Detection of W jj in Jets + MET Final State using New Data-Driven Technique
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1 Detection of W jj in Jets + MET Final State using New Data-Driven Technique Bi-Event Subtraction Technique Why? How? Where? Teruki Kamon Mitchell Institute for Fundamental Physics and Astronomy Texas A&M University & Department of Physics Kyungpook National University HEP Seminar Korea Institute for Advanced Study (KIAS), Seoul, Korea October 26, 2011 BEST 1
2 PPC Projects Experiment-Theory (ET) Collaboration Develop technique(s) a) To extract key final states; b) To measure SUSY masses in a minimal framework; c) To determine model parameters; d) To extract Ω (amount of the dark matter) at the LHC; Ω SUSY Ω DM e) To expand to non-minimal scenarios; f) To expand to non-susy scenarios (e.g., UED); and carry out at ATLAS and CMS! 2
3 PPC Projects at A Glance Phys. Lett. B 505 (2001) 161 (Tevatron) Phys. Lett. B 538 (2002) 121 (Tevatron) Phys. Lett. B 611 (2005) 223 (ILC) Phys. Lett. B 618 (2005) 182 (ILC) Eur. Phys. J. C46 (2006) 43 (LHC+ILC) Supersymmetry Parameter Analysis: SPA Convention and Project Phys. Lett. B 639 (2006) 46 (LHC) Phys. Lett. B 649 (2007) 73 (LHC) Phys. Rev. Lett. 100 (2008) (LHC) 1 Phys. Rev. D 79 (2009) (LHC) Phys. Rev. D 82 (2010) (LHC) 2 Phys. Lett. B 703 (2011) 475 ( BEST at LHC) 3
4 Probe Metric at the LHC We test msugra cases first, followed by a non-universal SUGRA case. Minimal SUGRA E LHC Future Collider Ω 2 ~ 0h A χ 1 = D ( m0, m1/2,tanβ, 0 ) 1 Non-Universal SUGRA Tevatron 2 Ω ~ 0h = D m, m,tanβ, A, µ ) 1 χ ( 0 1/2 0 2 Precision 4
5 BEST Part 1 : Why? Our studies have been based on msugra. 1 However, when we extend it to nonminimal scenarios, we see a case where W s become a key to reconstruct the SUSY masses. 2 We want to reconstruct W jj in all hadronic mode of SUSY events 5
6 Non-Universal SUGRA Dutta, Kamon, Kolev, Krislock, Oh Phys. Rev. D 82 (2010) [arxi: ] msugra: Unified masses at the GUT scale Parameters : m 0, m 1/2, A 0, tanβ, sign(μ) (*) Good enough to confirm that the dark matter is the SUSY weakly interacting neutral particle. nusugra: Unified masses at the GUT scale, except Higgs Parameters : m 0, m 1/2, A 0, tanβ, μ(m H ) (*) small μ makes neutralino Higgs-like annihilation cross section is large enough to have right amount of dark matter today. [Q] Is a cosmological measurement possible for non-minimal case? 6
7 Non-Universal SUGRA Project No. Suspect Report 5 Nonuniversal Higgs PRD82 (2010) Non-minimal SUGRA dn dt 2 = 3Hn σv 2 2 ( n ) n eq Is a cosmological measurement possible? 1) Start with over-abundance region in SSC-like msugra (e.g., m 1/2 = 500, m 0 = 360, m Hu = 360) 2) Reduce Higgs coupling parameter, µ, by increasing m Hu (e.g., m 1/2 = 500, m 0 = 360, m Hu =732) Extra contributions to Ωh 2 More annihilation (less abundance) Normal values of Ωh 2 3) Find smoking gun signals Non-U - UmSUGRA SSC ~ ± ± ~ % 0 χ1 W χ1 42% 2. 4 ντ~ 1 58% 98% ~ 0 χ ~ 2 ττ 1 92% 99% 4) Technique to calculate Ωh 2 7
8 Phys. Rev. D 82 (2010) (LHC) Phys. Lett. B 703 (2011) 475 ( BEST at LHC) W(s) in MET + Jets Next page 8
9 M(jj) Distribution E miss T > 180 GeV; N(J) > 2 with E T > 200 GeV; E miss T + E J1 T + E J2 T > 600 GeV N(j i ) > 2 with p T > 20 GeV M(j i j k ) 9
10 Data-Driven M(jj) Extraction Event Jets M(jj) M(jj) 1 1a, 1b, 1c 2 2a. 2b M(2a, 1a), M(2a, 1b), M(2a, 1c) M(2b, 1a), M(2b, 1b), M(2b, 1c) 3 3a, 3b, 3c, 3d M(3a, 2a), M(3a, 2b), M(3b, 2a), M(3b, 2b), M(3c, 2a), M(3c, 2b), M(3d, 2a), M(3d, 2b) M(2a, 2b) 4 For each j i in Event X, M(j i j k ) is calculated with j k in Event X 1 M(3a, 3b), M(3a, 3c), M(3a, 3d), M(3b, 3c), M(3b, 3d), M(3c, 3d) M(jj) > nnn GeV for normalization nnn M(jj) nnn M(jj) 10
11 Bi-Event Subtraction Technique m jj same m jj bi c m jj > 200 GeV for normalization m jj BEST For each j i in Event X, M(j i j k ) is calculated with j k in Event X 1 The method seems to be reasonable for SUSY 11
12 Start with JW E miss T > 180 GeV; N(J) > 2 with E T > 200 GeV; E miss T + E J1 T + E J2 T > 600 GeV & N(j) > 2 with p T > 30 GeV N(b) > 0 with p T > 30 GeV N(τ) = 0 with p T > 20 GeV & Jet Mix to extract W s Note there might be b-jets and/or τ-jets in event, but not counted as J nor j. Ture = 714 GeV (χ 1 +/ ) [Vetoing events with any τ s with p T > 20 GeV] Ture = 739 GeV (χ 40 ) Endpoint = 774 GeV Ture = 739 GeV (χ 40 ) M JW 12
13 Part 1: Summary We are pretty happy to be able to reconstruct the squark mass through W jj in all hadronic mode of SUSY events Can we validate with data? 13
14 BEST Part 2: Validation - How? TTbar events! 14
15 Brief Review: M(top) ATLAS and CMS reconstruct the top quark mass using kinematical constrains specific to TTbar events. 1) χ 2 2) M3 pp t t + j + ( W b) ( W b ) + j j l ν j 15
16 N(isolated lepton) = 1 N(jets) 4 [N(b-jets) 0] No MET cut CMS-TOP (PAS) 36pb -1 N(top) ~ 378 events 11 events / pb -1 N S / N + N = 13( for e & µ ) S B 16
17 CMS-TOP (PAS) 36pb -1 N = 392 N = 396 Fig. 1 N(top) = 209 (µ) N(BG) ~ 190 M(top) using kinematical fit; χ 2 < 10 χ 2 m = bjj σ m t t 2 m jj m + σ W W
18 N(isolated lepton) = 1 N(jets) 4 [N(b-jets) = 2] No MET cut Fig. 2 N(top) = 78 (e+µ) CMS-TOP (PAS) 36pb -1 M(top) and M(W) using M3 and M2 M 3 = M M 2 = M jjb ( max{ p }) jj( M 3) T ( jjb) 18
19 χ 2 and M3 Very powerful. However, those kinematical constraints would NOT be available for general searches A new technique? 19
20 Detection of W jj Bi-Event Subtraction Technique pp t t + j Phys. Lett. B 703 (2011); hep-ph/ ( W b) ( W b ) + j j l ν j pp W + jjjj l ν BEST: jet mixing from two different events (TTbar, TTbar), (TTbar,W), (W,W) = 20
21 LJ Sample Tai Sakuma (TAMU) = 21
22 TTbar in MadGraph (I) MC Closure Test 22
23 TTbar in MadGraph (II) N(isolated muon, pt > 20) 1 N(jets, pt >30) 3 [N(b-jets, pt>30) 1] MET > 20 ΔR(two jets)>0.4 3,701,947 events bi same a) Hadronization simulated by Pythia6 as well as the underlying events with the tune Z2. b) Pile-up events simulated comparable to the current LHC run c) CMS detector response simulated by a GEANT4 based program. W s M(jj) same /M(jj) bi normalized bi underestimating combinatorial M(jj) shape M(jj) M(jj) 23
24 BEST Part 3: Where? We are analyzing the CMS data and seeking any advice. Applications? Improvements? Next Step? 24
25 Potential Applications 25
26 Future BEST in SUSY m jj m jw?? 26
27 Phase Space Matching φ rotation 27 W Choice of Phase Space: p T, η, φ, MET, N j, H T
28 Summary BEST seems to be a powerful tool to reconstruct W jj in all hadronic mode of SUSY events Can we generalize? 28
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