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End now?

End now?. Régis Lefèvre Masterclass – Thursday, March 27th 2014. What we will look for. Invariant mass. In special relativity (you certainly know E=mc 2 ), using energy and momentum conservation, a relativistic invariant, called the invariant mass appears.

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End now?

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  1. End now? Régis Lefèvre Masterclass– Thursday, March 27th 2014

  2. What we will look for

  3. Invariant mass • In special relativity (you certainly know E=mc2), using energy and momentum conservation, a relativistic invariant, called the invariant mass appears. • If a particle decays, the invariant mass of the decay products (calculated in any referential) is the mass of the initial particle. • We will calculate (the software will do it in fact) the e+e-, 𝜇+𝜇-, 𝛾𝛾, e+e-e+e-, e+e-𝜇+𝜇- or 𝜇+𝜇-𝜇+𝜇- invariant mass of our different candidates.

  4. Beyond E = mc2

  5. In the case of Z → e+e-

  6. About histograms • Numbers between 0 and 10 • Distribution of occurrences

  7. About histograms The table can be represented as a graph: Each bar represents the number of occurrences of a given value. This one tells you that the value 7 appeared 16 times. This type of graph is an histogram.

  8. Examples from ATLAS

  9. Cuts we will use • We will only considered tracks with sufficient transverse momentum: pT≥ 5 GeV/c • Selected tracks should come from the same primary vertex (same proton-proton interaction): check it zooming in on the side-view window • If you have difficulties on a given event, you may use Pixel Hits ≥ 2 (tracks more likely to come from a primary vertex)and/or SCT Hits ≥ 7 (good quality tracks); do no forget to remove those cuts moving to the next event

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