1. Update on the Diphoton + MET Analysis Basckground Bruce Schumm, Osamu Jinnouchi (Tokyo Tech), Ryan Reese (SCIPP), Sheena Schier (SCIPP) 26 August 2014 SUSY Background Forum Meeting

2. 26 August 20142 Conference Note public in early January: Search for Supersymmetry in Diphoton Events with Large Missing Transverse Momentum in 8 TeV pp Collision Data with the ATLAS Detector ATLAS-CONF-2014-001 List of Tasks generated to move from note to paper…

3. 26 August 20143 Analysis Strategy (lower reach of Wino-Bino limits) Also: require E T > 75 GeV for each of the two photons

4. 26 August 20144 MC Generation/Simulation Tasks There were several issues to address that required more MC Low mass wino  Extend grid from 300 GeV down to 100 GeV  This is high cross-section/low-efficiency regime; required working out filtering mechanism Low mass bino  Extend explored bino mass reach down from 50 GeV to 10 GeV for all gluino, squark, and wino masses  Requires care to avoid metastable states, direct gravitino decays (our model requires decay through bino) Nearly degenerate case for EW production (M_bino close to M_wino)  Add points with  m of 25 and 10 GeV  Again need to watch for pathologies Now done; awaiting analysis

5. 26 August 20145 Analysis Tasks Increase jet E T cut from 20 to 40 GeV (M_eff reconstruction)  very little change to anything Evaluate p T dependence of e   fake rate  play role in determination of EW background  evaluated with “tag and probe” method  No significant p T dependence observed Check grids developed for other signatures  DISCUSS

6. 26 August 20146 Background Studies Estimate H   background  Use existing H   MC sample  Pass through all 5 analysese  Contributions at 10 -2 level or less DONE Re-evaluate  jet-MET uncertainty  Inclusion of overflow bin made diphoton and control distributions much more similar  Reduce uncertainty accordingly (small change in overall background uncertainty DONE Explore Wgg-background control region (  l sample) for non- Wgg backgrounds  This required developing the analysis from scratch since the sudden departure of Ben Aurebach  Also want to add tt  background just in case…  Nominal subject of this talk

7. 26 August 20147 New Wrinkle Comment on current version of Internal Note request that we update our analysis using BCH Cleaning In addition, we discovered that we had been unintentionally vetoing events containing identified muons, which was contrary to our intent  Are updating analysis, but need to see if this will have an appreciable effect on the backgrounds.  Note that this latter issue should not affect the Wgg analysis, since that explicitly requires events with muons, so no veto was applied.

8. 26 August 20148 Wgg Background Studies New developments on W  background calculation (Kaplan, Haas)  Our “enhancement factor” of ~3 is relative to Alpgen  Kaplan/Haas implement VBFNLO; see that Bozzi et al. NLO is consistent with Alpgen  Expect no need for enhancement factor Bozzi et al. Kaplan/Haas

9. 26 August 20149 Background Studies: New Issue Cont’d On the other hand, our W  background estimate based on (e,  )  control sample.  Our “enhancement factor” of ~3 is relative to Alpgen  Is this incompatible with Kaplan/Haas (phase space..)  Have we missed some background to the l  control sample?  Can just expand error to include Kaplan/Haas result (but we do simultaneous fit… so need to understand how to do that!) Includes x3 enhancement factor W  control region From CONF Paper Internal Note

10. 26 August 201410 Ed Board Request: Look for Z contamination in W  control sample Idea is to take l  control sample, divide it into low and high MET (below and above 50 GeV) and look at the following quantities: P T (e  ), P T (  ) M(e  1 ), M(e  2 ), M(e  ), M(  ), M(l  )  (MET,l),  (MET,e),  (MET,  ) But….

11. 26 August 201411 Re-Assessing the W  Control Analysis Re-invented Analysis Although signal selection was validated, lepton selection was not  Signal and MC down by x2 relative to CONF NOTE analysis  Exploring reasons for this  Have included tt  ; does not make much difference  X3 enhancement factor still consistent with data (see 3, expect 4.5), but based on 3 events rather than 8, so little statistical significance.

12. 26 August 201412 Summary Our tools for doing analysis and selecting events are largely back in place. While we seem to be able to reproduce our  sample, our l  sample has not been reproduced. If we decide current analysis is correct, could lower photon pT cut to get more statistics in control sample One bug (muon veto) and one analysis improvement (BCH cleaning) force us to recalculate backgrounds once again, but changes should be small. Should be quickly followed through upon once we work out the l  problem.

13. 22 April 201413 BACKUP

14. 17 June 201414 Interpretation/Limits Redo gluino/bino contour (changes very slight, except extension to M bino < 50 Set limit in squark/bino plane, including low bino mass Set limits in wino/bino plane, including lower limits (additional MC needed; hope to submit soon [Depending on manpower: Set limits in constrained SPS8 model (signal MC already in place)] Squark/bino limits done except low bino mass

15. 17 June 201415 5 fb -1 analysis required E T  > 50 GeV and Analysis Strategy Continued 1 fb -1 analysis required E T  > 25 GeV MET > 125 GeV These will likely place lower limits on the wino mass than those of the 8 TeV analysis (which are still being determined) Estimate of lower wino limit for 1 fb-1 analysis underway… but can we really include that in a paper? DISCUSS Not good

16. 17 June 201416