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1 A preliminary estimate of the beam e ’s from antineutrinos David Jaffe, Pedro Ochoa December 7 th 2006
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2 Data used: Horn-off: LE-10, Birch, 2.77x10 18 POT (couple of days Feb-2006) Horn-on: LE-10, Birch, 8.15x10 19 POT (Oct 2005 -Jan 2006) MC used: Horn-off: LE010000, Carrot, 1.32x10 19 POT Horn-on: LE010185, Carrot, 4.17x10 19 POT Data and MC used
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3 Preliminary results of from +: from + decay E < E cut data-(Fit or Scaled) MC, E cut < E < 30 GeV raw MC1553.7 ± 55.1 (stat)283.0 ± 23.0 (stat) reweighed MC1538.2 ± 54.8 (stat)386.5 ± 32.4 (stat) Scale method 14685.4 ± 367.4 (stat)-5914.9 Scale method 24628.8 ± 367.8 (stat)-5991.6 Stan’s method3163.6 ± 1122.0 (stat)-243.5 ± 1169.1 (stat) Scale method 33820.2 ± 374.5 (stat)584.3 ± 339.5 (stat) Scale method 46392.8 ± 355.1 (stat)412.4± 341.4 (stat) Fit method1735.5 ± 380.3 (stat)-357.1 ± 351.8 (stat) Note: talked with Zarko about using new neutrino-antineutrino combined fit in modified energy range for nubars. In progress. Should be real nubars from + if data/MC from horn-off is trust- worthy in this region Should be ~0 by construction Should be real nubars from + Expected to be highly negative by construction Details can be found in backup slides and in minos-docs 2421 and 2218).
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4 Systematics In addition, uncertainties when going from to e : from + selection efficiency: no systematic yet. ( )/ ( e ): Error in fit: no current estimate for SKZP “a la Boston” with antineutrinos. Will have one with new fit. How accurate is the Horn-off disagreement between data and MC to scale the Horn-on MC? No systematic yet Purity of antineutrino sample: see minos-doc-2205 For the atmospheric paper, Hugh G. estimated 13.5 % uncertainty in ( )/ ( ) (see minos-doc-1424). Should be almost identical for ( )/ ( e ) Main systematics for from + are: Deconvolution to extract e spectrum: no systematic yet ND-FD extrapolation: no systematic yet Cross-section shape uncertainty: see talk tomorrow Reconstruction efficiencies for and e ’s: small effect (?)
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5 Doing the numbers e from + e from +, 0 < E < 30 GeV Stan’s method2920.1 ± 1677.2(all) Fit method1378.3 ± 532.8(stat) Combination of scaling methods 1,2 and 4 gives: 5235.7 ± 629.6(stat) ± 818.5 (syst) from +: Necessary parameters from MC (all below 30 GeV): With Stan’s method, at 1x10 19 POT we get: e ’s from +, fid vol e ’s from + Stan’s method3,391.1±2017,417,091±10,178.8 Raw MC2,121.1±52.55(stat)10,691.4±118.0(stat) - Selection efficiency for from + is 31.38 % ± 1.9% (stat) - Ratio of e ’s from + to ’s from + is 2.97±0.14(stat) ±0.40(syst) - Ratio of e ’s from + in detector to those in fiducial volume is 5.04±0.14(stat) (this is reconstructed e ’s from +, not all e ’s that go through the detector) Assume we are dominated by statistics
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6 Backup
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7 Reweighting nubars from + from m+, raw MC from m+, reweighted MC
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8 Scaling method 1
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9 Scaling method 2
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10 Scaling method 3
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11 Scaling method 3-alt (no fit to ratio)
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12 Scaling method 4
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13 Fit method
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14 (Fit method 2 – discredited)
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15 (Fit method 3 – discredited)
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