(di-)photon + met status and plans for 5 fb -1 analysis

(Di-)Photon + MET Status and Plans for

5 fb-1 AnalysisWho plans to contribute?

• DESY (Ehrenfeld, Wildt, Vankov)• Annecy (Przysiezniak-Frey)• Penn (Williams, Bradmiller-Feld)• Santa Cruz (Damiani, Kim, Schumm)• La Plata (Dova, Alonso)• Tokyo (Jinnouchi)

Bruce Schumm3 Nov 2011

1 fb-1 Analysis: Thumbnail Sketch

(First-order) signal selection straightforward:• 2 tight isolated photons with ET 25 GeV

• ETmiss 125 GeV

Optimization based only on ETmiss cut value.

Compare to CMS analysis: • At least 2 isolated photons withET 45,30 GeV

• ETmiss 100 GeV

• At least one jet with ET 30 GeV

ATLAS CMS

# obs (exp) 5 (4.1) 0 (1.5)

Lum (fb-1) 1.07 1.14

Obs limit (fb) 26 27

Exp limit (fb) 23 33

Much time spent in deconstructing this difference, butat the end of the day, it all comes down to expected limit. How could these numbers be consistent?

The answer to the conundrum lies in the acceptance*efficiency:e.g. at (mg,mB,mq) = (880,375,1520)

ATLAS 27% CMS 12%But let’s look at backgrounds…

“Instrumental”

“Genuine”

But CMS made their cut at 100 GeV; for that cut

backgrounds CMS ATLASInstrumental 2.5 2.4

Genuine 0.3 6.1TOTAL 2.8 8.5

Our estimated backgrounds:

CMS significantly reduced the “genuine” component (jet requirement? e gamma fake rate?) at expense of efficiency.

In addition, examination of our high-PT events suggested• e fakes do indeed dominate• alignment of ETMiss with photon

This motivates• Studies to reduce backgrounds• Use of additional discriminating variables

Since we have a little time, we’ve tried to open things up a bit (but we are now beginning to refocus on optimization for final event selection)

Penn: Look at isolation, conversion category, pixel hits

0 conversion2 conversions

1 conversion

0 conversion 1 conversion2 conversions

6 Oct 2011 SUSY Photon Meeting 10

Bino-Like Grid Points• 2-d Gluino vs Bino grid– Gluino masses:

• 800, 850, 900, 950, 1000, 1050, 1100, 1200– Bino masses:

• 50, 100, 150, 300, 450, … , mgl – 20, mgl – 10• 79 points total – 5000 events per point

• 2-d Squark vs Bino grid– Mainly care about this grid to measure acceptance

differences with respect to the gluino-bino grid.– Same basic structure of points as above.

Status: Submitted; awaiting processing.

So where do we go from here?Penn/La Plata: Explore isolation w/ W sample; devise pragmatic suggestion for optimization:• ETCone_20,30,40?• Cut energy?• Energy-dependent cuts?• Leading vs. sub-leading?

La Plata/UCSC: Discrimination of other observables:Separate conversions categories, pixel hits for conversions, ETMiss (scaled?), Photon-ETMiss , Photon ET, Photon-ETMiss transverse mass, Meff/HT, jet activity

DESY: Contamination in QCD control sample (W, signal…)

Rough Calendar (Feedback?)

Preliminary studies (isolation, discriminating variables, QCD control sample) finish this week

Optimization over next two weeks (next week through 21-Nov?)

Un-blind (Through 1-Dec?)

Systematics (Through 15-Dec?)

What should target for support note be?

Photon + X + ETMiss

Starting to ask: what should “X” be?

CMS: X = 3 jets above 30 GeV

Have started to look at signal, background for single tight photon selection (MC; no trigger selection yet)

Signal: 800 GeV gluino, 400 GeV Bino, all else at ~

250 fb-1 of signal

1.8 fb-1 of W

6.8x10-5 fb-1 of QCD_J2

1.2 fb-1 of QCD_J5

Photon + X + ETMiss Next Steps

Look at full 1 fb-1 (5fb-1?) loose-tight ETMiss distributions to gauge QCD backgrounds from data.

Look at W+jets and ttbar for other possible contributions

To me, backgrounds look a little less daunting than I had feared (but this is all MC, and only a partial sampling so far)