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10th May 2013 Fergus Wilson, RAL 1
Experimental Particle Physics PHYS6011Looking for Higgs and SUSY at the LHCor...what can you get for $10,000,000,000
Lecture 5First LHC collisions at 4.0 TeV per beam 5th April 2012
http://hepwww.rl.ac.uk/fwilson/Southampton
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10th May 2013 Fergus Wilson, RAL 2
Search for the Higgs Boson Missing piece of Standard
Model Standard Model Higgs theory
well understood: Mass is only free parameter Clear predictions to test
Most “New Physics” models have something equivalent to a Higgs boson (“MSSM Higgs”, “little Higgs”, etc…).
Could be more than one type of Higgs boson
Current limit MH>115 GeV (LEP)
Particle masses are generated by interactions with the scalar (Higgs) field.
Couplings are fixed by the masses.
Once MH is known everything is predicted.
So by measuring the coupling of the Higgs to particles of known mass we can test theory.
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Higgs Mechanism in the Standard Model Need to accommodate massive gauge bosons
Strong and electromagnetism ok (photon, gluon) Weak force has two massive W and a Z
Step 1: Spontaneous Symmetry Breaking produces one massive and one massless gauge boson (Goldstone Boson).
Step 2: Introduce local gauge invariance : massive Higgs particle, three massive vector bosons and one massless boson.
Higgs mass a free parameter Gauge couplings of Higgs doublet give gauge boson masses:
Can calculate υ (=246GeV) but not λ before measuring Higgs mass. Higgs couplings to fermions depends on their mass and unique
coupling for each fermion:
10th May 2013 Fergus Wilson, RAL 3
2 42Modified potential V
22HM
2
min
/ 2 cos cos 0.8810W W Z W W WM g M M
f H fM M g
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What do we know about the Higgs?
10th May 2013 Fergus Wilson, RAL 4
No useful lower limit from theory. Upper limit from WW scattering
Above ~1TeV cross-section → ∞ Need Higgs to “regularise” cross-section
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10th May 2013 Fergus Wilson, RAL 5
What do we know about the Higgs?
2 22 2
2
2
8246 GeV
3logH
QCD
vM
v
If no new physics up to Planck scale (~1019GeV) small mass range for Higgs: 130 < MH< 190 GeV
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What do we know about the Higgs?
10th May 2013 Fergus Wilson, RAL 6
Direct searchesMH > 114.4 GeV
@ 95% C.L.
http://lepewwg.web.cern.ch/LEPEWWG
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How to discover a signal? Total number of events (nt) will have signal events (ns)
and background events (nb) Number of events follows a Poissonian distribution with σ
= sqrt(n). Require signal > 5σ above background for “observation”.
Require signal > 3σ above background for “first evidence”.
e.g. Measure 140 events and know 100 come from background:
How do you know the background? Monte Carlo or Look in areas where there is no signal.
Significance depend on how much data you have taken
10th May 2013 Fergus Wilson, RAL 7
Significance S 5s bn n
40 / 100 4S
LuminosityS
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Higgs Production Mechanisms
33 2 12 10L cm s
10th May 2013 Fergus Wilson, RAL 8
Gluon fusion most promising
Sometimes called “Associated ttH production”
Sometimes called “Associated WH,ZH production”
t
t
Gluon fusion looks most promising
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Higgs production and decay
10th May 2013 Fergus Wilson, RAL 9
How often is it produced? What does the Higgs decay into?
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Which Higgs decay to look for
10th May 2013 Fergus Wilson, RAL 10
08.0105.210
20)(
68
H
decays
N
NggHiggsBF
Branching Fraction: If produce 108 Higgs and measure only 20 decays H→gg with an efficiency of 0.00025% then Branching Fraction:
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10th May 2013 Fergus Wilson, RAL 11
Best Modes to look at
Compare to list on previous slides
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10th May 2013 Fergus Wilson, RAL 12
Huge stats for Standard Model signals. Rates @ 1033cm-2 s-1
~109 events/10 fb-1 W (200 Hz)~108 events/10 fb-1 Z (50 Hz)~107 events/10 fb-1 tt (1 Hz)
(10 fb-1 = 1 year of LHC running at low luminosity 1033 cm-2 s-1)
Backgrounds - Tevatron to the LHC
Background is anything with signature similar to signal
W+X (X can be W, Z or just 2 QCD jets)
ZZ-> qql+l- (one lepton not identified)
τ+τ-
b-tags can be real, charm or fakes
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10th May 2013 Fergus Wilson, RAL 13
Current Results - Tevatron At 120 GeV H->bb dominates Signature gg->H->bb:
2 jets One or two b-tags
Swamped by dijet production bb ~ μb qq ~ mb (fake b-tag rate small but not zero)
Have to use W/Z+H channel (Associated Production)
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10th May 2013 Fergus Wilson, RAL 14
Tevatron/CDF - Associated Production W->qq 70%
final state qqbb Four jet backgrounds still too large
W*H
Wq
qb
b
W-> eνe 10% W-> μνμ 10% Final state lνbb
One electron or muon Missing transverse momentum Two jets One or two b-tags
Easy to select in trigger and offline
σ×Br ≈ 0.02 pb
Qq->WH with H->bb
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Understanding “Higgs Exclusion Plot”
10th May 2013 Fergus Wilson, RAL 15
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Latest Higgs Results from Tevatron
10th May 2013 Fergus Wilson, RAL 16
Combined from many measurements.
10 years of data
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Latest Higgs Results from LHC
10th May 2013 Fergus Wilson, RAL 17
Nov 2011
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Is the Standard Model all there is? So far we have assumed a Standard Model Higgs but...
Does not explain Dark Matter Does not unify electromagnetism, weak and strong forces at high-energies (1016
GeV, Planck mass). Do not know the Higgs potential Calculations of Higgs mass using Standard Model produces a mass which is far
too high (>1 TeV) Need models beyond the Standard Model
10th May 2013 Fergus Wilson, RAL 18
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Supersymmetry
10th May 2013 Fergus Wilson, RAL 19
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Supersymmetric Higgs Need at least two Higgs doublets (H1,H2) to generate down- and up-type
particles. Physical particles:
Radiative corrections can change masses. Higgs sector now described by two free parameters (mh and tanβ=υ2/υ1). However, the exact SUSY symmetry has to be broken to reconcile the theory
with experiment (i.e. the standard model and SUSY particles have different masses).
The minimal extension to SUSY (MSSM) has 105 parameters! Have to assume a specific model e.g. mSUGRA
Modifies Higgs mechanism 5 free parameters:
tanβ (as before) m0 (universal scalar mass, includes Higgs) m½(gaugino mass) plus two others
10th May 2013 Fergus Wilson, RAL 20
2 1
2 1
2 2
cos sin ( )
sin cos ( )
CP-odd Higgs
H charged Higgs ( )
h Z
H Z
A WH
h H H m m
H H H m m
A
m m m
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Looking for SUSY Higgs at the LHC Small tanβ
gg→H,A production is enhanced due to stronger ttH coupling. H,A →tt decay gets enhanced.
Large tanβ H, A production is enhanced in bb-fusion H →ττ has a large branching ratio
Medium tanβ Only SM-like h visible. We could see a Higgs and not realise we
have seen SUSY! Charged Higgs
Clear signal for new physics (not predicted in Standard Model)
10th May 2013 Fergus Wilson, RAL 21
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Looking for other SUSY particles SUSY predicts that every Standard Model particle has a Super-
Symmetric partner Electron ↔ selectron, quark ↔ squark,W ↔ wino, etc... But masses not the same → SUSY not exact symmetry
SUSY can be a new source of CP-Violation Explain matter/anti-matter asymmetry of the Universe
A SUSY particle will quickly decay to the Lightest Supersymmetric Particle (LSP). Neutral (no charge) LSP is a candidate for Dark Matter
LSP will leave detector without interacting Large Missing energy, momentum (because LSP is massive)
What is the LSP? Don’t really know Likely to be a neutralino
10th May 2013 Fergus Wilson, RAL 22
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What a SUSY decay looks like
10th May 2013 Fergus Wilson, RAL 23
Lots of leptons produced. Easy to see and not produced in background events
Missing energy
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What theory predicts for SUSY at LHC
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What we currently (don’t) see (March 2012)
10th May 2013 Fergus Wilson, RAL 25
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What we currently (don’t) see (March 2012)
10th May 2013 Fergus Wilson, RAL 26
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Status of the LHC The Higgs mass has not been excluded around
~125GeV By the end of 2012, the LHC will be able to
confirm/deny presence of a Higgs below ~600 GeV. If 125 GeV Higgs confirmed
Could be a Standard Model Higgs (good). Could be a SUSY Higgs (also good).
If no Higgs below ~600 GeV Higgs mechanism (and therefore Standard Model) in big
trouble (bad). If no SUSY particles found below 1 TeV
SUSY models are “wrong” (bad) but theorists always have a back up plan.
10th May 2013 Fergus Wilson, RAL 27
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One final thought... John Ellis, Nature 481, 24 (2012)
“One option is that the evidence from the LHC will be confirmed, and a standard-model Higgs boson exists in the low-mass range below 130 GeV....But there is a catch. Within the standard model, it is possible to calculate the lowest energy state of the Universe. If the Higgs is light, this calculation predicts a lowest energy state totally unlike our current Universe. It implies that our Universe is in some other, unstable state that will eventually flip over to its lowest energy condition — next week, or in a few billion years, we could go down the cosmological tubes....”
10th May 2013 Fergus Wilson, RAL 28
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ATLAS detector
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ATLAS beam-pipe
10th May 2013 Fergus Wilson, RAL 30
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ATLAS construction
10th May 2013 Fergus Wilson, RAL 31
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ATLAS Tracker (silicon)
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ATLAS toroid magnet
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CMS detector
10th May 2013 Fergus Wilson, RAL 34
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10th May 2013 Fergus Wilson, RAL 35
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Inserting CMS tracker
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Inserting CMS tracker
10th May 2013 Fergus Wilson, RAL 37
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10th May 2013 Fergus Wilson, RAL 38
Damaged magnets 2009
QQBI.27R3 20/04/23 38LHC status and commissioning
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10th May 2013 Fergus Wilson, RAL 39
Which decay to look at? Depends on Higgs Mass
MH <100 GeV gg → H→γγ
MH <150 GeV H→ZZ* →4l H→bb H→WW* →2l 2ν H →τ+τ-
130 < MH <500 GeV H→ZZ →4l
600 < MH < 1000 GeV H→ZZ,WW → jets
Higgs Decay
08.0105.210
20)(
68
H
decays
N
NggHiggsBF
Branching Fraction: If produce 108 Higgs and measure only 20 decays H→gg with an efficiency of 0.00025% then Branching Fraction: