M. Dugger, February 2012 1 Triplet polarimeter study Michael Dugger* Arizona State University *Work at ASU is supported by the U.S. National Science Foundation.

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Presentation transcript:

M. Dugger, February Triplet polarimeter study Michael Dugger* Arizona State University *Work at ASU is supported by the U.S. National Science Foundation

M. Dugger, February Outline Triplet production Potential detector Event generator Comparison to previous triplet polarimeter Absolute polarization uncertainty for 4 hours of running Estimate of accidentals Testing a triplet polarimeter

M. Dugger, February Triplet production Pair production off a nucleon: γ nucleon → nucleon e + e -. For polarized photons σ = σ 0 [1 + PΣ cos(2φ)], where σ 0 is the unpolarized cross section, P is the photon beam polarization and Σ is the beam asymmetry Triplet production off an electron: γ e - → e R - e + e -, where e R represents the recoil electron Any residual momentum in the azimuthal direction of the e - e + pair is compensated for by the slow moving recoil electron. This means that the recoil electron is moving perpendicular to the plane containing the produced pair and can attain large polar angles.

M. Dugger, February Potential detector 96mm 48mm FrontBack Front: 4 sectors 16 strips/sector Back: 16 sectors Cost: $7500 (back stock) Manufacturer: Micron Semiconductor S1

M. Dugger, February Sample geometry 48mm 24mm eReR e+e+ e-e- converter Setting the detector distance from converter such that the largest polar angle measured is 45 o (results in θ min ~ 26 o )

M. Dugger, February Event generator Richard Jones provided an event generator that calculates QED tree level Feynman diagrams

M. Dugger, February kinetic energy of recoil versus polar angle for 26 o < θ < 45 o and E γ = 9 GeV Kinetic Energy (GeV) θ R (degrees)

M. Dugger, February Triplet asymmetry fits 10 million generated events using Richard’s code E γ = 9.0 GeV Fit each ring separately Fit function: A[1 + Bcos(2φ)] φ

M. Dugger, February Triplet asymmetry fit results A[1 + Bcos(2φ)] Parameter B from fit Results fairly consistent over ring number (inner most ring number = 1) Zero order fit: 22.7 ± 0.1 B Ring number

M. Dugger, February Comparison of GEANT4 study of triplet polarimeter to previous study The SAL detector δ-rays Pair to triplet ratio ASU simulation of SAL Could SAL have been modified to work in the Hall-D environment?

M. Dugger, February The GW SAL detector E γ = 220 to 330 MeV 2 mm scintillator converter Polarimeter located ~39 cm downstream of converter Recoil θ = 15 to 35 degrees Recoil φ = 0, 90, 180, 270 degrees with Δφ = 44 degrees Analyzing power at the event generator level = 12% Analyzing power from simulation 3-4% (post experiment) Measured analyzing power = 2.7% Quick check - Can ASU reproduce the GW results?

M. Dugger, February δ-ray comparison with Iwata 1993 simulation E δ is δ-ray kinetic energy after traveling through 1 mm of scintillator using Iwata’s polar geometry and scintillator widths BLUE: Current ASU GEANT4 results RED: Iwata GEANT3 (scaled to GEANT4 results by ratio of signal integration) Shapes of the distributions look similar E δ (MeV) ASU simulation E γ = 300 MeV Iwata simulation E γ = 250, 365, 450 MeV Note: ASU simulation did not wrap scintillators

M. Dugger, February NIST cross sections for triplet and pair production off carbon σ pair /σ triplet : 300 MeV 9.0 GeV Ratio does not vary much over large energy range

M. Dugger, February Comparison of ASU MC of SAL detector to GW results Note: ASU results are for E γ = 300 MeV and GW is of E γ = 220 to 330 MeV Analyzing power: At event generator level: 12.6 ± 0.1 % ASU; ~12% GW (no error reported) ASU simulation: 2.65 ± 0.05% ASU simulation (30 μm Al wrapped scintillators): 2.8 ± 0.1 % GW experiment: 2.7% (no error reported) GW simulation: 3-4% (range given with no error reported) ASU results are in agreement with the GW results for the SAL detector ☺

M. Dugger, February How could the SAL detector be modified to work in Hall-D environment?

M. Dugger, February Dependence of analyzing power on ΔE pair for 16 sector detector Same parameters as previous best configuration but now with 16 sectors instead of 4 paddle SAL design Analyzing power fairly constant for ΔE pair < 1750 MeV The 16 sector design increases the analyzing power to 19.1 ± 0.7 % from 17.5 ± 0.3 % of the 4 paddle design (ΔE pair < 1500 MeV) ΔE pair (MeV) Analyzing power (%)

M. Dugger, February Recap of modifications that would make SAL type detector work in Hall-D

M. Dugger, February Study of converter thickness, and placement of triplet polarimeter, to the absolute error in polarization measurement

M. Dugger, February Detector eReR e+e+ e-e- converter Figure not to scale 3cm scintillator 2.4 cm

M. Dugger, February Energy cut KE (MeV) θ cutoff energy = 0.5 MeV Cutoff energy of 0.5 MeV won’t cut out good recoil- electron events

M. Dugger, February NIST cross sections for triplet and pair production off Lithium σ pair /σ triplet : 300 MeV 9.0 GeV Ratio more favorable than when using carbon 9GeV) Will use lithium converter from here on

M. Dugger, February Radiation lengths of Li converter (10 -4 ) θ MAX Analyzing power (%) Rate surviving cuts (Hz) θ MAX Converter thickness and polarimeter placement study (slide 1)

M. Dugger, February Absolute polarization uncertainty in 4 hours of running σ p (for 4 hours) Radiation lengths (10 -4 ) θ MAX Assumed where N ≡ Rate * 4 hour, P ≡ Polarization = 0.4, and α ≡ analyzing power

M. Dugger, February Estimate of accidentals for the triplet polarimeter

M. Dugger, February GHz total rate 99 MHz rate E γ (GeV) Collimated photon distribution Potential accidentals Used Richard’s cobrems_root code to create shape of E γ distribution (top panel) Used shape of E γ to generate 1 million events (bottom panel) that were fed into the triplet-polarimeter Monte Carlo Rate (GHz) Counts

M. Dugger, February Accidental estimate For 1 million events thrown (N T ) there were 177 events seen (N S ) on the polarimeter Assumed a lithium converter of radiation lengths Total expected photon rate: R γ = 3.3 GHz Expected total photon rate seen on device: R S = R γ *(N S /N T ) = 3.3GHz*(177/1million) = 584 kHz Expected number of polarimeter hits for a 20 ns window: = R S *20ns = Probability of accidental coincidence between pair spectrometer and polarimeter: P acc = 1 – P 0 ( ) = 1.2 %

M. Dugger, February Testing a triplet polarimeter

M. Dugger, February Possibility of testing a device at Mainz Ken Livingston suggested trying to test a device similar to the ASU design at Mainz Ken might be able to borrow a ring detector (Micron semiconductor S2 design) Ken already has designed electronics that can read out the ring detector with possibility of timing widow as small as 20 ns Need to see if we can put all the pieces together and get permission for a parasitic test run at Mainz

M. Dugger, February Potential detector to borrow 70mm 22mm FrontBack Front: 4 sectors 48 rings/sector Back: 16 sectors Very similar to current ASU design Front: 4 sectors 16 rings/sector Back: 16 sectors S2

M. Dugger, February Expected Mainz photon polarization Distribution provided by Ken Livingston Electron beam energy = 1500 MeV Coherent edge = 600 MeV The rest of the slides will assume a 500 MeV photon beam with Polarization = 0.47 Polarization E γ (MeV) = 0.47 Should be able to use a much finer energy binning than what is shown on the plot, but just simulating a single energy for now

M. Dugger, February Dependence of analyzing power on ΔE pair for S2 geometry at Mainz photon energy Converter is radiation lengths of lithium No energy cut Symmetric pair definition of ΔE pair < 200 MeV seems reasonable and is used from here on Max(ΔE pair ) (MeV) Analyzing power (%)

M. Dugger, February Simulation results φ (degrees) cross section weighted counts Assumed collimated photon rate (over 200 MeV range) : 4.8x10 7 Hz Electron rate on device that survive cuts: 9 Hz Δt = 4 hours Analyzing power: 0.136(6) Polarization uncertainty: 0.029