Meson Exchange Current (MEC) model in Neutrino Interaction Generator
|
|
- Lester Wade
- 6 years ago
- Views:
Transcription
1 Meson Exchange Current (MEC) model in Neutrino Interaction Generator outline 1. Introduction 2. Letonic simulation in GENIE 3. Hadronic simulation in GENIE 4. Comarisons 5. Discussion Teei Katori Massachusetts Institute of Technology (and Cordão de Ouro Chicago) NuInt12, CBPF, Rio de Janeiro, Brazil, Oct. 22,
2 1. Introduction 2. Letonic simulation in GENIE 3. hadronic simulation in GENIE 4. Comarisons 5. Discussion 2
3 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e) N 3
4 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) N 4
5 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) e N A quasi-elastic e N A 5
6 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) e N A quasi-elastic e N A Δ-excitation e e Δ π N A A 6
7 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) e N A quasi-elastic e N A Δ-excitation e e Δ π N A A e N DIS e X 7
8 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) e N A quasi-elastic e N A Δ-excitation e e Δ π N A A di region e N DIS e X 8
9 1. Introduction of Meson Exchange Current (MEC) Benhar, Day, Sick Rev.Mod.Phys80(2008)189 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region e-beam Inclusive electron scattering with function of energy loss target e θ detector ω=e(e )-E(e ) e N A quasi-elastic e N A Δ-excitation e e Δ π N A A di region e MEC e A π N 1 N 2 A e N DIS e X 9
10 1. Introduction of Meson Exchange Current (MEC) Van Orden and Donnelly Annals.Phys.131(1981)451 Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region - MEC also contributes to QE eak (~10%) QE Δ-excitation MEC 10
11 1. Introduction of Meson Exchange Current (MEC) Carlson et al, PRC65(2002) Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region - MEC also contributes to QE eak (~10%) - MEC may contribute more than we thought Note: Calculation with good NN otential has correlations Light nuclei only Non-relativistic Longitudinal resonse of 4 He Transverse resonse of 4 He 40-50% 11
12 1. Introduction of Meson Exchange Current (MEC) Martini et al, PRC80(2009) Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region - MEC also contributes to QE eak (~10%) - MEC may contribute more than we thought - This rocess may be needed to describe recent QE ν-xs data ν µ CCQE total xs, RPA+n-nh effect RPA+n-nh RPA 12
13 1. Introduction of Meson Exchange Current (MEC) Nieves et al, Nucl.Phys.A627(1997)543 PRC83(2011) Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute at di region - MEC also contributes to QE eak (~10%) - MEC may contribute more than we thought - This rocess may be needed to describe recent QE ν-xs data - MEC verified in e-scattering agrees with ν-scattering Note, Local Fermi gas with extra correlations, MEC, ion roduction exclusive e-scattering on 12 C E=620MeV θ=60 o ν µ CCQE total xs on 12 C More about MEC theory, see all talks on Friday 13
14 1. Introduction of Meson Exchange Current (MEC) Meson Exchange Current (MEC) in e-scattering - MEC is conceived long time to contribute in di region - MEC also contributes to QE eak (~10%) - MEC may contribute more than we thought - This rocess may be needed to describe recent QE ν-xs data - MEC verified in e-scattering agrees with ν-scattering Goal of this rogram - Build the model consistent with both e-scattering and ν-scattering exeriments - Imlement such model in MC generator to simulate neutrino exeriments - Predict realistic signal of MEC in neutrino exeriments ν µ n 14
15 1. Introduction 2. Letonic simulation in GENIE 3. hadronic simulation in GENIE 4. Comarisons 5. Discussion 15
16 2. MEC simulation in GENIE Currently, hadronic kinematic distributions are not available from any models in the market ν µ n Therefore imlementation of MEC takes several stes (1) secify letonic model - Choose a model to generate leton differential cross section - Energy-momentum transfer is secified from the model - Verify the model using e-scattering data (2) secify hadronic model - Model how to ick u 2 nucleons - Model how to share the energy-momentum transfer, to knock-out 2 nucleons (3) secify FSI model - Outgoing leton and nucleons undertake standard FSI model in GENIE 16
17 2. MEC simulation in GENIE Currently, hadronic kinematic distributions are not available from any models in the market ν µ n Therefore imlementation of MEC takes several stes (1) secify letonic model - Choose a model to generate leton differential cross section - Energy-momentum transfer is secified from the model - Verify the model using e-scattering data (2) secify hadronic model - Model how to ick u 2 nucleons - Model how to share the energy-momentum transfer, to knock-out 2 nucleons (3) secify FSI model - Outgoing leton and nucleons undertake standard FSI model in GENIE 17
18 2. MEC simulation in GENIE Currently, hadronic kinematic distributions are not available from any models in the market ν µ n Therefore imlementation of MEC takes several stes (1) secify letonic model - Choose a model to generate leton differential cross section - Energy-momentum transfer is secified from the model - Verify the model using e-scattering data (2) secify hadronic model - Model how to ick u 2 nucleons - Model how to share the energy-momentum transfer, to knock-out 2 nucleons (3) secify FSI model - Outgoing leton and nucleons undertake standard FSI model in GENIE 18
19 2. MEC simulation in GENIE Currently, hadronic kinematic distributions are not available from any models in the market ν µ n Therefore imlementation of MEC takes several stes (1) secify letonic model - Choose a model to generate leton differential cross section - Energy-momentum transfer is secified from the model - Verify the model using e-scattering data (2) secify hadronic model - Model how to ick u 2 nucleons - Model how to share the energy-momentum transfer, to knock-out 2 nucleons (3) secify FSI model - Outgoing leton and nucleons undertake standard FSI model in GENIE 19
20 2. Letonic simulation in GENIE In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model MEC model requirement - It enhances total neutrino cross section ~30% - It enhances more high angle scattering due to transverse nature - It reroduces inclusive e-scattering data ν µ n 20
21 2. Letonic simulation in GENIE In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Dytman model - First MEC model in GENIE - Based on early work by Lightbody and O Connell - Easy to imlement, easy to tune ν µ n Feature - New MEC channel has only magnetic form factor (Pauli form factor) - MEC channel is Gaussian (mean~ 1.9 GeV width~150 MeV) - Linear A deendence to match revious studies Lightbody model Lightbody and O Connell Com in Phys. May/June(1988)57 QE (Gaussian) Δ (Cauchy) MEC (Cauchy) 21
22 2. Letonic simulation in GENIE In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Dytman model - First MEC model in GENIE - Based on early work by Lightbody and O Connell - Easy to imlement, easy to tune ν µ n Lightbody and O Connell Com in Phys. May/June(1988)57 ν µ - 12 C total cross section CCQE MEC CCQE MEC monotonically turn off (after 1 GeV) 22
23 2. Comarison with e-scattering data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model ν µ n Carbon target, 560MeV, 36 o (Q 2 ~0.1GeV 2 ) At low angle, RFG model overestimate QE eak MEC is small contribution at low angle 23
24 2. Comarison with e-scattering data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model ν µ n Carbon target, 560MeV, 60 o (Q 2 ~0.2GeV 2 ) MEC is related to transverse resonse function More imortant at larger scattering angle Pion roduction model is under develoment 24
25 2. Comarison with e-scattering data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model ν µ n Carbon target, 560MeV, 145 o (Q 2 ~0.5GeV 2 ) MEC is related to transverse resonse function More imortant at larger scattering angle Pion roduction model is under develoment 25
26 2. GENIE rediction for neutrino exeriment ν µ In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Neutrino interaction kinematics - with NuMI low energy configuration - matches MINERvA n - all (no π) - QE - MEC - all (no π) - QE - MEC 26
27 MiniBooNE collaboration, PRD81(2010) Comarison with MiniBooNE data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Comarison with MiniBooNE flux-folded ν µ CCQE double differential cross section data Tmu distribution, 0.8 < cosθ µ < 0.9 GENIE MiniBooNE data ν µ n Tmu distribution, 0.8 < cosθ µ < Slight over estimation at low angle muons 27
28 MiniBooNE collaboration, PRD81(2010) Comarison with MiniBooNE data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Comarison with MiniBooNE flux-folded ν µ CCQE double differential cross section data Tmu distribution, 0.8 < cosθ µ < 0.9 GENIE MiniBooNE data ν µ n Decomosition of GENIE rediction - it shows comlicated mix due to flux distribution Channels (no cut) - total - CCQE - MEC - RES - others 28
29 MiniBooNE collaboration, PRD81(2010) Comarison with MiniBooNE data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Decomosition of Valencia model - theory-based model is somewhat different - MiniBooNE data - Full model - Full QE (with RPA) - Multi-nucleon - No RPA, No Multi-nuc MA=1.049 GeV ν µ n Decomosition of GENIE rediction - it shows comlicated mix due to flux distribution Channels (no cut) - total - CCQE - MEC - RES - others 29
30 MiniBooNE collaboration, PRD81(2010) Comarison with MiniBooNE data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Comarison with MiniBooNE flux-folded ν µ CCQE double differential cross section data Tmu distribution, 0.5 < cosθ µ < 0.6 ν µ n Tmu distribution, 0.8 < cosθ µ < Slight over estimation at low angle muons GENIE MiniBooNE data Tmu distribution, 0.5 < cosθ µ < MC agrees with data at mild angle 30
31 MiniBooNE collaboration, PRD81(2010) Comarison with MiniBooNE data In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Comarison with MiniBooNE flux-folded ν µ CCQE double differential cross section data Tmu distribution, -0.1 < cosθ µ < 0.0 ν µ n Tmu distribution, 0.8 < cosθ µ < Slight over estimation at low angle muons GENIE MiniBooNE data Tmu distribution, 0.5 < cosθ µ < MC agrees with data at mild angle Tmu distribution, -0.1 < cosθ µ < Slight under estimation at high angle But remember the model is tested with electron data only! 31
32 2. Letonic simulation in GENIE In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Kinematic constraint - Letonic constraint (energy-momentum conservation) - Hadronic constraint (model deendent kinematic constraint) - Both CCQE and MEC show ~2% Hadronic constraint violation ν µ n Ankowski et al, PRD82(2010) ν µ - 12 C 800 MeV CCQE hase sace ν µ - 12 C 800 MeV MEC hase sace Letonic constraint Hadronic constraint 32
33 1. Introduction 2. Letonic simulation in GENIE 3. hadronic simulation in GENIE 4. Comarisons 5. Discussion 33
34 3. Hadron simulation in GENIE In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model Kinematic distribution of nucleon need to be modelled. MEC model defines leton kinematics, and Hadron model defines nucleon kinematics. Nucleon cluster model - Simle but reasonable model (GENIE, NuWro) - it has enough flexibility to add more features later ν µ n 34
35 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) Fermi gas - nucleon kinematics are randomly chosen from Fermi sea (GENIE, GiBUU, NuWro) Sectral function - nucleon kinematics can be chosen from sectral function Phase sace density - cross section is weighted with nucleon hase sace density (GiBUU) q 35
36 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed e.g.) ν µ - 12 C CC MEC interaction - It requires at least one neutron (- air is forbidden) - based on random choice, n- : n-n ~ 3 : 1 (NuWro, GiBUU) - based on isosin conjecture, n- : n-n ~ 1 : 4 (GENIE) - based on short range correlation n- : n-n ~ 90 : 5 Some theory also seculate n- >> n-n (Martini model) forbidden q q q n n n 36
37 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed 3. Energy-momentum conservation e.g.) GENIE - 2 nucleons make a on-shell cluster q q n P n nucleon cluster -P recoil nuclei 37
38 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed 3. Energy-momentum conservation e.g.) GENIE - 2 nucleons make a on-shell cluster - Energy-momentum transfer and nucleon cluster makes CM system (hadronic system) q n q 38
39 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed 3. Energy-momentum conservation e.g.) GENIE - 2 nucleons make a on-shell cluster - Energy-momentum transfer and nucleon cluster makes CM system (hadronic system) - Isotroic decay (random θ and φ) of hadronic system creates 2 nucleon emission q n q q θ 39
40 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed 3. Energy-momentum conservation e.g.) GENIE - 2 nucleons make a on-shell cluster - Energy-momentum transfer and nucleon cluster makes CM system (hadronic system) - Isotroic decay (random θ and φ) of hadronic system creates 2 nucleon emission - Boost back to lab frame µ ν q n q q θ 40
41 3. Nucleon cluster model in GENIE For a given Energy-Momentum transfer Choose 2 nucleons from secified kinematics (e.g., Fermi gas) 2. All n-n, n-, - airs are allowed, if interaction is allowed 3. Energy-momentum conservation e.g.) GENIE - 2 nucleons make a on-shell cluster - Energy-momentum transfer and nucleon cluster makes CM system (hadronic system) - Isotroic decay (random θ and φ) of hadronic system creates 2 nucleon emission - Boost back to lab frame µ Issues: - correlations may exist in initial 2 nucleons, any models? - certain airs may be favoured, any models? - searation energy, binding energy, etc, any measurements? The model can be extended to include these feature later ν 41
42 3. Nucleon cluster kinematics Nucleon cluster kinematic distribution - Isotroic momentum distribution - Nucleon cluster has more symmetric momentum distribution than CCQE, extends to higher energy q nucleon cluster n P θ -P recoil nuclei initial nucleon momentum black, CCQE red, CCMEC SRC tail 42
43 3. Nucleon cluster kinematics Nucleon cluster kinematic distribution - Isotroic momentum distribution - Nucleon cluster has more symmetric momentum distribution than CCQE, extends to higher energy - Isotroic angular distribution - Nucleon cluster has no referred direction against momentum transfer -P q nucleon cluster n recoil nuclei P θ initial nucleon momentum oening angle of initial nucleon to momentum transfer black, CCQE red, CCMEC black, CCQE red, CCMEC SRC tail 43
44 3. Nucleon cluster model kinematics for 800 MeV ν µ on 12 C 2 outgoing nucleon kinematics - 2 outgoing nucleons tend to be back-to-back (model deendent feature) θ -P recoil nuclei oening angle of 2 outgoing nucleons (before FSI) red, CCMEC Oening angle of 2 nucleons are naturally large 44
45 3. Nucleon cluster model kinematics for 800 MeV ν µ on 12 C In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model leading nucleons θ GENIE FSI model (ha FSI model) - After FSI, MEC still has larger oening angle for 2 nucleons than CCQE -P recoil nuclei oening angle of 2 outgoing nucleons (before FSI) oening angle of 2 leading outgoing nucleons (after FSI) red, CCMEC red, CCMEC 45
46 3. Nucleon cluster model kinematics for 800 MeV ν µ on 12 C In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model leading nucleons θ GENIE FSI model (ha FSI model) - After FSI, MEC still has larger oening angle for 2 nucleons than CCQE - This is rare configuration for CCQE and resonance -P recoil nuclei oening angle of 2 outgoing nucleons (before FSI) red, CCMEC oening angle of 2 leading outgoing nucleons (after FSI) black, CCQE red, CCMEC blue, CCRES 46
47 3. Nucleon cluster model kinematics for 800 MeV ν µ on 12 C In GENIE, Neutrino interaction is simulated in several stes (1) secify letonic model (2) secify hadronic model (3) secify FSI model leading nucleons f1 θ GENIE FSI model (ha FSI model) - leading outgoing nucleon momentum - leading outgoing nucleon angle -P recoil nuclei Nucleon cluster model may redict interesting event toologies black, CCQE red, CCMEC blue, CCRES black, CCQE red, CCMEC blue, CCRES 47
48 3. SciBooNE multi-track analysis Alcaraz-Aunion PhD thesis SciBooNE CC analysis - total rate is normalized to CC inclusive measurement - data is comared with NeuT rediction - 3 track data shows excess, this can be exlained by many ways - Resonance channel xs is underestimated? - FSI is not modelled correctly? - Indication of multi-nucleon emission? SciBooNE CC track number marker, data black, CCQE red, CCRES blue, others 48
49 1. Introduction 2. Letonic simulation in GENIE 3. hadronic simulation in GENIE 4. Comarisons 5. Discussion 49
50 4. MEC model in NuWro NuWro - 2 choices of MEC model - n-nh model (based on Marteau model) - TEM (Transverse enhancement model) - Nucleon cluster model similar to GENIE (more attention to energy balance) Sobczyk, PRD86(2012) Martini et al, PRC80(2009) Bodek et al, EUJC71(2011)
51 4. Sum of all nucleon kinetic energy NuWro - 2 choices of MEC model - n-nh model (based on Marteau model) - TEM (Transverse enhancement model) - Nucleon cluster model similar to GENIE (more attention to energy balance) Sobczyk, PRD86(2012) Martini et al, PRC80(2009) Bodek et al, EUJC71(2011)1726 Different redictions on energy transfer rovide different redictions on total kinetic energy, but after FSI, most of structure is gone 51
52 4. Sum of all nucleon kinetic energy Sobczyk, PRD86(2012) NuWro - 2 choices of MEC model - n-nh model (based on Marteau model) - TEM (Transverse enhancement model) - Nucleon cluster model similar to GENIE (more attention to energy balance) For GENIE, Dytman model has Gaussian energy transfer, therefore has symmetric kinetic energy distribution. GENIE ν µ - 12 C 800 MeV total outgoing nucleon kinetic energy CCMEC no FSI CCMEC with FSI 52
53 4. Max nucleon momentum Sobczyk, PRD86(2012) NuWro - 2 choices of MEC model - n-nh model (based on Marteau model) - TEM (Transverse enhancement model) - Nucleon cluster model similar to GENIE (more attention to energy balance) For GENIE, Dytman model has Gaussian energy transfer, therefore has symmetric kinetic energy distribution. GENIE ν µ - 12 C 800 MeV total outgoing nucleon kinetic energy CCMEC no FSI CCMEC with FSI 53
54 4. MEC model in GiBUU Lalakulich et al, PRC86(2012) One-article hase sace density Trile differential cross section (solution of couled Kadanoff-Baym eqn.) - A secial care is aid for the hase sace - 2 nucleons start from same location (effect of nuclear density is squared) Symmetry factor (n-n, - air=1/2, n- air=1) k q 1 (x) k 3 2 (x) 4 (=P- 3 ) 54
55 4. Total cross section, with N-nucleons GiBUU - A secial care is aid for the hase sace - 2 nucleons start from same location) - hadronic tensor is transverse rojector (model II) - FSI controls final state articles Lalakulich et al, PRC86(2012) GiBUU ν µ - 12 C total cross section for multi-nucleon knockout (after FSI) 2-2h doesn t contribute to 1 nucleon knockout - MEC model shouldn t enhance 1-nucleon knock out after FSI: QE Δ 22h k q 1 (x) k 3 2 (x) 4 (=P- 3 ) Eν (GeV)
56 4. Total cross section, with N-nucleons GiBUU - A secial care is aid for the hase sace - 2 nucleons start from same location) - hadronic tensor is transverse rojector (model II) - FSI controls final state articles Lalakulich et al, PRC86(2012) GiBUU ν µ - 12 C total cross section for multi-nucleon knockout (after FSI) 2-2h doesn t contribute to 1 nucleon knockout - MEC model shouldn t enhance 1-nucleon knock out 1 nucleon after FSI: QE Δ 22h GENIE ν µ - 12 C total xs for multi-nucleon knockout (after FSI) after FSI: QE 22h 2 nucleon 3 nucleon 10/22/ Teei 1 Katori, 1.5 MIT 2 Eν (GeV) Eν (GeV)
57 4. Summary GENIE NuWro GiBUU What kind of Letonic model? Dytman model n-nh model and TEM Transverse rojector for hadronic tensor how to choose 2 nucleon momentum? From Fermi sea, indeendently From Fermi sea, indeendently From Fermi sea, indeendently how to choose 2 nucleon location? both are random both are random both are random, but same location Any correlations? no no no, but xs is weighted by hase sace density what kind of airs? n- or n-n? n- : n-n = 1 : 4 n- : n-n = 3 : 1 n- : n-n = 3 : 1 How to share energymomentum transfer by 2 nucleons? nucleon cluster model nucleon cluster model not clear 57
58 1. Introduction 2. Letonic simulation in GENIE 3. hadronic simulation in GENIE 4. Comarisons 5. Discussion 58
59 5. Discussion The effort to imlement MEC model in MC is just started..., with many oen questions - How to choose 2 initial nucleon kinematics? - How to imlement 2 final nucleon FSI? - What kind of airs are referred, n-n, or n-, or -? - Where are 2 nucleons generated? - Do we assume any correlation of initial nucleon? (momentum and location) Some of them may be described in theoretical models, but what is best way to imlement in MC? (can have significant effect on redictions!) e.g.) Short Range Correlations (SRC) - Initial nucleons can be off-shell - from hadron exeriments, n- air is referred - 2 nucleons are close - initial momenta are correlated (back-to-back) We need more inut for a realistic rediction 59
60 5. Discussion GENIE v First tagged version with MEC - Leton kinematic is based on Dytman model, tests are ongoing with e-scattering data - Hadron kinematic is based on GENIE nucleon cluster model - Will be available Mar Acknowledgement - Costas Andreooulos - Steve Dytman - Hugh Gallagher - Ulrich Mosel - Jan Sobczyk Muito obrigado! 60
61 Backu 61
Neutrino Shadow Play Neutrino interactions for oscillation measurements
皮影 Shadow play Source: http://www.cnhubei.com/ztmjys-pyts Neutrino Shadow Play Neutrino interactions for oscillation measurements Xianguo LU / 卢显国 University of Oxford INT-18-1a: Nuclear ab initio Theories
More informationCharged Current Quasielastic Analysis from MINERνA
Charged Current Quasielastic Analysis from MINERνA Anushree Ghosh CBPF - Centro Brasileiro de Pesquisas F sicas, Rua Dr. Xavier Sigaud 150, Urca, Rio de Janeiro, Rio de Janeiro, 22290-180, Brazil on behalf
More informationNeutrino Interaction Physics for Oscillation Analyses
Neutrino Interaction Physics for Oscillation Analyses Patrick Stowell on behalf of the T2K Neutrino Interactions Working Group NuIntUK 20th July 2015 20th July 2015 Neutrino Interaction Physics for Oscillation
More informationNeutrino-Nucleus Scattering at MINERvA
1 Neutrino-Nucleus Scattering at MINERvA Elba XIII Workshop: Neutrino Physics IV Tammy Walton Fermilab June 26, 2014 2 MINERvA Motivation Big Picture Enter an era of precision neutrino oscillation measurements.
More informationThe Study of ν-nucleus Scattering Physics Interplay of Cross sections and Nuclear Effects
The Study of ν-nucleus Scattering Physics Interplay of Cross sections and Nuclear Effects Jorge G. Morfín Fermilab University of Pittsburgh, 8 December 2012 1 ν H / D Scattering Life was simpler when our
More informationMINERvA - Neutrino-nucleus cross sections are important!
MINERvA - Neutrino-nucleus cross sections are important! Steve Dytman, Univ. of Pittsburgh FUNFACT, JLab oscillations A cross sections MINERvA CC quasielastic results CC pion production results Big Picture
More informationHadronization model. Teppei Katori Queen Mary University of London CETUP neutrino interaction workshop, Rapid City, SD, USA, July 28, 2014
Hadronization model model tuning 4. Impact of Hadronization model for PINGU Teppei Katori Queen Mary University of London CETUP neutrino interaction workshop, Rapid City, SD, USA, July 28, 2014 Teppei
More informationNeutrino-Nucleus Interactions. Ulrich Mosel
Neutrino-Nucleus Interactions Ulrich Mosel Motivation Energy-Distributions of Neutrino Beams Energy must be reconstructed event by event, within these distributions Oscillation Signals as F(E n ) From:
More informationNUINT p2h or not 2p2h? Luis Alvarez Ruso
NUINT-2011 2p2h or not 2p2h? Luis Alvarez Ruso 2p2h Luis Alvarez Ruso 2p2h? 2-nucleon EW currents exist (are allowed by symmetries) 2p2h? 2-nucleon EW currents exist (are allowed by symmetries) Sizable
More informationarxiv: v1 [nucl-th] 26 Mar 2013
Superscaling in electron-nucleus scattering and its link to CC and NC E neutrino-nucleus scattering M.B. Barbaro Dipartimento di Fisica, Università di Torino and INFN, Sezione di Torino, 5 Torino, ITLY
More informationNeutrino cross sections for future oscillation experiments
Neutrino cross sections for future oscillation experiments Artur M. Ankowski SLAC, Stanford University based on A.M.A. & C. Mariani, J. Phys. G 44 (2017) 054001 Nuclear ab initio Theories and Neutrino
More informationNeutrino-Nucleus Interactions and Oscillations
Neutrino-Nucleus Interactions and Oscillations Ulrich Mosel Long-Baseline Experiment: T2K and NOvA Future (2027): DUNE From: Diwan et al, Ann. Rev. Nucl. Part. Sci 66 (2016) DUNE, 1300 km HyperK (T2K)
More informationQE or not QE, that is the question
Probing Neutrino-Nucleus ArgoNeuT event Interactions: New Results from ArgoNeuT QE or not QE, that is the question Ornella Palamara Yale University - INFN, Laboratori Nazionali del Gran Sasso INT Workshop
More informationNeutrinos Induced Pion Production in MINERvA
Neutrinos Induced Pion Production in MINERvA Aaron Higuera Universidad de Guanajuato, Mexico On behalf of the MINERvA collaboration Outline Neutrinos Induced Pion Production MINERvA Experiment E-938 CC
More informationStatus of Neutrino Cross Sections
1 Status of Neutrino Cross Sections Sam Zeller Fermilab U Pittsburgh Workshop December 6, 2012 what we know and don t know will point out well-known neutrino processes that can be used for flux determinations
More informationSam Zeller Fermilab. PANIC 2011 July 26, 2011
1 NEUTRINO CROSS SECTIONS Sam Zeller Fermilab PANIC 2011 July 26, 2011 this topic has become quite interesting lately revisiting ν scattering physics again for 1 st time in decades new data is revealing
More informationNuclear aspects of neutrino energy reconstruction in current oscillation experiments
Nuclear aspects of neutrino energy reconstruction in current oscillation experiments Tina Leitner Oliver Buss, Luis Alvarez-Ruso, and Ulrich Mosel Institut für Theoretische Physik Universität Gießen, Germany
More informationω γ Neutral Current Single Photon Production (NCγ) Outline 1. Oscillation physics 2. NOMAD 3. T2K/MINERvA 4. MicroBooNE 5. MiniBooNE+ 6.
Neutral Current Single Photon Production (NCγ) Outline physics ν Z ν N ω γ Teppei Katori Queen Mary University of London INT workshop, Seattle, USA, Dec. 12, 2013 N 1 2 NuSTEC protocol - way to avoid Donkey
More informationTina Leitner Oliver Buß, Ulrich Mosel und Luis Alvarez-Ruso
Neutrino nucleus scattering Tina Leitner Oliver Buß, Ulrich Mosel und Luis Alvarez-Ruso Institut für Theoretische Physik Universität Gießen, Germany XL. Arbeitstreffen Kernphysik, Schleching 26. Februar
More informationarxiv: v1 [nucl-th] 10 Apr 2018
Meson-exchange currents and quasielastic predictions for neutrino-nucleus scattering M.B. Barbaro Dipartimento di Fisica, Universita di Torino and INFN, Torino, Italy E-mail: barbaro@to.infn.it arxiv:.33v
More informationEffective spectral function for quasielastic scattering on nuclei
Eur. Phys. J. C (014) 74:3091 DOI 10.1140/epjc/s1005-014-3091-0 Regular Article - Experimental Physics Effective spectral function for quasielastic scattering on nuclei A. Bodek 1,a,M.E.Christy, B. Coopersmith
More informationNeutrino Energy Reconstruction Methods Using Electron Scattering Data. Afroditi Papadopoulou Pre-conference, EINN /29/17
Neutrino Energy Reconstruction Methods Using Electron Scattering Data Afroditi Papadopoulou Pre-conference, EINN 2017 10/29/17 Outline Nuclear Physics and Neutrino Oscillations. Outstanding Challenges
More informationNuclear effects in neutrino scattering
European Graduate School Complex Systems of Hadrons and Nuclei JUSTUS-LIEBIG- UNIVERSITÄT GIESSEN Copenhagen - Gießen - Helsinki - Jyväskylä - Torino L. Alvarez-Ruso, T. Leitner, U. Mosel Introduction
More informationLecture 2: Two body current contribution. Jan T. Sobczyk. Wrocªaw University. NuSTEC Neutrino Generator School, Liverpool, May 14-16, / 49
Lecture 2: Two body current contribution Jan T. Sobczyk Wrocªaw University NuSTEC Neutrino Generator School, Liverpool, May 14-16, 2014 1 / 49 Outline: history large M A controversy Marteau model basic
More informationQuasi-Elastic Cross Sections Pittsburgh Neutrino Flux Workshop
Quasi-Elastic Cross Sections Pittsburgh Neutrino Flux Workshop 2012-12-07 Laura Fields Northwestern University Outline Introduction Overview of quasi-elastic interactions Recent quasi-elastic measurements
More informationUlrich Mosel TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: AAAAAAA
Ulrich Mosel General Motivation: Interactions n Pions (from resonances and DIS) are the most dominant background to QE GiBUU : Theory and Event Simulation based on a BM solution of Kadanoff-Baym equations
More informationarxiv: v2 [nucl-th] 16 Jul 2018
EPJ manuscript No. (will be inserted by the editor) Removal and Binding Energies in Lepton Nucleus Scattering A. Bodek Department of Physics and Astronomy, University of Rochester, Rochester, NY 1467-0171
More informationOn the measurements of neutrino energy spectra and nuclear effects in neutrino-nucleus interactions
On the measurements of neutrino energy spectra and nuclear effects in neutrino-nucleus interactions Xianguo LU ( 盧 顕国 ) University of Oxford Kyoto HE Seminar 1 Outline 1. Introduction 2. Measuring nuclear
More informationJan T. Sobczyk. (in collaboration with K. Niewczas, T. Golan, C. Juszczak) (many discussions with Rik Gran) INT Workshop, March 5, 2018
Jan T. Sobczyk (in collaboration with K. Niewczas, T. Golan, C. Juszczak) (many discussions with Rik Gran) Wrocªaw University INT Workshop, March 5, 2018 1 / 43 Outline: Motivations. Attempts to estimate
More informationUnraveling the ν-nucleus Cross-Section
Unraveling the ν-nucleus Cross-Section Omar Benhar INFN and Department of Physics, Sapienza University I-00185 Roma, Italy Workshop on ν-nucleus Interaction in a Few-GeV Region KEK, Tokai Campus, November
More informationNeutrino Responses and the Long Baseline Program
Neutrino Responses and the Long Baseline Program - Review of existing plans: FermiLab to DUSEL - INT program critiques: challenge of event reconstruction with a broadband beam experiment - Possible contributions
More informationCamillo Mariani Center for Neutrino Physics, Virginia Tech
Camillo Mariani Center for Neutrino Physics, Virginia Tech Motivation and Contents Determination of neutrino oscillation parameters requires knowledge of neutrino energy Modern experiments use complicated
More informationDIS/Hadronization. Jarek Nowak
DIS/Hadronization Jarek Nowak Outline Deep Inelastic Scattering Cross section Parton Distribution Functions Hadronization Phenomenological approach (KNO scaling) Theoretical approach (Lund model) Resonance
More informationElectrons for Neutrinos
Electrons for Neutrinos 08/03/2018 INT Workshop INT-18-1a - Nuclear ab initio Theories and Neutrino Physics Or Hen, Larry Weinstein, Afroditi Papadopoulou,Mariana Khachatryan, Luke Pickering, Adrian Silva,
More informationQuasi-Elastic Scattering in MINERvA
Quasi-Elastic Scattering in MINERvA Kevin S. McFarland Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627 USA and Fermi National Accelerator Laboratory, Batavia, IL 60510
More informationarxiv: v4 [hep-ex] 29 Jan 2018
January 3, 28 Muon-neutrino-induced charged current cross section without pions: theoretical analysis U. Mosel Institut für Theoretische Physik, Universität Giessen, Giessen, Germany K. Gallmeister Institut
More informationNeutrino Scattering Results from MiniBooNE and SciBooNE
Neutrino Scattering Results from MiniBooNE and SciBooNE Outline: introduction, motivation MiniBooNE/SciBooNE experiments measurements, results interpretations future conclusions R. Tayloe, Indiana U. e-n
More informationResolving the axial mass anomaly
Neutrino Quasielas.c Sca1ering on Nuclear Targets Resolving the axial mass anomaly Eur.Phys.J.C71:1726,2011 arxiv:1106.0340 [hep- ph] Arie Bodek University of Rochester MIAMI 2011 Conference, Ft. Lauderdale,
More informationFINAL-STATE INTERACTIONS IN QUASIELASTIC ELECTRON AND NEUTRINO-NUCLEUS SCATTERING: THE RELATIVISTIC GREEN S FUNCTION MODEL
FINAL-STATE INTERACTIONS IN QUASIELASTIC ELECTRON AND NEUTRINO-NUCLEUS SCATTERING: THE RELATIVISTIC GREEN S FUNCTION MODEL Carlotta Giusti and Andrea Meucci Università and INFN, Pavia Neutrino-Nucleus
More informationarxiv: v2 [nucl-th] 1 Jul 2010
Neutrino-nucleus scattering reexamined: Quasielastic scattering and pion production entanglement and implications for neutrino energy reconstruction T. Leitner and U. Mosel Institut für Theoretische Physik,
More informationMany-Body Theory of the Electroweak Nuclear Response
Many-Body Theory of the Electroweak Nuclear Response Omar Benhar INFN and Department of Physics Università La Sapienza, I-00185 Roma Collaborators N. Farina, D. Meloni, H. Nakamura, M. Sakuda, R. Seki
More informationNEUTRINO CROSS SECTIONS
NEUTRINO 1 CROSS SECTIONS Sam Zeller Fermilab Final State Nucleons for Neutrino-Nucleus Interactions Workshop at JLAB May 14, 2015 this is a topic that has gotten a lot more interesting over the past several
More informationTheory overview on neutrino-nucleon (-nucleus) scattering
Theory overview on neutrino-nucleon (-nucleus) scattering Jan T. Sobczyk Wrocªaw University Neutrino 2014, Boston, June 3, 2014 1 / 42 Neutrina we Wrocªawiu Wszystko zacz ªo si od konferencji Epiphany
More informationNeutrino Cross Section Measurements for Long-Baseline Acceleratorbased Neutrino Oscillation Experiments
Neutrino Cross Section Measurements for Long-Baseline Acceleratorbased Neutrino Oscillation Experiments Katori, T arxiv record: http://arxiv.org/abs/0805.476 For additional information about this publication
More informationModel independent extraction of the axial mass parameter in CCQE anti neutrino-nucleon scattering
Model independent extraction of the axial mass parameter in CCQE anti neutrino-nucleon scattering Jerold Eugene Young III Department of Physics, Western Illinois University dvisor Dr. Gil Paz Wayne State
More informationUsing Electron Scattering Superscaling to predict Charge-changing Neutrino Cross Sections in Nuclei
Using Electron Scattering Superscaling to predict Charge-changing Neutrino Cross Sections in Nuclei Maria B. Barbaro University of Torino (Italy) and INFN Maria B. Barbaro NUFACT05, Frascati, June 21-26,
More informationNEUTRINO INTERACTIONS AT MINERvA. Kevin McFarland University of Rochester QMUL Seminar 14 January 2014
NEUTRINO INTERACTIONS AT MINERvA Kevin McFarland University of Rochester QMUL Seminar 14 January 2014 Outline Why study neutrino interactions? The MINERvA Experiment Results Quasi-Elastic Scattering in
More informationNEUTRINO ENERGY RECONSTRUCTION IN NEUTRINO-NUCLEUS INTERACTIONS
ELEMENTARY PARTICLE PHYSICS NEUTRINO ENERGY RECONSTRUCTION IN NEUTRINO-NUCLEUS INTERACTIONS D. CHEŞNEANU 1,2, A. JIPA 2,a 1 National Institute for Physics and Nuclear Engineering Horia Hulubei, Reactorului
More informationThe MINERnA Experiment
The MINERnA Experiment What is Minerna? Why Mienrna? n / n CCQE sections Inclusive n sections n beam and n flux Outlook INPC 2013 June 4 th 13 Alessandro Bravar for the Mienrna Collaboration The MINERnA
More informationIntroduction. Introduction to Elementary Particle Physics. Diego Bettoni Anno Accademico
Introduction Introduction to Elementary Particle Physics Diego Bettoni Anno Accademico 010-011 Course Outline 1. Introduction.. Discreet symmetries: P, C, T. 3. Isosin, strangeness, G-arity. 4. Quark Model
More informationPAVIA. Carlotta Giusti Matteo Vorabbi Franco Pacati Franco Capuzzi Andrea Meucci
PAVIA Carlotta Giusti Matteo Vorabbi Franco Pacati Franco Capuzzi Andrea Meucci ELECTROWEAK REACTIONS ON STABLE AND EXOTIC NUCLEI quasielastic electron and neutrino-nucleus scattering electron scattering
More informationStatus of experimental neutrino-nucleus scattering at a few GeV
Status of experimental neutrino-nucleus scattering at a few GeV Jeff Nelson William & Mary NuFact2016 Quy Nhon, Vietnam August 23nd, 2016 At the start of this workshop series The field was undergoing a
More informationInvestigation of Proton-Proton Short-Range Correlations via the Triple-Coincidence 12. C(e,e pp) Measurement at Jlab / Hall A
1935-2006 Investigation of Proton-Proton Short-Range Correlations via the Trile-Coincidence 12 C(e,e ) Measurement at Jlab / Hall A E01-105 20 October 2006 (Jefferson National Accelerator Facility ) e
More informationPRELIMINARY RESULTS OF NEUTRINO INTERACTIONS STUDY USING GENIE EVENT GENERATOR *
Romanian Reports in Physics, Vol. 64, No. 3, P. 695 701, 2012 ELEMENTARY PARTICLE PHYSICS PRELIMINARY RESULTS OF NEUTRINO INTERACTIONS STUDY USING GENIE EVENT GENERATOR * D. CHESNEANU 1,2, A. JIPA 2, I.
More informationApplication of the Spectral Function Formalism to Electronand Neutrino-Nucleus Scattering
Application of the Spectral Function Formalism to Electronand Neutrino-Nucleus Scattering Artur M. Ankowski Center for Neutrino Physics, Virginia Tech ECT* Doctoral Training Program 2017 Microscopic Theories
More informationN u P J-PARC Seminar August 20, 2015
Confronting Neutrino-Nucleus Interactions at Eν~1 GeV with the Detector Mark Hartz Kavli IPMU (WPI), University of Tokyo and TRIUMF N u P August 20, 2015 R I S M Outline Long baseline neutrino experiments
More informationarxiv: v1 [hep-ex] 30 Nov 2009
On extraction of oscillation parameters Jan Sobczyk and Jakub Zmuda Institute of Theoretical Physics, University of Wroclaw, plac Maxa Borna 9, 50-204 Wroclaw, Poland (Dated: November 28, 2017) arxiv:0912.0021v1
More informationLooking Forward to the Future QE* Needs of Oscillation Experiments
Looking Forward to the Future QE* Needs of Oscillation Experiments Deborah Harris Fermilab December 3, 2013 INT Workshop *U. Mosel, INT 2013: One always has to talk about QE and pions together Outline
More informationGENIE models and global fits of neutrino scattering data
GENIE models and global fits of neutrino scattering data Marco Roda - mroda@liverpool.ac.uk on behalf of GENIE collaboration University of Liverpool 7 September 17 NUFACT 17 Uppsala 1/49 Generators Neutrino
More informationSemi-inclusive neutrino-nucleus reactions
Final State Nucleons for Neutrino - Nucleus Interactions Thomas Jefferson National Accelerator Facility May 14th, 2015 Semi-inclusive neutrino-nucleus reactions Oscar Moreno Laboratory for Nuclear Science,
More informationO problemach z opisem produkcji pionów w oddziaªywaniach neutrin
O problemach z opisem produkcji pionów w oddziaªywaniach neutrin Jan T. Sobczyk Uniwersytet Wrocªawski Wrocªaw, 17 listopada 2014, seminarium ZFN 1 / 36 Outline: introduction puzzle 1: ANL and BNL normalization
More informationInclusive Electron Scattering from Nuclei and Scaling
Inclusive Electron Scattering from Nuclei and Scaling Donal Day University of Virginia NUINT12 October 22 - October 27, 2012 Rio de Janeiro, Brazil Outline Inclusive Electron Scattering from Nuclei General
More informationRecent results from MINERvA
Recent results from MINERvA Jonathan Miller for the MINERvA Collaboration Universidad Tecnica Federico Santa Maria 1 PANIC NOW Outline Introduction to MINERvA Recent important results: charged pion production
More informationHow I learned to stop worrying and love multi-nucleon effects (in neutrino-carbon interactions)
How I learned to stop worrying and love multi-nucleon effects (in neutrino-carbon interactions) new MINERvA measurement Phys. Rev. Lett. 116, 081802 arxiv.org:1511.05944 plus interpretation for oscillation
More informationarxiv: v3 [nucl-th] 8 Nov 2016
Neutrino Interactions with Nucleons and Nuclei: Importance for Long-Baseline Experiments Ulrich Mosel Institut fuer Theoretische Physik, Universitaet Giessen, Germany, D-35392 arxiv:1602.00696v3 [nucl-th]
More informationThe US Liquid Argon Time Projection Chamber (LArTPC) experiments
The US Liquid Argon Time Projection Chamber (LArTPC) experiments outline 1. Introduction 2. ArgoNeuT experiment 3. MicroBooNE experiment 4. Future large LArTPC experiments 5. Conclusion Teppei Katori for
More informationarxiv: v1 [nucl-ex] 7 Sep 2009
CCπ Event Reconstruction at MiniBooNE R.H. Nelson University of Colorado, Dept. of Physics, 39 UCB, Boulder, CO 839, USA arxiv:99.238v [nucl-ex] 7 Sep 29 Abstract. We describe the development of a fitter
More informationu-channel Omega Meson Production from the Fpi-2 Experiment
u-channel Omega Meson Production from the Fi- Exeriment Bill (Wenliang) Li Hall C Worksho. January, 015. Outline Where the data come from Theoretical justification Plan for data analysis Wenliang Li, Det.
More informationPossibilities for studying few nucleon correlations and Δ isobars in processes with several final state baryons.
Possibilities for studying few nucleon correlations and Δ isobars in rocesses with several final state baryons. Short-Range Structure of Nuclei at 12 GeV October 26-27, 2007 Jefferson Lab, Newort News,
More informationChallenges in ν-argon scattering and new results from the MicroBooNE experiment
Challenges in ν-argon scattering and new results from the MicroBooNE experiment Raquel Castillo Fernández, FNAL for the MicroBooNE collaboration ΙΝΤ Workshop 26 June 2018 Outline ν Oscillation phenomena
More informationGENIE. ! Physics Impact. Hugh Gallagher Tufts University Mar. 11, 2015
GENIE Project started in 2004; >100k line codebase. Simulates neutrino nucleus interactions from 100 MeV TeV on all nuclei, typical usage is as a front end to GEANT simulations. Additional capabilities
More informationRecent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012
Recent Results from Alysia Marino, University of Colorado at Boulder Neutrino Flux Workshop, University of Pittsburgh, Dec 6 8,2012 Outline T2K Beamline and Detectors Uncertainties from prior measurements
More informationWhy understanding neutrino interactions is important for oscillation physics
Why understanding neutrino interactions is important for oscillation physics Christopher W. Walter Department of Physics, Duke University, Durham, NC 27708 USA Unfortunately, we do not live in a world
More informationSimulation Studies Toward the Search for Neutron Antineutron Oscillation
Simulation Studies Toward the Search for Neutron Antineutron Oscillation By Joshua Barrow jbarrow3@vols.utk.edu For the Institute for Nuclear Theory Workshop on Neutron Oscillations: Appearance, Disappearance,
More informationCCQE and SciBooNE, T2K. 12/3/2013 K Mahn, INT
CCQE and SciBooNE, T2K 12/3/2013 K Mahn, INT Neutrino flux Neutrino flux neutrino energy (E ) in GeV Predominantly ~6%, ~0.5% ε + ε In MiniBooNE: ~1 per 1e15 POT In SciBooNE: ~0.5 per 1e15 POT ~5x closer,
More informationCharged current single pion to quasi-elastic cross section ratio in MiniBooNE. Steven Linden PAVI09 25 June 2009
Charged current single pion to quasi-elastic cross section ratio in MiniBooNE Steven Linden PAVI09 25 June 2009 Motivation Oscillation searches needed for leptonic CP violation. One approach: search for
More informationShort-range NN interactions: Experimental Past and Future
Short-range NN interactions: Experimental Past and Future 7th Workshop of the APS Topical Group on Hadronic Physics Nadia Fomin University of Tennessee February 1 st, 017 Independent Particle Shell Model
More information1 The pion bump in the gamma reay flux
1 The pion bump in the gamma reay flux Calculation of the gamma ray spectrum generated by an hadronic mechanism (that is by π decay). A pion of energy E π generated a flat spectrum between kinematical
More informationNeutrino Cross Sections and Scattering Physics
Neutrino Cross Sections and Scattering Physics Bonnie Fleming Yale University, New Haven, CT. Abstract. Large flux uncertainties and small cross sections have made neutrino scattering physics a challenge.
More informationThe search for the η -mesic nuclei in the LEPS2/BGOegg experiment
The search for the η -mesic nuclei in the LEPS2/BGOegg exeriment N. Tomida (RCNP, Osaka Univ.) 2018/Nov/13 QNP2018, Tsukuba Theory η -nucleus otical otential U(r) = ( V 0 + iw 0 ) x NJL model : V 0 = 150
More informationECT GENIE FSI overview. Trento 13 July, GENIE FSI strategy features comparisons looking to future
GENIE FSI overview Gabe Perdue, FNAL; Steve Dytman, Univ. of Pittsburgh Trento 13 July, 2018 GENIE FSI strategy features comparisons looking to future GENIE FSI strategy For better comparisons, goal always
More informationCharged Current Inclusive Scattering in MINERnA
Charged Current Inclusive Scattering in MINERnA What is Minerna? Why Minerna? n beam and n flux n / n inclusive x-sections x-section ratios (A-depndence) Outlook NUFACT 2013 August 21 st 13 Alessandro
More informationarxiv:hep-ex/ v1 18 Jan 2007
Jet roerties from di-hadron correlations in + collisions at s= GeV Jan Rak for the PHENIX collaboration arxiv:he-ex/77v 8 Jan 7 Abstract Deartment of Physics P.O.Box 5 (YFL) Jyväskylä FI-44 University
More informationNeutron Structure Function from BoNuS
Neutron Structure Function from BoNuS Stephen BültmannB Old Dominion University for the CLAS Collaboration The Structure of the Neutron at Large x The BoNuS Experiment in 005 First Results from the BoNuS
More informationSingle and double coincidence nucleon spectra in the weak decay of Λ hypernuclei
Single and double coincidence nucleon sectra in the weak decay of hyernuclei E. Bauer 1, G. Garbarino 2, A. Parreño 3 and A. Ramos 3 1 Deartamento de Física, Universidad Nacional de La Plata, C. C. 67
More informationNuclear effects on the determination of neutrino oscillation parameters
Nuclear effects on the determination of neutrino oscillation parameters Davide Meloni meloni@physik.uni-wuerzburg.de Wednesday, June 23 Electron-Nucleus Scattering XI Special thanks to Maria Barbaro, Omar
More informationNUCLEAR EFFECTS IN NEUTRINO STUDIES
NUCLEAR EFFECTS IN NEUTRINO STUDIES Joanna Sobczyk June 28, 2017, Trento 1 OUTLINE Motivation: neutrino physics Neutrino oscillation experiments: why nuclear physics is important Lepton-nucleus scattering:
More informationNeutrino interactions and cross sections
Neutrino interactions and cross sections ν scattering on a free nucleon ν electron scattering ν scattering on light nuclei at low energies ν quasielastic scattering ν pion production ν deep inelastic scattering
More informationThe short-range structure of Nuclei
The short-range structure of Nuclei 1. Beyond the nuclear mean-field the role of Nucleon-Nucleon correlations 2. Review of recent 2-N knockout experiments a) (γ,nn) and (e,e'nn) experiments at Mainz and
More informationConfronting electron and neutrino scattering Can the axial mass controversy be resolved?
Confronting electron and neutrino scattering Can the axial mass controversy be resolved? Omar Benhar Center for Neutrino Physics, Virginia Tech, Blacksburg, VA 24060 INFN and Department of Physics, Sapienza
More informationarxiv: v1 [hep-ex] 30 Dec 2018
Vector Boson roduction with heavy flavor quarks with the exeriment at LHC arxiv:8.633v [he-ex] 3 Dec 8 Université Libre de Bruxelles, Brussels, Belgium E-mail: bugra.bilin@cern.ch In this aer, a brief
More informationSIXTH INTERNATIONAL WORKSHOP
Ingenio SIXTH INTERNATIONAL WORKSHOP ON NEUTRINO-NUCLEUS INTERACTIONS IN THE FEW-GEV REGION NUINT-09 Stiges (Barcelona), Spain 18-22 May 2009 EDITORS Federico Sanchez IFAE Cerdanyola del Valles (Barcelona),
More informationHighlights from the ATLAS experiment
Nuclear Physics A Nuclear Physics A (28) 7 www.elsevier.com/locate/rocedia XXVIIth International Conference on Ultrarelativistic Nucleus-Nucleus Collisions (Quark Matter 28) Highlights from the ALAS exeriment
More informationNeutrino interaction at K2K
Neutrino interaction at K2K KEK Yoshinari Hayato for the K2K collaboration Contents Introduction Neutrino flux measurements and neutrino interaction studies in K2K Charged current quasi-elastic scattering
More informationStudy of e + e annihilation to hadrons at low energies at BABAR
Study of e + e annihilation to hadrons at low energies at BABAR V.Druzhinin Novosibirsk State University, BINP, Novosibirsk on behalf of the BABAR Collaboration International Symposium Advances in Dark
More informationRecent Results from T2K and Future Prospects
Recent Results from TK and Future Prospects Konosuke Iwamoto, on behalf of the TK Collaboration University of Rochester E-mail: kiwamoto@pas.rochester.edu The TK long-baseline neutrino oscillation experiment
More informationHADRON PRODUCTION IN WROCŁAW NEUTRINO EVENT GENERATOR
Vol. (00) ACTA PHYSICA POLONICA B No 8 HADRON PRODUCTION IN WROCŁAW NEUTRINO EVENT GENERATOR Jarosław A. Nowak, Jan T. Sobczyk Institute of Theoretical Physics, University of Wrocław M. Borna 9, 00 Wrocław,
More informationThe Quark-Parton Model
The Quark-Parton Model Before uarks and gluons were generally acceted Feynman roosed that the roton was made u of oint-like constituents artons Both Bjorken Scaling and the Callan-Gross relationshi can
More informationNuclear Physics and Astrophysics
Nuclear Physics and Astrophysics PHY-30 Dr. E. Rizvi Lecture 5 - Quantum Statistics & Kinematics Nuclear Reaction Types Nuclear reactions are often written as: a+x Y+b for accelerated projectile a colliding
More informationNeutrino Interaction Cross Sections
Neutrino Interaction Cross Sections Sam Zeller LANL INSS July 8, 2009 for the most part, in the context of ν oscillation experiments which neutrino interaction cross sections do we need to know and how
More information