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PICO-LON Project to search for WIMPs Dark Matter

ID-2. PICO-LON Project to search for WIMPs Dark Matter. Ken-Ichi Fushimi for PICO-LON Project. P lanar I norganic C rystal O bservatory for LO w-background N eutr(al)ino Aim Search for WIMPs dark matter Detector Thin NaI(Tl) 18cmX18cmX0.5cm. ID-11. ID-13.

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PICO-LON Project to search for WIMPs Dark Matter

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  1. ID-2 PICO-LON Project to search for WIMPs Dark Matter Ken-Ichi Fushimi for PICO-LON Project • Planar Inorganic Crystal Observatory for LOw-background Neutr(al)ino • Aim • Search for WIMPs dark matter • Detector • Thin NaI(Tl) 18cmX18cmX0.5cm

  2. ID-11

  3. ID-13

  4. From Scto Znin Hot bubblesof Sne~Origin of EMP stars: SNe or HNe ?~ ID-14 Natsuko Izutani (Univ. of Tokyo), Hideyuki Umeda (Univ. of Tokyo), Takashi Yoshida (Univ. of Tokyo) shock s/kb ～ 15 (HN) → high Zn, Co s/kb ～　3 (SN) → low Zn, Co HNe? or SNe? Fe,Zn,Co Fe,Cr,Mn Fe EMP star (high Zn, Co) Si Si C+O hot bubble (near Fe-core) He How the Abundance Patterns of Ejected Matter is changed ?? Ye > 0.5 Ye < 0.5 What is the origin of EMP stars ? 　　　　　ー HNe or SNe? center (Janka et al. 2003)

  5. ID-15

  6. ID-16 The neutron-rich matter in relativistic Hartree-Fock model with bare NN interaction Object of study: The equation of state of neutron-rich matter Methods: The relativistic Hartree-Fock (RHF) method The unitary correlation operator method (UCOM) NN Interactions: Bare interactions---- Bonn interactions Jinniu Hu, Hiroshi Toki, Wu Wen and Hong Shen

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