NMSSM & B-meson Dileptonic Decays Jin Min Yang ITP, Beijing arXiv: Heng, Wang, Oakes, Xiong, JMY 杨 金 民杨 金 民
Outline Introduction NMSSM Model B Dileptonic Decay Conclusion
1. Introduction Some B processes are sensitive to new physics B-physics is not over (super B-factory, LHCb) About B physics
About NMSSM Dynamical solution to -problem Solve little hierarchy problem What is -problem ? What is little hierarchy problem ?
-problem: only dimensionful parameter conserving SUSY should be at Planck scale only dimensionful parameter conserving SUSY should be at Planck scale
little hierarchy: Experimental lower bound m h 114 GeV (95 GeV) Theoretical upper bound m h 90 GeV ( tree-level) 135 GeV ( loop-level) we need sizable loop effects ! ~ 500 GeV 100 GeV
2. NMSSM Model NMSSM = MSSM + Singlet Symmetry H u ·H d
E6 models (superstring-inspired) SO(10) U(1) … string scale at low energy: S, H u, H d + heavy particles U(1) global PQ to explicitly break U(1) PQ: cubic term NMSSM naturally exist ?
Higgs potential: ( 0 ) U(1) PQ ( A 0, A 0 ) U(1) R NMSSM
Spectrum of NMSSM: One more CP-odd Higgs (A 1 ) One more CP-even Higgs One more neutralino
Before SUSY breaking: SUSY vacuum: VEVs = 0 EW; Z 3 are not broken With SUSY breaking: vacuum: VEVs 0 EW break at weak scale SUSY breaking scale (<TeV) term is generated at weak scale How to solve -problem ?
Z 3 symmetry is crucial ! Comment: Otherwise, introduce a singlet seems no good (except: in SUSY vacuum EW spontaneously breaking) Discrete symmetry may cause new problem
How to solve little hierarchy ? m h theoretical upper bound m h experimental lower bound suppressed ! MSSM: NMSSM: has singlet component
MSSM fraction of h V. Barger, et al, hep-ph/
3. B Dileptonic Decay
V KM In SM:
In SUSY:
g
Assume: soft-terms are flavor universal at GUT scale flavor mixings occur when evolving down to weak scale K. Hikasa, M. Kobayashi, PRD36, 724 (1987)
SM: only gauge bosons SUSY: gauge and Higgs bosons
A1A1 OPE:
=mb=mb =mA1=mA1 =mW=mW ( integrate out A 1 ) A 1 is heavy A 1 is intermediately heavy A 1 is very light
SU(2) gaugino = 200 GeV Sfermions = 500 GeV U(1) gaugino = 100 GeV Scan over NMSSM parameter space: Keep the points allowed by LEPII
expt data No expt data !
Sky-blue points excluded by
4. Conclusion In NMSSM a light A 1 is allowed B-meson dileptonic decays can be greatly enhanced in NMSSM (a) current data has already set on NMSSM (b) future high precision expt will be crucial test