SLHC detector upgrades

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SLHC detector upgrades Outline: LHC Machine Plans and Conditions ATLAS and CMS Detector Changes LHCb and ALICE Plans Some final comments More information: Slides/plots from R.Garoby, F.Gianotti, N.Hessey (mostly), J.Nash, F.Muheim, J.P.Revol Links to LHCC upgrade meetings: http://indico.cern.ch/categoryDisplay.py?categId=1949

description

Outline: LHC Machine Plans and Conditions ATLAS and CMS Detector Changes LHCb and ALICE Plans Some final comments More information: Slides/plots from R.Garoby, F.Gianotti, N.Hessey (mostly), J.Nash, F.Muheim, J.P.Revol - PowerPoint PPT Presentation

Transcript of SLHC detector upgrades

Page 1: SLHC detector upgrades

SLHC detector upgrades

Outline: LHC Machine Plans and Conditions ATLAS and CMS Detector Changes LHCb and ALICE Plans Some final comments

More information: Slides/plots from R.Garoby, F.Gianotti, N.Hessey (mostly), J.Nash, F.Muheim, J.P.Revol Links to LHCC upgrade meetings: http://indico.cern.ch/categoryDisplay.py?categId=1949

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SLHC perspectives

Planning based on the assumption that it is well worth increasing the integrated luminosity of LHC by a factor 4-7, running well beyond 2020 SLHC has the potential to deliver large data sets, making new

measurements accessible

It is possible that some of the energy scales for new physics can be determined already next year (Higgs, Supersymetry, etc), but it is not at all certain – so the only reasonable assumption is that we need to plan for detector performance at least as today. Also that Inner Detectors are needed with similar performances as

today

The current ID detectors will fail around 2015-18 (500-1000 fb-1) Constructions of new IDs takes 6-7 years

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Detector Needs at SLHC

Detector performance needs to be maintained despite the pile-up! High-mass (~TeV) can

tolerate some degradation; low backgrounds

But WW scattering (Higgs couplings or vector boson fusion) needs forward jet trigger and central jet veto

Vertex, missing Et, pt resolution remain important, and efficiencies, for many channels of interest

Electron ID and muons for W/Z, W'/Z', and SUSY

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b-tag eff

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Anticipated Peak and Integrated Luminosity

LHC, ATLAS and CMS have agreed to use this as basis for planning

Discussed at LHCC meeting 1 July 2008 Sets the conditions and timescale

Phase 1 starts with 6 – 8 month shutdown end 2012 Peak luminosity 3 x 10-34 cm-2 s-1 at end of phase 1

Phase 2 will start with an 18 month shutdown at end of 2016 Peak 10 x 10-34 cm-2 s-1 in phase 2

3000 fb-1 integrated luminosity lifetime of detectors minimum in phase 2

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LHC Evolution – Phase 1

LHC is complete apart from full collimation Limited to 40 % of nominal for protection until collimators installed Collimators to be completed in 2010/11 shutdown, allowing rise to

~nominal luminosity of 10-34 cm-2 s-1

Best current estimate is that one nominal year will deliver 60 fb-1 Phase-1: 2013-2016

Linac-4 Approved and work has started; higher brightness

Allows higher LHC current, to “Ultimate” which is 2.3 times nominal Ready to run in 2013

New Inner Triplet focusing magnets Use spare super-conductor from LHC magnets Larger aperture, allows β* of 0.25 m instead of 0.55 m Install in 2012/13 shutdown In principle also gives factor 2 on nominal

Expectation is that these two improvements will allow a ramp-up to 3 x nominal; Conditions: 70 minimum bias events per BC; ~700 fb-1 before phase 2

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LHC Evolution – Phase 2

Several ideas being explored to see the best way to achieve 10 x nominal in 2017

Injector improvements – higher current, higher reliability, shorter fill time

New machine elements and ideas: Magnets inside the experiments for “Early Separation” schemes Crab cavities Wire correctors Luminosity Leveling

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What are the conditions at SLHC?

300 – 400 pile-up events at start of spill (unless luminosity leveling)

Want to survive at least 3000 fb-1 data

taking

B-layer at 37 mm:

~30 tracks per cm-2 per bunch

crossing

>1016 1 MeV n-equivalent non-

ionising

Few 10s of MGray

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Non-ionising fluence

ATLAS 1 MeV neq cm-2 fluence at 1000 fb-1 (Ian Dawson)

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Detector Plans – Phase 1 Limited time for installation – 6 to 8 months in 2012/13 shutdown Small increase in peak rate above previous estimates (2 --> 3 x 1034) Total integrated luminosity similar to previous expectations ~700 fb-1

Limited changes needed; some completion of staged items e.g. CMS muons

CMS pixel detector is fast to replace Will replace at least the B-layer, and investigating substantial more

ambitious plans to replace the whole pixel detector

ATLAS pixel takes ~ 1 year to replace B-layer ATLAS will insert a new B-layer inside the current detector, along with a

new smaller diameter beam pipe, in 2012/13 shutdown TDAQ

Both experiments will continuously upgrade TDAQ to cope with rates and take advantage of new processing power

CMS investigate track triggers at Level-1 with new pixel (see later) ATLAS look at topological triggers – combining different trigger elements,

e.g. muon with no jet and fast track finding (associative memory) at LVL2

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Detector Changes for Phase 2

Most of ATLAS and CMS will cope well with SLHC Keep magnet systems and the basic elements of

the muon systems and calorimeters Inner trackers in both experiments need complete

replacement: Radiation damage limit will have been reached Need to replace them even if no SLHC! Higher rates cause dead time (e.g. ATLAS TRT) Need finer granularity detectors for good pattern recognition

And parts of all systems need upgrading, even if most of the basic detector parts remain

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Inner detectors - B-layers Most challenging for track

density, radiation damage, SEU

Highest requirements: efficiency, coverage, position resolution

Sensors: current planar-Si sensor technology is not rad-hard enough to survive to end of sLHC. Either new sensors, or replace every few years 3D silicon, thin silicon,

diamond, MPGD (Gossip) as alternatives

Smaller beampipes --> b-layer closer to beam

Si pixel sensorBiCMOS analogue

CMOS digital

Cluster3

Cathode (drift) plane

Integrated Grid (InGrid)

Cluster2

Cluster1

Slimmed Silicon Readout chipInput pixel

1mm,100V

50um, 400V

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Pixel Detectors

Read-out architecture and front-end chips under development 130 nm; low power; minimum

pixel length; high data rates

High power levels -> look at new cooling, including CO2

Lighter mass supports and services?

Cheaper production – more pixels?

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CMS

ATLAS

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New Strips Detectors

Switch to n-in-p sensors At high dose, may not achieve full

depletion Still have readout junction in the depleted

region, no big signal loss Prototype sensors reach 1000 V after

irradiation -> good charge collection efficiency

Short strips (~25 mm) at inner region for lower occupancy

Mechanics and assembly Take into account need for low radiation

length and rapid installation in a short shutdown

Both experiments insert complete ID's

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Electromagnetic Calorimeters

Both ATLAS and CMS EM calorimeters should perform well at SLHC

Pileup worsens the resolution a little, partially compensated by optimising the sampling

New electronics can allow more flexibility in trigger; all data read out

Worst affected region is forward Remains important for WW-scattering triggers

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Electromagnetic Calorimeters: Atlas LAr

ATLAS forward calorimeter may suffer a number of problems: Boiling of LAr, ion build up between electrodes, voltage drop over HV resistor Studies underway; If these show action is needed, two solutions considered:

Warm calorimeter in front of current calorimeter Open cryostat, insert complete new FCAL with smaller gaps and more

cooling

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FCAL

HEC

ELECTRONICS

HEC2

HEC1

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Hadronic Calorimeters - CMS Most of hadron cal is fine Forward region suffers: few towers blacked by SLHC (tower 1

~ 4 % of original light output; tower 2 ~23%) Also, machine magnets (“D0”) block forward calorimetry

Hadronic ForwardHadronic Forward HEndcapHEndcap

HBarrelHBarrel

HOHO

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Muon Systems CMS has a lot of shielding, rate probably OK for current

chambers Need to see backgrounds to confirm; possibly η > 2 need

changing, or limit trigger region New readout electronics? FPGA not rad hard enough

ATLAS air core toroids have higher backgrounds; need to replace forward chambers (CSCs mainly) at nominal background. Very important to measure actual background to see how

much of “safety factor 5” is used up to see if significantly more needs replacing

Both experiments are looking into improved shielding Difficult : current design is highly optimised Other possibility is to develop single chambers to do both

triggering and precision read-out: thinner chambers leave more space for shielding – see talk later on

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ATLAS Muon Chamber Replacement Range

Depending on backgrounds, either minimal or very large fraction of Atlas muon system needs replacing, unless backgrounds can be reduced (in relation to luminosity)

Both Atlas and CMS have to wait for data

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Muons - example of chamber R&D

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Beam-pipe and shielding

All-Be beam pipe reduces muon BG considerably Expensive beampipe, but much cheaper than new muon chambers

CMS consider more shielding to η = 2 Add borated polythene; better shielding of PMTs

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Main Electronics Needs – Readout chips

The ATLAS and CMS Upgrades need new electronics throughout the detector: power supplies of calorimeters, data transfer and handling for all detectors; some cases highlighted below

Read-out chips for pixels and strips Under development for ATLAS and CMS; ABCNext, FE-I4, Timepix-2, CMS Controller chips High speed data links Requirements

Very challenging: rad hard, SEU tolerant, low analogue noise. Low power: number of channels increases by large factors between current and

upgraded detectors. Bringing power in and removing it are major contributors to the material budget

High data rates: e.g. develop per-pixel storage, read pixel to end of column only at level-1 trigger

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Powering and data transfer Powering scheme

Cannot have individual module LV – no space, too much material DC/DC or serial very important; many possible schemes Look beyond the basic requirements of high power efficiency and low

noise Safety: overcurrent, overvoltage, overtemperature Monitoring

Can we avoid copper sense lines, e.g. local safety; local ADC; send DCS information along with data on fibre optics

Data transfer High-speed electrical and optical links

Calorimeters may want to read out all data to RODs: a lot of data better triggering capability

How rad hard can we get optical links? Affects where we make the optical-electronic transition in the ID

Multiplexing and redundancy schemes Error correction schemes (SEU tolerance)

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Powering

Need to supply ~ 50kW at 1-2 V – hugely inefficient with large losses in cables (P=RI2, so we end up introducing a large amount of copper)

New detectors – lower voltages in DSM processes, higher granularity – we need to change approach and think new

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From F.Faccio

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Track trigger Inner Tracker Triggers at Level-1

Muon trigger rate ~constant above ~20-30 GeV/C; both ATLAS and CMS

Current understanding is this is due to multiple scattering at CMS and width of RPC strips at ATLAS

Cannot improve muon situation at CMS; difficult at ATLAS (new muon trigger chamber layer with higher resolution?)

Several ideas to investigate inner tracker triggers both Pt and vertex displacement

triggers

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Track trigger (Cont)

SearchWindow

γ

High momentum tracks are straighter so pixels line up

High momentum tracks are straighter so pixels line up

Pairs of stacked layers can give a PT

measurement

Pairs of stacked layers can give a PT

measurement

Several ideas to investigate inner tracker triggers

both Pt and vertex displacement triggers

E.g. local coincidences separated by >~ 1 mm in pixels read to end-of-stave

then check for pairs of these in different layers

Micropattern gas detectors also interesting – collect the “coincidence” over ~17 mm gap onto one chip

Requires a lot of processing on the chip

Challenge is to develop new chips in time, without increasing the material budget too much (power as well as chip material)

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LHCC meetingCERN, 22/23 Sept 2008F. Muheim

LHCb Upgrade Strategy LHC Machine Upgrade (LHCC upgrade session 1th July 2008)

Tentative LHC schedule Phase 1 - IR Upgrade, new triplets, 8 months shutdown in 2012/13 Phase 2 – ATLAS & CMS replace inner detectors

18 months shutdown in 2017 Propose two-step approach consistent with LHC schedule

(LHCb upgrade does not require SLHC)

LHCb Upgrade Phase 1 Upgrade all front-end detector electronics to 40 MHz by 2014

do not run in 2013 (Nov 2012 – Mar 2014 with 12 months access) Run at 1x1033 until Phase 2 shutdown Increase hadron data sample by factor ~10 reach detector design lumi of ~20 fb-1 (except VELO)

LHCb Upgrade Phase 2 Upgrade all detectors such that LHCb can operate at a luminosity

of at least 2x1033 during 18 months shutdown in 2017 Operate at highest possible luminosity for five years

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LHCC meetingCERN, 22/23 Sept 2008F. Muheim

VELO → VESPA

VErtex LOcator replacement called VESPA

Solution for first upgrade phase (2013) Keep mechanical structure and silicon strip sensors Replace FE chip with 40 MHz readout This device will be rad hard to ~20 fb-1

and will collect data until 2017

Solution for 2017 will be a complete overhaul Pixels/3D detectors

better resolution lower occupancy

Possible magnetic field to improve trigger by taking advantage of improved pattern recognition

Remove bulky RF shield and replace with wires? Could use liquid N2 cooling with cold fingers to create good vacuum, making VESPA a cryo-pump at the LHC

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LHCC meetingCERN, 22/23 Sept 2008F. Muheim

Muon System

The major part of the muon detector can very likely operate at 2×1033 for 5 years Muon detector electronics is already at 40 MHz

Upgrade of M1 station is not required, it will likely be removed Momentum of muon candidates determined by tracking stations

Aging Okay for up to 100 fb-1 with the possible exception of region M2R1 technology presently adopted for region M1R1 (triple-GEM) will work

Further studies are required to understand the effects of a larger occupancy of the muon detector on the

tracking and the purity of muon identification.

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Scenario for ALICE

2008-2011 Detector Completion (TRD, PHOS, EmCal, PMD), data taking/analysis; some maintenance.

2009-2011 Detector R&D and definition of upgrade plan (requires significant simulation effort, not possible so far)

2010-2011 Decision on upgrade, funding approval, etc.

2011-2014 Construction of new detectors

2013-15 Installation of upgraded detectors

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VHMPID – for ALICE Would be located on both sides of PHOS, below space frame;

RICH-like detector with mirrors, Gas radiator (C4F10?) maximum length ~80cm;

PHOS

VHMPID

Photon detector: MWPC with CsI photon converter and pad readout

(current HMPID technology);

Resistive Thick GEM (≥2 layers) with CsI photon converter (promising preliminary results).

Dedicated trigger logic to select high pT

use of TRD detector;

4 layer GEMs detector with algorithm selecting high pT particles (new trigger detector);

use of EMCAL detector, opposite to beam line, triggering on high energy jets.

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Summary There is every hope there will be a rich field of

physics to explore at the LHC into the 20's The LHC expects

Phase-1 upgrade 2012 leading to 3 x 1034 cm-2 s-1 peak luminosity

Phase-2 upgrade 2016 leading to 10 x 1034 cm-2 s-1 peak luminosity (restart in 2017)

Atlas and CMS require major upgrades (even without Phase-2) installed in long shutdown 2016

LHCb and ALICE are also formulating upgrade programs

Overall very ambitious detector development and construction periods

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Backup slides

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