present and future of high energy physics - cern · present and future of high energy physics...
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![Page 1: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/1.jpg)
Present and Future of High Energy Physics
Hitoshi Murayama (IPMU Tokyo, Berkeley)EPAC 2008, Genoa, Italy
June 27, 2008
!"#$
%&'()*+,-./01
2!#3(*
2004.2.12
456
789:
;<9:
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Accelerators and Particle Physics
accelerators have been the enabling technology for particle physicsnon-accelerator experiments are becoming more important partly because of price tagsHowever, I expect & hope that accelerator-based HEP remains main drivers in the foreseeable future
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non-accelerator physics
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non-accelerator physics
Many non-accelerator physics discoveries had to be confirmed, studied, and improved using accelerators
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non-accelerator physics
Many non-accelerator physics discoveries had to be confirmed, studied, and improved using acceleratorsbatteries: electrons as cathode ray
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non-accelerator physics
Many non-accelerator physics discoveries had to be confirmed, studied, and improved using acceleratorsbatteries: electrons as cathode raycosmic-ray: muons, pions, kaons
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non-accelerator physics
Many non-accelerator physics discoveries had to be confirmed, studied, and improved using acceleratorsbatteries: electrons as cathode raycosmic-ray: muons, pions, kaonsatmospheric neutrinos: oscillations
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non-accelerator physics
Many non-accelerator physics discoveries had to be confirmed, studied, and improved using acceleratorsbatteries: electrons as cathode raycosmic-ray: muons, pions, kaonsatmospheric neutrinos: oscillationsdark matter: LHC & ILC?
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Major Achievements >2000
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Major Achievements >2000
amazing precision measurements from PEP-II/KEK-B establishing KM theory
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Major Achievements >2000
amazing precision measurements from PEP-II/KEK-B establishing KM theory
large data set from Tevatron discovering Bs mixing, precision studies of W, top, narrowing range for the SM Higgs
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Major Achievements >2000
amazing precision measurements from PEP-II/KEK-B establishing KM theory
large data set from Tevatron discovering Bs mixing, precision studies of W, top, narrowing range for the SM Higgs
K2K/MINOS confirmation of neutrino oscillation
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Outline
IntroductionEnergy Frontier
Firm and established needs for TeVless firm but exciting needs for beyond
Intensity Frontierneeds for intense neutrinoshigh precision flavor physics
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Energy Frontier
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New Era
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cm
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cmknown since Fermi (1933), finally there!
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cmknown since Fermi (1933), finally there!presumably it is also a derived scale more fundamental theory
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cmknown since Fermi (1933), finally there!presumably it is also a derived scale more fundamental theorysupersymmetry? extra dimensions? string theory?
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cmknown since Fermi (1933), finally there!presumably it is also a derived scale more fundamental theorysupersymmetry? extra dimensions? string theory?If so, we expect rich spectrum of new particles!
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New Era
∼1900 reached atomic scale 10-8cm≈α/me
∼1970 reached strong scale 10-13cm≈Me-2π/αs b0
∼2010 will reach weak scale 10-17cmknown since Fermi (1933), finally there!presumably it is also a derived scale more fundamental theorysupersymmetry? extra dimensions? string theory?If so, we expect rich spectrum of new particles!
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TeV
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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!]
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Something is in the Universe
There is something filling our UniverseIt doesn’t disturb gravity or electric forceIt does disturb weak force and make it short-rangedIn fact, it is the “mother of mass” for all elementary particlesWhat is it??
gravity
electric force
weak force
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Like a superconductor
In a superconductor, magnetic field gets repelled (Meißner effect), and penetrates only over the “penetration length” ⇒ Magnetic field is short-ranged!
Imagine a physicist living in a superconductorShe finally figured:
magnetic field must be long-ranged there must be a mysterious charge-two condensate in her “Universe”But doesn’t know what the condensate is, nor why it condensesDoesn’t have enough energy (gap) to break up Cooper pairs
That’s the stage where we are!
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Large Hadron Collider (LHC):Exploring the TeV-scale
1
10
100
100 120 140 160 180 200
Sig
nal
sig
nif
ican
ce
Total significance
!Ldt = 30 fb"1
(no K-factors)
ATLAS
5#
mH (GeV/c2)
H $ %%
ttH (H $ bb)H $ ZZ(*) $ 4l
H $ WW(*) $ l&l&qqH $ qqWW(*)
qqH $ qq''
Robust discovery
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Questions to be answered
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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 JP=0+?Is it condensed in the Universe?
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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 JP=0+?Is it condensed in the Universe?
Prove it is the “Mother of Mass”Spin/Parity CouplingsBranching RatiosSize of the condensate
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Linear Collider
International Linear Collider (ILC)
ElectronsPositrons
Drawing not to scale
February 2007
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Linear Collider
International Linear Collider (ILC)
ElectronsPositrons
Drawing not to scale
February 2007 ! !-
-+
+
(GeV)
10
10
1
-3
-2
10-1
SM
Hig
gs
Bra
nch
ing
Ra
tio
bb
ggcc
""
MH
W W
100 110 120 130 140 150 160
Branching Fractions test the relation: coupling ∝ mass
⇒ proves that Higgs Boson is the Mother of Mass
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TeV to multi-TeV
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Three reasons beyond Higgs
Hierarchy Problem
Dark Matter of the Universe
Physics behind Higgs
all suggest rich physics at
sub-TeV to multi-TeV
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Evidence for Dark Matter
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Evidence for Dark Matter
Galaxy is held together by mass far bigger than all stars
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WMAP satellite result ΩMh2=0.135±0.009Ωbh
2=0.0224±0.0009ΩM/Ωb=5.70+0.39-0.61dark matter is not atoms!
Cosmic Microwave Background
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WIMP
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WIMP
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It must be WIMP (Weakly Interacting Massive Particle)
Stable heavy particle produced in early Universe, left-over from near-complete annihilation
WIMP
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It must be WIMP (Weakly Interacting Massive Particle)
Stable heavy particle produced in early Universe, left-over from near-complete annihilation
WIMP
ΩM =0.756(n +1)x f
n+1
g1/2σannMPl3
3s08πH0
2 ≈α 2 /(TeV)2
σann
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Post-Higgs Problem
We see “what” is condensedBut we still don’t know “why”From Ginzburg-Landau to BCS theoryTwo problems:
Why anything is condensed at allWhy is the scale of condensation ~TeV<<MPl=1015TeV
Explanation most likely to be at ~TeV scale because this is the relevant energy scalestudy Higgs properties and interaction in detail!
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Once upon a time,there was a hierarchy problem...At the end of 19th century: a “crisis” about electron
Like charges repel: hard to keep electric charge in a small packElectron is point-likeAt least smaller than 10–17cm
Need a lot of energy to keep it small!
Correction Δmec2 > mec
2 for re < 10–13cmBreakdown of theory of electromagnetism ⇒ Can’t discuss physics below 10–13cm
Δmec2 ~ α
re~ GeV10
−17cmre
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Anti-Matter Comes to Rescueby Doubling of #Particles
Electron creates a force to repel itselfVacuum bubble of matter anti-matter creation/annihilationElectron annihilates the positron in the bubble⇒ only 10% of mass even
for Planck-size
e–
!
e–
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Anti-Matter Comes to Rescueby Doubling of #Particles
Electron creates a force to repel itselfVacuum bubble of matter anti-matter creation/annihilationElectron annihilates the positron in the bubble⇒ only 10% of mass even
for Planck-size
e–
e+
!
e–
!
e–
22
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Anti-Matter Comes to Rescueby Doubling of #Particles
Electron creates a force to repel itselfVacuum bubble of matter anti-matter creation/annihilationElectron annihilates the positron in the bubble⇒ only 10% of mass even
for Planck-size
e–
e+
!
e–
!
e–
e–
e+
!
e–
22
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Anti-Matter Comes to Rescueby Doubling of #Particles
Electron creates a force to repel itselfVacuum bubble of matter anti-matter creation/annihilationElectron annihilates the positron in the bubble⇒ only 10% of mass even
for Planck-size
e–
e+
!
e–
!
e–
e–
e+
!
e–
!me
me
!
!
4"
log(mere)
22
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Higgs repels itself, too
Just like electron repelling itself because of its charge, Higgs boson also repels itselfRequires a lot of energy to contain itself in its point-like size!Breakdown of theory of weak forceCan’t even think about short distance physics!
€
ΔmH2 c4 ~ c
rH
2
shorter
distance
EW scale
SM breaks
down here
physics that
answers
questions
~100GeV
~1TeV
???
H H
H
23
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History repeats itself?
Double #particles again ⇒ superpartners
“Vacuum bubbles” of superpartners cancel the energy required to contain Higgs boson in itselfStandard Model made consistent with whatever physics at shorter distances
24shorter
distance
EW scale
SM breaks
down here
physics that
answers
questions
~100GeV
~1TeV
???
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History repeats itself?
Double #particles again ⇒ superpartners
“Vacuum bubbles” of superpartners cancel the energy required to contain Higgs boson in itselfStandard Model made consistent with whatever physics at shorter distances
€
ΔmH2 ~ α
4πmSUSY2 log(mHrH )
H H
H
H H
H~
W~
24shorter
distance
EW scale
SM breaks
down here
physics that
answers
questions
~100GeV
~1TeV
???
![Page 52: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/52.jpg)
History repeats itself?
Double #particles again ⇒ superpartners
“Vacuum bubbles” of superpartners cancel the energy required to contain Higgs boson in itselfStandard Model made consistent with whatever physics at shorter distances
€
ΔmH2 ~ α
4πmSUSY2 log(mHrH )
H H
H
H H
H~
W~
24shorter
distance
EW scale
SM breaks
down here
physics that
answers
questions
~100GeV
~1TeV
???
shorter
distance
EW scale
SUSY
physics that
answers
questions
~100GeV
~1TeV
???
![Page 53: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/53.jpg)
25
Three Directions
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25
Three Directions
History repeats itselfCrisis with electron solved by anti-matterDouble #particles again ⇒ supersymmetry
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25
Three Directions
History repeats itselfCrisis with electron solved by anti-matterDouble #particles again ⇒ supersymmetry
Learn from Cooper pairsCooper pairs composite made of two electronsHiggs boson may be fermion-pair composite ⇒ technicolor
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25
Three Directions
History repeats itselfCrisis with electron solved by anti-matterDouble #particles again ⇒ supersymmetry
Learn from Cooper pairsCooper pairs composite made of two electronsHiggs boson may be fermion-pair composite ⇒ technicolor
Physics as we know it ends at TeVUltimate scale of physics: quantum gravityMay have quantum gravity at TeV ⇒ hidden dimensions (0.01 cm to 10–17 cm)
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Need absolute confidence for a major discovery
![Page 59: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/59.jpg)
Need absolute confidence for a major discovery
As an example, supersymmetry
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Need absolute confidence for a major discovery
As an example, supersymmetry“New-York Times level” confidence
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Need absolute confidence for a major discovery
As an example, supersymmetry“New-York Times level” confidence
The Other Half of the World Discovered
July 23, 2009
Geneva, Switzerland
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Need absolute confidence for a major discovery
still a long way to
As an example, supersymmetry“New-York Times level” confidence
The Other Half of the World Discovered
July 23, 2009
Geneva, Switzerland
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Need absolute confidence for a major discovery
still a long way to
“Halliday-Resnick” level confidence
As an example, supersymmetry“New-York Times level” confidence
The Other Half of the World Discovered
July 23, 2009
Geneva, Switzerland
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Need absolute confidence for a major discovery
still a long way to
“Halliday-Resnick” level confidence
“We have learned that all particles we observe have unique partners of different spin and statistics, called superpartners, that make our theory of elementary particles valid to small distances.”
As an example, supersymmetry“New-York Times level” confidence
The Other Half of the World Discovered
July 23, 2009
Geneva, Switzerland
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28
Hidden Dimensions
Hidden dimensions
Can emit graviton into the bulk
Events with apparent energy imbalance
⇒ How many extra dimensions are there?
G
e
e
!
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28
Hidden Dimensions
Hidden dimensions
Can emit graviton into the bulk
Events with apparent energy imbalance
⇒ How many extra dimensions are there?
G
e
e
!
LC
5
10
20
30
50
100
200
400 450 500 550 600 650 700 750 800 850 900
ECM (GeV)
!G / (
fb)
D=6
D=7
D=8
D=9
D=10ILC
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29
Supersymmetry
Tevatron/LHC will discover supersymmetry
Can do many measurements at LHC
! L dt = 1, 10, 100, 300 fb-1
A0= 0, tan! = 35, µ > 0
ET
(300 fb-1)miss
ET
(100 fb-1)miss
ET
(10 fb-1)miss
ET
(1 fb-1)miss
g(1000)~
q(1500)
~
g(1500)~
g(2000)~
q(2500)
~
g(2500)~
q(2000)
~
g(3000)~
q(1000)
~
q(500)
~g(500)~
!h2 =
0.4
!h2 =
1
!h 2 =
0.15
h(110)
h(123)
1400
1200
1000
800
600
400
200
50000
1000 1500 2000
m0 (GeV)
m1
/2(G
eV
)
EX
TH
CMS
one year
@1033
one year
@1034
one month
@1033
Fermilab reach: < 500 GeV
one week
@1033cosmologically plausible
region
0
50
100
150
200
250
300
350
400
0 50 100 150 200 250 300 350 400
S5
O1
M! (GeV)"1
0
Ml (
Ge
V)
" R
LHC LHC
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30
Prove Superpartnershave different spin
Discovery at Tevatron Run II and/or LHCTest they are really superpartners
Spins differ by 1/2Same SU(3)×SU(2)×U(1) quantum numbersSupersymmetric couplings
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30
Prove Superpartnershave different spin
Discovery at Tevatron Run II and/or LHCTest they are really superpartners
Spins differ by 1/2Same SU(3)×SU(2)×U(1) quantum numbersSupersymmetric couplings
Spin 0?
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30
Prove Superpartnershave different spin
Discovery at Tevatron Run II and/or LHCTest they are really superpartners
Spins differ by 1/2Same SU(3)×SU(2)×U(1) quantum numbersSupersymmetric couplings
Spin 0?
#E
vents
cos !
150
100
50
0–1 –0.5 0 0.5 1
e+e" # µ+µ"
$s = 350 GeV
% %
Tsukamoto, Fujii, HM, Yamaguchi, Okada
ILC
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31
Creating Dark Matter
Look for reactions where energy and momenta are unbalanced
“missing energy” Emiss
Something is escaping the detectorelectrically neutral, weakly interacting⇒Dark Matter!?
4.8Gev EC19.Gev HC
YX hist.of BA.+E.C.0| ! 500cm 500cm|X
0|!500cm
500cm|
Y
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Dark Matter Concordance
abundance
32
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Dark Matter Concordance
abundance direct detection
32
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Required New Facilities
LHC & ILC may do it if new particles are light enoughPossibly, we need to go beyond themneed a tandem of proton & leptonneed to keep eyes on a few to 10 TeVhigher gradient cavities, CLIC, high-field magnets, muon collider, plasma
33
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Intensity Frontier
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35
Baryon AsymmetryEarly Universe
10,000,000,001 10,000,000,000
q q_
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36
Baryon AsymmetryCurrent Universe
1us
The Great Annihilationq q
_
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37
CP Violation
Is anti-matter the exact mirror of matter?1964 discovery of CP violation in neutral kaon systemBut only one system, hard to tell what is going on.2001 Found kaon and anti-kaon decay differently at 10–6 level2002 Found CP violation also in B-meson systemBut no CP violation observed so far is large enough to explain the absence of anti-matter
Entr
ies
/ 0.6
ps
B0 tags
B! 0
tags
Background
"t (ps)
Raw
Asy
mm
etry
0
50
100
150
-0.5
0
0.5
-5 0 5
BaBar
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38
Leptogenesis
Neutrinos may be their own anti-particles
They can transform matter to anti-matter and vice versa
Maybe they are responsible for our existence!
![Page 80: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/80.jpg)
38
Leptogenesis
Neutrinos may be their own anti-particles
They can transform matter to anti-matter and vice versa
Maybe they are responsible for our existence!
• CP-violation may be observed in neutrino oscillation
• Plans to shoot neutrino beams over thousands of kilometers to see this
P (!µ ! !e)" P (!̄µ ! !̄e) = "16s12c12s13c213s23c23
sin " sin
!!m2
12
4EL
"
sin
!!m2
13
4EL
"
sin
!!m2
23
4EL
"
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First Steps
39
Neutrino beam
Far detector
NOνAMINOS
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First Steps
39
Neutrino beam
Far detector
NOνAMINOS
T2K startsnext year
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40
Very Long Baseline Experiment
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40
Very Long Baseline Experiment
Shoot the beams over thousands of kilometers to see
CP violation in neutrinos
![Page 85: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/85.jpg)
Once new particles at TeV
41
What do they do with flavor?Do they come in three generations?If so, do they mix the same way as quarks and leptons?If not, do their interactions preserve or violate flavor?
Ultimately, what is the origin of flavor?need a large sample of kaons, muons, B’s
![Page 86: Present and Future of High Energy Physics - CERN · Present and Future of High Energy Physics Hitoshi Murayama (IPMU Tokyo, Berkeley) EPAC 2008, Genoa, Italy June 27, 2008 !"#$ %&’()*+,-./01](https://reader031.vdocuments.net/reader031/viewer/2022011901/5f06dc347e708231d41a18c9/html5/thumbnails/86.jpg)
Required New Facilities
high-intensity proton machine (4MW?)to produce intense neutrino beamsto create kaons for precision studies
high-intensity electron machine (1036?)to create B mesons for precision studies
high-intensity muon source (1020?)neutrino factorymuon flavor physics
42
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Required New Facilities
high-intensity proton machine (4MW?)to produce intense neutrino beamsto create kaons for precision studies
high-intensity electron machine (1036?)to create B mesons for precision studies
high-intensity muon source (1020?)neutrino factorymuon flavor physics
42much stronger case with LHC discoveries
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Conclusions
43
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Conclusions
Accelerators will remain critical drivers for particle physics research
43
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Conclusions
Accelerators will remain critical drivers for particle physics researchFirm case for LHC & ILC followup
43
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Conclusions
Accelerators will remain critical drivers for particle physics researchFirm case for LHC & ILC followupGood reasons to except more excitement, likely to need to go multi TeV scales
dark matter, beyond Higgs, hierarchy
43
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Conclusions
Accelerators will remain critical drivers for particle physics researchFirm case for LHC & ILC followupGood reasons to except more excitement, likely to need to go multi TeV scales
dark matter, beyond Higgs, hierarchyNeed high intensity neutrinos
43
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Conclusions
Accelerators will remain critical drivers for particle physics researchFirm case for LHC & ILC followupGood reasons to except more excitement, likely to need to go multi TeV scales
dark matter, beyond Higgs, hierarchyNeed high intensity neutrinosneed to study consequences of new particles on flavor physics
43
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Our Future Rests On You!
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