The SLHC
description
Transcript of The SLHC
14/09/2007
The SLHCThe SLHC
Cartigny, le 14 Septembre 2007 SLHC, Didier 1
Centre de rencontre de CartignyD. Ferrère, 14 septembre 2007
Team: G. Barbier, A. Clark, D. Ferrère, D. Lamarra, S. Pernecke, E. Perrin, M. Pohl
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“The LHC will be the energy frontier machine for the foreseeable future, maintaining European leadership in the field; the highest priority is to fully exploit the physics potential of the LHC, resources for completion of the initial program have to be secured such that machine and experiments can operate optimally at their design performance. A subsequent major luminosity upgrade (SLHC),
motivated by physics results and operation experience, will be enabled by focused R&D; to this end, R&D for machine and detectors has to be vigorously pursued now and centrally organized towards a luminosity upgrade by around
2015.”
Draft Strategy Document Initiatives:
http://council-strategygroup.web.cern.ch/council-strategygroup/
The European Strategy for Particle PhysicsThe European Strategy for Particle Physics
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SLHC status:• R&D towards a realistic Upgrade scenario is active (Machine and Detectors) • SLHC is not approved yet!• Exact time schedule is unknown• Machine scenarios exist but not frozen
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The ATLAS ID current status at LHCThe ATLAS ID current status at LHC
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All services (pipes, cables, fibers,..) Installed
TRT barrel & Endcap cabled and connected - 1.8% problematic channels out of 105K, noise figure as on surface – Cosmics collected in M4 runs
SCT barrel and Endcap signed off on surface - < 0.3% problematic channels out of 6.3 M, >99% efficiency on cosmics. Commissioning in Progress, ongoing delays due to cooling and environmental gas.
Pixel signed off on surface and installed and waiting for connection and tests
… towards the end …December 07: End of the ATLAS InstallationJan-Feb 08: Overall ATLAS commissioningMarch/April 08: Close Access
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Machine and ScenariosMachine and Scenarios
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3 phases considered:
Phase 0: Push the machine to its maximum performance without hardware changeLuminosity of 2.3x1034 cm-2s-1. and ultimate energy 7.54 TeV (dipole field @ 9T)
Phase 1 (SLHC): Interaction Region (IR) quadrupoles life expectancy < 10 years Modify the insertion quadrupoles and their layout *
Phase 2: Rebuild the SPS with superconducting magnets, the transfer line to inject into LHC at 1 TeV and new 15T dipoles proton energy of 12.5 TeV
ParametersLHC SLHC - Phase1
Nominal Ultimate Scenario 1 Scenario 2
Bunch spacing [ns] 25 25 50 25
Proton/bunch Nb[1011] 1.15 1.7 4.9 1.7
* at IP1&5 [m] 0.55 0.5 0.25 0.08
Longitudinal profile Gaussian Gaussian Flat Gaussian
Rms bunch length z[cm] 7.55 7.55 11.8 7.55
Peak luminosity [1034 cm-2s-1] 1 2.3 10.7 15.5
Effective luminosity (5h) [1034 cm-2s-1] 0.56 1.15 3.5 3.6
Peak events per crossing 19 44 403 294
CommentsWire comp. Crab + D0
(+ Q0)
NB: Original scenario of 12.5 ns excluded since exceed the max local cooling capacity
Ba
se
lin
e
Alt
ern
ati
ve
Far future
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Physics BenchmarksPhysics Benchmarks
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The future observations at LHC should drive physics investigations at SLHCThe future observations at LHC should drive physics investigations at SLHC •Higgs:
- H couplings to bosons and fermions- WW scattering and resonances
• SUSY spectroscopy:- mass reconstruction, sparticle ID, BR measurements, …- performances for heavy SUSY (> 2 TeV) – impact and statistics
• EW physics:- Boson self-couplings: focus on those for which the sensitivity is close to ILC
• Super-heavy stuff:- Multi-TeV region: light Higgs decay to new gauge bosons Z’, W’
Ideally it is desired to increase the luminosity and get a better
detector performance
Luminosity should be 10 times higher & Upgrade is considered for the detectors
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ATLAS UpgradeATLAS Upgrade
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Due to increase of radiation level, pile-up, background Due to increase of radiation level, pile-up, background each sub-detectors has to think of the consequences in each sub-detectors has to think of the consequences in term of detector performance, aging, radiation hardness!term of detector performance, aging, radiation hardness!
Inner Detector (ID):Completely new design and detectors – No TRT, more pixel and strips: New detector and ASICs technologies to withstand the radiation level Simulations drive optimal geometry (Strawman layers) and occupancies
LAr Calorimeter:FCAL: To be replaced with smaller gap size and special cooling close to the beam pipe.HEC: Cold electronics may have to be replaced (no need to get HEC wheels apart)Others: More R&D require about the Ion buid-up
Tile Calorimeter:Front-end electronics and Low Voltage Power Supplies
Muon System:MDT: Chambers and readout electronics are radhard at LHC or can stand 10 times the max nominal flux but further studies need to be performed in SLHC environment
2008: detail upgrade plan based on some tests and R&DTGC: Thick GEMs can possibly replace forward chambers due to high occupancy.
Focus
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Radiation Background in ATLAS at SLHCRadiation Background in ATLAS at SLHC
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1 MeV equivalent neutron fluences assuming an integrated luminosity of 3000fb-1 and 5cm of moderator lining the calorimeters (reduces fluences by ~25%)
•With safety factor of two, design short microstrip layers to withstand 1015neq/cm2 (50% neutrons)
•Outer layers up to 4×1014neq/cm2 (and mostly neutrons)
Thermal management and shot noise. Silicon looks to need to be at ~ -25oC (Thermal runaway).Si power: 1W @ -20°C
4W @ -10°C10W @ 0°C
High levels of activation will require careful consideration for access and maintenance.
IssuesIssues
Simulation using FLUKA2006
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Inner Detector Upgrade - LayoutInner Detector Upgrade - Layout
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The goal for b-layer replacement is fall 2012Actual b-layer is expected to survive 3 years at LHC design luminosity
(~300fb-1)The Upgrade of the entire tracker should take place in 2016
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Silicon SensorsSilicon Sensors
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Choice of adequate material thanks to RD50 collaboration
Pixel and Strips: n-in-p (planar technology)
No type inversion, full depletion is on structured side
Collection of electrons (faster than p-in-n)
0 20 40 60 80 100 120eq [1014 cm-2]
0
5000
10000
15000
20000
25000
sign
al [e
lect
rons
]
3D FZ Si, 235 m, (laser injection, scaled!), pad [Da Via 2006]n-FZ Si, 280 m, (-10oC, 40ns), n-in-n pixel [Rohe et al. 2005]p-FZ Si, 280 m, (-30oC, 25ns), strip [Casse 2004]p-MCZ Si, 300 m, (-30oC, s), pad [Bruzzi 2006]n-epi Si, 150 m, (-30oC, 25ns), pad [Kramberger 2006]n-epi Si, 75 m, (-30oC, 25ns), pad [Kramberger 2006]sCVD-Diamond, 770m, (RT, s), [RD42 2006] (preliminary data, scaled)pCVD-Diamond, 500m, (RT, s), strip, [RD42 2002-2006] (scaled)SiC, n-type, 55 m, (RT, 2.5s), pad [Moscatelli et al. 2006]
M.Moll 2007
Pixel b-layer: 3D technology is an option(should be ready for b-layer replacement in 20012)
electrons swept away by transversal field holes drift in
central region and diffuse towards p+
contact
Exist in single and double column type
n+-columns
ionizing particle
p-Si
3D FZ 235m
P-FZ 280m
Still ~15000e- at 1.1015 cm-2s-1 (FZ or MCZ)
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Electronics for StripsElectronics for Strips
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ABC-N Readout architecture
Minimum requirements:
Implementation of an on-chip shunt regulation to allow any powering scheme (Serial or DC-DC)
Increased data bandwidth of 160 Mb/s
Compatibility with existing ATLAS SCT DAQ ROD hardware
Front-end for two signal polarities, 3 to 12 cm long silicon strips
Minimum power circuit techniques
Delay adjustment for control and data signals
Similar “core” functionality as for the present silicon strip tracker: signal amplification, discriminator, binary data storage for L1 latency, readout buffer with compression logic, and data serializer.
Goal: Prepare a design of the FE ASIC in deep submicron radiation tolerant.Design and evaluation with 250 nm towards 130 nm technology
• Daniel La Marra, Sebastien Pernecker, Geneva University• Wladek Dabrowski, Krzysztof Swientek, AGH-Cracow• Jan Kaplon, Karolina Poltorak, Francis Anghinolfi, CERN• Mitch Newcomer, Pennsylvania University
Design team:
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Module IntegrationModule Integration
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Focus on the most challenging modules with Short-Strips, 80 chips (24W), 4 hybrids, 160MHz clocking to FE chips, and readout by group of 10 modules.
3 flavors are considered: Staves, Super-Modules, Modules
Service bus
TTC, Data & DCS fibers
PS cable
DCS env. IN
Cooling
Opto
BGT
DCSinterlock
SMC
Module #1 Module #2 Module #10
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Power DistributionPower Distribution
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Services are clearly an issue for the material budget as well as for the system design
Tracker Upgrade should leave with the existing ID services and optimize the power distribution: Serial Powering or DC-DC (Individual Powering is abandoned)
SCT - 4mW/ch 24 kW (excl. cable losses)Strip Upgrade - 2mW/ch 90 kW only for FE (45 Mch)
1 2 3 4 5 6 n-1 n
SPIPS=IH=4.2AVPS=nVABCN=24V
PPg= GAINDC-DC=20IPS=n/g.IH=2AVPS=gVABCN=24 V
Short-Strip Super-Module configuration
n is hybrid number = 20; VH (0.13m)=1.2V
NB: Here only 2 cables/SM needed but for IP it would be 40 cables
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CoolingCooling
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Cooling System is one of the key points for ID operationHeat density is 4-7 times higher than the current SCT module
Detector thermal runaway impose to operate the silicon wafer below -20ºCTsensor = Tcoolant + THeat_Path
Coolant: Less than -30 C is considered for the pipe temperature Module design and choice of material is critical – Thermal FEA
3 candidates for the cooling:• CO2 (~100 bar)• C2F6 (Low pressure)• C3F8 (Low pressure)
1g of evaporation @ -30ºC ~280 J(Where for C3F8 it is 100 J/g)
CO2Enthalpy [kJ/kg]
Pre
ss
ure
[b
ar]
Existing pipes are considered:-SCT & Pixel (ok for C2F6, C3F8)-TRT (ok for CO2 but limited number)
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Status in the various working groupsStatus in the various working groups
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Pixel:3D sensors:
-ATLAS geometry evaluated: Laser and capacitance measurements- proton and neutron irradiations will soon come- H8 TB will be in September/October 2007
Readout chips: Prototyping activity in 0.13 m technology – chip FE 14 Powering: Promising results for SP – Using current ATLAS Pixel modules
Strips:Sensors: 10X10 cm2 short strip sensors ordered (15 units for UniGe) Readout chips ABC-n: Specification document created and under design. The submission is foreseen at the beginning of 2008Powering: Promising results for SP – Using current ATLAS SCT modules on
staves and with individual modules. DC-DC is also investigated!Module Integration:
- Concept proposed and some Thermal FEA showed- Prototypes with ABC-n and new n-in-p sensors in 2008- TB and irradiation will follow
Structure and Services: On going discussions and specifications expected soon
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UniGe InvolvementsUniGe Involvements
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Asics: Digital Architecture & Simulation: pipeline, Derandomizer, Data Compression Logic, Readout Logic and Control; Check after place and route!
250nm submission January 2008 130nm design from January 2008
Detectors: 135 sensors of size10X10cm2 ordered to HamamatsuUniGe ordered 15 sensors: 12 p-stop and 3 p-spray Sensor characterization will be made and compared with other institutes
Module Concept: UniGe investigated 2 concepts module directly mounted on barrel or mounted on an intermediate local support!
UniGe operates 3D Thermal FEA to evaluate and optimize the designStrategy is to make prototype modules in 2008 with above detectors and Asics
DCS: Involvement in the strategy and decision for the detector safety. DCS will be part of the system design to optimize the service and resource issues.
Mechanical Engineering: Involvement in the structure and service design.
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Important Milestones DraftedImportant Milestones Drafted
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1. Beam off – start decommissioning 1/7/2014 (18 month for installation) 2. Ready for beam: 1/1/2016
• Straw man Layout - December 2006 (Modification/changes to be made in
term of performance /Risk/Cost etc.)• TDR - Feb/2010• Cooling PRR April/2010 • Mechanical Support Design complete Oct/2010• Sensor PRR July/2010• FE-electronics Sept/2010• Surface Assembly March/2012
B-Layer replacement • Ready for Installation August/2014• Barrel Installation Feb/2015• B-layer/beam pipe August/2015
Conceptual Design R&D
Prototypes
Pre-Series
Production
Assembly & Installation
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ConclusionsConclusions
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SLHC is clearly in the continuity of the machine and detector operation Phase 1 will be to increase the luminosity up to a factor 10 (1035 cm-2s-1 ) ATLAS and CMS are considering options to Upgrade the detectors in 2016 The ATLAS Inner Tracker will be completely renewed (no TRT) and is in a design and specification phase The B-layer replacement is foreseen already in 2012 using 3-D sensors The major challenges are: Service and material reductions, Cooling, Powering scheme The time scale is short and there is almost no time for R&D Working groups start smoothly to grow and to be active UniGe involved in various topics and keep an eye on the B-layer replacement activities Next events:
• Pixel Upgrade Workshop 28-29 September at CERN• ID Upgrade Workshop 12-14 Dec 2007 in Valencia
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Back-up slidesBack-up slides
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Appendix - Tracker Organizational StructureAppendix - Tracker Organizational Structure
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new upgrade bunch structures
25 ns
50 ns
nominal
25 ns
ultimate& 25-ns upgrade
50-ns upgrade,no collisions @S-LHCb!
50 ns
50-ns upgradewith 25-ns collisionsin LHCb
25 ns
new alternative!
new baseline!
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25 ns scenario 50 ns scenario
Merits •Negligible long-range collisions,•No geometric luminosity loss,•No increase in beam current beyond ultimate
•No elements in detector,•No crab cavities,•Lower chromaticity,•Less demand on IR quadrupoles (NbTi possible)
Challenges •D0 dipole deep inside detector (~3 m from IP),•Q0 doublet inside detector (~13 m from IP),•Crab cavity for hadron beams (emittance growth),•4 parasitic collisions at 4-5s separation,•“Chromatic beam-beam” Q’eff~sz/(4pb*sd),•Poor beam and luminosity lifetime ~b*
•Operation with large Piwinski parameter unproven for hadron beams, •High bunch charge,•Beam production and acceleration through SPS,•“Chromatic beam-beam” Q’eff~sz/(4pb*sd),•Larger beam current,•Wire compensation (almost etablished)
Two scenarios Luminosity UpgradeTwo scenarios Luminosity Upgrade
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Heat loadPer GrafstromCERN
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B-Layer Replacement
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B-Layer Replacement & Tracker UpgradeB-Layer Replacement & Tracker Upgrade
• ATLAS considers to have a B-layer replacement after ~3 year of integrated full LHC luminosity (2012) and replace completely the Inner Tracker with a fully silicon version for SLHC (2016).
• The B-layer replacement can be seen as an intermediate step towards the full upgrade. Performance improvements for the detector (here some issues more related to FE chip):– Reduce radius and design for > 1034cm-2s-1 luminosity Improve radiation
hardness ( 3D sensor, p-type bulk materials)– Reduce pixel cell and architecture related dead time ( deign FE for
higher luminosity)– Reduce material budget of the b-layer (~3% X0 <2.5% X0) stave
replaces module as the basic building block.– increase the module live fraction ( increase chip size, > 1214 mm2),
optimize inactive chip periphery, use “active edge” technology in the sensor.– Use faster R/O links, move MCC at the end of stave– FE chip technology will use 0.13 µm 8 metal CMOS.
• The B-layer for the upgrade will push even more technological/ design/ architectural issues of the FE chip radiation hardness (1015 1016 neq/cm2) and detector occupancies ( 15)
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Half barrel
10-Module Structure
Reference (r, Z) + fixation
Barrel end
Reference (r+ alignment
Intermediate support bracket+ insertion guide
End view
LSR on BarrelLSR on Barrel(UniGe Concept)(UniGe Concept)
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SS disks
SS+LS disks
EC disks – Petal optionEC disks – Petal option
C. Lacasta
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Data Transmission
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0
2
4
6
8
10
12
-60 -40 -20 0 20 40
T [°C]
p [
ba
ra]
-35
1.1 bara
7.6 bara
C3F8
Low evaporation pressure limit
• Limit from return line impedance and compressor suction pressure.
• Mostly of concern for C3F8
– TRT pipes would give ~70% more flow → return pipe Δp would have to increase (α ~P2),
– Heaters/HEXs (diameter) need to be bigger, – Alternative pev control: cold condenser
(needs development),– Surface condensers to reduce compression
ratio → allows to reduce suction p.– Mix with C2F6:
• Allows to tailor saturation properties,• Lower HTC to wall (~50%),• Mixture control by measurement of vsound.
SCT return p budget Δp [bar]
Heaters & HEXs ~0.2
Return pipes ~0.1
Back pressure regulators ~0.5
Compressor suction p p ~ 0.7
Total p ~ 1.5
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Run conditions @ -35C
C3F8 C2F6
Pevaporation 1.1 bar 6 bar
ΔT for ΔP=+-0.1bar +2 C / -2 C
ΔT for ΔP=+-1.0bar +20 C / ~-44 C
ΔH for evaporation 100 J/g 100 J/g
Flow for 100 W 1.0 g/s 1.0 g/s
Volume flow 0.6 cm3/s 0.6 cm3/s
HTC [W/cm2/K] 3000 W/cm2/K
Major difference for CO2 with respect to C3F8 cooling is the increase by a factor of 10 of the evaporation pressure for T=-35C.
CO2
12 bar
+0.2 C / -0.2 C
+1.8 C / -1.9 C
280 J/g
0.4 g/s
0.4 cm3/s
8000 W/cm2/K
Advantages….
Coolant propertiesCoolant properties