search for bottom counterparts of x(3872) and y(4260) via p + p -
DESCRIPTION
Search for Bottom Counterparts of X(3872) and Y(4260) via p + p - . July 28, 2006, ICHEP ’ 06 @ Moscow. Outline. I Introduction II X b p + p - at Tevatron/LHC III Y b p + p - in e + e - ( g ISR ) Y b IV Discussion and Conclusion. based on hep-ph/0606016 - PowerPoint PPT PresentationTRANSCRIPT
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 1
Search for Bottom Counterparts ofX(3872) and Y(4260) via
July 28, 2006, ICHEP’06 @ Moscow
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 2
Outline
I Introduction
II Xb at Tevatron/LHC
III Yb in ee (ISR) Yb
IV Discussion and Conclusion
A simple talk to motivate the experts
based on hep-ph/0606016 (published in PRD)
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 3
I. Introduction
J/Xb, Yb
Bottomonium?
[X(3940), Z(3940)]
J/J/
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 4
Narrow
DD* threshold
preferred
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 5
Direct Scan
ISR
~ MeVeeBJ~ eV
vs eV
Large Y
2005
2006
The Y(4260)
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 6
II. Xb at Tevatron/LHC
Mass: If BB* ➯ 10640 MeV If coupled BB* and s/d-wave ➯ ~10560 MeV
Production: - No B KX analogue - Fortunately prompt X(3872) dominant (~ (2S))
Will check if dominant when seen
~ 3000 X(3872) evts / fb1
[ J/
Xb analogue: ~ 180 evts ~ 180 evts / 8fb/ 8fb11
4.4K/77pb1 vs 300K/40pb1 J/
PRL’02
PRD’05
TooOptimistic?
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 7
More conservative: Take ratio of peaks ~ 1/800 ➯ ~ 30 evts ~ 30 evts / 8fb/ 8fb11
To Do
bbbb
- benchmark: (2S) - Look for high mass, narrow statesLook for high mass, narrow states
???
(seems on-going at CDF)
Promising at Tevatron Run II
N.B. BR, production frac., etc.
CDF, PRL’02
CDF, PRD’05
J/
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 8
Assured at LHC (if exist)
Huge cross section over 102 increase ➯ Expect > > 10103 3 evts / evts / fbfb11
Xb Domenech-Garret, Sanchis-Lozano, NPB’01
PYTHIAfitting CDF J/
Remarks - Much work to do to estimate cross sections - Forward cross sections even less known Should be larger ! - LHCb has forward design (w/ RICH/ECAL)
➯ Spectroscopy May be best @ LHCbMay be best @ LHCb
Any narrow state, e.g. J/(KKJ/?)
“Y(3940)”
To Do
bbbb
- benchmark: (2S) - Look for high mass, narrow statesLook for high mass, narrow states
???
for ATLAS, CMS, LHCb
CDF, PRL’02
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 9
II. Yb in ee (ISR) Yb
ee+J/pb
~ 125 evts
BaBar, PRL’05
233 fb-1
Analogy: Do bothboth ee ISR and ee
CLEO-c, PRL’06
ee J/ee ISR J/
~ 35 evts
13 pb-1
stimulate
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 10
Belle (5S) Runs
June 21-23, 2005 1.86 fb
10825 10845 10865 10885 10905
each 30 pb
@ 10869 MeV
Repeated June, 2006
21.7 fb !
~ 1 fb/day
Do Both ee and ee ISR
~ 24 fb on (5S) at handDirect Scan Quick and Easy
Yb Mass ? Cross Section ?
Bs motivated
EnergyEnergyscan:scan:
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 11
Mass: Use QQg hybrid (CLEO favored) lattice work to illustrate
- 10600 - 10900 MeV (Michael) Could scale down, ∵ ccg prediction typically higher than Y(4260)
➯ Could show up in ISR on Could show up in ISR on (5S)(5S)
- 10900 – 11000 MeV (Juge, Kuti, Morningstar)
Predicted ccg state ~ 4260 ➯ Prefers Higher Energy ScanPrefers Higher Energy Scan
Width: 100 MeV (~ Yc = Y(4260)) plausible
Product BR:
Assume
~
Could be smaller or larger
Guestimates
BaBar/CLEO
─
─
─
10865
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 12
Cross Section:
energy fraction in CM
Direct
ISR on (5S)
─ ─~1/s scaling
Even for ~ 1 eV,
~ 125 ISR evts @ 10700 MeV, for 25 fb on (5S)
~ 45 Direct Scan evts / 30 pb
Comparable toBaBar
CLEO-cfor Y(4260)
Yb Evt Guestimates
More effective ?More effective ?
10900 11000
Promising !
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 13
IV. Discussion and Conclusion
• Only Tevatron confirmed X(3872) — Need Highest Energy - Only narrow states at hadronic colliders: Go for Xb
- Too much combinatorics () for heavy ion collisions
• not easy at ee, so/but LHCb should - Be prepared for other Narrow States - Aim for diverse modes (e.g. KK or ) and JPC determination
• Available (5S) at Belle should be exploited for ISR Yb
Probably hard for BaBar to collect equivalent data
• Both Belle and BaBar should try Quick energy scan 10600 – 11000 MeV Profitable ! (?)Quick energy scan 10600 – 11000 MeV Profitable ! (?)
• If Yb found, can run a little longer around direct eeYb
Study different channels (KK ? ?) and properties (be ingenious)
Xb/Yb George W.S. Hou (NTU) ICHEP’06, 7/28/06 14
Conclusion
at Tevatron/LHC ? ISR at B Factories ?
233 fb
125 evts
Xb, Yb Maybe Discovered in Near Future !
BaBar