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2015:groups:higgs:diff [2015/06/07 09:27]
frank.tackmann
2015:groups:higgs:diff [2015/07/14 08:22]
philippe.gras Added instructions for CERN account
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 ====== Discussion on Differential Higgs Cross Section Measurements ====== ====== Discussion on Differential Higgs Cross Section Measurements ======
  
-  ​* Discussion focused on H->​gammagamma and H->​4leptons (and maybe H->WW)+//If you are interested in contributing please subscribe to the [[https://​e-groups.cern.ch/​e-groups/​EgroupsSearch.do?​searchValue=houches-2015-topics-higgs-diff-xsection|mailing list]]. You will be asked to log in with your CERN account. If you don't have a CERN account, please fill [[https://​account.cern.ch/​account/​Externals/​RegisterAccount.aspx|this form]] to create a lightweight account.//​ 
 + 
 +== Session 1 discussion == 
 + 
 +  ​* Discussion focused on H->​gammagamma and H->​4leptons (and H->WW)
  
   * Currently available measurements:​   * Currently available measurements:​
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     * ATLAS combination of H->​gammagamma and H->​4leptons:​ http://​arxiv.org/​abs/​1504.05833 (https://​atlas.web.cern.ch/​Atlas/​GROUPS/​PHYSICS/​PAPERS/​HIGG-2014-11/​)     * ATLAS combination of H->​gammagamma and H->​4leptons:​ http://​arxiv.org/​abs/​1504.05833 (https://​atlas.web.cern.ch/​Atlas/​GROUPS/​PHYSICS/​PAPERS/​HIGG-2014-11/​)
     * Results from CMS will hopefully be available soon.     * Results from CMS will hopefully be available soon.
 +    * //​[Update]//​ Several talks with details on current and planned measurements were presented at the LHC Higgs XS WG kick-off meeting on fiducial cross sections: https://​indico.cern.ch/​event/​399923/​
  
   * What would be other useful observables and/or corners of phase space that are not currently measured by the experiments?​   * What would be other useful observables and/or corners of phase space that are not currently measured by the experiments?​
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                 * for CP studies in ggH: use loose delta eta_jj cut (some separation between jets, but looser than one would use for VBF studies)                 * for CP studies in ggH: use loose delta eta_jj cut (some separation between jets, but looser than one would use for VBF studies)
         * While statistics is limited, measurement of the 1st, 2nd moments of distributions is useful\\ (binning effects should be investigated).         * While statistics is limited, measurement of the 1st, 2nd moments of distributions is useful\\ (binning effects should be investigated).
 +
 +
 +  * H->​WW(->​lnulnu)
 +    * Most promising: 0-jet (smaller uncertainties from ttbar backgrounds)
 +    * Definition of fiducial region should include cuts on mll and mT
 +      *mT<mH reduces off-shell component to avoid associated uncertainties (~10%)
 +    * Interesting measurement:​ 0-jet cross section as a function of the pT cut in the jet veto, going as low as possible
 +    * Do not subtract pp->WW contribution to avoid associated uncertainties (quote estimated contribution)
 +    * Harmonized fiducial cross section measurements between Higgs and SM would be nice
 +
 +
 +  * Possibility of a measurement of VH?
 +    * high pT(V) (easier experimentally) or m(VH) (more direct from the theory perspective) would be interesting from the BSM perspective
 +    * H->bbbar 0-jet selection is likely the most promising, large uncertainties with the present statistics
 +      * NB: pT(V) and m(VH) very correlated in 0-jet selection
 +
 +
 +  * Isolation for photons and leptons
 +     * Some measurements include an isolation requirement for the photons or leptons into the definition of the fiducial region as the isolation efficiency depends on the production mode.
 +     * Provide corrections from isolated to full phase space in publications,​ preferably by production mode.
 +
 +  * Normalized or non-normalized measurements?​
 +    * Potential advantage: reduction of some experimental uncertainties,​ which will become more relevant when we are no longer dominated by statistical uncertainties.
 +    * As theoretical predictions are for cross sections, non-normalized cross sections are preferred in general. They also contain more information.
 +    * If the full experimental covariance matrix is provided, the normalization can be done easily. ​
 +
  
   * Information that is useful to include in publications to allow making maximal use of the results   * Information that is useful to include in publications to allow making maximal use of the results
-    * cross correlations between different spectra+    * cross correlations between different spectra. In addition, it would also be useful to provide the correlation between the differential distributions and the measured total (fiducial) cross section.
     * estimated nonperturbative effects     * estimated nonperturbative effects
     * estimated contributions of non-ggH modes     * estimated contributions of non-ggH modes
     * acceptance corrections to allow extrapolation from fiducial region to full phase space (for convenience)     * acceptance corrections to allow extrapolation from fiducial region to full phase space (for convenience)
  
 +  * Background subtraction?​
 +    * Experimentally H->​gammma gamma makes more sense fully background subtracted
 +    * H->​ZZ->​4l or H->​WW->​2l2nu could give measurements including irreducible background (with appropriate fiducial phase space definition including eg suitable m4l window in that case)
 +    * In that case prediction for irreducible background should also be provided to allow theorists to easily subtract it if desired
 +
 +
 +
 +== Session 2 discussion ==
 +
 +jet selection anti-kT R=0.4, pt>25-30 GeV, |eta|<​4.5
 +
 +== ggF ==
 +
 +(|eta|<​2.5)
 +
 +0j : sigma times BR
 + 
 +1j : pT 100,​200,​(300,​400)_mt,​overflow
 +
 +2j : bin in 2j exclusive and 3j inclusive, distributions mjj, Delta eta_jj, Delta Phi_jj
 +
 +== VBF ==
 +
 +2j : mjj, Delta eta_jj, Delta Phi_jj
 +
 +== VH ==
 +
 +fully leptonic: mVH 300...500, overflow
 +
 +1l, 0l: mT>200 GeV
  
-Points for further discussion: 
-  * Background subtraction for H->ZZ should be done or not? 
-  * More details to be discussed for gamma gamma? 
-  * How to deal with interference?​ 
-  * Should spectra be measured normalized or not normalized? 
-        * not normalized (normalization can always be done later)? 
-  * What is possible for H->WW? 
  
 +== ttH ==
  
 +m_T(ttH) ...,500,...
2015/groups/higgs/diff.txt · Last modified: 2015/07/14 08:22 by philippe.gras