%Z&$s?<9/<k2013 918e<k

2n13| (e)!ZB9'a0J#tK"aeJb]K[

9'30 ] 9'50 uU

9'50 ] 10'00 Opening

10'00 ] 11'30 G3R*'h@ I (4 BO a (KEK))

11'30 ] 13'00 k)

13'00 ] 14'30 SUSY=]@ I (s# p a (lg))

14'30 ] 14'45 YF

14'45 ] 16'15 Ee:),jH new physi s (b p/ a (*cg))

16'15 ] 17'30 Free Dis ussion

2n14| (Z)!ZB9'a0J>DK"aeJb]K[

9'30 ] 11'00 G3R*'h@ II (4 BO a (KEK))

11'00 ] 11'15 YF

11'15 ] 12'45 SUSY=]@ II (s# p a (lg))

12'45 ] 14'30 k)u Free Dis ussion

14'30 ] 16'00 Muon g � 2KpE/77$*}N=u

(s# p a (lg))

16'00 ] 16'15 YF

16'15 ] 17'45 Ele troweak data and its impli ations for new physi s

(b p/ a (*cg))

18'30 ] )Fq

2n15| (b)!ZB9'a0J#mK"aeJ#tK[

9'00 ] 10'30 G3R*'h@ III (4 BO a (KEK))

10'30 ] 10'45 YF

10'45 ] 12'15 'h@Khkxu9k3RXN)B

(4 BO a (KEK))

12'15 ] 13'30 k)

13'30 ] 14'30 Cosmi R-string/ R-tube in the thermal history

(gOb - a (~g))

14'30 ] 15'00 Cosmologi al onstraints on spontaneous

R-symmetry breaking models (@D :@ a (~g))

15'00 ] 15'15 YF

15'15 ] 15'45 $sUl<7gsHi|'h'l8.

(#D R0 a (lg Kavli IPMU))

15'45 ] 16'15 6PNO?K*1klWHsUl<P<NKl

(f< B4 a (lLg))

16'15 ] 16'45 ILCKhkWinoEu*AN!ZD=-

(Tn ,K a (lg Kavli IPMU))