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Gustaaf Brooijmans CERN 2017 The Road to Discovery Searching for BSM Physics at Hadron Colliders Gustaaf Brooijmans 1

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Page 1: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

The Road to Discovery Searching for BSM Physics at Hadron Colliders

Gustaaf Brooijmans

1

Page 2: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Goals❖ Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

- Challenges posed at hadron colliders

- Ease of generating false positives

- Techniques to deal with limited knowledges

- But far from exhaustive!

❖ Thread in results - Hints?

2

Page 3: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Standard Model Today

3

Triumph of Gauge Theories!

Page 4: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Standard Model Today❖ Higgs discovery completes the

Standard Model - Fully consistent, complete, precise

description of strong, electromagnetic and weak interactions

❖ Even generate fermion masses - But that is the only property of

fermions we “understand”

4

Page 5: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

In Words❖ Matter is built of spin 1/2 particles that interact by exchanging 3 different

kinds of spin 1 particles corresponding to 3 different (gauge) interactions

❖ There appear to be 3 generations of matter particles

❖ The 4 different matter particles in each generation carry different combinations of quantized charges characterizing their couplings to the interaction bosons

❖ The matter fermions and the weak bosons have “mass”

❖ Gravitation is presumably mediated by spin 2 gravitons

❖ Gravitation is extremely weak for typical particle masses

❖ There appear to be 3 macroscopic space dimensions

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Page 6: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

About the Standard Model❖ It’s a theory of interactions: - Properties of fermions are inputs

- In gauge paradigm, fermion properties “generate” interactions

- Properties of interaction bosons in terms of couplings, propagations, masses are linked:

- Measuring a few allows us to predict the rest, then measure and compare with expectation

❖ It’s remarkably successful: - Predictions verified to be correct at sometimes incredible levels of precision

- After ~40 years, still no serious cracks

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Page 7: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Precision Results

7

muon g-2: 0.7 ppm!

B, K physicsLEP, SLD & Tevatron

Page 8: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Lacking in the Standard Model❖ Clear structure in fermionic sector

unexplained - No understanding of the “charges”

- Evidence of selective principle(s) - E.g. no neutral colored fermions

- q(down) = q(e)/Nc

- Interpreted as evidence for (grand) unification

- Grand or less grand? (One or more scales?)

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Page 9: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Lacking in the Standard Model❖ Many cosmological issues - Dark matter and dark energy

- Not enough CP violation in the quark sector for baryogenesis

- Baryon number violation - Present in the SM through B-L (sphalerons)

- Baryogenesis through leptogenesis and B-L?

‣ Untestable?

9

Page 10: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Many Fundamental Questions❖ What exactly is spin? Or color? Or electric charge? Why are they

quantized? ❖ Are there only 3 generations? If so, why? ❖ Why are there e.g. no neutral, colored fermions? ❖ What is mass? Why are particles so light? ❖ Is there a link between particle and nucleon masses? ❖ How does all of this reconcile with gravitation? How many space-time

dimensions are there really? ❖ ...

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Page 11: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Particles Solve Problems

(Problems Predict Particles)

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Page 12: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Vector Boson Scattering

12

• There was in fact one known problem with the Standard Model (+ a second, related, lesser one):

• If we collide W’s or Z’s (not so easy...), the scattering cross-section grows with the center of mass energy, and gets out of control (violates unitarity) at about 1.7 TeV: σ(WW → WW) ∼ s

• This is similar to “low” energy neutrino scattering:

• If q2 << (MW)2, looks like a “contact interaction”, and cross-section grows with center of mass energy: σ ∼ s

• But when q2 ≈ (MW)2, W-boson propagation becomes visible, and “cures” this problem

Page 13: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Vector Boson Scattering

13

• There was in fact one known problem with the Standard Model (+ a second, related, lesser one):

• If we collide W’s or Z’s (not so easy...), the scattering cross-section grows with the center of mass energy, and gets out of control (violates unitarity) at about 1.7 TeV: σ(WW → WW) ∼ s

• This is similar to “low” energy neutrino scattering:

• If q2 << (MW)2, looks like a “contact interaction”, and cross-section grows with center of mass energy: σ ∼ s

• But when q2 ≈ (MW)2, W-boson propagation becomes visible, and “cures” this problem

Page 14: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

The Higgs Boson❖ One way to solve WW, is to introduce a massive, spinless particle (of

mass < ~1 TeV) - Couplings to W and Z are fixed, quantum numbers are known...

- .... to be those of the vacuum

- Its mass is unknown, and its couplings to the fermions are unknown.... well, maybe

- Fermions can acquire mass by coupling to this Higgs boson, so their couplings could be proportional to their masses. This is called the “Standard Model Higgs”

14

Page 15: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Precision Measurements❖ In fact, we were able to say

something about the standard model Higgs mass

- If the fermions get their masses from the Higgs, we know all couplings and can infer the Higgs mass from precision measurements

- Result is very sensitive to measured top quark, W boson masses

- Really wants a “light” Higgs boson15

Page 16: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Precision Measurements❖ In fact, we were able to say

something about the standard model Higgs mass

- If the fermions get their masses from the Higgs, we know all couplings and can infer the Higgs mass from precision measurements

- Result is very sensitive to measured top quark, W boson masses

- Really wants a “light” Higgs boson16

Page 17: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

The Plot Thickens

17

Page 18: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

New Physics?

18

Could this be it?

Page 19: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Higgs Mass❖ Higgs, in fact, also acquires

mass from coupling to W’s, fermions, and itself!

- These “mass terms” are quadratically divergent

- Drive mass to limit of validity of the theory

❖ So we expect the Higgs mass to be close to the scale where new physics comes in....

19

Page 20: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

New Physics?

20

Could this be it?

Page 21: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

New Physics?

21

Could this be it?

Page 22: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Nevertheless❖ Clear structure in fermionic sector

unexplained - Evidence of some selective principle

(why are there no neutral colored fermions?)

- Proton stability, running of couplings suggestive of at least one other scale relevant to SM particles and interactions, ~1015 GeV

- Either fine-tuning, or a closer scale

22

Page 23: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

The Tools

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Page 24: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Energy Frontier❖ Currently, hadron colliders: - High energy implies probing of short

distances, and production of other, massive particles

24

7 - 14 TeV center of mass energy

VLHCLHC

Page 25: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Hadron Colliders❖ Incoming longitudinal momentum not known: - “Hard interaction” is between one of the quarks and/or gluons from each

proton, other quarks/gluons are “spectators”

❖ Longitudinal boost “flattens” event to a pancake ➡ We usually work in the plane transverse to the beam

25

Page 26: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Detectors❖ Make best possible measurement of all particles coming out of collisions

26

Page 27: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

CMS

27

456%3.8T Solenoid

0>?@!76k scintillating PbWO4 crystals A>?@!Scintillator/brass

Interleaved ~7k ch

•  Pixels (100x150 µm2) " ~ 1 m2 ~66M ch"• Si Strips (80-180 µm)" ~200 m2 ~9.6M ch!

g8T.#@%o%970>G.7!

5p+_%XQqqfZ!250 Drift Tubes (DT) and 480 Resistive Plate Chambers (RPC)

473 Cathode Strip Chambers (CSC) 432 Resistive Plate Chambers (RPC)

5p+_%f_i4Qg6!

!+&)1%B'#9"&%%%%%%%%%=4<<<%&%CD',)11%2#)('&',%%%=6%(%CD',)11%1'*9&"%%%%%%%;E:5%(%

eq+_%r+sf%

YBO YB1-2

Preshower Si Strips ~16 m2

~137k ch

Foward Cal Steel + quartz Fibers 2~k ch

16

Page 28: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Charged Particles❖ Combination of pixels, silicon strips (“SCT”) and straw tube transition

radiation tracker (TRT)

28

Page 29: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Calorimetry❖ Liquid Argon & Pb accordion (EM & forward),

crystals ❖ Scintillator & steel/copper/tungsten (hadronic)

29

Page 30: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Muons❖ Air-core toroids/flux return; wire chambers

and RPCs

30

Page 31: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Neutrinos*

31

*(100% acceptance)

Page 32: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017 32

✓✓

✓✓✓

✓ ✓ ✓

✓: Detect with high efficiency

✓: Detect by missing transverse energy

✓: Detect through decays: t→Wb, W/Z → leptons, ...

H125500

0

Detecting Particles

Page 33: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

The Work

33

Page 34: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Steps in a Physics Analysis❖ Choose a topic (often theory-motivated) ❖ What is the final state? ⇒ “Preselection”

- For a search, sufficiently loose to be signal-poor - Prove you understand the detector response, physics processes contributing

- But sufficiently tight to have a manageable data volume - ATLAS/CMS write 1000 Hz × 1+ MB/event = 1+ GB/s

- “4-vectors” is not enough, need some amount of detector info

- In practice, often have preselected sample for frequent analysis, + looser sample for e.g. multijet background with rare passes

❖ Note that data volume ∝ running time, not ∫L34

Page 35: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Steps (II)❖ Determine preselected sample’s composition - MC and data to understand each contribution

- Multijet background to leptons often extracted from data: rejection factor ~10-4, difficult for simulation to be that accurate

- MC for most other processes, with corrections from data, since generators are (LO,) NLO, NNLO, (LL,) NLL, NNLL

- Also need to correct MC for real-life data conditions - Different alignment, dead channels etc.

- As statistics increase, more difficult, since mis-modelings not hidden by statistical uncertainties anymore

- Mis-modelings often show up in tails

35

Page 36: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Anecdotes From the Field (I)❖ Everybody wants experimenters to produce results fast - Lots of pressure in the early days of LHC...

36

Only jets, background easy

Page 37: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Anecdotes From the Field (I)

37

GEANT bug

❖ Everybody wants experimenters to produce results fast - Lots of pressure in the early days of LHC...

Page 38: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Anecdotes From the Field (I)

38

GEANT bug

Cosmics

❖ Everybody wants experimenters to produce results fast - Lots of pressure in the early days of LHC…

- Sometimes it’s better to take the time needed to understand strange things…

Page 39: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

A Semi-Challenging Search: Higgs to τ µ

39

Page 40: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

❖ 20 fb-1 collected by end 2012 at 8 TeV

40

400000 events in direct productioncan look for rare decays!

Producing Higgses

Page 41: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Higgs Decay: 125 GeV is Golden

41

Low MassH → bb, ττ, γγ

High MassH → WW, ZZ

Page 42: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

µ+τ❖ Indirect constraints fairly weak (as opposed to e.g. e+µ)

- Indirect: BR(µτ) < ~10%; BR(eµ) < ~10-8

❖ Lepton Flavor remains a mystery - Observing LFV crucial in understanding origin

- Know it exists in the neutrino sector

❖ Experimentally: - With 400k Higgses produced,1% BR yields 4000 signal events (x efficiency)

- Two leptons ⇒ small to moderate background at hadron collider

42

Page 43: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Tau decays❖ Exploit two channels: - τ→eνν: BR = 18%

- τ→hν: BR = 49% (one charged particle) + 15% (three charged particles)

- Avoid Z → μμ background

❖ Final states are μτe and μτh - Irreducible background is Z → ττ

- Primary discriminating variable is μ-τ invariant mass - Unfortunately not directly reconstructible: neutrinos escape!

43

Page 44: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Collinear Mass❖ m(H) = 125 GeV, m(τ) = 1.8 GeV ➡ Tau is heavily boosted

➡ Tau decay products are collinear with tau

❖ Under that assumption, know neutrino direction - From direction and missing transverse momentum infer neutrino longitudinal momentum

44

CMS: arXiv:1502.07400PreselectionPhys. Lett. B 749 (2015) 337

Page 45: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Categorize!❖ Different production mechanism (gluon

fusion vs. vector boson fusion) lead to different topologies

- In practice number of jets

❖ Different decay channels have different reducible backgrounds

- Hadronic tau decays are low multiplicity jets

❖ Categorize to exploit different S/B! - Assign corresponding weights (typically

ln(1+S/B)), to increase sensitivity

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hτµ

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Page 46: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Backgrounds❖ Small signal ⇒ need very accurate

background estimate - Use data where possible

❖ In this case: - Z → ττ (irreducible): take Z → µµ events from data,

replace one muon with simulated tau

- Misidentified leptons: get control sample, and independently measure probability to fake e or τh, check in control region

- Rest: simulation46

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Page 47: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Finally❖ Tighten cuts and look for signal ❖ Don’t forget systematic uncertainties - Difficult topic: estimators often have known

flaws, but “best we can do”

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Gustaaf Brooijmans CERN 2017

Run 2

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Page 49: The Road to Discovery · 2018-11-21 · Gustaaf Brooijmans CERN 2017 Goals Searches span very wide spectrum - Overview of many types of searches, with focus on experimental aspects

Gustaaf Brooijmans CERN 2017

Higgs Drawbacks❖ So with the addition of a Higgs boson around 125 GeV particle

physics could be “complete” - Like Mendeleev’s table for chemistry, but not understood. By itself, the

Higgs is very unsatisfactory: - Why are the couplings to the fermions what they are?

‣ Dumb luck (aka landscape)?

- What is the link to gravity?

- What about Dark Matter?

- Why does the Higgs break the symmetry?

- Why are there 3....?

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