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ID-28

ID-28. ID-32. Unified studies of reactions and structures in a N-rich system: M. Ito. N. Resonance. Slow RI beam. 4 He. 8 He. Strongly Polarized !!. Interact. Threshold. Inclusions of neutrons’ rearrangements. 1. Consistency with low lying states. 2. Extraction of cross

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ID-28

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  1. ID-28

  2. ID-32 Unified studies of reactions and structures in a N-rich system: M. Ito N Resonance Slow RI beam 4He 8He Strongly Polarized !! Interact Threshold Inclusions of neutrons’ rearrangements 1 Consistency with low lying states 2 Extraction of cross sections for low spin (Analysis of angular dis.) Application of the new cluster model to the a+a+4N system (Poster 32) Low-lying states

  3. ID-34

  4. ID-36

  5. Cooling of Exotic Stars with Quark-Hadron Mixed Phase in the Colour Superconductive State ID: 38 • Cassiopeia A Observation (Ho & Heinke, 2009) • Young (~330 yr), Hot and Heavy (>1.5M8) Compact Object • Suggesting Standard Nuclear Matter (No Quark!?) • Not match with some cooler stars (3C58/Vela) • Creating consistent model with both case (Cas A 3C58/Vela) • EOS with Quark-Hadron Mixed Phase (Maruyama 2007/2008) • Using Colour Superconductivity • Assuming large gap D (~100MeV), Enable to suppress quark cooling • Heavy stars cool slower, light stars cool faster. Tsuneo NODA (Kyushu Univ.) M. Hashimoto (Kyushu Univ.), N. Yasutake (NAOJ), T. Maruyama (JAEA), T. Tatsumi (Kyoto Univ.) & M. Fujimoto (Hokkaido Univ.)

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