1 LoI FCAL Takashi Maruyama SLAC SiD Workshop, SLAC, March 2-4, 2009 Contributors: SLAC M. BreidenbachFNALW. Cooper G. Haller K. Krempetz T. MarkiewiczBNLW.

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Presentation transcript:

1 LoI FCAL Takashi Maruyama SLAC SiD Workshop, SLAC, March 2-4, 2009 Contributors: SLAC M. BreidenbachFNALW. Cooper G. Haller K. Krempetz T. MarkiewiczBNLW. Morse T. MaruyamaOregonD. Strom M. Oriuno Colorado U. Nauenberg J. Gill G. Oleinik

2 SiD Forward Region Beampipe LumiCal W Mask BeamCal Borated Poly Support Tube

3 SiD Forward Region LumiCal 20 layers of 2.5 mm W + 10 layers of 5.0 mm W BeamCal 50 layers of 2.5 mm W 3cm-thick Tungsten Mask 13cm-thick BoratedPoly Centered on the outgoing beam line ECAL Beampipe +/- 94 mrad (detector) +101 mrad, -87mrad (ext. line)

4 Calorimeter coverage –41    120 mrad Precision integrated luminosity measurement –Fiducial volume: 46    86 mrad Luminosity spectrum dL/dE –  s is not monochromatic due to beamstrahlung emission LumiCal

5 Energy resolution Energy resolution parameter is dependent on energy –15%/  E at low energy –20%/  E at high energy Energy leakage is small even at 500 GeV.   E/E =  /  E 20 layers of 2.5mm W+ 10 layers of 5.0mm W

6 Luminosity measurement Luminosity precision goal  L / L < –10 6 W + W - events in 5 years (500 fb -1 )  L/L=(N rec -N gen )/N gen –Bhabha d  /d  ~ 1/  3 –  L/L~2  /  min,  is a systematic error.  must be less than ~20  rad to reach  L/L = –Detector radial location must be know within 30  m. Bhabha event rate –N ev / 500 Nominal= 5.9 [1/  2 min – 1/  2 max ] (  in mrads) –30 ev/sec for  min =46 mrad,  max =86 mrad  (mrad) E (GeV) 46 mrad86 mrad 1/  3 dN/d 

7  L/L vs. segmentation  r (mm)  (mrad)  (mrad)  L/L       (mrad)  (mrad)  L/L     Radial segmentation  segmentation N  = 32  r = 2.5 mm  L / L < can be reached by  r < 3mm. Finer  segmentation helps, but not much. –Finer  segmentation will help shower separation.

8 Max Energy Deposition in Si channel Max energy deposition –160 MeV (7010 fC*) MIP –MPV~ MeV (4.1 fC) Bhabha ~ 1710 MIP If we want S/N ~ 10 for MIP, we need 17,000 dynamic range. –2 gains + 10 bit ADC Max Energy Deposition (MeV) 250 GeV e GeV  - Energy Deposition (MeV) 160 MeV * 3.65 eV to generate e-h pair  r = 2.5mm N  = 32

9 Pairs in LumiCal 1.5 e+/e- / BX hit LumiCal 282 BXs (10% train) R=6 cm ANTI-DID ILC 500 Nominal are confined within ~4 cm. However, there are pairs outside the ring of death, and >4000 e+/e-/train hit the LumiCal. X (cm) Y (cm)

10 Pair occupancy in LumiCal 1.5 e+/e- / BX reaching LumiCal Hits are mostly in the front ~10 layers. Inner most channels have more than 4 hits. Hits per Train  r = 2.5 mm, N  = 32 Inner most channels KPiX has only 4 buffers. Need a new chip being developed for the BeamCal.

11 LumiCal sensor design Based on 6” wafer. The inner radius centered on the out-beam, while the outer radius on the detector. 14 petals are all different; need different Masks.  r = 2.5 mm,  = 10  Radial division varies from 46 to 54 channels. Non-projective geometry; same sensors in depth-wise.

12 Bhabha events in LumiCal BHWIDE to generate Bhabha events Move to 14 mrad crossing angle system Simulate LumiCal response Reconstruct showers Move back to CM system Look at the distributions  1 (rad)  -  2 (rad)  (deg) E 1 + E 2 (GeV) E 1 (GeV) E 2 (GeV)

13 BeamCal Extend calorimeter coverage to small angle –7    44 mrad High energy electron detection –Provide two-photon veto for new particle searches Instantaneous luminosity measurement using beamstrahlung pairs –Pair production is proportional to luminosity

14  Veto in Pair Backgrounds Under SUSY dark matter scenarios, slepton & neutralino masses are nearly degenerate. M. Battaglia et al. hep-ph/ Search & measure stau with  m = 3 – 9 GeV P. Bambade et al. hep-ph/ SignalMajor background ee →  ee → (e)(e)   ~ 10 fb  ~ 10 6 fb  veto is crucial. –High energy electron detection in beamstrahlung pair background

15 Detector-Integrated-Dipole Total pair energy into BeamCal is half. –10 TeV/BX vs. 20 TeV/BX with NO-DID. Pair distribution is symmetric and more confined. No. photons backscattering to the tracker is half. NO DIDAnti-DID X (cm) Y (cm) We want Anti-DID. DID Pair energy distribution SiD Solenoid

16 High energy electron detection A lookup table to correlate energy deposition and incident energy. – ,  dependence –Geometry dependence Overlay high energy electron shower and one bunch crossing of beamstrahlung background. Subtract average beamstrahlung energy. Cluster algorithm to find high energy electron. Two talks in Parallel session by Jack Gill and Gleb Oleinik Detection efficiency

17 BeamCal Sensor Based on 6” Si wafer Centered on the outgoing beam line Two regions –R= cm (7 mrad – 25 mrad) BeamCal where beamstrahlung pairs hit. –R= cm (25 – 42 mrad) LumiCal extension, no beamstrahlung pairs 2.0 cm 7.5 cm 12.5 cm Incoming beamOutgoing beam

18 High occupancy and high radiation 100% occupancy R < 5 cm. –Need a new chip to store every bunch crossing.  R&D Highest radiation dose ~100 MRad/year. Neutron fluence 5  n s /cm 2 /year –Need radiation hard sensors.  R&D

19 Unresolved Issues LumiCal –Readout design –Petal-to-Petal dead space –Reproducible alignment to  30 um and verification BeamCal –Choice of sensor –Readout design –Petal-to-Petal dead space –Electronics cooling BeamPipe –HOM heating, cooling & wakefields due to abrupt radial transitions Global FCAL –Integration –Installation and servicing

20 Deformations in mm QD0 Lumi (220 kg) Mask (507 kg) LowZee&Beamcal (136 kg) Support Clam-shell Forward Integration 10mm steel 1616 mm  392

21 Summary Good enough progress has been made to write the LoI. We still have to resolve many issues before we can write TDR.