Vishnu V. Zutshi for NIU/NICADD

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Presentation transcript:

Vishnu V. Zutshi for NIU/NICADD Prototyping Studies for a Scintillator (semi)Digital HCal and a Tail-Catcher/Muon Tracker Vishnu V. Zutshi for NIU/NICADD

Outline A scintillator-based 2-bit hadron calorimeter MC studies Hardware Prototyping Plans Tail-catcher/Muon tracker V. Zutshi, ICLC04, Paris 1/18/2019

N vs. E (single hadrons) 0.25mip threshold V. Zutshi, ICLC04, Paris 1/18/2019

Single Particle E Resolution Simple counting of cells above threshold Single Particle E Resolution Non-projective geometry V. Zutshi, ICLC04, Paris 1/18/2019

Parameterized Jet E Resolution Energy Smearing Fit s as a function of incident E (slide4) and smear neutral hadrons accordingly g ~ 17%/sqrt(E), generated E for charged hadrons Jet Reconstruction pT order stable MC particles (ignoring neutrinos) start with highest pT particle and cluster in 0.7 cone repeat for remaining particles V. Zutshi, ICLC04, Paris 1/18/2019

Single Particle Resolution (10GeV) 9cm2 cells Single Particle Resolution (10GeV) s/E=0.183 s/N=0.166 V. Zutshi, ICLC04, Paris 1/18/2019

Single Particle Resolution (50GeV) 9cm2 cells Single Particle Resolution (50GeV) s/E=0.101 s/N=0.153 V. Zutshi, ICLC04, Paris 1/18/2019

The Culprit Can be flattened with multiple thresholds V. Zutshi, ICLC04, Paris 1/18/2019

Single Particle Resolution (50 GeV) After threshold-based weighting of cells Single Particle Resolution (50 GeV) s/E=0.101 s/E=0.092 V. Zutshi, ICLC04, Paris 1/18/2019

Similar treatment to 10 GeV…. s/E=0.183 s/N=0.164 V. Zutshi, ICLC04, Paris 1/18/2019

Applying Photo-Statistics Smearing V. Zutshi, ICLC04, Paris 1/18/2019

Layer Stack V. Zutshi, ICLC04, Paris 1/18/2019

Cosmic Data with PMT Started with 11pe now ~14 p.e being regularly achieved V. Zutshi, ICLC04, Paris 1/18/2019

Efficiency vs. Noise Rejection V. Zutshi, ICLC04, Paris 1/18/2019

Si-PM and MRS Pixilated (500 to 1000 on ~1mm2) Geiger mode sensor with high gain and modest Quantum*geom. efficiency P. Buzhan et. al V. Zutshi, ICLC04, Paris 1/18/2019

Si-PM’s V. Zutshi, ICLC04, Paris 1/18/2019

Cosmic Data with Si-PM nPE V. Zutshi, ICLC04, Paris 1/18/2019

MRS Dark Noise Rate V. Zutshi, ICLC04, Paris 1/18/2019

Surface Treatment/Wrapping UNPOLISHED TOP AND POLISHED BOTTOM POLISHED TOP AND UNPOLISHED BOTTOM 0.98 1.00 1.02 Tyvek Paint VM 2002 Mylar CM590 CM500 Alum Foil 1.00 0.89 1.08 0.83 0.28 0.44 0.63 V. Zutshi, ICLC04, Paris 1/18/2019

Thickness vs. weight If weight and thickness track each other, then it may be possible to monitor paint application via weight only Check to see if thickness and weight track each other by plotting thickness vs. weight: 2nd set V. Zutshi, ICLC04, Paris 1/18/2019

X-talk Optical x-talk + source spillage All cells connected to pmt Only central cell connected Only neighbors connected 1.000 0.985 0.008 0.006 V. Zutshi, ICLC04, Paris 1/18/2019

Cells Fabricated V. Zutshi, ICLC04, Paris 1/18/2019

Normalized Response Eljen extruded Bicron Cell Groove Area Response Hexagon Sigma 9.4 1.0 Square 0.88 6 0.92 1.05 Straight 0.81 4 0.85 0.46 0.48 0.58 Since light ample, can optimize for ease of construction V. Zutshi, ICLC04, Paris 1/18/2019

Sigma Groove Uniformity V. Zutshi, ICLC04, Paris 1/18/2019

Straight Groove Uniformity V. Zutshi, ICLC04, Paris 1/18/2019

Scanning over the neighbors V. Zutshi, ICLC04, Paris 1/18/2019

Rainbow Groove V. Zutshi, ICLC04, Paris 1/18/2019

Response Dispersion Overall dispersion<10% V. Zutshi, ICLC04, Paris 1/18/2019

RESPONSE LONG AFTER PRODUCTION 0.993  0.006 RESPONSE LONG AFTER PRODUCTION Column1 Mean 0.992641 Standard Error 0.005622 Median 0.994932 Mode #N/A Standard Deviation 0.030794 Sample Variance 0.000948 Kurtosis -0.64168 Skewness 0.171597 Range 0.117636 Minimum 0.935048 Maximum 1.052684 Sum 29.77922 Count 30 V. Zutshi, ICLC04, Paris 1/18/2019

Summary/Plans Scint. (s)DHCAL looks like a very competitive option…. Simulations indicate approach competitive with analog Prototypes indicate there is sufficient sensitivity (light x efficiency) & uniformity. Outlook for optimizing materials & construction to minimize cost looks promising Intend to take part in the CALICE test beam in collaboration with the Tile-Cal group V. Zutshi, ICLC04, Paris 1/18/2019

Tail-catcher/Muon System V. Zutshi, ICLC04, Paris 1/18/2019

Goals for the TC/Muon System Provide a reasonable snapshot of the tail-end of the shower for simulation validation Prototype detector with high-fidelity to what is imagined for a generic LCD correcting for leakage understanding the impact of coil muon reconstruction + eflow fake rate V. Zutshi, ICLC04, Paris 1/18/2019

On tail-catching For charged pions with >5% of E inside TC 10cm absorber plates V. Zutshi, ICLC04, Paris 1/18/2019

Accounting for material in the coil... 135%/sqrt(E) V. Zutshi, ICLC04, Paris 1/18/2019

Erec/Egen 50 GeV p V. Zutshi, ICLC04, Paris 1/18/2019

Fake Jets Needed to judge the hit occupancy near the muon track B*  B + p(35GeV) | D* + m(15GeV) | p(20GeV)+K(15GeV)+p(10GeV) Particles are produced in 0.05 cone individually and G4 simulated hits are combined in the analysis program V. Zutshi, ICLC04, Paris 1/18/2019

Fake Jet Angular Width (dR = 0.05) ECal view TC view V. Zutshi, ICLC04, Paris 1/18/2019

s(X) w.r.t. previous layer V. Zutshi, ICLC04, Paris 1/18/2019

Stripification Assign tail-catcher hits to strips of a given size in analysis software Obtain x or a y co-ordinate from alternate lyrs Take all combinations Efficiency is defined as the ratio of the no. of times a pairwise muon hit is found within a road in lyrs N+1 and N+2 when it was present in N and N+1 Rejection = 1-p where p is the fraction of times a non-muon hit combination was present in the road V. Zutshi, ICLC04, Paris 1/18/2019

s(X) with strips Sets the size of the search road V. Zutshi, ICLC04, Paris 1/18/2019

Pairwise ‘Efficiency’ 1cm wide strips Pairwise ‘Efficiency’ V. Zutshi, ICLC04, Paris 1/18/2019

1cm wide strips ‘Rejection’ V. Zutshi, ICLC04, Paris 1/18/2019

For >99% efficiency…. V. Zutshi, ICLC04, Paris 1/18/2019

Current Guess “Fine” section (8 layers) 2cm Steel, 0.5 cm thick scintillator Following “coarse” section (8 layers) 10cm Steel, 0.5 cm scintillator 5cm wide strips, 1m long Tyvek wrapping Alternating x-y orientation Si-PM photo-detection V. Zutshi, ICLC04, Paris 1/18/2019

Fermi-NICADD Extruder Line 10cm wide, 5mm thick Fermi-NICADD Extruder Line V. Zutshi, ICLC04, Paris 1/18/2019

First Measurements V. Zutshi, ICLC04, Paris 1/18/2019

Uniformity V. Zutshi, ICLC04, Paris 1/18/2019

Separation Grooves Provides better rigidity Epoxy/paint mixture 1 2 3 4 5 Epoxy/paint mixture V. Zutshi, ICLC04, Paris 1/18/2019

Response V. Zutshi, ICLC04, Paris 1/18/2019

X-talk V. Zutshi, ICLC04, Paris 1/18/2019

Response and Strip Fabrication V. Zutshi, ICLC04, Paris 1/18/2019

Uniformity Scan V. Zutshi, ICLC04, Paris 1/18/2019

Strips Wrapped in Tyvek Each strip wrapped in 2 layers of Tyvek Strips Wrapped in Tyvek Compare to separation groove V. Zutshi, ICLC04, Paris 1/18/2019

S/N Signal amplitude Noise amplitude MRS Si-PM V. Zutshi, ICLC04, Paris 1/18/2019

15 p.e. Strip Light Yield V. Zutshi, ICLC04, Paris 1/18/2019

Summary/Plans 5mm thick Fermi-NICADD produced extruded strips used in combination with Si-PM/MRS adequate for tail-catcher/muon tracker. Strip-fiber configuration nearly finalized. Putting together mechanical module to understand and resolve assembly issues. Talking with Fermi for cart design and construction. V. Zutshi, ICLC04, Paris 1/18/2019