X iv : n uc l - th / 0 11 10 82 v 1 2 9 N ov 2 00 1 Lattice Study of the High Density State of SU ( 2 ) - QCD

ar X iv : n uc l - th / 0 41 10 83 v 1 1 9 N ov 2 00 4 Electromagnetic transitions for A = 3 nuclear systems

Recent advances in the study of pd radiative capture in a wide range of center-of-mass energy below and above deuteron breakup threshold are presented and discussed.

X iv : n uc l - th / 0 21 10 45 v 1 1 4 N ov 2 00 2 Novel Phases at High Density and their Roles in the Structure and Evolution of Neutron Stars ∗

Despite decades of study, the question What is the ground state of dense baryonic matter? remains in the realm of theoretical speculation. Advances in our understanding of strongly interacting many-particle systems and QCD suggests numerous candidate states which have competitive free energy. Conventional many-body techniques, including those of lattice gauge theory and non-relativistic variati...

ar X iv : n uc l - th / 0 21 10 85 v 1 2 7 N ov 2 00 2 1 Medium effects to the N ( 1535 ) resonance and η mesic nuclei

ar X iv : h ep - p h / 97 10 23 0 v 2 1 9 N ov 1 99 7 KEK - TH - 546 Oct . ’ 97 Domain wall solution for vectorlike model

Domain wall solution for Nc = Nf supersymmetric QCD is constructed. Astrophysical implications of the domain wall configuration is also discussed. [email protected] 1

iv : n uc l - th / 0 11 00 25 v 2 2 8 N ov 2 00 1 Nuclear masses : evidence of order – chaos coexistence

Shell corrections are important in the determination of nuclear ground– state masses and shapes. Although general arguments favor a regular single– particle dynamics, symmetry–breaking and the presence of chaotic layers cannot be excluded. The latter provide a natural framework that explains the observed differences between experimental and computed masses.