Presentation Transcript
Physics with 500 GeV LC : Physics with 500 GeV LC Hitoshi Murayama (UC Berkeley)
LC Retreat
Santa Cruz, June 27, 2002
We are interested inthings we don’t see : We are interested in things we don’t see
Energy budget of Universe : Energy budget of Universe Stars and galaxies are only 0.1%
Neutrinos are ~0.1–10%
Rest of ordinary matter (electrons and protons) are ~5%
Dark Matter ~25%
Dark Energy ~70%
Anti-Matter 0%
Higgs boson ~1062%??
The Cosmic Questions : The Cosmic Questions What is Dark Matter?
What is Dark Energy?
How much is Neutrino component?
Is Higgs Boson really there?
Where did Anti-Matter go?
Synergy at TeV scale : Synergy at TeV scale Dark Matter
Fermi (Higgs) scale
v~250GeV
Dark Energy
rL~(2meV)4 vs (TeV)2/MPl~0.5meV
Neutrino
(Dm2LMA)1/2~7meV vs (TeV)2/MPl~0.5meV
TeV-scale physics likely to be rich
Fermi’s dream era : Fermi’s dream era Fermi formulated the first theory of weak force (1933)
Knew the required energy to study the problem: ~TeV
We are finally getting there!
Higgs Boson : Higgs Boson
Mystery of the “weak force” : Mystery of the “weak force” Gravity pulls two massive bodies (long-ranged)
Electric force repels two like charges (long-ranged)
“Weak force” pulls protons and electrons (short-ranged) acts only over 10–16 cm [need it for the Sun to burn!]
Something is in the Universe : Something is in the Universe There is something filling our Universe
It doesn’t disturb gravity or electric force
It does disturb weak force and make it short-ranged
What is it??
Like a superconductor : Like a superconductor In a superconductor, magnetic field gets repelled (Meißner effect), but penetrates only over “penetration length”
Magnetic field is short-ranged!
Imagine a physicist living in a superconductor
Finally figured:
magnetic filed must be long-ranged
there must be mysterious charge-two condensate in his “Universe”
But doesn’t know what the condensate is, nor why it condenses
Doesn’t have enough energy to break up Cooper pairs
That’s the stage where we are!
Higgs Boson is Most Likely “Just Around the Corner” : Higgs Boson is Most Likely “Just Around the Corner” All current data combined, sensitive to quantum effects of the Higgs boson
mH<196GeV (95%CL)
(LEPEWWG Winter 2002)
Tevatron at Fermilab, IL, has chance to discover Higgs boson by 2008
Higgs Boson at LHC : Higgs Boson at LHC LHC would discovery Standard Model Higgs boson of any mass within 3 years! (2011?)
Does it settle the issue? I’m afraid not.
Suppose Hgg discovered, cross checked by ttH final state
Technipion? Scalar or pseudo-scalar? Does it couple to W/Z?
Questions to be answered : Questions to be answered Is the particle discovered really the Higgs boson?
Is it really responsible for particle masses?
Does this have the right quantum number 0+?
Is it condensed in the Universe?
Prove it is the “Origin of Mass”
Spin/Parity
Couplings
Vacuum expectation value
Branching Ratios
Higgs Boson at LC : Higgs Boson at LC Angular distribution in e+e–ZX depends on X=h, A, V Is it a 0+ boson?
Higgs Boson at LC : Higgs Boson at LC Branching Fractions test the relation coupling mass
proves that Higgs Boson is the “Origin of Mass”(Battaglia)
Higgs Boson at LC : Higgs Boson at LC ZH final state
ALR proves it is due to s-channel Z-exchange
Higgs Boson at LC : Higgs Boson at LC ZH final state
ALR proves it is due to s-channel Z-exchange
We know Z:gauge boson, H: scalar boson only two vertices
Higgs Boson at LC : Higgs Boson at LC ZH final state
ALR proves it is due to s-channel Z-exchange
We know Z:gauge boson, H: scalar boson only two vertices
Need a VEV to get ZZH vertex
Higgs Boson at LC : Higgs Boson at LC ZH final state
ALR proves it is due to s-channel Z-exchange
We know Z:gauge boson, H: scalar boson only two vertices
Need a VEV to get ZZH vertex proves it is the origin of mZ
HM, LBNL-38891
Absolute confidence is crucialfor a major discovery : Absolute confidence is crucial for a major discovery “New York Times” level confidence
“Origin of Mass Uncovered”
still a long way to
“Halliday-Resnick” level confidence
“We have learned that masses of all elementary particles originate in the condensate of so-called Higgs boson of mass 124GeV/c2.”
Post-Higgs Problem : Post-Higgs Problem
Post-Higgs Problem : Post-Higgs Problem We see “what” is condensed
But we still don’t know “why”
Two problems:
Why anything is condensed at all
Why is the scale of condensation ~TeV<
Three Directions : Three Directions History repeats itself
Crisis with electron solved by anti-matter
Double #particles again supersymmetry
Learn from Cooper pairs
Cooper pairs composite made of two electrons
Higgs boson may be fermion-pair composite
technicolor
Physics ends at TeV
Ultimate scale of physics: quantum gravity
May have quantum gravity at TeV
hidden dimensions
Task : Task Find physics responsible for condensation
We can eliminate many possibilities at LHC
But new interpretations necessarily emerge
Elucidate what that physics is
Reconstruct the Lagrangian from measurements
Many theories look alike : Many theories look alike Supersymmetry
Missing energy, high pT jets, leptons, b, t, t
Fourth generation
Missing energy, high pT jets, leptons, b, t, t
Many theories look alike : Many theories look alike Pseudo-Nambu-Goldstone bosons in technicolor
Universal Extra Dimensions (Cheng, Matchev, Schmaltz)
Lightest Kaluza-Klein states ~ LSP
If models well-defined and only a few parameters, LHC can exclude many interpretations of data
Race will be on:
theorists coming up with new interpretations
experimentalists excluding new interpretations
A loooong process of elimination
Crucial information is in details
LC is good at details : LC is good at details Supersymmetry Fourth generation Ejj distribution tells if mB 0
Cross sections vs polarization determine quantum numbers ~
Supersymmetry at LC : Supersymmetry at LC Discovery at Tevatron Run II or LHC
Test they are really superpartners
Spins differ by 1/2
Same SU(3)SU(2)U(1) quantum numbers
Supersymmetric couplings Spin 0?
Supersymmetry at LC : Supersymmetry at LC Is gaugino coupling = gauge coupling? Mass Measurement
Superpartners as probe : Superpartners as probe Most exciting thing about superpartners beyond existence:
They carry information of small-distance physics to something we can measure
“Are forces unified?”
Hidden Dimensions : Hidden Dimensions Randall-Sundrum scenario with warped extra 1D
TeV-scale KK gravitons
determine the shape of the hidden dimension
Produce Dark Matter : Produce Dark Matter Dark Matter likely to be TeV-scale electrically neutral weakly interacting particle (e.g., LSP, Lightest KK)
With LC, measure its mass, couplings
Can calculate its cosmic abundance
If it agrees with cosmological observation, we understand Universe back to 10–12 sec after the Big Bang
Conclusion : Conclusion Physics at TeV scale likely to be rich
To fully understand it, we will likely need a lot of detailed information
LC will study new particles one by one
reconstruct the fundamental Lagrangian
Then we would like to move on further with absolute confidence
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