Charged Higgs

Europe/Zurich
EVO Instructions
################################################### LHC Higgs Cross Section: Charged Higgs meeting 22/02/2010, 14:00 Present: Elias Coniavitis, Patrick Czodrowski, Martin Flechl, Michael Krämer, Sami Lehti, Allison McCam, Michael Spira, Reisaburo Tanaka Chair: Martin Flechl Minutes: Martin Flechl ################################################### Please have a look at the slides. The following only summarizes additional discussions. ################################################### 1. Intro (Martin) ################################################### 2. Theory Overview (Michael) Reisaburo/Martin: Group is not supposed to discuss analysis strategies; first task are inclusive distributions, then differential incl. k factors Martin: ATLAS uses Matchig and Pythia for the H+ signal Reisaburo: slide 5 - differences 4FS vs 5FS look larger. ->Michael & Michael: indeed... 5FS includes Delta b corrections, 4FS does not Michael K: plot has been corrected in current version of slides. Reisaburo: different low-mu behavior for 4FS and 5FS... why? ->Michael: Yes... 4FS as expected, but 5FS unusual. Should try to get Tilman's opinion on this. Martin: Investigating differences 4FS vs 5FS important in the context of this group. ################################################### 3. CMS Status (Sami) Martin: Slide 4 - for 7 TeV? -> Sami: Yes Michael K: All work-in-progress or already done? -> Sami: in progress Martin: Which tools used for xsec, BR? -> Sami: Numbers from Tilman; CMS top xsec; BR(H+ -> taunu)=1 assumed for low mass Sami: Signal generation - Pythia6+Tauola, Bkg: Madgraph, Alpgen ################################################### 4. ATLAS Status (Martin) Michael S: Systematic uncertainties for BR seem large -> Martin: Yes, they are very conservative limits; and not result of a rigorous investigation. Should ask Sven for an updated opinion. Michael K: slide 8: due to large uncertainties for gluons at large x Michael K: slide 9: used MRST2004 as no newer 4FS-pdfs available. Have now a private version of MSTW2008 4FS PDFs, will redo exercise. b PDFs etc might not have been optimally described in the old version. Michael S: slide 11 - same xsec for both H+ masses?? -> Martin: This is normalized to the 14-TeV cross section, to get scale factors Michael K: Any idea how appropriate adding incoherently H+ from ttbar and heavy H+ cross sections? -> Martin: Yes, from recent gb->tH+ MC@NLO paper. Typically smaller than our uncertainties. ################################################### 5. Discussion Martin: procedure could be 1) agree on tools, 2) obtain numerical results, 3) investigate these: comparisons between tools, uncertainties, differential distributions, ... Michael S, Reisaburo: Higgs BR, also for MSSM, done by BR group. But not t->bH+ -> Martin: Need to make sure Higgs and top BR and Higgs xsec are treated consistently (delta b corrections etc) Michael S: SUSY corrections factorize... can do that later -> Michael K: Yes, let's start with the QCD part -> Martin: Ok, but eventually need to also provide numbers for specific benchmark scenarios like mh-max Michael S: HDecay implements NNLO Delta b, only 1-2% scale uncertainties (compared to 10% at NLO). Important esp. for BR. Martin: Will 4FS ever become public code? -> Michael & Michael: not secret - but should only be run in close contact to experts, thus prefer to only share it upon request. Michael K: Need to check if MSTW private 4FS PDFs will be public on time so that we can show results. Reisaburo / Martin: 7 TeV highest priority; and setting up machinery to look at other sqrt(s) Michael K., Michael S., Martin: For Freiburg, would be nice to have 4FS and 5FS grids. Need to start thinking about t->bH+ and delta b corrections as well, in close touch with MSSM neutral and BR groups. ################################################### Action List: 1. Produce 4FS grid (Michael K) 2. Produce 5FS grid (Tilman) 3. Start thinking about t->bH+ and discuss with MSSM neutral and BR groups 4. Contact MSTW to have PDFs public (Michael K) 5. Set up an email list for our subgroup (Martin). Please send a mail to Martin if you would like to be included in H+ email discussions. Next meeting: probably in about 4 weeks, but will fix ad-hoc when we have something to discuss
There are minutes attached to this event. Show them.
    • 14:00 14:05
      Introduction 5m
    • 14:05 14:25
      Theory Overview 20m
      Speaker: Michael Krämer
      Slides
    • 14:25 14:45
      CMS Status 20m
      Speaker: Sami Lehti (Helsinki Institute of Physics HIP)
      Slides
    • 14:45 15:05
      ATLAS Status 20m
      Speaker: Martin Flechl (Uppsala Universitet)
      Slides
    • 15:05 15:25
      Discussion 20m
      -Scope of the group -Plans for Freiburg -?