Title: Beam Delivery System / Machine Detector Interface
1Beam Delivery System / Machine Detector Interface
- BDS Area leaders
- Deepa Angal-Kalinin, Andrei Seryi, Hitoshi
Yamamoto - ILC MAC meeting, January 10-12, 2007
2BDS design optimization and evolutionVancouver
gt MAC(Sep06) gt Valencia gt MAC(Jan07)
- Configuration changes (CCRs) after Vancouver
- Baseline configuration to 14/14, single collider
hall - 5m muon walls instead of 918m CCR approved
23rd Sep - On surface detector assembly CCR approved 2nd
Nov - Evaluations by WWS, MDI panels CCB
- MAC (Sep 06)
- Further cost optimizations studies
- Shorter BDS and shorter extraction lines
- Several optics versions proposed, extraction
lines shortened - Single IR evaluation of push-pull
- Task force charged to report at Valencia
- CCR submitted 19th Nov, on 23rd Dec CCB issued
recommendation for the EC to approve the CCR. The
EC approved it last Thursday
3Vancouver baseline to Valencia baseline
Vancouver baseline
Diagnostics BSY tune-up dump
2mr IR
b-collim.
E-collim.
20mr IR
Two collider halls separated longitudinally by
138m
FF
Valencia baseline
14mr IR
14mr IR
One collider hall
4 Valencia 14/14 baseline. Conceptual CFS layout
muon wall tunnel widening
polarimeter laser borehole
9m shaft for BDS access
IP2
10m
IP1
beam dump service hall
alcoves
1km
5CFS designs for two IRs
Vancouver
Valencia
6Beam Delivery System tunnels
9m shaft for BDS access service hall
muon wall tunnel widening
alcoves
beam dump service hall
beam dump and its shield
7Muon walls
- Purpose
- Personnel Protection Limit dose rates in one IR
when beam sent to other IR or to the tune-up beam
dump - Physics Reduce the muon background in the
detectors
Scheme of a muon wall installed in a tunnel
widening which provides passage around the wall
Baseline configuration 18m and 9m walls in each
beamline
85m muon walls instead of 918m
- Reduction of 18m muon spoilers to 5m and
elimination of 9m muon spoilers CCR submitted
8th September - Considered that
- The estimation of 0.1 beam halo population is
conservative and such high amount is not
supported by any simulations - The minimum muon wall required for personnel
protection is 5m - Detector can tolerate higher muon flux
- Cost of long muon spoilers is substantial,
dominated by material cost and thus approximately
proportional to the muon wall length - The caverns will be built for full length walls,
allowing upgrade if higher muons flux would be
measured - MDI panel accepted this change
- CCB approved this request on 23rd September
contingent upon continuation of detailed detector
studies to ensure that the occupancy due to muons
does not affect the high precision physics
measurements
9On-surface assembly CMS approach
- CMS assembly approach
- Assembled on the surface in parallel with
underground work - Allows pre-commissioning before lowering
- Lowering using dedicated heavy lifting equipment
- Potential for big time saving
- Reduces size of required underground hall
10On-surface detector assembly CCR
- According to tentative CFS schedule worked out
by M. Gastal, CERN, the detector hall is ready
for detector assembly after 4y11m after project
start - If so, cannot fit into the goal of 7years until
first beam and 8years until physics run - Surface assembly allows to save 2-2.5 years and
allows to fit into this goal - The collider hall size may be smaller (40-50)
in this case - A building on surface is needed, but savings may
be still substantial - Discussing possible variations
- pure CMS assembly (config B)
- modified CMS assembly (config A)
- Assemble smaller (than CMS) pieces on surface,
lower down and perform final assembly underground - May affect schedule (?), but preliminary looks by
a small bit less expensive than B - The change request not intended to specify all
the details for the schedule, hall sizes,
capacity of cranes etc. - Such optimisation is being done in details by
BDS, CFS and Detector concept groups. - CCB approved this CCR on 2nd November.
11 CERN LHC-ILC engineering forum Participation by
MDI members (Oct. 12,13)
- Tour of ATLAS, CMS and ALICE
- Presentations on
- Radiation protection issues
- CMS services
- ATLAS installation
- CMS installation infrastructure
- ILC MDI present status and understanding H.
Yamamoto and A. Seryi - Assembly and installation of an ILC detector N.
Meyners - Extremely useful information from CERN colleagues
based on real experience.
12Optimizing the design and tweaking it to
understand its position w.r.to the optimum
- Since Vancouver, incorporated other cost saving
changes - redesigned tail folding octupoles, final doublet,
refined vacuum requirements, redesigned CFS
tunnels, changed design of water and air cooling
systems, decimated bends, removed any spares and
overheads, scrutinized all tech area for cost
savings, etc. - Other design optimization studies that were
performed, but were not included, as not giving
performance improvement and/or cost savings - studied shorter BDS or its subsystems
- studied lowering power of tune-up dumps
- studied replacing magnetized muon walls with
magnetized muon doughnuts
13Single IR questions
- GDE suggested evaluation of push-pull at the end
of September. - Questions to be evaluated
- Organizational and historical questions
- Accelerator design questions
- Detector design questions
- Engineering integration questions
- Detailed list of questions to be studied
developed - Technical evaluation of push-pull option by an
extended task force, which include more than 60
detector and accelerator experts from ILC
community and beyond. Detailed summary presented
at Valencia. - Conclusions from task force should be feasible,
provided careful design and sufficient RD
resources - Conclusions from detector concept groups do not
see show stoppers, detailed engineering design
studies are needed to give confidence, in
meantime would like to see two IR option kept as
an alternative - WWS comments H. Yamamoto (next talk)
http//www-project.slac.stanford.edu/ilc/acceldev/
beamdelivery/rdr/docs/push-pull/
14Single IR BDS (version 2006e)
e-
e
- Upgrade to 1 TeV CM involves adding magnets only
no geometry changes - Total BDS Z-length is 4452 m (2 IRs5100m)
- Removed dedicated energy error dianostics (MPS)
and replaced with polarimeter chicane (some
issues)
hybrid BSY (x 2)
14 mrad ILC FF9 hybrid (x 2)
IR 14 mrad
?Z -650 m w.r.t. ILC2006c
2226 m
14 mrad (L 5.5 m) dump lines
M. Woodley et al
15BDS with single IR
BSY
Sacrificial collimators
b-collim.
E-collimator
Diagnostics
FF
14mr IR
Tune-up dump
Extraction
16betatron collimation
septa
skew correction / emittance diagnostic
MPS coll
polarimeter
fast kickers
fast sweepers
tuneup dump
beta match
final transformer
polarimeter
energy collimation
IP
primary dump
energy spectrometer
fast sweepers
final doublet
energy spectrometer
17500GeV gt 1TeV CM upgrade in BSY of 2006e
Magnets and kickers are added in energy upgrade
M. Woodley et al
18Single IR BDS optics (2006e)
BSY
FF
Polarimeter
E-spectrometer
E-collimator
b-collim.
Diagnostics
19Concept of single IR Final Doublet
vacuum connection feedback kicker
common stationary cryostat
Detector
QD0
QF1
warm
IP
Original FD and redesigned for push-pull (BNL)
Redesigned FD
20IR magnets
BNL prototype of sextupole-octupole magnet
BNL prototype of self shielded quad
cancellation of the external field with a shield
coil has been successfully demonstrated at BNL
21New optics for extraction FD push pull
compatible
- Rearranged extraction quads are shown. Optics
performance is very similar. - Both the incoming FD and extraction quads are
optimized for 500GeV CM. - In 1TeV upgrade would replace (as was always
planned) the entire FD with in- and outgoing
magnets. In this upgrade, the location of
break-point may slightly move out. (The
considered hall width is sufficient to
accommodate this).
Nominal scheme
Push-pull scheme
B.Parker, Y.Nosochkov et al.
http//ilcagenda.cern.ch/conferenceDisplay.py?conf
Id1187
22Extraction Lines shortened by 100m
For undisrupted beam reliance on beam sweeping on
beam dump window using kickers.
high L parameters (500 GeV CM)
Total loss before and at collimators for High L
parameters is within acceptable levels. Losses
for the nominal case are negligible.
23Concept of single IR with two detectors
The concept is evolving and details being worked
out
may be accessible during run
detector A
accessible during run
Platform for electronic and services (1088m).
Shielded (0.5m of concrete) from five sides.
Moves with detector. Also provide vibration
isolation.
24Detector systems connections
25Push-pull cryo configuration
Optimized for fast switch of detectors in
push-pull and fast opening on beamline
QD0 part
QF1 part
This scheme require lengthening L to 4.5m and
increase of the inner FD drift Opening of
detectors on the beamline (for quick fixes) may
need to be limited to a smaller opening than what
could be done in off-beamline position
door
central part
26Shielding the IR hall
Self-shielding of GLD
Shielding the 4th with walls
27Working progress on IR design
Mobile Shield Wall
Illustration of ongoing work Designs are
tentative evolving
Structural Rib
3m Thickness
Overlapping Rib
Mobile Platform 20m x 30m
Electronics/Cryo Shack 1m Shielded
9m Base
25m Height
John Amann
28CFS layout for single IR central DR
29CFS layout for single IR
30Single IR push pull schedule
- The hardware can be designed to be compatible
with a one day move, and this can be a design
goal - Need to study cost and reliability versus the
move duration - Need to study regulations in each regions
- A.Yamamoto presented a scheme (which includes
warming-up the cold-box and disconnecting room T
lines) and give an estimation of one week (many
other tasks can be done in parallel with cryo
work), which can serve as conservative boundary
of the range - Recalibration (at Z) may or may not be needed,
and may be independent on push-pull to be
studied - BDS group will study the range between one day
and one week and optimize the design versus cost,
performance, reliability, etc.
31Single IR, push-pull cost
- Cost difference of two IR versus single IR
push-pull as reported to CCB on Dec.15 (based on
Valencia wbs) - baseline 14/14 100
- estimate for single p-p IR 69.1, with further
updates 67.6 - Estimation of saving, in Value cost, is 31-32 of
BDS cost - Using single push-pull IR saves about one third
of two IR BDS cost, or in other words the two IR
BDS is by about 50 more expensive than single
push-pull IR BDS - Estimation of additional hardware that is needed
to make push-pull feasible is small fraction of
the savings
32From summary of CCB response on Single IR
push-pull
- CCB agrees that .. CCR qualifies as Class-2.
Consequently, CCB assumes that its role is to
make recommendation to EC rather than to make a
decision. - CCB recommends EC to accept CCR23, whereby
incorporating the "1IR with two detectors
push-pull" as Baseline Configuration. - CCB recommends EC to maintain the previous
Baseline with "2IR, single hall, two detectors"
as part of Alternative Configuration. - CCB recommends EC to reinforce a taskforce on
Machine-Detector-Interface issues. The taskforce
should be specifically charged to facilitate
pertinent design development efforts and
discussions on relevant executive matters.
33Briefly on other systems
- Magnets and PS
- Vacuum system
- Crab cavities
- Beam dumps collimators
- IR hall, surface buildings cranes
34Magnets and PS
- Most of the magnets are rather standard, but
require good magnetic and mechanical stability - All PS are high availability design, stability in
several ppm range (building 40 PS for ATF2 now) - PS are placed in the service tunnel, cable
penetrations are every 100m, which reduces heat
load in the tunnel helping thermal and mechanical
stability - All BDS magnets in incoming beamlines except
bends are on movers with 50nm step - Special magnets except FD and first extraction
quads - SC tail folding octupoles (BNL design)
- beam sweepers
- Kickers with option of DC bends
- Antisolenoids embedded in the detector
- Detector integrated dipoles (part of detector
solenoid) - Magnetized muon walls
35Vacuum system
- Material choice
- is defined by the resistive wall effects for
off-centered bunch preserving the beam emittance
discourage use of SS chambers - Considered Al version and Cu plated SS chambers.
Chosen the latter as more reliable, keeping Al
for backup option. Chambers in the places where
SR is expected (e.g. chicanes) are Cu - Vacuum pressure
- determined by the need to minimize background due
to beam-gas. - Need 1nTorr in 200m upstream of IP (may need in
situ baking), 10nTorr in 200-800m and 50nTorr
in the rest of the system
36Crab cavities
- BDS has two SC 9-cell cavities located 13 m
upstream of the IP operated at 5MV/m peak
deflection. - Based on a Fermilab design for a 3.9GHz TM110
mode 13-cell cavity. - The uncorrelated phase jitter between the
positron and electron crab cavities must be
controlled to 61 fsec to maintain optimized
collisions. - A proof-of-principle test of a 7 cell 1.5GHz
cavity at the JLab ERL facility has achieved a 37
fsec level of control. - Other key issues to be addressed are LLRF
control and higher-order mode damping.
- Top earlier prototype of 3.9GHz deflecting
(crab) cavity designed and build by Fermilab.
This cavity did not have all the needed high and
low order mode couplers. - Bottom Cavity modeled in Omega3P, to optimize
design of the LOM, HOM and input couplers.FNAL
T. Khabibouline et al., SLAC K.Ko et al. - Design is being continued by UK-US team
3.9GHz cavity achieved 7.5 MV/m
3718MW Water Dump design features
- BDS features
- Optics drift to increase undisrupted beam spot
size on window - Raster beam in 30mm radius circle in 1 ms
interlock to MPS - Hi-power donut collimators to protect vessel
window - Vessel
- 6.5m (18X0) water followed by 1m water-cooled Cu
(22X0) - 1.5m diameter with vortex flow water, v1.0-1.5
m/s , at r30cm - 10 atm to prevent boiling
- 30 cm diameter 1mm Ti vessel window with water
cooling nozzles - Rad water system
- 2300 gpm three loop water system
- 18 MW heat exchanger 400HP of pumps per loop
- Catalytic H2-O2 recombiner
- Mixed bed ion exchange column to filter 7Be
- Containment for tritiated water
- Shielding
- 50cm Fe 150cm concrete local protection for
personnel beamlines - 200cm site dependent to protect ground water
3818MW Dump design
- Two companies Fichtner Framatome, design and
cost estimate for TESLA TDR - Fichtner design for TESLA reworked by RAL
- Taken into account recent RAL experience with
industry - RAL design included additions for window remote
handling, air exchange and control, air drying
and recovery, etc.
39IR surface area
40Included in IR hall and surface buildings
- IR halls
- finished civil engineering works, plus
- movable concrete intermediate shielding wall in
two parts (on air pads) - steel platforms with staircases and all fittings
- two 1.6t elevators between steel platforms plus
two 2.8t in shafts, - steel plates on the floor of the Hall
- one 400t and two 20t overhead cranes in Hall
- etc
- Included in surface assembly building
- 400t and 20t overhead cranes
- Requirements for detector assembly are different
(table on the next slide). Since we cannot tell
now which detectors will be used, assumed
Configuration A - This choice can suite some detectors better than
other (one size does not fit all) and is the
reason for concerns - Further adjustments of IR hall and surface
building are needed, and detector colleagues
should be more deeply involved in this design and
also cost optimization
41Table of IR assumptions
continued
42Summary
- Several configuration changes since Vancouver to
Valencia and final RDR version. - Single IR with two complementary detectors in
push-pull configuration has been recommended by
CCB to EC as a baseline for the RDR. The EC
approved it last Thursday - This configuration gives 30 saving compared to
two IR 14/14 mrad configuration. - Single IR BDS optics design allows upgrade to 1
TeV in the same tunnel. - The on surface detector assembly will save 2-2.5
years and has been accepted by the MDI panel. - The engineering details will be carried out in
the EDR phase.
43Backup slides
44500 GeV cm
1 TeV cm
45 continued
46Power cooling in BDS
Table as of Valencia, 1TeV CM, two IR.
Table is as of 11/26/2006
9.768 0.862 218 MW gt Power from Magnets, PS
Dumps to LCW 0.726 MW gt Cables to Airgt
approximately 60W/m in average 0.712 MW gt PS to
Air gt taken out by Chilled water
47Cost breakdown for single IR
(Labor person-hours, such as installation, was
converted to dollars to produce this chart)
48Beam Dump Vessel
49Beam Dump Service Cavern Layout
50If detector does not provide any radiation
protection
18MW loss on Cu target 9r.l \at s-8m. No
Pacman, no detector. Concrete wall at 10m. Dose
rate in mrem/hr.
- For 36MW maximum credible incident, the concrete
wall at 10m from beamline should be 3.1m
Wall
25 rem/hr
10m
Alberto Fasso et al
51IR hall radiation safety criteria
- BDS produces and uses ILC radiation guidance
document - beam containment policies and devices, conditions
for occupancy - For IR region, in particular, defines
- Normal operation dose less than 0.05 mrem/hr
(integrated less than 0.1 rem in a year with 2000
hr/year) - allows non-rad workers in IR hall
- Accidents dose less than 25rem/hr and
integrated less than 0.1 rem for 36MW of maximum
credible incident (MCI)
52Detector sizes opening on beamline
SiD (opened)
GLD
Since opening of detectors on the beamline is
intended only for quick fixes, the required width
for opening may be smaller that for opening
off-beamline
53FD with L4.5m lengthened warm drift section
by 0.7m
Detector opened on beamline (GLD opening reduced
to 1.5m) still leaves 0.5m of not-overlapped
space for config.C
54Instrumentation
- Laser wire
- Deflecting cavity Y-T
- Loss monitors ion chamber PMT
- Cav BPM C-band, S-band, L-band
- Stripline or button bpm
- X sync light tr. profile imager
- OTR, OTRI
- Current monitors
- Pickup phase monitors
- Feedbacks
- Polarimeter laser upstream downstream
- E-spectrometer
55IR coupling compensation
When detector solenoid overlaps QD0, coupling
between y x and y E causes large (30 190
times) increase of IP size (greendetector
solenoid OFF, redON)
without compensation sy/ sy(0)32
Even though traditional use of skew quads could
reduce the effect, the local compensation of the
fringe field (with a little skew tuning) is the
most efficient way to ensure correction over wide
range of beam energies
antisolenoid
QD0
SD0
with compensation by antisolenoidsy/ sy(0)lt1.01