Title: Physics Division Plans
1Physics Division Plans
- Engineering Division - Mechanical
- Retreat
- June 26, 2001
2Overview
- Attempt to cover this decade
- ATLAS
- BaBar
- SNAP
- Linear Collider
- Other
- Caveats
- Not a complete look at all Phys. Div. Activities
- Uncertainties grow with time
- Talk reflects my opinions
3ATLAS(1)
- Now - 2006
- Lead role in mechanical structure for ATLAS pixel
project - Deliverables requiring composite structures and
close electrical/mechanical integration built at
LBNL or under contract to LBNL. - Fabrication in Bldg. 77s, including(I hope) final
assembly/test in new clean room in 77. - CERN final assembly and installation
- ATLAS pixel upgrades(after initial running)
- Pixel system will be upgraded.
- Lower mass in structures/services is one of the
goals. This requires development, starting(if
possible) even before first collisions(eg in 2004
onwards) and should continue as long as there are
good ideas. - Production could even start before first
collisions in 2006 if ideas are compelling. Need
to be ready by 2008/2009. - LBNL can be leader in this area(if we dont get
worn out building first detector).
4ATLAS(2)
- Major ATLAS upgrades
- LHC luminosity upgrade in long-range plan.
- LHC luminosity above 1034 requires both new ideas
and replacement of entire ATLAS tracking system. - Very likely this would mean expansion of pixel
system to larger radii - bigger system - and new
and larger silicon strip system. - This would be very large effort(some hundreds of
M) - Timescale obviously depends on LHC operation,
physicsbut installation by 2014 is a reasonable
guess. Would require about 5 year
development/production time, preceded by
RD(above 1034 is hard).
5ATLAS Pixel Detector
6(No Transcript)
7ATLAS -gt ME
- Design and FE modeling of composite structures
- Fabrication of composite structures
- Design validation for ultra-stable structures.
Acquisition of TV holography system a significant
step in improving LBNL capability. Should expand
on this area(environmental chamber, coincident IR
thermography, improved computing power,) - Optical and touch CMM will continue to be needed.
- Electrical/mechanical integration. This should
mean joint modeling of electrical and mechanical
properties(not currently done in any systematic
way). This also includes the subject of cable
design and modeling, custom design and sometimes
fabrication of low mass cables. - Clean room space and fabrication equipment(wire
bonders, plasma cleaning, glue robots, .) - Innovations in stable, low mass structures and
power, signal and cooling integration will be key
to future involvement.
8BaBar(1)
- Middle 2002
- Remove the SVT so PEPII can have access to the
beam pipe for modifications. Only moderate rework
of the SVT. - Need from engineering mechanical technician and
electrical coordinator help. - Electrical coordinator a few man months from now
to June 2002. Full time for one man month June
2002. - Mechanical technician 20 now to Jan 2002. Full
time Jan to Aug. 2002. - Middle 2004
- Remove the SVT bring to LBNL for refurbishing.
Manpower similar to above with the addition of
two full time mechanical technicians for three
months during the rework at LBNL - In addition need to share the clean room in
77(assuming it exists). - (Note may not have Fred Goozen at this time as he
may retire.)
9BaBar(2)
- 2005
- BaBar and PEPII upgrade path not entirely clear
but increased luminosity will be key gt replace
SVT(radiation damage) - LBNL would be natural location for design,
fabrication, integration as before - lead role - Need both design and technical support. Composite
structures, electrical/mechanical integration,.. - Even later - new machine(1036)?
- Silicon based detectors - larger scale, new
techniques. - Starts to look like hadron collider, but low mass
structure even more important.
10BaBar -gt ME
- Immediate(and critical) need over next few years
is for technical support familiar with silicon
systems or to become rapidly familiar with
silicon systems. - If warranted by physics need, by mid-decade,
LBNL would be natural site to lead replacement of
SVT. This would require design, fabrication
facilities, technical support.at least similar,
probably larger, scale to existing SVT.
11SNAP(1)
- SNAP and related instrumentation
- CCD instrumentation, packaging and use
- SNAP project development
- Active projects
- Package development for backside illumination
- Molybdenum fabrication
- Alignment mechanism
- Glue/epoxy research
- Glue/epoxy application techniques
- SNAP-specific implementation of LBNL chicken
feeder dewar - Package existing devices to deliver to NOAO,
SNIFS, ESI, . - 3D conceptual modeling
12SNAP(2)
- Near term projects
- Mechanical/thermal model of assemblies
- Measure material properties to feed model
- Performance measurements of prototypes to
validate model - Scale up the model to the full detector
- Incorporate test dewars into optical test system
- Build small focal plane containing 4 to 8 CCDs to
use in a ground-based telescope. - 3D conceptual modeling
13SNAP(3)
- Longer term
- Mass production
- CCD assembly parts
- CCD mechanical assembly
- Cryostats for mass production of CCDs
- Focal plane
- Base plate design and fabrication - no longer a
flat plate, rather, it is highly faceted. - Probable that we will have to design the shutter
mechanism. - Focal plane base plate attachment to passive
cooling radiator - Particle/thermal/light shield cone design.
- Mounting system for focal plane and shield
- Modeling of thermal/mechanical performance
- Integration and testing
- Test chamber (150 K)
- Mechanical survey of CCDs.
- Operational testing of entire CCD array.
- NB, integration of instruments with spacecraft is
scheduled for mid-07
143D conceptual modeling
15GigaCam Assembly
Particle/thermal/light shield
CCDs
Support plate
Heat Radiator
Base plates
16Mosaic Packaging
Plug and play Precision CCD modules, precision
baseplate, and adequate clearances designed
in. Focal plane tolerance is ?25 ?m. Final
assembly can be xyz surveyed cold.
Recent development, focal plane will now be
curved requiring a faceted base plate.
Cable
150 K plate attached to space radiator.
17CCD Packaging
Prototypes are being assembled with dummy silicon
that includes all steps including wire
bonding. Want to deliver functional packages to
telescopes by the end of summer.
- Support CCD
- Connection to cold plate
- Four-side abuttabe for dense mosaic.
- Built-in mechanical precision no shimming.
- Access to bonding pads
- Local electronics
- Cable connector
- Low mechanical stress in silicon from -150 C to
150 C. - Low background radiation materials
- Low chemical reactivity with silicon
18Cosmology/SNAP -gt ME
19Linear Collider
- Linear Collider will likely be next focus of
world-wide, accelerator-based HEP, following LHC. - Location not known. Timescale for completion
uncertain. - LBNL detector development
- TPC improvements and related studies
- CCD vertex detector
- TPC
- Readout/gas studies
- Reduce structural mass(composites?)
- Integration of electronics(eg. in 0.25 micron
processes) on endplanes -gt electrical/mechanical
issues, including reduced mass - CCD
- Utilize SNAP rad-hard CCD technology
- Vertex detector similar to one built for SLD
20Other
- Cosmic Microwave Background instrumentation
- Effort to utilize large-scale HEP techniques
for CMD instruments - Cryogenic systems, superconducting detectors
- Underground laboratory
- Effort to push for US underground laboratory for
dark matter searches, next generation solar
neutrino experiments, detector for neutrino
oscillation experiments from accelerator beams - Cryogenic detectors, big detectors(large mass
needed), low background - Neutrino beams/muon storage ring
- Big neutrino detectors. Need innovations
- Astrophysical neutrinos
- ICECUBE.
21Implications
- Diverse effort, hard to give common theme
- ATLAS, BaBar, SNAP, LC possible commonalities
- Clean space.
- Silicon fabrication equipment
- FE structural/thermal modeling, verification via
TVH, CMMs, IR - Composite structures
- Combined electrical/mechanical design,modeling
- Other potential experiments have additional needs