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    <pubDate>Fri, 14 Jul 2006 10:15:10 +0200</pubDate>
    <lastBuildDate>Fri, 14 Jul 2006 10:15:10 +0200</lastBuildDate>
    <item>
      <title>Transition to delta matter from hot, dense nuclear matter within a relativistic mean field formulation of the nonlinear sigma and omega model</title>
      <link>http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/2382</link>
      <description>An investigation of the transition to delta matter is performed based on a relativistic mean field formulation of the nonlinear sigma and omega model. We demonstrate that in addition to the Delta-meson coupling, the occurrence of the baryon resonance isomer also depends on the nucleon-meson coupling. Our results show that for the favored phenomenological value of m* and K, the Delta isomer exists at baryon density ~ 2–3 p0 if beta=1.31 is adopted. For universal coupling of the nucleon and Delta, the Delta density at baryon density ~ 2–3 p0 and temperature ~ 0.4–0.5 fm-1 is about normal nuclear matter density, which is in accord with a recent experimental finding.</description>
      <author>Zhuxia Li; Guangjun Mao; Yizhong Zhuo; Walter Greiner</author>
      <category>article</category>
      <guid>http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/2382</guid>
      <pubDate>Fri, 14 Jul 2006 10:15:10 +0200</pubDate>
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      <title>Relativistic transport theory of N, Delta and N* (1440) interacting through sigma, omega and pi mesons.</title>
      <link>http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/3048</link>
      <description>A self-consistent relativistic integral-di erential equation of the Boltzmann- Uehling-Uhlenbeck-type for the N*(1440) resonance is developed based on an effective Lagrangian of baryons interacting through mesons. The closed time-path Green s function technique and semi-classical, quasi-particle and Born approxima- tions are employed in the derivation. The non-equilibrium RBUU-type equation for the N*(1440) is consistent with that of nucleon s and delta s which we derived before. Thus, we obtain a set of coupled equations for the N,Delta and N*(1440) distribution functions. All the N (1440)-relevant in-medium two-body scattering cross sections within the N,Delta and N*(1440) system are derived from the same effective Lagrangian in addition to the mean field and presented analytically, which can be directly used in the study of relativistic heavy-ion collisions. The theoreticalprediction of the free pp - pp* (1440) cross section is in good agreement with the experimental data. We calculate the in-medium N+N - N+N* , N* +N - N+N and N*+N - N* +N cross sections in cold nuclear matter up to twice the nuclear matter density. The influence of different choices of the N* N* coupling strengths, which can not be obtained through fitting certain experimental data, are discussed. The results show that the density dependence of predicted in-medium cross sections are sensitive to the N* N* coupling strengths used. An evident density dependence will appear when a large scalar coupling strength of g^(sigma) N*N* is assumed. PACS number(s): 24.10.Cn; 25.70.-z; 21.65.+f</description>
      <author>Guangjun Mao; Ludwig Neise; Horst Stöcker; Walter Greiner; Zhuxia Li</author>
      <category>preprint</category>
      <guid>http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/3048</guid>
      <pubDate>Wed, 21 Dec 2005 11:00:59 +0100</pubDate>
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