Engineering Runs on Y(3S). The Cosmic Mystery-Pie o% antimatter WIMPs...
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Transcript of Engineering Runs on Y(3S). The Cosmic Mystery-Pie o% antimatter WIMPs...
![Page 1: Engineering Runs on Y(3S). The Cosmic Mystery-Pie o% antimatter WIMPs (Weakly-Interacting-Massive-Particles) are good dark matter candidates.](https://reader030.fdocuments.in/reader030/viewer/2022032522/56649d6d5503460f94a4d75a/html5/thumbnails/1.jpg)
Engineering Runs on Y(3S)
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The Cosmic Mystery-Pie
o% antimatter
WIMPs (Weakly-Interacting-Massive-Particles) are good dark matter candidates
![Page 3: Engineering Runs on Y(3S). The Cosmic Mystery-Pie o% antimatter WIMPs (Weakly-Interacting-Massive-Particles) are good dark matter candidates.](https://reader030.fdocuments.in/reader030/viewer/2022032522/56649d6d5503460f94a4d75a/html5/thumbnails/3.jpg)
DAMA NaI 3Region
CDMS 04
CDMS 05
90% CL upper limits assuming standard halo A2 scaling
Upper Limits from Direct Measurements
Predictions: Ellis & Olive, Baltz & Gondolo, Mandic & all
Direct measurements have no sensitivity for ~GeV mass regionLHC will reach ~TeV mass regionWho will search ~GeV mass region ?
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Possibility of Dark Matter Search in B-factory
PRD 72, 103508 (2005)
Br( Y(1S) ) ~ 0.0041 (m<4.73GeV/c2)
Y(3S)ISR
Y(3S) +-Y(1S), Y(1S) invisibleHowever …Two-photon backgrounds are quite high …Hard to reach Br ~ O(0.001)
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Idea to improve S/N ratio
(e+e- Y(3S)ISR ) ~ 0.02 nb
(e+e- Y(3S)) ~ 3 nb
S/N ratio x150
Energy scan in CLEO
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Y(3S) run w/o TRG modification
Expected Sensitivity on Y(3S) run
Current trigger condition is too tight for this channelLoose trigger condition gives large the sensitivity
*) Syst. error is not considered
Y(4S) run460 /fb
Theory prediction
90 %C.L
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Y(3S) run w/o TRG modification
Expected Sensitivity on Y(3S) run
Current trigger condition is too tight for this channelLoose trigger condition gives large the sensitivity
*) Syst. error is not considered
Y(4S) run460 /fb
Theory prediction
90 %C.L
Y(3S) run x 4 trigger efficiency
We took engineering data taking on Y(3S) to check the sensitivity with different trigger logic to check the capability of DAQ with such trigger to check the sensitivity for other physics topics
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We took data for 4.5 days(end of Feb, 2006)
Energy scan ~ 4hoursWe set E(4S)-223.6 MeV~ 3 /fb on 3S resonance ~0.25 /fb on 30MeV below 3S
CLEO
3 times hadrons~0.47 on Y(4S)~0.33 off-resonance
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Trigger logic was optimized for DM channel
Control sample data(3S) (1S)(1S) Eff. depends on opening angle
opening angle (degree) 4 times efficiency gain is expected - loose opening angle cut 135 45 degree - loose pt cut pt>350 MeV for both tracks for one (or both) track
x
y
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Trigger RateT
rig
ger
Rat
e (H
z)
Trigger rate was rather higher than usual condition (~460Hz)
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w/o Event Builder
Upgrade
w/Event BuilderUpgrade
Last BGM slide by Ito-san
DAQB
elle
Dea
d T
ime
(%)
Trigger Rate (Hz)
Dead time was consistent with expectationWe confirm great advantage of event builder upgrade (2005 summer)However, there were frequent DAQ errors remaining subject …
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Summary• Invisible decay of Y(1S) is sensitive for light Dark
– Y(3S) p+p-Y(1S)invisible
– Direct search has no sensitivity ~GeV mass region
• We took Y(3S) engineering runs for 4.5 days– (~3 /fb on-reso. , ~0.25 /fb off-reso.)
• Trigger was optimized for DM channel loose opening angle, pt-cutquite high trigger rateDAQ capability was checkedFrequent fatal errors are next subject…
• Offline analysis are on going