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Linear Collider Physics

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Title: Linear Collider Physics


1
Linear Collider Physics
  • Tohru Takahashi
  • Hiroshima Univerisity

Aug. 10, 2000 3rd ACFA-LC WS Taipei
2
Introduction
K.Fujii
  • The First ACFA LC WS ,,,,,Beijing
  • Justification is over.
  • More
  • detailed simulation
  • for detector design
  • with realistic beam related backgrounds
  • theoretical insight
  • to expand the potential of the collider

3
  • The Second ACFA LC Ws Seoul
  • talks on detailed simulation
  • theoretical insight
  • The Third one has to see
  • where we are toward the ACFA Report.

draft by the end of 2000 submitted in spring 2001
4
Issues to be covered in the ACFA report
  • Physics
  • How well we can explore mechanism of the symmetry
    breaking?
  • Higgs, SUSY, top, anomalous coupling, contact
    interaction,,,,,,,,
  • Detectors
  • good enough for precise measurement?
  • tough enough with beam background?
  • Options gg/ge, e-e-,
  • Well justified?
  • thechnically feasible?

5
Physics to be explored
  • mechanism of the electroweak symmetry breaking

LC has to find it, identify itself
something, called Higgs, somehow, condensed to
the vacuum
world we live,,,, electroweak superconductors
6
Some scenario
  • Promising?
  • light higgs boson
  • most lucky
  • light higgs, Heavy Higgs, SUSYs
  • Grand Unification
  • ,,,,,,,,,,
  • no higgs at LC lt 500 GeV
  • strong coupling in Higgs sector

always have top, Ws
7
Light Highs boson
A.Gurtu, ICHEP2000
Mh lt 175 GeV _at_ 95 C.L.
8
If light higgs bosons
  • Discovery seems ok

even in NMSSM
9
Precise measuremt of Higgs property
  • Once a Highs boson is discovered
  • s(hz), Br(h-gtWW)
  • Higgs gauge coupling
  • branching ratio to fermion
  • Higgs Yukawa coupling
  • has information on heavy mass content
  • CP
  • SM, or exotic

Which/what highs it is.
w
h
h
z
z
w
mass
f
h
f
g
h
g
10
Mass
Lhomann, LCWS99
11
Branching Ratio etc
I.Nakamura, LCWS99
hep-ex/007022
only assuming
12
two photon decay width
  • ee-
  • gg

Ohgaki,Watanabe,TT
13
higgs coupling CP
  • light h ee-
  • gg
  • Linear Polarization
  • H,A interference

Kamoshita, Seoul
Asakawa, LCWS99
14
If SUSY,,,,
Planc scale Physics
SUSY breaking
SUSY spectra coupling
SUSY Spectroscopy
15
Example

W
W
e-R
e-R
ne
W0
W-
e
W-
e
WW background suppressed by pol beam!
16
Demonstration of the measurements
  • Chargino and neutrarino mass

jets
17
Scalar muon mass
18
Selectron production
ee-
e-e-
eg
19
Test of SUSY GUT
20
If no new particles
  • Try to get information of physics of high energy
  • which energy we have to go next
  • Anomlous coupling of W bosons
  • contact interaction
  • Top quark property,,,,,,,,
  • In other word,,,,,,,
  • these physics are most promising in some sense

21
Anomalous coupling of W bosons
  • ee-
  • gg
  • do good a job up to 500 GeV

gg 10fb-1
gg 10fb-1
50fb-1
100fb-1
200fb-1
22
contact interactions
  • e-e- ,ee-

positron polarization?
23
top quark physics
GD
GP
GD
  • Promising
  • does not depend on scenarios.
  • large decay width allow us to see top decay
    properties

24
next step
  • more precise measurement
  • testing CP in top production/decay
  • requires full reconstruction of the top quark
    final state

ISR, beamstrahlung, missing P, top, W
width, b-tagging
a most tough test channel
25
Detector-Beam related Issues
  • Physics at the Linear Collider must be physics
    of precise measurement.
  • 1) High energy interaction
  • high energy narrower jets.
  • high energy particles
  • 2) High luminosity
  • beam-beam interaction
  • beamstrahlung
  • incoherent pairs
  • 1)2)
  • hadronic background

26
TeV Gravity
Moller
BhaBha
27
Beam-Beam Interaction
A field of the bunch seen by an electron ,,,,,,
O(kT)
critical energy of synchrotron rad.
(beamstrahlung)
pair background
Lum dist.
28
(No Transcript)
29
Tauchi, Beijing
30
Interaction Region
31
(No Transcript)
32
Effect of beam interaction
  • beamstrahlung

33
Interaction region
34
Incoherent pairs
35
Minimum veto angle
  • pair production

acoplanar tau pairs
36
Hadronic background
  • resolved photon process
  • bunch ID
  • good t0 resolution of the CDC

overlap prob.
37
Linear Collider options
scenario
ee-
gg/ge
e-e-
light Higgs only
SUSY
Strong int.
W coupling
WW scatt.
others extradimension,,,
better than ee-?
better than ee-?
38
Summary
  • Let see
  • where we are toward the ACFA report
  • we should fully explore the potential of the
    linear collier with possible options

39
Effect on the Highs properties of a new physics
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