Search for the Higgs Boson at DØ in the Trilepton Channel
James Kraus University of Mississippi
1 Outline
The Standard Model and the Higgs Boson Fermilab Tevatron and the DØ experiment Higgs Production and Higgs Searches at DØ – Motivation for the trilepton Higgs search Search for the Higgs in the trilepton + Missing Transverse Energy (MET) final state Discussion of DØ and Tevatron combinations – Comparison with LHC results
2 Standard Model
Describes 3 of the 4 Fundamental Forces – Strong Force • Force carrier is gluon • Binds quarks into protons, neutrons • Holds protons & neutrons in nucleus – Electromagnetic Force • Force carrier is photon • Acts on charged particles • Responsible for electricity, chemical bonds
3 Standard Model
Describes 3 of the 4 Fundamental Forces – Strong Force – Electromagnetic Force – Weak Force νe ± 0 137 137 • Force carriers W , Z Cs Ba • Responsible for some radioactive 55 56 decays, nuclear fission e- – Gravity • Planetary motion, falling apples
4 Standard Model
Describes 3 of the 4 Fundamental Forces – Strong Force – Electromagnetic Force – Weak Force νe ± 0 137 137 • Force carriers W , Z Cs Ba • Responsible for some radioactive 55 56 decays, nuclear fission e- – Gravity • Planetary motion, falling apples Gravity is not
included in 5 Standard Model Standard Model
The Standard Model arranges 6 quark flavors and 6 lepton flavors into 3 generations of matter
Quarks experience The generations strong, weak, and are arranged by electromagnetic forces increasing mass, but are otherwise Leptons do not similar experience the strong force. Neutrinos only interact via the weak 6 force Electroweak Theory
Salam, Glashow, & Weinberg develop Electroweak theory in 1967 (Nobel prize in 1979) – Describes EM and Weak forces with a single theory – Predicted existence of massive, neutral Z boson Electroweak symmetry must be broken to give us the observed electromagnetic and weak forces With electroweak symmetry unbroken, particles are massless...
7 A Massive Problem
u d s c b W Boson Z Boson 80 GeV 91 GeV
(Photon & Gluon = Massless)
Top Quark e e 173 GeV
1 GeV ≈ mass of the proton 8 A Massive Solution
2010 Sakurai Prize ... for "elucidation of the properties of spontaneous symmetry breaking in four-dimensional relativistic gauge theory and of the mechanism for the consistent generation of vector boson masses."
Englert Brout Higgs Guralnik Hagen Kibble
PRL 13, 321-323 PRL 13 508-509 PRL 13, 585-587 9 (1964) (1964) (1964) The Higgs Boson in the Standard Model
Higgs mechanism responsible for electroweak symmetry breaking Interactions with Higgs field gives particles their masses – No prediction of the strength of this interaction The Higgs is the last undiscovered particle predicted by the Standard Model
– Standard Model does not predict the mass of the Higgs 10 Fermilab
Fermilab is a national lab located in Batavia, IL, outside Chicago − Is home to US-based high energy physics experiments, including Tevatron
To Chicago
11 The Fermilab Tevatron DØ Run II of Fermilab Tevatron March 2001 to Sept. 2011 − p-p collisions with energy of
1.96 TeV = 1960 mp One collision every 396 ns − >1.7 million collision/min Technology − Superconducting magnets Size − 4 mile circumference CDF 12 Fermilab Site Home to a healthy herd of bison
13 Fermilab at Night
14 The DØ Experiment
η θ A multipurpose Pseudorapidity = -ln(tan( /2)) particle detector Innermost detectors are the trackers, followed by calorimetry and muon chambers
Using information from all subdetectors, we can reconstruct the pp collision 15 Electrons, Photons
Lighter particles (e, γ) are stopped in the first few layers of the the calorimeter Hadrons make it farther into the detector
Only charge particles leave tracks Track matching allow us to distinguish e from γ 16 Hadronic Jets
When a high momentum quark or gluon is produced in a collision, results in a jet of hadronic particles into the detector
17 Muons
Muons can pass through our entire detector – µ are massive enough not to be stopped like e or γ in EM calorimeter – Don't feel strong force, so hard interactions are rare Muons are charged, so they leave tracks
Place trackers outside the calorimeter to detect
passage, and match to a 18 track in inner tracker Missing Transverse Energy Neutrinos do not interact with our detector MET muons – Infer their presence through missing transverse energy jet – Transverse = ⊥ to beamline
To conserve momentum,
vector sum pT = 0 – If non-zero, then either
• Energy Mis-measurement electron • Missed one or more particles (usually neutrinos)
19 Higgs Production at the Tevatron
The Higgs at Tevatron produced by gluon fusion (gg→H), associated production (qq→W/Z+H), and vector boson fusion (qq→qqH)
20 Higgs Decay Modes
The Higgs decays primarily to bottom quarks at low mass, WW at higher mass
The searches for the Higgs at the Tevatron focus on H→bb at low mass, H→WW at high mass.
Also use H → ττ, H → γγ due to low backgrounds
21 Higgs Backgrounds Or, You've been looking for over 10 years, why haven't you found it already?
The rate of Higgs production is small compared to backgrounds − Bottom decays swamped by QCD background except for associated ZH/WH production − WW cleaner, but still large backgrounds
22 Trilepton Higgs Search
New search channel at DØ – not in July 2011 combination
H0 ZH and WH production followed by H → WW decay
For WH → WWW → lνlνlν, where l = e, µ – Ratio of eee:eeµ:µµe:µµµ = 1:3:3:1 For ZH → ZWW → lllνX, ratio is 1:2:2:1 Currently, only considering the eeµ and µµe final states, with others to be added in future 23 Higgs Decay Modes
The expected Higgs signal from VH→VWW is between one tenth and one hundreth that from H→WW
However, eliminates almost all W, Z, Wγ, and WW backgrounds
So there is a gain in the signal over background in the three lepton channels compared to the 2 lepton channels
24 Trilepton Backgrounds
Principle backgrounds for the trilepton search – WZ → lνll – ZZ → llll Also have backgrounds with 2 real leptons and a jet or photon fake – Z + jets – Z + γ ν ν – tt→l bl b 25 Z + jets
q Z/γ* Z→l+l- + jets cross section is the largest of all the backgrounds Fakes lepton However, it is suppressed by low q g j→l fake rates – Z + jet fake rate is estimated by passing simulated Z+jet events through our MC detector model Z + jet events have no real missing energy – Variables that are sensitive to the missing energy separate this background from our signal
26 Z + γ
Z + γ significant background for µµe final state Only difference between electrons and photons in our detector is a track
27 Z + γ
Z + γ significant background for µµe final state Only difference between electrons and photons in e + - our detector is a track γ e Sometimes the photon undergoes interaction with the tracker, leading to γ→ee – If one electron gets most of the photon energy, will
be reconstructed as an electron 28 Estimating the Z + γ Background
Correctly estimating the γ→e fake rate in MC difficult
We use a data-driven method to estimate this background – Calculate the γ→e fake ratio from a photon sample in data – Reconstruct µµγ events, where the photon is not matched to a track – Apply the fake ratio to the data events to get the background estimate 29 Top Background
Like Z + jets, tt requires jet to fake lepton – tt events have real missing energy – b-quark jets have a higher fake rate than light quark jets – The tt background is the smallest SM background, but tends to be more signal-like, so it is significant
Fakes lepton
30 WZ and ZZ Backgrounds
WZ → lνll and ZZ → llll are estimated from MC – Currently, there is no dedicated 4l Higgs search at DØ, so these events are included in our search – Of all backgrounds, WZ most closely mimics signal
31 Trilepton Selection Cuts
We have requirements on both eeµ and µµe channels – 3 good leptons must be found – M(ee) or M(µµ) > 15 GeV
– One lepton with pT > 15 GeV,
all with pT > 10 GeV – All leptons from same pp collision – Δ R = √ Δ η 2 + Δ ϕ 2 > 0.3 between any two leptons
32 Reducing Backgrounds in µµe Channel
The µµe channel has larger backgrounds than eeµ – From Z backgrounds – jet → e fake rate higher than jet→µ fake rate, γ fake e but not µ Have additional cuts on µµe to reduce backgrounds – Remove final state radiation (FSR) – Photon is radiated off a muon after Z decay, so µµγ will have Z mass – Also, no real missing energy, so can keep most signal in the Z mass range by cutting only low MET events 33 Reducing Backgrounds in µµe Channel
The µµe channel has larger backgrounds than eeµ – From Z backgrounds – jet → e fake rate higher than jet→µ fake rate, γ fake e but not µ Have additional cuts on µµe to reduce backgrounds
34 Reducing Backgrounds in µµe
To reduce background more, turn to variables related to MET Special MET – If ∆φ between MET and nearest object < 90°. specialMET = MET×sin∆φ, otherwise = MET MET Significance – Based on the uncertainty on the energy measured in the 35 detector Reducing Backgrounds in µµe
We require either – Special MET > 15 GeV
or – MET Significance > 3 Removes most Z + jets and Zγ, leaves most signal
36 Event Yields
After all cuts, have 175 trilepton events
Less than 3 expected signal events S/B ~ 0.15
Errors reflect uncertainty due to sample size. With all statistical and systematic errors, expected 37 and observed agree within 1σ Signal vs. Background
Once we have a good background model, we look for differences between signal and background Example – ∆φ between leptons The Higgs is a spin-0 particle; W is spin-1 ⇒ small opening angle in leptons from the W decays Leptons from Z tend to be back-to-back 38 Signal vs. Background
Once we have a good background model, we look for differences between signal and background Example – ∆φ between leptons
39 Signal vs. Background
Once we have a good background model, we look for differences between signal and background Example – ∆φ between leptons The signal to background ratio is so small that any one variable will not be sufficient to isolate the Higgs Instead, we look at many variables associated with each event at once – multivariate analysis
40 Multivariate Analysis
Take multiple variables, each of which has some separating power Combine them into one variable that separates the signal and background
41 Limit Setting
Multivariate discriminants are used to hunt for signal If there is a significant amount of signal, will see pile-up of events near one, in excess of background
42 How We Set Limits
Based on log-likelihood ratio
– L is the Poisson likelihood that the s+b (b) correctly models the data – θ represents the systematic uncertainties on the measurements (luminosity, energy scale, etc.) Calculate probability density of LLR based on models of signal and background
43 How We Set Limits
Based on log-likelihood ratio
CLb and CLs+b are given by the integrals of the b and s+b LLR distributions above observed LLR – Represents how well the given model agrees with data We vary the signal content of the s+b model to find
where CLs = CLs+b/CLb < 0.05 – We exclude those points at the 95% Confidence Level (CL)44 Limit Setting vs Mass
No prediction of Higgs mass, so calculate LLR at multiple mass points – Set limits at 5 GeV intervals between 100 and 200 GeV – Solid black observed, dashed black b, dashed red s+b for signal set to SM expectation
45 Limit Setting vs Mass
Data consistent with background, so set limits – 95% CL limits shown for each mass point, adjusted for expected Higgs cross section at that mass – If observed limit falls below 1, we exclude SM Higgs at that mass point
46 Trilepton Higgs Limits
47 We expect a 95% CL limit of 12x SM expectation at mH = 125 GeV, measure a limit of 18x SM expectation DØ Combination
Trileptons only one channel out of many
48 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb,
49 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb,
50 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb,
51 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb, H→WW→lνlν,
52 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb, H→WW→lνlν, VH→l+l+X,
53 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb, H→WW→lνlν, VH→l+l+X, H→ττ,
54 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb, H→WW→lνlν, VH→l+l+X, H→ττ, H → γγ, and more
55 DØ Combination
Trileptons only one channel out of many – Others include ZH→llbb, WH→lνbb, ZH → ννbb, H→WW→lνlν, VH→l+l+X, H→ττ, H→γγ, and more – Below 145 GeV, H→bb searches dominate, but H→WW still contributes significantly
56 DØ Combination
Exclude 159 to 166 GeV
57 We expect a 95% CL limit of 1.85x SM expectation at mH = 125 GeV, measure a limit of 2.53x SM expectation Previous Higgs Search
The Tevatron Higgs search limits from July `11
156–177 GeV
58 Current Large Hadron Collider Results
The highest energy collider in the world is now the LHC at CERN
– 122.5 < mH < 127.5 allowed at 95% CL
59 Tevatron Combination
The CDF experiment does similar Higgs searches – CDF sees larger excess at low mass than DØ
149–178 GeV
60 Tevatron Combination
147 – 179 GeV
61 We expect a 95% CL limit of 1.1x SM expectation at mH = 125 GeV, measure a limit of 2.2x SM expectation Tevatron and LHC results
62 Magnitude of Excess Most significant local excess – Tevatron: 2.7σ at 120 GeV – CMS: 2.8σ at 125GeV – ATLAS: 2.6σ at 126 GeV • H→γγ+H→ZZ channels 3.4σ
63 Global Excesses
However, need to consider look-elsewhere effect – The more independent mass points examined, the more likely it is that at least one of them will be found to be high due to a statistical fluctuation – The look-elsewhere factor scales the probability for the number of independent mass points After application of look-elsewhere factor – Tevatron global excess of 2.1σ over 100 GeV – 200 GeV – ATLAS global excess of 2.2σ over 110 GeV – 146 GeV σ – CMS global excess of 2.1 over 110 GeV – 145 GeV 64 Plans for Improving Results
Tevatron no longer taking data, but we are still refining our search to improve our limits For the trilepton search, we are looking into – Improving our multivariate analysis by including jet information – Adding eee and µµµ channels – Improving jet modeling More is still to come – Tevatron is close to having the expected limits less than the SM expectation between 100 and 180 GeV 65 Conclusions
Have set limits on the Higgs in the trilepton channel at DØ – First time this has been done at DØ was in Feb. 2012
Tevatron excludes Higgs masses 147 – 179 GeV @ 95% CL – 110 – 122.5 GeV, 127 – 600 GeV excluded by LHC experiments
The global excesses are – Tevatron: 2.1σ for 100–200 GeV – σ ATLAS: 2.2 for 110 – 146 GeV 66 – CMS: 2.1σ for 110 – 145 GeV Backup Slides
67 Feynman Diagrams
A pictorial way to depict particle interactions = quark, lepton, or hadron = gamma, W Z = gluon
e+ e+ e- becomes e m
i e- t photons time 68 The Higgs Field
The Higgs field is everywhere The Higgs field impeded the progress of a particle, slowing it from speed of light – Effectively giving it mass The Higgs boson is the quanta of the Higgs field
69 Indirect Measurements
Because of quantum mechanics, the Higgs bosons can influence other particles without being directly detected
More mass ⇒ more interactions with virtual Higgs bosons
Measuring the mass of the W boson and top quark can tell us about the Higgs boson
t t 70 Indirect Measurements
Fit to the precision EW data Prefers a low mass Higgs
⇒ MH ≈ 94 GeV
⇒ MH ≤ 152 GeV at 95% CL
t t 71 Look-Elsewhere Effect
Consider a simple case – flipping a coin 100 times – Expect it to come up heads about 50 times – Not exactly 50 each time – probability distribution of number of heads – If we perform this task 1000 times (100, 000 coin flips) we may have a case where we find 65 heads, and not 50 – Does not mean coin is broken – The probability of getting 65 heads is 0.00087 – but if you perform the experiment 1000 times, there is a 87% chance72 this will happen at least once – “look elsewhere effect” eeμ/μμe Systematics Uncertainties
• Apply both flat and shape systematics; shape systematics include Z-pT smearing, electron pT smearing, and muon pT smearing
73 The Standard Model of Particle Physics
The Standard Model describes the strong, electromagnetic, and weak forces – Strong force – holds quarks together in protons and neutrons, protons and neutrons in atomic nuclei – Electromagnetic force – runs your iPod, etc.
– Weak force – responsible for some nuclear decays 74 The Standard Model of Particle Physics
The Standard Model (SM) describes the electromagnetic, weak, and strong forces Only quarks feel the strong force Force carrier is the gluon
75 The Standard Model of Particle Physics
The Standard Model (SM) describes the electromagnetic, weak, and strong forces All charged particles feel the electromagnetic force Force carrier is the photon
76 Searching For The Higgs at DØ
In all decay modes, there are at least 100 background events for every expected signal event There is no one variable, such as dilepton mass or missing transverse energy, that can separate the Higgs signal from background However, by looking at multiple variables, we can separate the signal and background sufficiently to possibly find the Higgs
77 The Weak Force
Henri Becquerel discovered radioactivity in 1896 “missing” energy (neutrino) 137 137 Cs Ba 55 56
β particle (electron) Enrico Fermi proposes model for beta decay in 1934 p
– Point interaction with strength GF -5 -2 n GF = 1.166x10 GeV 78 ν e- The Weak Force
Fermi's point interaction fails at high energies – Weak force is short range: Massive force carrier – EM is long range: photon massless - - p e e e n W - W ( q ) ( q ) α2 W ν W p p q 2+M 2 e W e-
α2 α2 α2 ≪ W ≃ e e G = If q MW ⇒ 2 F 2+ 2 2 MW 79 q M γ q
Assume αe = αW ⇒ MW ≈ 100 GeV The Weak Force
Henri Becquerel discovered radioactivity in 1896 “missing” energy (neutrino) 137 137 Cs Ba 55 56
β particle (electron) Enrico Fermi proposes model for beta decay in 1934 p
– Point interaction with strength GF -5 -2 n GF = 1.166x10 GeV 80 ν e- The Weak Force
Fermi's point interaction fails at high energies – Weak force is short range: Massive force carrier – EM is long range: photon massless - - p e e e n W - W ( q ) ( q ) α2 W ν W p p q 2+M 2 e W e-
α2 α2 α2 ≪ W ≃ e e G = If q MW ⇒ 2 F 2+ 2 2 MW 81 q M γ q
Assume αe = αW ⇒ MW ≈ 100 GeV The Standard Model of Particle Physics
The Standard Model describes the electromagnetic, weak, and strong forces However, we have not yet found the last particle predicted by the Standard model, the Higgs Boson
82 WZ, ZZ, and top Backgrounds
WZ → lνll and ZZ → llll are estimated from MC – Currently, there is no dedicated 4l Higgs search at DØ, so these events are included in our search Like Z + jets, tt requires jet to fake lepton – tt events have real missing energy – b-quark jets have a higher fake rate than light quark jets – The tt background is the smallest SM background, but tends to be more signal-like, so it is significant
83