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In this same place teachers and pupils are storing topics that they do not like to get lost. Carved on the stone architrave of the Old Library, Conques Abbey, X th Century, Aveyron (Massif Central), France
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In this same place teachers and pupils are storing topics that they do not like to get lost. Carved on the stone architrave of the Old Library, Conques Abbey, X th Century, Aveyron (Massif Central), France.
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We remark here that also all relativistic mean field approaches in the presently used approximation scheme are predicting a stiff-like symmetry term, proportional to the baryon density, coming from the ρ-meson field contribution, see Ref. [10]. Actually, a superstiff-like behavior is obtained when a coupling to the scalar charged meson δ is added, see Refs. [11-13]
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We remark here that also all relativistic mean field approaches in the presently used approximation scheme are predicting a stiff-like symmetry term, proportional to the baryon density, coming from the ρ-meson field contribution, see Ref. [10]. Actually, a superstiff-like behavior is obtained when a coupling to the scalar charged meson δ is added, see Refs. [11-13].
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17
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85060509628
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Contributions of GR98
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Contributions of P.G. Reinhard, H. Sagawa, M. Di Toro, G. Colo' E.G. Lanza, in: GR98, Nucl. Phys. A 649 (1999) 1c-446c.
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(1999)
Nucl. Phys. A
, vol.649
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Reinhard, P.G.1
Sagawa, H.2
Di Toro, M.3
Colo', G.4
Lanza, E.G.5
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37
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17244371114
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EOS of asymmetric nuclear matter
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Bao-An Li, W. Udo Schröder (Eds.) Nova Science Publishers, New York and references therein
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U. Lombardo, W. Zuo, EOS of asymmetric nuclear matter, in: Bao-An Li, W. Udo Schröder (Eds.), Isospin Physics in Heavy-ion Collisions at Intermediate Energies, Nova Science Publishers, New York, 2001, pp. 1-34 and references therein.
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(2001)
Isospin Physics in Heavy-ion Collisions at Intermediate Energies
, pp. 1-34
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Lombardo, U.1
Zuo, W.2
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57
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0038117151
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EOS for isospin-asymmetric nuclear matter for astrophysical applications
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Bao-An Li, W. Udo Schröder (Eds.) Nova Science Publishers, New York and references therein
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I. Bombaci, EOS for isospin-asymmetric nuclear matter for astrophysical applications, in: Bao-An Li, W. Udo Schröder (Eds.), Isospin Physics in Heavy-ion Collisions at Intermediate Energies, Nova Science Publishers, New York, 2001, pp. 35-81 and references therein.
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(2001)
Isospin Physics in Heavy-ion Collisions at Intermediate Energies
, pp. 35-81
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Bombaci, I.1
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67
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17244366237
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Diploma Thesis
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V. Greco, Diploma Thesis (1997)
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(1997)
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Greco, V.1
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68
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0033248730
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V. Greco, A. Guarnera, M. Colonna, M. Di Toro, Phys. Rev. C 59 (1999) 810;
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Phys. Rev. C
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Greco, V.1
Guarnera, A.2
Colonna, M.3
Di Toro, M.4
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69
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0040585042
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V. Greco, A. Guarnera, M. Colonna, M. Di Toro, Nuovo Cimento A 111 (1998) 865.
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(1998)
Nuovo Cimento A
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Greco, V.1
Guarnera, A.2
Colonna, M.3
Di Toro, M.4
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75
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0004056428
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Pergamon Press, New York
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L.D. Landau, E.M. Lifshitz, Statistical Physics, Pergamon Press, New York, 1989, p. 288.
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(1989)
Statistical Physics
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Landau, L.D.1
Lifshitz, E.M.2
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97
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17244378293
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and http://www.phy.anl.gov/ria/
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http://www.nscl.msu.edu/ria/index.php and http://www.phy.anl.gov/ria/
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142
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Ph.D. Thesis
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V. Greco Ph.D. Thesis 2002
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Greco, V.1
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149
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TWINGO code, Ph.D. Thesis, University of Caen, July
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A. Guarnera, TWINGO code, Ph.D. Thesis, University of Caen, July 1996.
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(1996)
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Guarnera, A.1
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150
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0032536309
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and references therein
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G. Westfall Nucl. Phys. A 630 1998 27c and references therein
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Nucl. Phys. A
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Westfall, G.1
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153
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max is the sum of the two nuclear radii
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max is the sum of the two nuclear radii.
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We like to call the r-r1-correlation plot as Wilczynski-2 plot. Indeed this correlation, very important to rule-out a statistical fission scenario for fragments produced at mid-rapidity, nicely emerged during hot discussions with Janusz the LNS - INFN, Catania. As shown in the discussion this correlation represents also a chronometer of the fragment formation mechanism. In this sense it is the nice Fermi energy complement of the famous Wilczynski plot which gives the time-scales in deep inelastic collisions
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We like to call the r-r1-correlation plot as Wilczynski-2 plot. Indeed this correlation, very important to rule-out a statistical fission scenario for fragments produced at mid-rapidity, nicely emerged during hot discussions with Janusz the LNS - INFN, Catania. As shown in the discussion this correlation represents also a chronometer of the fragment formation mechanism. In this sense it is the nice Fermi energy complement of the famous Wilczynski plot which gives the time-scales in deep inelastic collisions.
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250
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0002050965
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It is important to put the properties of neutron matter at subnuclear densities on as firm a footing as possible not only for astrophysical applications, but also for interpreting terrestrial experiments with coming radioactive beam facilities, The Lives of Neutron Stars
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C.J. Pethick, D.G. Ravenhall, It is important to put the properties of neutron matter at subnuclear densities on as firm a footing as possible not only for astrophysical applications, but also for interpreting terrestrial experiments with coming radioactive beam facilities, in: The Lives of Neutron Stars, NATO ASI Series C, vol. 450, 1995, p. 59.
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(1995)
NATO ASI Series C
, vol.450
, pp. 59
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Pethick, C.J.1
Ravenhall, D.G.2
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253
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F) which is of the order ∼-30 MeV. In the relativistic case it becomes slightly positive due to the density dependence of the nucleon effective mass
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F) which is of the order ∼-30 MeV. In the relativistic case it becomes slightly positive due to the density dependence of the nucleon effective mass.
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254
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The solid lines in Fig. 4 are not fully symmetric with respect to the α=0 dashed line. This is due to the fact that, for fixed baryon density, the total scalar density which gives the σ field contribution (first part of the Eq. (6)) is also slightly N/Z dependent
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The solid lines in Fig. 4 are not fully symmetric with respect to the α=0 dashed line. This is due to the fact that, for fixed baryon density, the total scalar density which gives the σ field contribution (first part of the Eq. (6)) is also slightly N/Z dependent.
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264
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J. Klug et al. Phys. Rev. C 68 2003 064605
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Klug, J.1
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ρS
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ρS
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275
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private communication and Collective Modes of Nuclear Matter in Relativistic Mean Field Theories, Preprint LMU-Physik Sektion, Munich
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S. Typel, H.H. Wolter, private communication and Collective Modes of Nuclear Matter in Relativistic Mean Field Theories, Preprint LMU-Physik Sektion, Munich, 2002.
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Typel, S.1
Wolter, H.H.2
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0030268591
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and references therein
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C.H. Lee Phys. Rep. 275 1996 255 and references therein
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(1996)
Phys. Rep.
, vol.275
, pp. 255
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Lee, C.H.1
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In our framework this is a characteristic relativistic effect that should be somewhat included in the corresponding non-relativistic models. The importance of this contribution was not realized so far in previous non-relativistic studies [281], where no isospin effects were included in the momentum-dependent part of the effective forces. In this case the differences in the used symmetry energy parametrizations at supra-normal densities were very pronounced and therefore they resulted in very large effects with respect to earlier neutron emission and particle production
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In our framework this is a characteristic relativistic effect that should be somewhat included in the corresponding non-relativistic models. The importance of this contribution was not realized so far in previous non-relativistic studies [281], where no isospin effects were included in the momentum-dependent part of the effective forces. In this case the differences in the used symmetry energy parametrizations at supra-normal densities were very pronounced and therefore they resulted in very large effects with respect to earlier neutron emission and particle production.
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289
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(FOPI collaboration), private communication of very preliminary data
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W. Reisdorf (FOPI collaboration), private communication of very preliminary data.
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Reisdorf, W.1
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290
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Isospin effects in intermediate energy heavy-ion collisions
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arXiv:nucl-th/0402041 Bormio, Italy
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T. Gaitanos, M. Di Toro, G. Ferini, M. Colonna, H.H. Wolter, Isospin effects in intermediate energy heavy-ion collisions, arXiv:nUcl-th/ 0402041, Proceedings of the XLII International Winter Meeting On Nuclear Physics, Bormio, Italy, 2004.
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(2004)
Proceedings of the XLII International Winter Meeting On Nuclear Physics
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Gaitanos, T.1
Di Toro, M.2
Ferini, G.3
Colonna, M.4
Wolter, H.H.5
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(FOPI Collaboration)
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B. Hong, et al. (FOPI Collaboration), Phys. Rev. C 66 (2002) 034901
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(2002)
Phys. Rev. C
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Hong, B.1
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293
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and very preliminary data taken from (FOPI collaboration), GSI-Report
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and very preliminary data taken from B. Hong, Y.J. Kim, Y. Leifels, et al. (FOPI collaboration), GSI-Report, 2002.
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(2002)
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Hong, B.1
Kim, Y.J.2
Leifels, Y.3
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Of course we can have other asymmetric NM instability regions, at higher baryon densities, with a different structure of the unstable modes [20]. Here some interactions are even predicting quite exciting isovector-like (species separation) unstable oscillations. Unfortunately all that appears out of the present experimental possibilities
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Of course we can have other asymmetric NM instability regions, at higher baryon densities, with a different structure of the unstable modes [20]. Here some interactions are even predicting quite exciting isovector-like (species separation) unstable oscillations. Unfortunately all that appears out of the present experimental possibilities.
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