

Screening of nuclear pairing in nuclear and neutron matter [PDF]

Phys.Rev. C71 (2005) 054301, 2005
The screening potential in the $^1S_0$ and $^3S_1$ pairing channels in neutron and nuclear matter in different approximations is discussed. It is found that the vertex corrections to the potential are much stronger in nuclear matter than in neutron matter.
Shen, Chao, Lombardo, U., Schuck, P.
arxiv   +7 more sources

Phase transition from hadronic matter to quark matter [PDF]

, 2006
We study the phase transition from nuclear matter to quark matter within the SU(3) quark mean field model and NJL model. The SU(3) quark mean field model is used to give the equation of state for nuclear matter, while the equation of state for color ...
A. G. Williams, A. W. Thomas, A. W. Thomas, P. Wang, Ping Wang   +4 more
core   +2 more sources

Saturation properties and incompressibility of nuclear matter: A consistent determination from nuclear masses [PDF]

, 1995
Starting with a two-body effective nucleon-nucleon interaction, it is shown that the infinite nuclear matter model of atomic nuclei is more appropriate than the conventional Bethe-Weizsacker like mass formulae to extract saturation properties of nuclear ...
A. Seeger, A.H. Wapstra, F. Buchinger, F. Tondeur, H. de Vries, J. Decharge, J.M. Pearson, J.M. Pearson, L. Satpathy, L. Satpathy, L. Satpathy, L. Satpathy, L. Satpathy, M. Brack, M.D. Myers, N.H. Hugenholtz, P. Moller, P. Moller, R. Nayak, V. S. Uma Maheswari, Y. Aboussir   +20 more
core   +2 more sources

Isospin Physics in Heavy-Ion Collisions at Intermediate Energies [PDF]

, 1997
In nuclear collisions induced by stable or radioactive neutron-rich nuclei a transient state of nuclear matter with an appreciable isospin asymmetry as well as thermal and compressional excitation can be created.
Aim T., Alkahzov G., Ayik S., Ayik S., Bao-An Li, Barranco M., Bauer W., Bauer W., Bauer W., Baym G., Bernard V., Bertsch G. F, Bertsch G. F, Bertsch G. F., Bohnet A., Bombaci I., Borderie B., Brockmann R., Brueckner K. A., Charagi S. K., Che Ming Ko, Chomaz Ph., Christley J. A., Cole A. J., Colonna M., Csernai L. P, Danielewicz P, Danielewicz P., Danielewicz P., Das Gupta S., de la Mota V., Dean D. J., Dempsey J. F., Farine M., Friedman B., Gale C., Gale C., Gatty B., Glasmacher T., Glendenning N. K., Glendenning N. K., Glendenning N. K., Gonin M., Haar B., Hamamoto I., Hanold K. A., Haustein P. E., Hilscher D., Hirata D., Horowitz C. J., Huang M. J., Huber H., Jaqaman H. R., Jaqman H. R., Johnston H., Khoa T., Klakow D., Kortmeyer G., Krofcheck D., Krofcheck D., Kutschera M., Lagaris I. E., Lamb D. Q., Lattimer J. M., Li B. A., Li B. A., Li B. A., Li B. A., Li B. A., Li B. A., Li B. A., Li B. A., Li G. Q., Lopez-Quelle M., Ma Y. G., Miiller A. C., Miiller H., Miither H., Mishra V. K., Molitoris J., Molitoris J., Nagamiya S., Noren B., Ogawa Y., Ogilvie C. A., Ono A., Pak R., Pak R., Pak R., Pandharipande V. R., Pearson J. M., Peter J., Peter J., Pethick C. J., Polster D., Prakash M., Remaud B., Ren Z. Z., Rufa M., S., Schafmer J., Sharma M. M., Shen W. Q., Shlomo S., Sobotka L. G., Sobotka L. G., Sugahara Y., Sullivan J. P., Sumiyoshi K., Sumiyoshi K., Suzuki T., Thorsson V., Toke J., Tsang M. B., Uma Maheswari V. S., Werner T. R., Werner T. R., Westfall G. D., Wilson W. K., Wiringa R. B., Wolfgang Bauer, Xu H. M., Yabana K., Yariv Y., Yennello S. J., Zhang J., Zhang W. M.   +126 more
core   +3 more sources

Nuclear charge and neutron radii and nuclear matter: trend analysis [PDF]

Phys. Rev. C 93, 051303(R) (2016), 2016
Radii of charge and neutron distributions are fundamental nuclear properties. They depend on both nuclear interaction parameters related to the equation of state of infinite nuclear matter and on quantal shell effects, which are strongly impacted by the presence of nuclear surface.
arxiv   +1 more source