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JAROSLAW NOWAK For the MiniBooNE Collaboration LOUISIANA STATE UNIVERSITY Sixth International Workshop on Neutrino-Nucleus Interactions in the Few-GeV.

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Presentation on theme: "JAROSLAW NOWAK For the MiniBooNE Collaboration LOUISIANA STATE UNIVERSITY Sixth International Workshop on Neutrino-Nucleus Interactions in the Few-GeV."— Presentation transcript:

1 JAROSLAW NOWAK For the MiniBooNE Collaboration LOUISIANA STATE UNIVERSITY Sixth International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region May 18th - 22nd, 2009 Sitges, Barcelona (Spain)

2 Rein-Sehgal model of resonance excitations with M A =1.1GeV [Annals of Physics, 133, 79 (1981)] Rein-Sehgal model for coherent π + production with M A =1.03 GeV [Nucl. Phys. B223, 29, (1983)] Rescale to reproduce MiniBooNE NC π 0 results (PLB 664, 1, 2008) ProcessFraction of reconstructed CC1π + events CC1 π + Resonant81 CC1 π + Coherent5.9 CCQE5.3 Multi-pion3.8 CC1 π 0 1.5 No muon mass in dynamics in CCπ + 5/22/092J. Nowak - NuInt09 The Q 2 distribution has been presented by Bonnie Fleming at NuInt 07 #events / 5.58E20POT/bin

3 Graczyk and SobczykPhys.Rev.D77:053001,2008 ANL Lalakulich et al., Phys.Rev.D71:074003,2005 Hernandez et al, Phys.Rev.D76:033005,2007 All models are described by the Rarita-Schwinger formalism Vector form factors from Lalakulich et al. Phys.Rev.D74:014009,2006 Axial-vector form factors: Adler model – used also in The analyses for ANL and BNL With the biggest contribution From C 5 A (Q 2 ) 3

4 Muon mass in resonace excitation model  Muon mass included only in the leptonic current –KLN model [Kuzmin, Lyubushkin and Naumov, Phys. Part. Nucl. 35, S133 (2004)]  Improving the KLN model by adding the pion-pole terms – BRS model [Berger and Sehgal, Phys. Rev. D 76, 113004 (2007)]  Similar prediction by Graczyk & Sobczyk [ Phys.Rev.D77:053003,2008 ] 5/22/09J. Nowak - NuInt09 Muon mass in coherent π + production is introduced by applying Adler’s screening factor [D. Rein and L. M. Sehgal, Phys. Lett. B 657, 207 (2007) ] Multiply by Adler’s screening factor With muon mass partial cross sections depend on the helicity Only three Functions Modified 4

5 Axial vector form factor Vector form factor The relationship between vector form factor in the Rein-Sehgal model and the Rarita-Schwinger form factors taken from Graczyk and Sobczyk, Phys.Rev.D77:053001,2008 5/22/09J. Nowak - NuInt095

6 Model (M A =1.1GeV)χ 2 /ndf Rein-Sehgal280/39 BRS(m μ )341/39 + new G V 138/39 +C 5 A (dipole)24.7/39 Data/MC (absolutely normalized) Improvement In the agreement With data for Q 2 And for E ν vs. Q 2 PRELIMINARY 5/22/096 PRELIMINARY Reconstructed Q 2 (GeV 2 ) #events /5.58E20POT/bin

7 Modelχ 2 /ndf Rein-Sehgal280/39 Lalakulich v1, C 5 A (0)=1.2, M A =0.95188/39 Lalakulich v2, C 5 A (0)=1.2, M A =1.05391/39 Hernandez, C 5 A (0)=0.867, M A =0.985353/39 Graczyk v1, C 5 A (0)=1.2, M A =0.9490/39 Graczyk v2, C 5 A (0)=0.98, M A =1.15109/39 All models but the Rein-Sehgal are with muon mass effect and new vector form factor PRELIMINARY 5/22/097J. Nowak - NuInt09 Lalakulich v.1 Lalakulich v.2 Hernandez Graczyk v.1Graczyk v.2 Reconstructed Q 2 (GeV 2 ) #events for 5.58E20POT/bin

8 The fit for the M A 1π has been performed for the improved Rein-Sehgal model: Absolutely normalized distributions Fit for entire range of Q 2 and without the coherent π + production M A 1π =1.16±0.15 GeV with χ 2 /ndf =22/39 For 0.0<Q 2 /GeV 2 <1.0 M A 1π =1.17±0.13 GeV with χ 2 /ndf =14/32 For Q 2 >0.2 GeV 2 PRELIMINARY Rein-Sehgal The same analysis for the default model In Nuance gives M A 1π =1.77±0.27 GeV with χ 2 /ndf =22/39 5/22/098J. Nowak - NuInt09

9 GA M A 1π PRELIMINARY Keeping the dipole form of the C 5 A we performed two-parameter fits Default contribution to CCπ + events M A only fit 1σ contour Best fit M A 1π =1.37 GeV C 5 A (0)=0.97 Best fit M A 1π =1.15 GeV Coherent<0.04 G A RS (0)=0.764 M A 1π and coherent contribution M A 1π and C 5 A (0) 5/22/099J. Nowak - NuInt09

10 PRELIMINARY The new model of charged Current pion production Improved agreement with data We performed fits for three models 5/22/0910J. Nowak - NuInt09 2a. Coherent contribution and M A 1π M A 1π =1.15 GeV Coherent<0.04 2b. M A 1π and C 5 A (0) M A 1π =1.37 GeV C 5 A (0)=0.97 1. The fit result for M A 1π for Q 2 >0.2GeV 2 M A 1π =1.17±0.13 GeV. #events / 5.58E20POT/bin PRELIMINARY Best fit values obtained for the new model with BRS (muon mass), new G V and C 5 A

11 5/22/09J. Nowak - NuInt0911

12 5/22/09J. Nowak - NuInt0912 M A 1π =1.16±0.15 GeV with χ 2 /ndf =22/39 For 0.0<Q 2 /GeV 2 <1.0 M A 1π =1.17±0.13 GeV with χ 2 /ndf =14/39 For Q 2 >0.2 GeV 2 M A 1π =1.06±0.1 GeV For shape Q 2 >0.2 GeV 2 with χ 2 /ndf =110/39 (absolutely normalized)

13  SciBooNE K2K, PRL 95, 252301 (2005) 1.1 GeV 2.2 GeV 1.3 GeV MiniBooNE, PHLTA,B664,41 NC coherent pion production is Of all NC π 0 (19.5 ±1.1 (stat) ±2.5 (sys))% 5/22/0913J. Nowak - NuInt09


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