Thoughts on TPC Optimization Xin Qian BNL 1. Outline Detector Parameters – TPC angle – Wire pitch – Wire angle – Wire pattern – Wire plane gap Basic reconstruction.

Slides:



Advertisements
Similar presentations
0 - Electron Discrimination in Liquid Argon Time Projection Chamber.
Advertisements

CBM Calorimeter System CBM collaboration meeting, October 2008 I.Korolko(ITEP, Moscow)
Proposal for a new design of LumiCal R. Ingbir, P. Ruzicka, V. Vrba October 07 Malá Skála.
Analysis for J2 chamber Yousuke Kataoka (University of Tokyo) Atsuhiko Ochi, Yuki Edo (Kobe University) 11 / 12 / 2012 Micromegas weekly meeting 1.
The performance of Strip-Fiber EM Calorimeter response uniformity, spatial resolution The 7th ACFA Workshop on Physics and Detector at Future Linear Collider.
May 14, 2015Pavel Řezníček, IPNP Charles University, Prague1 Tests of ATLAS strip detector modules: beam, source, G4 simulations.
Simulation Studies of a (DEPFET) Vertex Detector for SuperBelle Ariane Frey, Max-Planck-Institut für Physik München Contents: Software framework Simulation.
Standalone VeloPix Simulation Jianchun Wang 4/30/10.
Off-axis Simulations Peter Litchfield, Minnesota  What has been simulated?  Will the experiment work?  Can we choose a technology based on simulations?
Introduction to Hadronic Final State Reconstruction in Collider Experiments Introduction to Hadronic Final State Reconstruction in Collider Experiments.
Introduction to Hadronic Final State Reconstruction in Collider Experiments Introduction to Hadronic Final State Reconstruction in Collider Experiments.
Far Detector Fiducial Volume Studies Andy Blake Cambridge University Saturday February 24 th 2007.
The Origins of X-Rays. The X-Ray Spectrum The X-Ray Spectrum (Changes in Voltage) The characteristic lines are a result of electrons ejecting orbital.
Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope J.D. Zornoza 1, A. Romeyer 2, R. Bruijn 3 on Behalf of the ANTARES Collaboration 1.
Jianchun Wang Marina Artuso Syracuse University 11/06/00 MC Simulation of Silicon Pixel Detector.
LBNE R&D Briefing May 12, 2014 LBNE R&D Briefing May 12, 2014 LArIAT and LBNE Jim Stewart LArIAT EPAG Chair BNL LBNE LARIAT-EPAG J. Stewart BNL T. Junk.
SPiDeR  First beam test results of the FORTIS sensor FORTIS 4T MAPS Deep PWell Testbeam results CHERWELL Summary J.J. Velthuis.
Atmospheric Neutrino Oscillations in Soudan 2
Study of FPCCD Vertex Detector 12 Jul. th ACFA WS Y. Sugimoto KEK.
Tracking within hadronic showers in the SDHCAL Imad Laktineh.
Status of DRIFT II Ed Daw representing the DRIFT collaboration: Univ. of Sheffield, Univ. of Edinburgh, Occidental College, Univ. of New Mexico Overview.
PERFORMANCE OF THE MACRO LIMITED STREAMER TUBES IN DRIFT MODE FOR MEASUREMENTS OF MUON ENERGY - Use of the MACRO limited streamer tubes in drift mode -Use.
Status of W analysis in PHENIX Central Arm Kensuke Okada (RBRC) For the PHENIX collaboration RHIC Spin Collaboration meeting November 21, /21/20091K.Okada.
A study of systematic uncertainties of Compton e-detector at JLab, Hall C and its cross calibration against Moller polarimeter APS April Meeting 2014 Amrendra.
Chevron / Zigzag Pad Designs for Gas Trackers
EAS Reconstruction with Cerenkov Photons Shower Simulation Reconstruction Algorithm Toy MC Study Two Detector Configuration Summary M.Z. Wang and C.C.
Yosuke Watanabe….. University of Tokyo, RIKEN A, KEK C, Development of a GEM tracker for E16 J-PARC 1 Thanks to ???????????
Poster Design & Printing by Genigraphics ® Neutrino Interactions Studying the properties of neutrinos will shed light on the origin of the.
1 Energy loss correction for a crystal calorimeter He Miao Institute of High Energy Physics Beijing, P.R.China.
1 Calorimeter in G4MICE Berkeley 10 Feb 2005 Rikard Sandström Geneva University.
Simulation of Beam-Beam Background at CLIC André Sailer (CERN-PH-LCD, HU Berlin) LCWS2010: BDS+MDI Joint Session 29 March, 2010, Beijing 1.
1 Performance of a Magnetised Scintillating Detector for a Neutrino Factory Scoping Study Meeting Rutherford Appleton Lab Tuesday 25 th April 2006 M. Ellis.
LM Feb SSD status and Plans for Year 5 Lilian Martin - SUBATECH STAR Collaboration Meeting BNL - February 2005.
Secondary Vertex reconstruction for the D + Elena Bruna University of Torino ALICE Physics Week Erice, Dec. 6 th 2005.
David Finley, Fermilab / October 3, 2005 on LArTPC Slide 1 LArTPC: Large Liquid Argon TPC for the NuMI Off-axis Beam First Point: Try to recognize intellectually,
Bangalore, India1 Performance of GLD Detector Bangalore March 9 th -13 th, 2006 T.Yoshioka (ICEPP) on behalf of the.
3D Event reconstruction in ArgoNeuT Maddalena Antonello and Ornella Palamara 11 gennaio 20161M.Antonello - INFN, LNGS.
Bartol Flux Calculation presented by Giles Barr, Oxford ICRR-Kashiwa December 2004.
Jonathan BouchetBerkeley School on Collective Dynamics 1 Performance of the Silicon Strip Detector of the STAR Experiment Jonathan Bouchet Subatech STAR.
K.T. McDonald  BooNe Electronics Meeting Jan. 13,  BooNE Comments on  BooNE Readout Parameters Based on the Electronics Meeting of Jan. 7, 2009.
November 4, 2004Carl Bromberg, FNAL LAr Exp. Workshop Nov. 4-6, Liquid argon as an active medium Carl Bromberg Michigan State University & Fermilab.
Goddard February 2003 R.Bellazzini - INFN Pisa A new X-Ray Polarimeter based on the photoelectric effect for Black Holes and Neutron Stars Astrophysics.
1 Nick Sinev, ALCPG March 2011, Eugene, Oregon Investigation into Vertex Detector Resolution N. B. Sinev University of Oregon, Eugene.
1 Constraining ME Flux Using ν + e Elastic Scattering Wenting Tan Hampton University Jaewon Park University of Rochester.
Muons at CalDet Introduction Track Finder Package ADC Corrections Drift Points Path Length Attenuation Strip-to-Strip Calibration Scintillator Response.
meeting, Oct. 1 st 2015 meeting, Oct. 1 st Gas Pixel: TRD + Tracker.
Scan Rules Introduction –Overview –Justification –Approach Neutrino Event Type Assignment –Strategy –Muon-Flavor Reaction (mu) Type –Electron-Flavor Reaction.
1 Limitations in the use of RICH counters to detect tau-neutrino appearance Tord Ekelöf /Uppsala University Roger Forty /CERN Christian Hansen This talk.
18 Sep 2008Paul Dauncey 1 DECAL: Motivation Hence, number of charged particles is an intrinsically better measure than the energy deposited Clearest with.
Small, fast, low-pressure gas detector E. Norbeck, J. E. Olson, and Y. Onel University of Iowa For DNP04 at Chicago October 2004.
David Finley / PPD Engineering Meeting / June 24, Fermilab Slide 1 R&D Toward Large Liquid Argon Time Projection Chambers “Large” means up to 100.
BESIII offline software group Status of BESIII Event Reconstruction System.
Introduction to Hadronic Final State Reconstruction in Collider Experiments Introduction to Hadronic Final State Reconstruction in Collider Experiments.
Lessons Learned from Real Data Xin Qian BNL 1. Outline Space Charge effect for LArTPCs on surface Field Response Calibration How to deal with noises and.
View of TPC Optimization from Reconstruction Working Group Xin Qian and Tingjun Yang 1.
Recent Progress on Wire-Cell Xin Qian and Chao Zhang BNL 1.
Low-energy Sim/Reco Capability Xin Qian (BNL) Tingjun Yang (FNAL) 1.
By: Daniel Coelho Matthew Szydagis Robert Svoboda Improving Electron / Gamma Separation LBNE Software Fermilab, ILFebruary 1, 2013.
1 straw tube signal simulation A. Rotondi PANDA meeting, Stockolm 15 June 2010.
High Energy Physics experiments.
Activities on straw tube simulation
Comparison of GAMMA-400 and Fermi-LAT telescopes
GLAST LAT tracker signal simulation and trigger timing study
HARPO Analysis.
Detector Configuration for Simulation (i)
5% The CMS all silicon tracker simulation
Study of dE/dx Performance in TPC at CEPC
Special Considerations for SIDIS
p0 detection and reconstruction with the
A. Menegolli, University of Pavia and INFN Pavia
Presentation transcript:

Thoughts on TPC Optimization Xin Qian BNL 1

Outline Detector Parameters – TPC angle – Wire pitch – Wire angle – Wire pattern – Wire plane gap Basic reconstruction – Charge resolution – Position resolution – Image reconstruction quality High level physics – Particle identification – Resolution 2

Gain and Shaping Time Optimization for Cold Electronics 3

time Overview of Signal Processing 4 Number of ionized electrons Signal on Wire Plane Field Response Signal to be digitized by ADC Electronics Response High-level tracking … (Deconvolution) V. Radeka TPC signal consists of time and charge information from induction and collection planes Same amount charge was seen by all the wire planes

Deconvolution 5 Fourier transformation Time domain Frequency domain Back to time domain Anti-Fourier transformation Time Domain Frequency Content Deconvoluted Signals The goal of deconvolution is to help extract charge and time information from TPC signals Bruce Baller developed during Argoneut

Field and Electronics Response 6 Cold electronics: 4 shaping time (0.5, 1.0, 2.0, 3.0 us) 4 gain (4.7, 7.8, 14, 25 mV/fC) Leon, SLAC Charge vs. Time averaged for a single electron Difference between simulation and data (bigger signal in LongBo arXiv:1504:00398)

Discussion about Noise There are two components of noise – Electronic noise (ENC) The signal to noise ratio does not depend on the gain Longer shaping time has smaller noise Longer shaping time has slightly worse two-peak separation – Digitization noise due to 12-bit ADC At 3 ms and 4.7 mV/fC, the electronic noise at collection plane is expected to be 0.58 ADC 1/sqrt(12.) ~ 0.29 ADC 11.7 ENOB  1.23/sqrt(12.) ~ bit ADC is enough so that “digitization noise” << “electronic noise” 7

Discussion about Gain and Shaping Time The choice of gain will not affect the signal to noise ratio – Higher gain could lead to more chances of overflow – Also need to take into account the zero-suppression algorithm Longer shaping time would – Increase the size of signal higher chance to overflow – Reduce noise, thus increase signal/noise ratio – Slightly worse two-peak separation (difference between 2.5 and 3 us) – Also less digitization time (Nyquist: T shaping >= 2 T digitization ) Less data 8

Optimization of Field Response Functions 9

Gap between Wire Plane, Bias Voltage, and Grid Plane The raw signal (digits) consists of both signal and (electronic) noise – An ideal deconvolution will recover signal completely  number of electrons reached – The deconvolution on the electronic noise will thus determine the signal to noise ratio – Change in the gap distance and bias voltage will change  response function R  signal to noise ratio – To be worked out 10

MicroBooNE Case In MicroBooNE, the second induction plane has the worst signal to noise ratio 11 Jyoti Joshi

Some Questions Preliminary results for 1D deconvolution What’s the impact of dynamic induced charge? – Data validation 12

TPC Angle(I) LArTPC High density (Z ~ 18) – Event are more compact Parallel wire readout w.r.t. the beam direction – More ambiguities Slow detector response (~ms) – Challenges in rejecting cosmics for detector on surface Ultra-high resolution – A layer ~ 3.5% X 0 (14 cm R.L.) Higher physics requirement – ~ 80% efficiency Liquid Scintillator Low density (Z ~ 6) Perpendicular wire readout w.r.t. the beam direction Fast detector response (~10 ns) High resolution – A layer ~ 0.15 X 0 (44 cm) ~35% efficiency in NOνA 13

TPC Angle (II) In a neutrino event, because of incident neutrino energy, the entire event is more boosted toward forward region Due to nucleon response, the lepton tends to going more forward in the center-of-mass frame TPC with wire readout has more trouble to reconstruct “tracks” which are parallel to the wire plane  charges arrive at various wire-plane at same time  ambiguity to figure out the proper correlation bee/set/4/event/2/ 14

Detector Angle cell/bee/set/7515fe16-d163-4df8-ad87- 09f7c809dc7e/event/0/ cell/bee/set/7515fe16-d163-4df8-ad87- 09f7c809dc7e/event/0/ Same events (rotate 0-19 degrees) – Event 0  0 degrees – Event 10  10 degrees – Event 19  19 degrees 15

16 0 degrees 10 degrees One can click the web-site to look at events in 3D and rotate to get a better understanding. 10 degrees (truth)

17 19 degrees10 degrees MC truth: one electron, one neutral pion, and one positve pion

First Look at the TPC Orientation Generated by GENIE Look at the electron angle for two configurations: default vs. 10 degrees rotation Integrated over all the energy, oscillation added ~ 20 % effect at the 0 degrees with rotating 10 o Effect is expected to be strongly energy-dependent – Right plot shows the expected distribution at Argoneut (5-6 GeV) energy 18

Questions How to evaluate which angle is good enoug? Is perpendicular wire-readout completely hopeless? Can we add in intended distortion in electric field? – How to calibrate its effect? 19

Wire Pitch’s impact on Charge For a electron drift at different locations within a wire pitch – Field response has a strong dependence on the location of electron Deconvolution was performed with average field response Large wire pitch  smaller (electronic) noise to signal ratio  smaller resolution Large wire pitch  larger spread at response function  larger resolution 20

Questions What’s the expected charge resolution and its dependence on the wire pitch? How important is dynamic induced charge effect? How to calibrate the 2D response function? 21

About Wrapping (Wire Angle) Wire angle would impact the wire wrapping scheme What’s the problem of wire wrapping? – The wrapping of wire would lead to more crossings of wires  the wires originally won’t cross can cross with wrapping  the crossing of wires will introduce ambiguities 22 True Hits Fake Hits u1 u2 v2 v3 At fixed time v1 H1 H2 H3 H4 H5 H6 The amount of ambiguities strongly depends on the event activity For a simple track, it is not a problem For multiple tracks, more difficult For showers, much more difficult For shower + track + crossing APA  extremely difficult Wire-cell imaging step is an ideal tool to study this (use both charge and time to do reconstruction)

Wire Pitch/Angle on Position Resolution Along the drift direction, the digitization length is 0.5 us * 1.6 mm/us  V/cm – Average diffusion σ=0.9 mm for 2.5 m drift distance – Signal shaping time 2 us  2 us / 2.45 * 1.6 ~ σ=1.3 mm For wire plane, the digitization length is related to the wire pitch (3 ~ 5 mm) – For a continuous track, not a problem to calculate dE/dx – For the end points of track, the resolution in “dx” is about “0.3 * L” – Perpendicular to vertical wire: L = wire pitch – Parallel to vertical wire: L ~ (wire pitch)/sin(theta) – Consequences in short tracks (PID, angle, energy through range …) – Gap identification (i.e. for e/gamma separation) Likely need “2 * L” to identify a gap 23 θ

More about Gap Identification Radiation length ~ 14 cm  for high-energy photon, the mean free path 9/7 * 14 ~ 18 cm Assumption – Along the drift direction: 4 us for two-peak separation – Perpendicular to drift direction  2 * L 24 Observations: 3 mm  5 mm, gap identification efficiency is reduced by about 2.x% ~ (1- exp(-4/180)) ~60% more background 36  45 degrees, the impact of gap identification efficiency is one order smaller Also varied pitch for different planes (Maxim)

Discussions For bigger wire pitch, the gap identification efficiency will be reduced without a doubt – 3 mm  5 mm wire pitch leads to about 2.2 % reduction in efficiency – But this number corresponds to ~60% more background There are three weapons to differentiate electron from gamma: – Gap identification – dE/dx (initial track is about 3 cm long, what’s the impact of wire pitch?) – Shower topology (i.e. gamma is always from neutral pion decay, thus multiple gammas) The real question is “which wire pitch is good enough to reject background?” Also engineering considerations – Will small wire pitch leads to more chance of wire touching and high noise? 25

These two would explain the shape of dE/dx plot 26 Compton Scattering I calculated 5 cm mean free path based on moller scattering cross section, cross checked with MC

e/gamma separation dE/dx Compton ~ Z Pair production ~ Z^2 Compton scattering could lead to confusion of dE/dx 27

Summary From reconstruction point of view, the priority (from high to low) is – TPC angle (5-10 degrees from the beam direction) Within this range, larger angle is better When will be enough (i.e. increment is modest)? – Wire Pitch (gap identification, dE/dx) 3 mm is better Will 5 mm be enough? – Wire Angle (reduce ambiguity, position resolution) To be studied – Wire gap and bias voltage (charge resolution) To be studied 28