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1 Using the pHE data to measure the beam e ’s from + decay David Jaffe and Pedro Ochoa April 12 th 2007 Reminder Systematic from background Horn 1 systematics Conclusion
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2 Reminder x parLE ( + ) pHE ( ,K) pHE - ( ,K) LE x parHE ( + ) LE Procedure: - Take pHE-LE difference. Correct for - Fit using MC shapes. Scale ( + ) LE and ( + ) pHE by parameters parLE and parHE. Recent study showed that this procedure yields a ~13% statistical error when applied to the ~2x10 19 POT of existing pHE data (doc-2783) Need to assess systematics associated with this measurement. Two main concerns: C= ( ,K) pHE - ( ,K) LE correction. Background in nubar selection. both addressed in this talk
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3 Expanded feasibility study to include background: Background in pHE and LE samples obtained with the nubar-PID cut at 0.9 (mostly CC neutrinos; see doc 2783) ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE Bkgd. pHE Bkgd. LE Systematic from background Please note that vertical scale is not the same in all 6 plots
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4 Create fake data in which background level is shifted by a given amount. Fit is done assuming nominal background levels: Results: Shifting only LE backgroundShifting only pHE background Background shifted by +10%-10%+30%-30%+50%-50%+10%-10%+30%-30%+50%-50% Bias in parLE +2%-2%+7%-7%+12%-13%-2%+3%-8%+8%-13%+13% Bias in parHE -0%+0%-0%+0%-0%+0%+3%-2%+7%-7%+12%-12% Background shifted by +10%-10%+30%-30%+50%-50% Bias in parLE -0%+0%-1%+0%-1%+1% Bias in parHE +2%-2%+7%-7%+11%-12% If shift is in same proportion & direction for the two backgrounds then bias in parLE is considerably reduced: Example: parHE background shifted up by 10% ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE Bkgd. pHE Bkgd. LE (These are scaled to 2.0x10 20 POT)
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5 It seems background is not that big of a problem. Tools like the MuonChopper may assist us in determining this error. (minos-doc 2841) Main concern is C = ( ,K) pHE - ( ,K) LE : Work by David suggests differences are due mostly to geometry, as one would expect: Note: nomenclature and drawing follow scheme for focussing Horn 1 systematics
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6 Ex: horn1 current increase by 2% in pHE neutrino beam First obtained ratios of spectra with systematics over nominal spectra: Recommended in minos-doc-1283 Used for this study horn 1 offset1.0 mm4.0 mm horn 1 angle0.2 mrad0.4 mrad horn current offset1.0 %2.0 % Using gnumi, looked at the effect of varying the following horn1 parameters: Then converted these ratios to reconstructed energy using the ntuples: Good agreement with pbeam Ex: horn1 current increase by 2% in pHE antineutrino beam Note: scale is different than above Convert to E reco Might have been too pessimistic. See conclusion
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7 The obtained ratios for the antineutrinos with hadron parents are: The ratios are smoothed due to lack of statistics. LE-10 pHE
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8 LE-10 pHE But also have to consider effect on antineutrinos with muon parents: Large effect ! + ’s depend directly on focusing.
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9 Applied these systematics in our feasibility study: The nominal spectra are used to do the fit. Assume infinite pHE and LE statistics. Horn current shift -2%: Systematics: Results of fit: ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE with systematics result of fit ( + ) pHE ( + ) LE fit pHE-LE corrected for background and nominal C Bias of -18.0% Bias of -21.9% with systematics nominal
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10 Horn current shift of +2%: Systematics: ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE Results of fit: with systematics nominal with systematics result of fit ( + ) pHE ( + ) LE fit pHE-LE corrected for background and nominal C Bias of -26.8% Bias of -67.2%
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11 Horn angle shift by 0.4mrad: Bias of -7.2% Bias of -16.9% Systematics: ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE Results of fit: with systematics nominal with systematics result of fit ( + ) pHE ( + ) LE fit pHE-LE corrected for background and nominal C
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12 Horn offset by 4mm: Bias of -35.7% Bias of -66.1% Systematics: ( + ) pHE ( + ) LE ( ,K - ) pHE ( ,K - ) LE Results of fit: with systematics nominal with systematics result of fit ( + ) pHE ( + ) LE fit pHE-LE corrected for background and nominal C
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13 It seems that worse sources of systematics are increase in horn current and horn offset: Also need to add the error associated with hadron production. Work is in progress to assess it. Horn I -2%Horn I +2%Horn angle 0.4mrHorn offset 4mm Bias in parLE-18.0%-26.8%-7.2%-35.7% Bias in parHE-21.9%-67.2%-16.9%-66.1% This assumed same horn conditions for pHE and LE running. If that is not the case need to blend with other combinations & scenarios: Horn I -2%Horn I +2%Horn angle 0.4mrHorn offset 4mm Applying systematics to LE beam only Bias in parLE+4.8%-9.1%-2.0%-19.8% Bias in parHE+9.5%-4.5%-2.6%-7.6% Applying systematics to pHE beam only Bias in parLE-24.9%-24.8%-4.7%-17.8% Bias in parHE-34.7%-46.9%-14.2%-58.8% + recently discovered target z position offset of ~1cm between the two LE-10 datasets
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14 The geometric systematics associated with the measurement of ( + ) LE seem to be very large. However, a recent discussion between Sacha and David revealed that the assumed horn 1 systematics were too pessimistic. Study will have to be repeated using horn 1 offset of 1mm and horn current shift of ±1% In addition, maybe can improve situation by modifying fit: Ignore 15-30 GeV region where systematics which pull parLE (and parHE) down are largest? Use information at > 30 GeV to constrain the fit? Add an extra parameter to scale the C correction up and down? Summary & Ongoing work Measurement of ( + ) pHE seems severely hampered by systematics. Fortunately we don’t care.
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