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Rambling Thoughts on Further Photon(s) + MET Analysis SUSY EtMiss Subgroup Meeting 17 February 2011 Bruce Schumm, SCIPP/UCSC, For the SUSY Photon + MET.

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Presentation on theme: "Rambling Thoughts on Further Photon(s) + MET Analysis SUSY EtMiss Subgroup Meeting 17 February 2011 Bruce Schumm, SCIPP/UCSC, For the SUSY Photon + MET."— Presentation transcript:

1 Rambling Thoughts on Further Photon(s) + MET Analysis SUSY EtMiss Subgroup Meeting 17 February 2011 Bruce Schumm, SCIPP/UCSC, For the SUSY Photon + MET Group

2 Neutralino NLSP Signatures For Bino, branching is 77% , 23% Z. For Wino, branching properties are switched. For Higgsino, no photonic decay, but actual NLSP may be Higgsino/Bino/Wino admixture All can be prompt or metastable (“non-pointing” photons)

3 No visible jet activity when M g ~ M  Tevatron Limit Current state-of-the-art: (Semi-) Generalized GMSB MGM Trajectory Generalized by decoupling neutralino and gluino mass scales, but… Neutralino purely Bino- like Prompt neutralino decay

4 CMS limits: “simplified model” approach identical in spirit to ours; adds third dimension (squark mass) to parameter space I’d guess: up to color factors (that favor gluinos), squark and gluino channels essentially identical. Convert from one to another via net color factor.

5 2011 Data Sentiment (?) Likelihood of SUSY discovery much higher in 2011 than ever before Most important question: what can we do to baseline analysis to ensure that a discovery would be convincing Re-evaluate background estimation techniques, think about independent modes of confirmation Next priorities: improve model-independence (see photon+MET trigger), think of clever ways to extend reach That said…

6 2011 Wish List (probably partial… just some things that have occurred to me over the past few months) Use photon+MET trigger to look for non-pointing signatures and Higgsino/Bino admixture Explore photon+lepton signature for Wino-like case Fit to MET distribution rather than simple cut to improve sensitivity Explore additional selection variables (HT, m , , etc) Explore ISR as model-independent tag (SLAC theory development) Explore further ways to suppress backgrounds (brehmstrahlung veto…) Parameter-space dependent optimization

7 There is much to do, much opportunity for additional people to contribute Note that much of this is signature-related, and not a matter of physics-model interpretation  Joining forces with UED 2  +MET group would make a lot of sense. We should make sure this conversation continues to unfold

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