Based on N. Nagata, S. Shirai, JHEP 1403 (2014) 049.
Ø Ø Y. Okada, M. Yamaguchi, T. Yanagida (1991), H. E. Haber, R. Hempfling (1991) J. R. Ellis, G. Ridolfi, F. Zwirner (1991)
Scalar Par cles Gravi no Higgsinos M S = 10 (2-4) TeV Gauginos ( ) Gluino Bino Wino O(1) TeV pure gravity media.on, M. Ibe, T. T. Yanagida (2012) simply unnatural supersymmetry, N. Arkani- Hamed, et.al. (2012) spread supersymmetry, L. J. Hall and Y. Nomura (2012) mini- split, A. Arvanitaki, et.al. (2012)
q i q I q j g g g γ (g) q J u L ũ L t L t R ũ R u R q j q i M S O(10 2 )TeV T. Moroi and M. Nagai (2013), D. McKeen, M. Pospelov, A. Ritz (2013) W. Altmannshofer, R. Harnik, J. Zupan (2013), K. Fuyuto, J. Hisano, N. Nagata, K. Tsumura (2013)
α 1 50 40 30 SU(2) U(1) α 1 28 27 26 High- scale SUSY 20 10 SU(3) 10 6 10 8 10 10 10 12 10 14 10 16 Scale (GeV) Zoom 25 10 16 Scale (GeV) Low- scale SUSY J. Hisano, T. Kuwahara, N. Nagata (2013).
U i U k d R (s R ) u R t R τ R H C H C E j D l H u Hd lifetime (years) 10 36 10 35 10 34 10 33 M S = μ M 2 = 3 TeV M 16 = 1.0 10 GeV tanβ = 3 tanβ = 5 Hc tanβ = 10 tanβ = 30 tanβ = 50 s L (d L ) (b) (ν τ ) L T. Goto and T. Nihei (1999) V. Lucas and S. Raby (1997) 10 2 10 3 10 4 10 5 M S (TeV) J. Hisano, D. Kobayashi, T. Kuwahara, N. Nagata (2013).
Ø Ø
Sfermion Flavor Viola^on s ν µ,ν τ δ Q L 13 t b δ Q L 13 ũ d g u d
10 37 10 36 10 35 1/Γ(p K + ν) [year] 10 34 10 33 10 32 10 31 10 30 δ Q L 13 δ Q L 12 M S = 100 TeV, M 1 = 600 GeV," M 2 = 300 GeV, M 3 = -2 TeV," μ = M S, M Hc = 10 16 GeV," tanβ = 5" 10 29 10 28 10 27 δũr 13 δ Q L 23 SK Limit 0.01 0.1 δ N. Nagata, S. Shirai (2013).
Minimal Flavor Violation 10 31 10 32 10 33 10 34 10 35 10 36 10 37 lifetime (years) 10 31 10 32 10 33 10 34 10 35 10 36 10 37 lifetime (years)
U i D j U k E l X X Q k L l Q i Q j
10 38 1/Γ(p π 0 µ + ) [year] 10 36 10 34 10 32 10 30 δ Q L 13 δ Q L 12 δũr 13 SK Limit M S = 100 TeV, M 1 = 600 GeV," M 2 = 300 GeV, M 3 = -2 TeV," μ = M S, M Hc = 10 16 GeV," tanβ = 5" 0.01 0.1 δ N. Nagata, S. Shirai (2013).
Summary
Backup
10 9 8 7 Theory Experiment δ Q L 23 = δũr 23 =0.9 Q L 3 =4 tan β 6 5 4 3 2 1 10 1 10 2 10 3 10 4 10 5 m 0 [TeV] N. Nagata, S. Shirai (2013).
q i q I q j g g q j q J q i 1 1 0.1 Uppuer bound 0.1 δũr 13 = δũr 23 (D0 ) δ d R 13 (Bd 0) δ d R 23 (Bs) 0 0.01 10 1 10 2 10 3 10 4 m 0 [TeV] δ d R 12 (K 0 ) δũr 12 (D0 ) δ d R 13 = δ d R 23 (K 0 ) Uppuer bound 0.01 δũr 13 = δũr 23 = δ Q L 13 = δ Q L 23 (D0 ) δ d R 13 = δ Q L 13 (B0 d ) δ d R 23 = δ Q L 23 (B0 s) 0.001 10 1 10 2 10 3 10 4 m 0 [TeV] δ d R 12 = δ Q L 12 (K0 ) δũr 12 = δ Q L 12 (D0 ) δ d R 13 = δ d R 23 = δ Q L 13 = δ Q L 23 (K0 ) N. Nagata, S. Shirai (2013).
1 Uppuer bound 0.1 m 0 [TeV] d R 12 = QL 12 ũr 12 = Q L 12 d R 13 = QL 13 Q L 13 ũr 13 = 0.01 10 1 10 2 10 3 10 4 g γ (g) u L ũ L t L t R ũ R u R N. Nagata, S. Shirai (2013).
M Hc 10 18 10 17 10 16 10 15 M 3 /M 2 = 3 M 3 /M 2 = 9 M 3 /M 2 = 30 10 2 10 3 μ H = M S M 2 = 3TeV tanβ = 3 M S (TeV) J. Hisano, T. Kuwahara, N. Nagata, Phys. Le_. B723 (2013) 324.
S. Dimopoulos and H. Georgi (1981) N. Sakai (1981) (M HC : )
Q i Q k U i U k H C H C H C H C LLLL Q i L l E j D l RRRR LLLL RRRR
LLLL RRRR
Sfermion Flavor Viola^on
-< 0 (ud) R u L p> < 0 (ud) L u L p> <K 0 (us) R u L p> <K 0 (us) L u L p> -<K + (us) R d L p> <K + (us) L d L p> -<K + (ud) R s L p> <K + (ud) L s L p> -<K + (ds) R u L p> -<K + (ds) L u L p> < (ud) R u L p> < (ud) L u L p> N f =2+1 "direct" N f =2+1 "indirect" 0 0.05 0.1 0.15 0.2 W 0 (µ=2gev) [GeV 2 ] Y. Aoki, E. Shintani, and A. Soni, arxiv:1304.7424
10 35 Γ 1 (p K + ν)[year] 10 34 10 33 10 32 Long-Distance Theory Short-Distance 0.01 0.1 δ Q L 13 N. Nagata, S. Shirai (2013).
s ν τ B s δ Q L 23 b ν τ t b δ Q L 13 δ Q L 13 ũ d g u d
ηµ + ηe + K + ν K 0 µ + K 0 e + π + ν M S = 100 TeV, M 1 = 600 GeV," M 2 = 300 GeV, M 3 = -2 TeV," μ = M S, M X = 10 16 GeV," tanβ = 5" π 0 µ + π 0 e + 10 30 10 32 10 34 10 36 10 38 10 40 Γ 1 [year]
Dim- 5 proton decay via Planck suppressed operators 12 M scalar, no f mixing 11 m h excl tan 1 Log 10 MScalar GeV 10 9 8 m h excl tan 2 Hyper K p K excl Hyper K 7 p e excl 6 4 2 0 2 4 Log 10 M ino M Scalar M. Dine, P. Draper, W. Shepherd, arxiv: 1308.0274.
Soudan Frejus Kamiokande IMB Super-K p e + 0 n e + n + - p + 0 n + p + n 0 p e + p + n p e + 0 n e + n 0 p + 0 p + p e + p + n p e + K 0 n e + K - n e - K + p + K 0 n + K - p K + n K 0 p e + K*(892) 0 p K*(892) + n K*(892) 0 10 32 10 33 10 34 /B (years) 10 35 Super- Kamiokande
1 0.1 Uppuer bound 0.01 δ Q L 13 δ Q L 12 δ Q L 23 M S = 100 TeV, M 1 = 600 GeV," M 2 = 300 GeV, M 3 = -2 TeV," μ = M S, M Hc = 10 16 GeV," tanβ = 5" 0.001 10 1 10 2 10 3 10 4 m 0 [TeV] δũr 13 N. Nagata, S. Shirai (2013).