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General issues with the implementation of theory models in generators A. Nikolakopoulos , N. Jachowicz, K. Niewczas, J. T. Sobczyk , R. Gonzalez-Jimenez, J.M. Udias 1 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos Outline I. Nucleon


  1. General issues with the implementation of theory models in generators A. Nikolakopoulos , N. Jachowicz, K. Niewczas, J. T. Sobczyk , R. Gonzalez-Jimenez, J.M. Udias 1 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  2. Outline I. Nucleon complexity II. Nuclear complexity III. Final state interaction Underlying message: → More exclusive signals higher dimensional problems 2 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  3. → π + N + l : counting variables v+N 5 Four vectors = 5x4 = 20 variables - 4 : on mass shell relations - 4 : initial nucleon known (at rest) - 4 : Energy-momentum conservation - 3 : Freedom to choose reference frame And invariance along q (known direction of one four vector) = 5 independent variables E v , cosθ l , E l , Ω π * or E v, Q 2 ,W, Ω π * 3 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  4. → π + N + l : Born approximation v+N → Leptonic part ( PW approximation ) known → Hadronic part modelling effort Exploit these facts: -Lepton tensor is known -Hadronic part is invariant under rotation along q and is the product of Hadronic current with its conjugate → Separate the φ* dependence 4 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  5. Separating the variables Example for the A structure function: Here the Hadron tensor depends on 3 variables: W, Q 2 , cosθ π * and φ π * = 0 And in total one needs 15 elements of the hadron tensor For inclusive: Only A survives integration over pion angles: And responses depend on Q 2 and W 5 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  6. What we know from electro- and photoproduction What we know from electro- and photoproduction Many approaches in the literature: -MAID07 -DCC ( e.g. Sato and Lee) -Effective Lagrangian approaches,ChpT , ... Ingredients: -Nucleon resonances -Background terms : Born term, Vector meson exchanges -cross channel resonances -Final state interactions - … - Many parameters fitted to > 20000 datapoints: 6 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  7. What we know from electro- and photoproduction What we know from electro- and photoproduction Many approaches in the literature: -MAID07 -DCC ( e.g. Sato and Lee) -Effective Lagrangian approaches, ... Ingredients: -Nucleon resonances -Background terms : Born term, Vector meson exchanges -Final state interactions - … - Many parameters fitted to > 20000 datapoints: 7 NuFA FACT19, Daegu Korea A. Nikolakopoulos

  8. What we know from electro- and photoproduction What we know from electro- and photoproduction Many approaches in the literature: -MAID07 -DCC ( e.g. Sato and Lee) -Effective Lagrangian approaches, ... Ingredients: -Nucleon resonances -Background terms : Born term, Vector meson exchanges -Final state interactions - … - Many parameters fitted to > 20000 datapoints: For neutrinos no such dataset is available 8 NuFA FACT19, Daegu Korea A. Nikolakopoulos

  9. Electroproduction data Write lepton tensor for polarized electron explicitly 9 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  10. → Electroproduction data: e+p n + π + LEM from R. Gonzalez-Jimenez et al. Phys. Rev. D 95, 113007 (2017) Based on HNV model Data from E89-038 CLAS experiment, 1999, V. Burket, R. Minehart MAID07 : Drechsel, D., Kamalov, S.S. & Tiator, L. Eur. Phys. J. A (2007) 34: 69 10 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  11. → Electroproduction data: e+p n + π + LEM from R. Gonzalez-Jimenez et al. Phys. Rev. D 95, 113007 (2017) Based on HNV model Data from E89-038 CLAS experiment, 1999, V. Burket, R. Minehart MAID07 : Drechsel, D., Kamalov, S.S. & Tiator, L. Eur. Phys. J. A (2007) 34: 69 11 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  12. → Electroproduction data: e+p n + π + LEM from R. Gonzalez-Jimenez et al. Phys. Rev. D 95, 113007 (2017) Based on HNV model Data from E89-038 CLAS experiment, 1999, V. Burket, R. Minehart MAID07 : Drechsel, D., Kamalov, S.S. & Tiator, L. Eur. Phys. J. A (2007) 34: 69 12 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  13. Structure functions for neutrinos 13 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  14. Angular distributions for neutrinos HNV, DCC and LEM vary in structure functions, still more or less agree on angular cross section. (Around Delta peak) Could this influence neutrino oscillation analysis ? 14 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  15. Angular distributions for neutrinos In (most) event generators: Isotropic distribution in CMS. → Computationally easy What is the difficulty ? ✗ Time to compute cross section → Actually rather fast The problem is efficiency in Sampling the phase space 15 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  16. How to introduce the fivefold CS ? Sample inclusive cross section in the traditional way: Tabulate or Calculate in situ inclusive structure functions for the interaction Functions only of Q2 and W, very fast interpolation in 2D. This gives an event with Q2 and W 16 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  17. How to introduce the fivefold CS ? given a Q2 and W, distribution of cosθ * is determined by A A is a smooth function and can usually be interpolated by a polynomial of degree 2 17 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  18. How to introduce the fivefold CS ? given a Q2 and W, distribution of cosθ * is determined by A A is a smooth function and can usually be interpolated by a polynomial of degree 2 18 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  19. How to introduce the fivefold CS ? given a Q2 and W, distribution of cosθ * is determined by A A is a smooth function and can usually be interpolated by a polynomial of degree 2 Calculation of A(cos) for fixed Q2 and W is very cheap Interpolation with degree 2 polynomial means: Cumulative distribution function Is a monotonic degree 3 polynomial → Can be inverted analytically → Inversion sampling 19 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  20. How to introduce the fivefold CS ? given a Q2 and W, distribution of cosθ * is determined by A A is a smooth function and can usually be interpolated by a polynomial of degree 2 Calculation of A(cos) for fixed Q2 and W is very cheap Interpolation with degree 2 polynomial means: Cumulative distribution function Is a monotonic degree 3 polynomial → Can be inverted analytically → Inversion sampling 20 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  21. How to introduce the fivefold CS ? By calculation of A at 3 points one gets a cosine according to the theoretical distribution With efficiency 100% given a Q2 , W, and cos θ * distribution of φ * is Again we determine the CDF algebraically. → The CDF can be inverted numerically to give φ * 21 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  22. How to introduce the fivefold CS ? By calculation of A at 3 points one gets a cosine according to the theoretical distribution First results, sampling in the full phase space, With efficiency 100% still some issues to be checked and algorithms to be explored given a Q2 , W, and cos θ * distribution of φ * is Again we determine the CDF algebraically. → The CDF can be inverted numerically to give φ * 22 NuStec workshop, Pittsburgh A. Nikolakopoulos

  23. → π + N + X+l : counting variables v+A 6 Four vectors = 6x4 = 24 variables - 4 : on mass shell relations - 4 : initial nucleus known (at rest) - 4 : Energy-momentum conservation - 3 : Freedom to choose reference frame And invariance along q (known direction of one four vector) = 9 independent variables interaction - 1 : Final nucleus left in a hole state (i.e. integrate over final nucleus energy) = 8 independent variables E v , cosθ l , E l , Ω π , Ω N, k π → → We go from a 2 3 process to a 2 4 process But there are no additional constraints because residual nucleus can be in any state. → So from 5 9 variables (one can also interpret the extra 4 variables as four-vector of initial bound nucleon) 23 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  24. How to introduce the fivefold CS ? By calculation of A at 3 points one gets a cosine according to the theoretical distribution With efficiency 100% given a Q2 , W, and cos θ * distribution of φ * is Again we determine the CDF algebraically. → The CDF can be inverted numerically to give φ * 24 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  25. → π + N + X+l : Born approximation v+A interaction Ψ i and Ψ f contain the whole initial and final state Nuclear modeling = finding a good approximation for the wavefunctions 25 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  26. Impulse approximation I. Interaction with only one particle of complex system II. The incident particle (Q) is unaffected by the system (in BA) Reduces the problem to finding single particle states in nuclear medium: 26 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  27. Impulse approximation I. Interaction with only one particle of complex system II. The incident particle (Q) is unaffected by the system (in BA) Reduces the problem to finding single particle states in nuclear medium: With p = p m = q – p’ N -k’ π This is a six dimensional integral with a lot of matrix multiplication… 27 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

  28. Factorization Replace these by asymptotic momenta 28 NuSTEC workshop, Pittsburgh USA A. Nikolakopoulos

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