Tuesday round table,
Collider issues
a compilation by Fawzi Boudjema and Stefano Moretti. Send any
comments,, additions to Fawzi
and Stefano |
Wednesday round
table, Dark Matter issues
a compilation by Fawzi Boudjema and JeanOrloff. Send any comments,
additions to Jean and
Fawzi
|
*C++: do experiments really require C++ software (for event generations, etc.) ? Or would they be equally happy with wrappers around whichever code/language ? What is the status in this respect ? C++ is certainly good for authors (OO helps multi-editing, etc) but many insist FORTRAN is still faster, more accurate/efficient. That is, there any point for a single author to convert his/her code to C++ to have it used by the experiments ? Probably not ? Are C++ (ThePEG) libraries/repositories useful to whom, other than the authors ?
* e-Science Data Analysis Resource HEP tools (like CEDAR), more of those ? What has the impact been so far on the experiments, real (Tevatron) or simulated (LHC) ?
* Top-down (start from known theory and generate data) vs Bottom-up (start from data and parametrize theory).
Much of the former, very little of the latter at present. Possibly apart from LHC Olympics, which assume second approach, but maybe still biased towards standard scenarios (SUSY, Xdim) ? How general can we be in the second approach. Would be good to have overview of experiences from LHC Olympics. LANHEP approach (whatever Lagrangian) can be useful ? Or effective theories ? Bard approach? Global approach?
* Experimenters to declare data handling policy. Who can accesses them , how will they be presented (unfolded, raw, etc.). Other ?
* Experimenters to make sure tools used are up-to-date, authors' approved versions, all settings (if defferent from default) are declared, which data are used for tuning, version #'s specified, interferfaces used are declared, etc.
* Related to previous point: do LHC experiments have a cutoff date to make a code part of the collaboration tool repository or will they keep updating/enlarging the latter as the need arises ? That is, will they maintain manpower dedicated to this tasks throughout the experiment lifetime ?
* How to normalise MC event generators especially in multi-leg hadronic final states (many jets beyond MC@NLO). Establish control sample of data for overall normalisation ? Extrapolation to other final states/data sets possible ? Any experiences so far with real data (from Tevatron) ?
|
* What does it take to validate
a ``dark matter model"
* What are the most important cross checks to perform, for indirect,
direct and collider observables.
* What to do with pseudo signals, like some signals that we have now
and that cover a wide range of energy..?
*How to merge dark matter codes, especially the particle physics part
with the propagation codes.
Can we find a general parametrisation of the latter, based of course on
few key parameters.
*How to aim at the best precision on the relic density (from
colliders). Shall we start to incorporate
unconventional cosmological scenarios (non thermal production,
entropy,..)
*Revival and major update of DarkMatter Tools (New experiments,
improved theory). DarkMatter tools is webpage on direct detection that
had been maintained by Rick Gaitskell.
|