(r6) SusySubjet < Main

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---+ Identifying massive hadronic decays in SUSY decay chains.

This page is intended to help discussion between Are, Erckan, John and Jon and isn't intended to be used by anyone else.

---++ Project plan

We'll start by assuming that in a SUSY pair production, one decay chain has allowed us to remove all non-SUSY backgrounds, and what we are trying to do is interrogate/unpick the second decay chain to learn more about the SUSY spectrum. In particular we are looking at high ET jets and seeing they come from hadronic decays of W or Z.

John: I suggest that we use the benchmarks postulated in [[http://www-spires.dur.ac.uk/cgi-bin/spiface/hep/www?rawcmd=FIND+EPRINT+HEP-PH+AND+EPRINT+0508198][hep-ph/0508198]], particularly scenarios \alpha, \beta, \gamma and \delta. The first three have neutralino dark matter but non-universal Higgs mases (NUHM), with parameters chosen to get varying branching ratios for \chi_2^0 \to Z,H \chi_1^0, as seen in Fig. 2. I do not know offhand about the \chi^\pm \to W \chi decays. 

The point \delta has gravitino dark matter, but the neutralino is the next-lightest sparticle and its decays are invisible. Hence, all four points have 'standard' missing energy signatures.

Since there are issues in treating NUHM models using ISAJET, we might want to start with point \delta. It is in any case the most interesting, as it has relatively large masses and hence is quite challenging using conventional techniques (see Fig. 9).

After our discussion at CERN on 19 July, we decided the immediate way ahead was as follows:

   * Are to produce the PYTHIA config files from these and upload to this page. 
   * Are to run the [http://hepforge.cedar.ac.uk/hzsteer HZSteer] analysis and show us the key distributions (mass, y, ET, eta etc... as shown previously).
   * Erckan to run similar jobs with Athena ATLFast and compare to Are's.

After this, we should have a good idea how much mileage there is in this kind of study, and hopefully be in a position to start looking at more challenging SUSY scenarios and treating non-SUSY background events.

The SLHA file for John's \delta point has been generated with ISAJET 7.69, and SUSY decays added with SDecay 1.1. I checked the decays with the ones given by ISAJET and modulo small numerical differences they look the same.
 


-- Main.JonButterworth - 19 Jul 2006

-- Main.ErkcanOzcan 
   * [[%ATTACHURL%/delta_slha.dat][delta_slha.dat]]: SLHA (SUSY Les Houches Accord) file for the \delta benchmark point