Summary
STAR Inner Silicon tracking detector review :: abstracts
2398 - Benefit of the removal of the SVT for e- measurement
Introduction , 10:15Presenter : Thomas Ullrich
2401 - Overview of progress and current status of the SVT/SSD tracking effort
Software focused effort outcome and perspectives , 10:50Presenter : Spiros Margetis
2394 - Overview of STAR's BUR and main physics goals for the near term future
Introduction , 09:00Presenter : James Dunlop
2404 - Self-alignment status and perspectives
Software focused effort outcome and perspectives , 11:45Presenter : Victor Perevoztchikov
2421 - SSD Software and hardware maintainability and plans
Project(s) Management session , 11:20Presenter : Howard Matis
3034 - STAR Inner Silicon tracking detector committee report
Committee summary report , 15:00Presenter :
2403 - SVT calibration issues and remaining tasks for the future
Software focused effort outcome and perspectives , 11:30Presenter : Yuri Fisyak
2420 - SVT Software and hardware maintainability
Project(s) Management session , 11:00Presenter : Rene Bellwied
2402 - The use of Silicon detectors for future TPC Calibration
Software focused effort outcome and perspectives , 11:10Presenter : Gene Van Buren
2413 - Using the SVT for rejection of photon conversion
Status and analysis , 15:00Presenter : Frank Laue
2393 - Welcome
Introduction , 08:45Presenter :
Email from Tim Hallman, Spokesman for STAR sent on 5/27/2006 14:50
Dear STAR Collaborators,
The email concerns an upcoming planning exercise related to
STAR's inner tracking detectors. The review, which will take place
just before the Collaboration meeting (July 7-8) at BNL, will place
particular emphasis on understanding how a plan which optimizes our
physics program in the next few years (including planned upgrades
of STAR's capability) informs the question of future utilization of
the SVT and when it should be taken out of the STAR set-up.
The draft charge for the SVT Review Committee is attached below.
The agenda and the membership of the review panel will be announced
in the coming week.
As a final comment, I would like to thank, in advance, Jerome Lauret,
and Spiros Margetis for organizing the necessary effort for this review, as
well as all the members of the STAR software and SVT analysis teams who
have been working steadily behind the scenes for close to a year now to
produce the necessary understanding to inform this important
discussion.
Sincerely,
Tim Hallman
Charge to the SVT Review Panel:
The charge to the committee is to comment on how a plan
which optimizes the scientific output of the STAR Collaboration
in the next 3-5 years influences the issue of whether and
when the STAR Silicon Vertex Tracker should be removed.
The core physics goals of the STAR Collaboration in the
next 3-5 years include:
1) measurements which confirm the existence of and
characterize the quark-gluon plasma
2) measurements which illuminate the spin dependence
of the parton distribution functions within the
proton; measurements which delineate the contribution
of orbital motion to the proton spin
3) measurements which illuminate the initial state wave
function of entrance channel relativistic heavy ion
collisions; measurements which explore the QCD processes
which underly diffractive scattering in high energy
hadron-hadron interactions.
To achieve these goals, a strategy which optimizes the science
within the constraints of running time, machine performance,
detector configuration and performance, and manpower/resources
(hardware and software) is essential. This strategy should
take into account the timeliness and urgency of planned measurements.
Taking into account the physics goals of STAR as well as the expected
operating envelopes for STAR and RHIC, the committee is charged with
recommending a strategy for the future utilization and eventual removal
of the STAR Silicon Vertex Tracker. In developing its recommendation,
the review panel should take into account known constraints, including,
but not limited to, factors that relate specifically to possible changes
in detector configuration and continued operation of the STAR Silicon
Vertex Tracker and Silicon Strip Detector.
Factors specific to the SVT and SSD which impact this consideration are:
1) the ultimate precision/performance the SVT can be expect to
achieve a) standalone and b) in conjunction with the SSD
2) what compelling physics may be afforded by an optimized
SVT+SSD tracking system? What beams are required for these
measurements and how soon can they be completed?
3) what compelling physic measurements are compromised and/or
delayed if the SVT or SVT + SSD support structure remain in place
(e.g. direct photons, semi-leptonic decays of open charm, charmonium).
What is the impact on the STAR scientific program and what
if anything can be done to moderate it (e.g. Can spin physics
compromised by the SVT at 200 GeV in the near term be
accomplished with the SVT in place at 500 GeV?)
4) what level of software/hardware maintainability for the SVT and
SSD is required to achieve No. 2. Is this realistic?
5) What impact does experience with the SVT + SSD microvertexing
effort have on the future STAR tracking upgrades? What is the
interface between the SVT and the future tracking upgrade
detectors and what conflicts with the needs of the tracking upgrade
detectors does it pose?
To inform the panel, in addition to SVT/SSD specific presentations
the review will contain reports on:
a) specific measurements key to STAR's science goals; their feasibility,
timing, and factors which may compromise them or their timeliness
b) Issues related to STAR detector hardware/maintenance/operations
c) Issues related to STAR software and computing
