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Identifying massive hadronic decays in SUSY decay chains. | ||||||||
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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. | ||||||||
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< < | John: I suggest that we use the benchmarks postulated in hep-ph/0508198![]() | |||||||
> > | John: I suggest that we use the benchmarks postulated in hep-ph/0508198![]() | |||||||
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. |