Re: Minutes of OPC meeting (08/Sep/'01)

From: seki@neutrino.kek.jp
Date: Mon Sep 17 2001 - 19:25:17 JST

  • Next message: Dave Casper: "RE: Minutes of OPC meeting (08/Sep/'01)"

    Date: Mon, 17 Sep 2001 19:25:17 +0900 (JST)
    From: <seki@neutrino.kek.jp>
    To: dcasper@uci.edu
    cc: Makoto Sakuda <sakuda@neutrino.kek.jp>, opc.nuint01@neutrino.kek.jp
    Subject: Re: Minutes of OPC meeting (08/Sep/'01)
    Message-ID: <Pine.LNX.3.95LJ1.1b3.1010917191626.20893A-100000@neutrino.kek.jp>
    
    Dave,
    Let's have a TV conference at 8;00am on Wednesday in Japan time (4:00pm
    on Tuesday there).  This seems to be the only window this week on our
    side.  Otherwise, it has to be a week later, but we won't be able to 
    afford much delay.  Hope you can be available.
    Seki
    p.s. I am scheduled to fly back to LAX on Oct. 1.
    
    
    On Mon, 17 Sep 2001, Makoto Sakuda wrote:
    
    > Dear Dave,
    > 
    > Shall we (Session 5 conveners, ie Seki/Hayato) meet via
    > Video this week and discuss more about benchmark calculations, 
    > or do you have any idea about how you plan to organize session 5?
    > 
    > If you tell us your convenient time this week, we will set
    > up the Video connection.
    > 
    > Regards,
    > Makoto 
    > -----------------------------------------------------------
    > 5. Comparison of the benchmark MC and theoretical calculations
    >              Conveners: Casper*/Seki/Hayato/H.R.Gallagher
    > 
    >   **) Casper will discuss with Seki, update the benchmark calculations
    >    and propose to the following people a concrete scheme to 
    >    compare the distributions/calculations before the meeting:
    >      Hayato, Gallagher, Zucchelli, Mills, Rubbia ?, Seki/Nakamura, 
    >      Marteau, Paschos, Lipari ,....
    >    Good communication and coordination before the workshop are important.
    >   **) E_nu=0.3-0.5 (low energy) and 5 GeV (high energy) 
    >     will be included in the benchmarck calculations.
    >   
    >     i) MC Generators:
    >     > It is important that all groups use the same
    >     >parameters for the neutrino-nucleon cross sections, for
    >     >example, vector and axial form factors. Then, specify which
    >     >models or papers they use for nuclear effects (Fermi-gas model etc). 
    >           1) NEUT   (Hayato)
    >           2) NUANCE (Casper)
    >           3) MINOS/Soudan II (Gallagher)
    >           4) OPERA/NOMAD/DONUT (Piero Zucchelli) 
    >   **      5) MiniBooNE  (Mills?)
    >           6) A brief summary of MC results
    > 
    >    ii) Theoretical calculations
    >            7) J. Marteau
    >            8) E. Paschos 
    >            9) H. Nakamura 
    >   **      10) P. Lipari
    > 
    >    iii) Summary of comparison of benchmark calculations (MC+Theory)(0.5 hours)
    > 
    >    ----  Coffee break ---
    > 
    



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