Optical Reconstruction of Proton Decay Events π " β πΏ " πΜ Kevin R. Wood kevin.wood@stonybrook.edu June 22, 2016
Overview β’ Characterization of photon detectors + reconstruction performance. Revisiting studies done last year* with 200MeV energy deposition and simulated information. Now we take advantage of reconstructed proton decay events. β’ Attenuation length β’ Reconstruction efficiency (flash finding) β’ And, additionally, timing resolution β’ PDK photon reconstructed signals β’ Towards incorporating PD information into PDK background rejection β’ Effect of radiological activity * http://lbne2-docdb.fnal.gov:8080/cgi-bin/RetrieveFile?docid=10896&filename=2015-05-19- Himmel-PDSim-Review.pdf&version=6 6/22/16 Optical Reconstruction of PDK Events 2
π " β πΏ " πΜ sample β’ Gabriel Santucci has generated, simulated, and reconstructed a sample of 10,000 βgolden channelβ proton decay events β’ /pnfs/dune/persistent/users/gsantucc/correct_flat_dist/reco/8011111_*/p2K+nuba r_2_g4_detsim_reco.root β’ Uniformly distributed inside the 1x2x6 geometry β’ Reconstructed using standard configurations (v05_13_00) β’ standard_reco_dune10kt_1x2x6.fcl 6/22/16 Optical Reconstruction of PDK Events 3
π " β πΏ " πΜ sample π " π " πΏ " 0.4 GeV π " β π " π ' π * π " β πΏ " π ' πΏ " β π " π * ( π - ~10 12 π‘ π * ~10 14 s πΆπ = 63.5% 6/22/16 Optical Reconstruction of PDK Events 4
(A. Himmel) Attenuation Energy deposited into the central region of the APA (yz plane); uses photon library information LHS incorporates APA edge effects and reconstruction β’ Reconstructed information from PDK suggest an attenuation length of ~114 cm while the β’ photon libraries give ~136cm 6/22/16 Optical Reconstruction of PDK Events 5
Optical Reconstruction Efficiency β’ How often do we reconstruct a flash given a PDK event? (5PE threshold) PDK 200 MeV (A. Himmel) β’ Covers everything at >97.5% efficiency (early + late light). >99% until last ~13cm. β’ Appreciable portion of Kaons deposit <200MeV, which affects our flash finding. 6/22/16 Optical Reconstruction of PDK Events 6
Optical Reconstruction Efficiency β’ Threshold for flash finding on the previous slide was set to 5 PE. β’ Radiological backgrounds (and noise levels) dictate where this threshold should be set. 39 Ar The effect that the presence of 39 Ar has on (From 10K PDK) 2 PE threshold finds everything efficiency/purity will be studied in more detail. 6/22/16 Optical Reconstruction of PDK Events 7
Timing Resolution β’ Important for non-beam events β’ PD gives us T 0 and therefore X coordinate (distance from APA) β’ (t true is the time associated with the Kaons) β’ Time resolution O(10 ns) β’ TDC DAQ sampling rate of 500 ns would make this negligible 6/22/16 Optical Reconstruction of PDK Events 8
PE Yield vs. Kaon Momentum β’ Characteristic photon yield from PDK ranges from a few hundred PEs to a few thousand PEs β’ Can we use PD information to help separate PDK from backgrounds (e.g. atmospheric, cosmogenic)? 6/22/16 Optical Reconstruction of PDK Events 9
Summary/Moving Forward β’ Weβve improved upon some initial estimations of the PD performance with a sample of π " β πΏ " πΜ events β’ Non-beam events drive the PD requirements β’ Found reasonable agreement, but some expected deviations from the cruder study (200 MeV, no reconstructed information) β’ ~114cm attenuation length β’ >99% reconstruction efficiency in all but the last ~15 cm furthest from the APA where it dropped to ~97.5% β’ Time resolution O(10 ns) β’ Begin incorporating radiologicals and cosmogenics into the study β’ Also start thinking about incorporating PD information into PDK signal/background separation (see A. Higueraβs work) 6/22/16 Optical Reconstruction of PDK Events 10
Backup (new) vertex distribution If you have been using the PDK sample G. Santucci has produced, make sure you are using the newly (in the past week or two) generated sample with these vertex distributions. See slide 3 for location. Old vertex distribution on next slide.
Backup (old) vertex distribution This is from the sample that lives in /pnfs/dune/persistent/users/gsantucc/bugfix/* β’ β’ Gaussianβ¦ why? β’ Buildup on detector edge: most of these tracks will exit the detector. β’ If you happen to be using it... donβt. Should be deleted soon
Recommend
More recommend
