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Coordinators:
Marco
Battaglia (CERN), Ian Hinchliffe
(LBNL),
John Jaros (SLAC),
James Wells(UC Davis)
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Physics Contacts:
Higgs: R. Van Kooten
(Indiana) and
J. Conway (Rutgers U.),
SUSY: G. Blair
(Royal Holloway Coll.),
Exotics: M. Perelstein (LBL) and
S. Mrenna (UC Davis)
Strong Symmetry Breaking:
T. Barklow (SLAC),
T. Han (Wisconsin)
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We will consider the following
physics scenarios
in order to assess what impact measurements from a linear collider will
have on what will already have been learned from Tevatron and LHC running.
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SO1 -
Precision EW Data: (Coordinator
K. Moenig (DESY))
SO2 -
Photon and Electron Collider:
(Coordinators:
J. Gronberg (LLNL) and
M. Velasco (Northwestern U.))
SO3 - Positron Polarization: (Coordinators:
P. Rowson (SLAC) ,
E. Torrence (Oregon U.))
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How does each of these special options contribute
to the physics scenarios listed above?
What other new measurements are possible
with each option?.
What are the special machine and detector requirements for
each option, and what R&D is required before the option is feasible?
In what scenarios is the physics case for the special option so
compelling that running time should be shared between a high energy e+e- IR
and one devoted to the special option?
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DQ1 - LC Performance Trade-offs:
How may the design differences between
the different LC projects impact the physics that can be done at each machine?
What are the trade-offs between energy and luminosity, luminosity and
backgrounds, polarisation and luminosity for each LC project ?
(Discussion Leader: M. Battaglia)
DQ2 - LC Planning:
What are the pros and cons of proceeding to the
construction of a Tev Class LC before results are available from the LHC ?
(Discussion Leader: J. Wells)
DQ3 - Luminosity Management: For each of the
physics scenarios, what is the best way to distribute
running time over various center of mass energies to optimize the physics
output ? How much time is required ? (Discussion Leaders: H. Montgomery and
J. Siegrist)
DQ4 - LC Expandability:
What is the energy for the initial phase of the LC
(350 GeV, 500 GeV)? Assuming the energy reach is expanded using the same
technology as in the initial phase, what is the high energy goal for a
secondary phase of the LC? What R&D issues remain before such an expansion
is possible? What constraints on the initial phase would ultimate
conversion to two-beam drive impose? (Discussion Leader: P. Burrows)
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Wed July 4
(11:30 - 13:00)
Start of Sub-group Activities
Parallel SG1
Charge to Physics Contacts and Physics Issues
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Fri July 6
(8:00 - 12:15)
General Announcements
Plenary SG1 - TeV-class LC
Sub-group:
Plenary SO1 - Physics at the GigaZ
(speaker: K. Moenig)
Plenary SO2 - Physics at gamma-gamma and electron
Colliders (speaker: M. Velasco)
Plenary SO3 - Introduction and Production of Polarized
Positrons (speaker: P. Rowson and K. Floettman)
Plenary DQ4 - LC Energy and Expandability
(Discussion Leader: P. Burrows)
Plenary DQ2 - LC Planning
(Discussion Leader: J. Wells)
Parallel SO1
Parallel SO2
Parallel SO3
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Tue July 10
(14:00 - 18:00)
General Announcements
Plenary SG1 - TeV-class LC
Sub-group
Higgs Physics: LC issues
Plenary DQ4 - LC Energy and Expandability
(discussion leader: P. Burrows )
Plenary SO2 - Techniques for the gamma-gamma
Collider
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Wed July 11
(8:15 - 12:15)
General Announcements
Plenary SG1 - TeV-class LC Sub-group
SUSY Models: LC issues
Plenary DQ3 - LC Luminosity Management
(Discussion Leaders: H. Montgomery and J. Siegrist)
Plenary SO3 - Techniques for polarized beams
Parallel DQ3
Parallel SO3
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Fri July 13
(8:15 - 12:15)
General Announcements
Plenary SG1 - TeV-class LC
Sub-group
Physics Beyond SM and Strong Symmetry Breaking: LC issues
Plenary SO1 - Physics with Precision EW Data
Plenary DQ3 - LC Luminosity Management
(Discussion Leaders: H. Montgomery and J. Siegrist)
Plenary DQ4 - LC Energy and Expandability
(discussion leader: P. Burrows )
Parallel SO1
Parallel DQ3 and DQ4
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| Last update June 21st, 2001 by M.B. |
