Physics at the Large Hadron Collider (LHC)hep.ucsb.edu/people/claudio/talks/ucsb_coll.pdfLarge...
Transcript of Physics at the Large Hadron Collider (LHC)hep.ucsb.edu/people/claudio/talks/ucsb_coll.pdfLarge...
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Physics at the Large Physics at the Large HadronHadronColliderCollider (LHC)(LHC)
Claudio Claudio CampagnariCampagnariUC Santa BarbaraUC Santa Barbara
June 2, 2009June 2, 2009
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OutlineOutline
What and Why? What and Why? The LHCThe LHC A detector (CMS), how we do physics at A detector (CMS), how we do physics at
the LHCthe LHC How to look for "New Physics"How to look for "New Physics" StatusStatus
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Electroweak
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Standard Model (SM) works very well and Standard Model (SM) works very well and has been tested to E~O(100 GeV)~10has been tested to E~O(100 GeV)~10--1818mm
Several open questionsSeveral open questions Why 3 generationsWhy 3 generations Why matterWhy matter--antimatter asymmetry antimatter asymmetry Dark matter?Dark matter? Dark energy?Dark energy? How does the How does the ElectroWeakElectroWeak interaction break interaction break
into EM and Weak interaction at low energies into EM and Weak interaction at low energies (electroweak symmetry breaking)(electroweak symmetry breaking)
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ElectroWeakElectroWeak Symmetry BreakingSymmetry Breaking
Occurs at E ~ 1000 Occurs at E ~ 1000 GeVGeV (1 (1 TeVTeV)) In the SM realized through interaction with In the SM realized through interaction with
Higgs fieldHiggs field Results in a yetResults in a yet--toto--bebe--discovered Higgs discovered Higgs
particleparticle
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Do not know if the Higgs mechanism is the Do not know if the Higgs mechanism is the right answerright answer
But, if it is not the answer, something else But, if it is not the answer, something else must be operational at the must be operational at the TeVTeV scalescale
The LHC is the machine that will allow us The LHC is the machine that will allow us to explore the to explore the TeVTeV scalescale
Find the Higgs (if it's there) and study its Find the Higgs (if it's there) and study its propertiesproperties
And/Or see if there is New PhysicsAnd/Or see if there is New Physics
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OutlineOutline
What and Why?What and Why? The LHCThe LHC A detector (CMS), how we do physics at A detector (CMS), how we do physics at
the LHCthe LHC How to look for "New Physics"How to look for "New Physics" StatusStatus
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Large Large HadronHadron ColliderCollider (LHC)(LHC)
A 14 A 14 TeVTeV protonproton--proton proton collidercollider 1 1 TeVTeV = 10= 101212 eVeV A factor of 7 more energy than the A factor of 7 more energy than the FermilabFermilab
TevatronTevatron 27 Km long tunnel, 100 m below ground27 Km long tunnel, 100 m below ground 9300 superconducting magnets (1232 dipoles)9300 superconducting magnets (1232 dipoles)
60 tons of liquid helium60 tons of liquid helium 11,000 tons of liquid nitrogen 11,000 tons of liquid nitrogen
Energy stored in magnets = 10 GJEnergy stored in magnets = 10 GJ
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Each of the 1232 dipoles....Each of the 1232 dipoles.... is 15 m longis 15 m long carries 11.8 kA of currentcarries 11.8 kA of current provides a field of 8.3 Tprovides a field of 8.3 T
There are 2808 "bunches" of protons in There are 2808 "bunches" of protons in each beameach beam 10101111 protons per bunchprotons per bunch 11,245 turn11,245 turn
When brought into collision the transverse When brought into collision the transverse size of the bunches is of order 10 size of the bunches is of order 10 mm
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Picture of the tunnelPicture of the tunnel
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OutlineOutline
What and Why? What and Why? The LHCThe LHC A detector (CMS), how we do physics at A detector (CMS), how we do physics at
the LHCthe LHC How to look for "New Physics"How to look for "New Physics" StatusStatus
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Coil insertion. 4T superconducting solenoid
Magnet is 12,000 tons. Stores enough energy to melt 18 tons of gold.
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Insertion of HCAL
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Insertion of ECAL super modules
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Insertion of tracker
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closing of detector for magnet test
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What does the detector do?What does the detector do? The detector tries to measure the 4The detector tries to measure the 4--momenta of all momenta of all
particles in a pp collisionsparticles in a pp collisions 33--momenta of charged particles are inferred by momenta of charged particles are inferred by
reconstructing tracks as it bends in a 4T magnetic fieldreconstructing tracks as it bends in a 4T magnetic field For neutrals (For neutrals (, neutrons), energy is measured by size , neutrons), energy is measured by size
of "shower" in instrumented material (calorimeter)of "shower" in instrumented material (calorimeter) The interactions patterns of particles with the detector The interactions patterns of particles with the detector
elements allows to "identify" the particle specieselements allows to "identify" the particle species e.g.,e.g., electron electron vsvs muonmuon vsvs protonproton
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They do not interactThey do not interact Their presence is inferred by conservation of Their presence is inferred by conservation of
momentummomentum In practice this can only be done in the plane In practice this can only be done in the plane
transverse to the beam direction, since transverse to the beam direction, since particles escaping down the particles escaping down the beampipebeampipe are are not measurednot measured Missing Transverse Momentum, or Missing Missing Transverse Momentum, or Missing
Transverse EnergyTransverse Energy
Neutrinos (or dark matter particles)Neutrinos (or dark matter particles)
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Gluons and quarks Gluons and quarks jetsjets
They do not They do not directlydirectly show up in the detectorshow up in the detector Quarks and Quarks and antiquarksantiquarks are pulled from the are pulled from the
vacuum and bound states are formed (hadrons, vacuum and bound states are formed (hadrons, egeg, , pionspions, protons, etc), protons, etc)
If the original gluon or quark is energetic If the original gluon or quark is energetic enough, the result is a spray of hadrons (jet) enough, the result is a spray of hadrons (jet) that preserves the direction and energy of the that preserves the direction and energy of the original gluon or quark (more or less) original gluon or quark (more or less)
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A two jet event from D0 (A two jet event from D0 (didi--jet)jet)
Two jets back-to-back in Note: 45 GeV of MET
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What happens when two protons What happens when two protons collide?collide?
Most of the times: not very muchMost of the times: not very much The protons might break up with most The protons might break up with most
daughter particles going down the daughter particles going down the beampipebeampipe. A few ( ~50. A few ( ~50--100) particles with 100) particles with small transverse momentum (Psmall transverse momentum (PTT) show up ) show up in the detectorin the detector
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Physics 105B: Billiard ball scattering:=4 R2
Rproton ~ 10-15 m (pp)~10-29 m2=100 mb
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The gardenThe garden--variety collisions are not interesting (to variety collisions are not interesting (to most people)most people)
The interesting collisions are the "violent" collisions The interesting collisions are the "violent" collisions where a lot of transverse momentum is exchangedwhere a lot of transverse momentum is exchanged
Here we can think of collisions between the Here we can think of collisions between the components of the proton (quarks, components of the proton (quarks, antiquarksantiquarks, and , and gluons, gluons, akaaka partonspartons))
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Think of the LHC as a Think of the LHC as a partonparton--partonparton collidercollider BroadbandBroadband collidercollider. . PartonsPartons in the proton can in the proton can
take any fraction of the proton momentum.take any fraction of the proton momentum. In a probabilistic way, that we cannot calculate In a probabilistic way, that we cannot calculate
from first principles from first principles measure itmeasure it
ffii(x(x) = ) = probprob of of partonparton i i having momentum x*having momentum x*PPprotonproton
PartonParton Distribution Distribution Function (Function (pdfpdf))
Note that there are many Note that there are many manymany manymany gluons.gluons.
LHC = gluon LHC = gluon collidercollider
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Moving on to harder scattersMoving on to harder scatters
Jets have large crossJets have large cross--sections because they sections because they are strong processes, are strong processes, egeg, , gggggggg
To look for "New Physics" To look for "New Physics" require presence of require presence of or or leptons (e, leptons (e, , , ) or ) or missing energymissing energy BackgrondsBackgronds are electroare electro--
weak processesweak processes There are exceptionsThere are exceptionsNote: TeV-scale SUSY, ~ 10-9mb
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OutlineOutline
What and Why? What and Why? The LHCThe LHC A detector (CMS), how we do physics at A detector (CMS), how we do physics at
the LHCthe LHC How to look for "New Physics"How to look for "New Physics" StatusStatus
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What Physics should I do at the LHC?What Physics should I do at the LHC?
To Higgs or not to Higgs? To Higgs or not to Higgs? Should I look for the Standard Model Higgs, Should I look for the Standard Model Higgs,
or for "New Physics"?or for "New Physics"? Interestingly enough all of us at UCSB Interestingly enough all of us at UCSB
have answered "not to Higgs"have answered "not to Higgs"
Remainder of the talk on searches for New Remainder of the talk on searches for New PhysicsPhysics
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3+1 Ingredients for New Physics 3+1 Ingredients for New Physics Discoveries at the LHCDiscoveries at the LHC
0.0. Machine/detector:Machine/detector: if they if they dontdont work, forget itwork, forget it1.1. Trigger:Trigger: if you did not trigger on it, it never if you did not trigger on it, it never
happenedhappened2.2. Backgrounds:Backgrounds: It's the background, stupidIt's the background, stupid
Need to understand instrumental and Standard Need to understand instrumental and Standard Model physics backgroundsModel physics backgrounds
3.3. Searches:Searches: If you look for something, you may not find If you look for something, you may not find it. But if you don't look, you will never find itit. But if you don't look, you will never find it
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What is the "trigger"?What is the "trigger"? (pp) ~ 100 (pp) ~ 100 mbmb Gives an "event rate" of order 100 MHzGives an "event rate" of order 100 MHz Each event is ~ 250 kbEach event is ~ 250 kb 250 kb x 100 MHz = 25 250 kb x 100 MHz = 25 TbytesTbytes/second/second
Trigger is the system that Trigger is the system that selects the ~ 200 selects the ~ 200 events/second that are events/second that are saved for further studysaved for further study
Most of the events are Most of the events are thrown away!!!!thrown away!!!!
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Trigger (2)Trigger (2) The decision on what to trigger on has enormous impact on The decision on what to trigger on has enormous impact on
the physics that we can dothe physics that we can do Trigger selects objects (e, Trigger selects objects (e, , jets..) or combinations thereof , jets..) or combinations thereof All kinematical distributions fall steeply with PAll kinematical distributions fall steeply with PTT trigger trigger
selects objects above a thresholdselects objects above a threshold It is always a compromiseIt is always a compromise A balance between competing A balance between competing
prioritiespriorities A source of great debate in the A source of great debate in the
collaboration collaboration If you, as a theorist have a great If you, as a theorist have a great
idea for NPidea for NP……....1.1. Check that your events have been Check that your events have been
triggered ontriggered on2.2. If not, try to convince people to If not, try to convince people to
devote bandwidth to your theorydevote bandwidth to your theoryAnd your argument better be goodAnd your argument better be good……
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CMS "Trigger Menu"CMS "Trigger Menu"
From the Technical Design Report. Obsolete. There are now close to 100 different triggers in the menu.....
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New Physics discoveries @ LHCNew Physics discoveries @ LHCBroadly speaking, three typesBroadly speaking, three types1.1. Self CalibratingSelf Calibrating
•• A signal that stands out, where you do not really A signal that stands out, where you do not really need to understand the background very wellneed to understand the background very well
2.2. Counting experimentsCounting experiments•• The number of observed events of some type is The number of observed events of some type is
>> than the SM prediction>> than the SM prediction3.3. DistributionsDistributions
•• The distribution of some kinematical quantity is The distribution of some kinematical quantity is inconsistent with the SM prediction inconsistent with the SM prediction
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Self Calibrating Signals (SCS)Self Calibrating Signals (SCS)
A NP signal that obviously stands outA NP signal that obviously stands out where you do not need to know the SM BG very where you do not need to know the SM BG very
preciselyprecisely
For example:For example: A mass peakA mass peak
XXAB, measure the 4AB, measure the 4--momenta of A & B, then, momenta of A & B, then, (P(PAA+P+PBB))22=M=MXX
22
A A hugehuge distortion to some kinematical distributiondistortion to some kinematical distribution
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DrellDrell--YanYane- or -
e+ or +
SM Drell-Yan
Di-jet backgroundWW background
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SCS example: Z' SCS example: Z'
What a 100 pb-1 exptmight look like
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Another SCS example: Another SCS example: didi--jet mass distributionjet mass distribution
Distorts angular distributionsDistorts angular distributions More scatters at high anglesMore scatters at high angles
More jets at high PMore jets at high PTT
More More didi--jets at high massjets at high mass
Quark Contact Interaction
M ~
Quark Compositeness New Interactions
M ~
Dijet Mass <<
q
q
q
q
q
q q
qQCD Background
QCD + Signal
Dijet Mass or jet PT
d/ d
Mor
d/
dPT
If the "edge" is low enough, thiscould be a relatively easy discovery
(Self-calibrating variety)
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DiDi--jet mass distribution distortionjet mass distribution distortion Ratio of events at highRatio of events at high--low low is a sensitive is a sensitive
variable that eliminates many variable that eliminates many systsystuncertaintesuncertaintes
95% CL Exclusion95% CL Exclusion 14.814.810.410.46.26.2
12.012.07.87.84.74.755σσ DiscoveryDiscovery
++ forfor10 fb10 fb--11
((TeVTeV))
++ for for 1 fb1 fb--11
((TeVTeV))
++ forfor100100 pbpb--11
((TeVTeV))
LeftLeft--HandedHandedQuark ContactQuark Contact
InteractionInteraction
CMS CMS
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What was just described is like What was just described is like Rutherford Scattering, but with quarks!Rutherford Scattering, but with quarks!
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SCS: EdgesSCS: Edges
M(l+l-)
10 fb-1
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3+1 Ingredients for New Physics 3+1 Ingredients for New Physics Discoveries at the LHCDiscoveries at the LHC
0. 0. Machine/detector:Machine/detector: if they if they dontdont work, forget itwork, forget it1. 1. Trigger:Trigger: if you did not trigger on it, it never if you did not trigger on it, it never
happenedhappened2.2. Backgrounds:Backgrounds: It's the background, stupidIt's the background, stupid
Need to understand instrumental and Standard Need to understand instrumental and Standard Model physics backgroundsModel physics backgrounds
3. 3. Searches:Searches: If you look for something, you may not find If you look for something, you may not find it. But if you don't look, you will never find itit. But if you don't look, you will never find it
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Not all NP signals are as dramatic as a mass peakNot all NP signals are as dramatic as a mass peak Particularly for signal with dark matter particles, Particularly for signal with dark matter particles, egeg, ,
SUSYSUSY Because dark matter particles are not detected, only Because dark matter particles are not detected, only
inferred from Missing Transverse Energyinferred from Missing Transverse Energy And most often you have two per eventsAnd most often you have two per events
Less dramatic signalsLess dramatic signals
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Signal can be Signal can be "number of events passing selection" > SM "number of events passing selection" > SM
expectationexpectation "kinematical distributions" inconsistent with SM"kinematical distributions" inconsistent with SM
Example: pp b'�' tW ŧW. HT=sum of PT of all objects
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Understanding the SM background is keyUnderstanding the SM background is key This is were most of the work goesThis is were most of the work goes Difficult because background is usually an Difficult because background is usually an
"unlikely" SM event"unlikely" SM event In the tail of distributions In the tail of distributions
Methods that try to estimate the background Methods that try to estimate the background from the data itself using clever tricks are the from the data itself using clever tricks are the most robustmost robust
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ExampleExample pp pp jets + MET is a generic signature of SUSY jets + MET is a generic signature of SUSY
pp pp Z + jets, with Z Z + jets, with Z gives similar signaturegives similar signature Crucial to have an estimate of itCrucial to have an estimate of it But SM theory is uncertain to factors O(2) or moreBut SM theory is uncertain to factors O(2) or more
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Clever Clever data drivendata driven ideaidea
pp pp Z + jets and pp Z + jets and pp + jets have similar + jets have similar production propertiesproduction properties
Use pp Use pp + jets + jets datadata, delete , delete from the event, from the event, apply some well understood corrections, predict apply some well understood corrections, predict pp pp Z(Z() + jets) + jets
or Z
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Test this idea on simulated dataTest this idea on simulated data
(J. Incandela et al)
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5757M. Mangano, Int.J.Mod.Phys.A23:3833-3848,2008
• Important to come up with clever tricks • Lots of work to validate theoretical tools when clever
tricks do not quite work
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3+1 Ingredients for New Physics 3+1 Ingredients for New Physics Discoveries at the LHCDiscoveries at the LHC
0. 0. Machine/detector:Machine/detector: if they if they dontdont work, forget itwork, forget it1. 1. Trigger:Trigger: if you did not trigger on it, it never if you did not trigger on it, it never
happenedhappened2. 2. Backgrounds:Backgrounds: It's the background, stupidIt's the background, stupid
Need to understand instrumental and Standard Need to understand instrumental and Standard Model physics backgroundsModel physics backgrounds
3. 3. Searches:Searches: If you look for something, you may not find If you look for something, you may not find it. But if you don't look, you will never find itit. But if you don't look, you will never find it
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Model dependent vs. model Model dependent vs. model independent searchesindependent searches
Can search for generic NP signaturesCan search for generic NP signatures e.g., the e + e.g., the e + + MET+ MET
Or, for very specific, complicated signaturesOr, for very specific, complicated signatures e.g., e.g., ppppTTTT, , TTtZtZ TTbWbW, , tteebb ZZ, W, W
Because we do not know what the NP is, Because we do not know what the NP is, generic searches are very powerfulgeneric searches are very powerful
But in a generic search But in a generic search worry about missing worry about missing complicated signature that nobody thought complicated signature that nobody thought about......about......
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Palano (Bari)DsJ(2317) DS 0
PRL90 242001 (2003)
BaBar
This huge signal had been in various data This huge signal had been in various data sets for many years!!sets for many years!!
c�meson. Was expected to havemass ~ 2.5 GeV, decay strongly toDK, and therefore have broad width
So: noone bothered to look!
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OutlineOutline
What and Why? What and Why? The LHCThe LHC A detector (CMS), how we do physics at A detector (CMS), how we do physics at
the LHCthe LHC How to look for "New Physics"How to look for "New Physics" StatusStatus
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Where are we nowWhere are we now
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Current ScheduleCurrent Schedule
After extensive repairs the machine is After extensive repairs the machine is scheduled to come on line this Fallscheduled to come on line this Fall
Energy of 10 Energy of 10 TeVTeV (design is 14)(design is 14) Low intensity to commissionLow intensity to commission
First results in 2010First results in 2010
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In the meantime the experiments are getting ready for data.Using cosmic rays to debug detector, align components, etc
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ConclusionsConclusions
The LHC era is (finally) about to beginThe LHC era is (finally) about to begin
We are looking forward to finding out what We are looking forward to finding out what nature has in store for usnature has in store for us
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The EndThe End
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Interim Summary Report on the analysis of the 19th Interim Summary Report on the analysis of the 19th September 2008 incident at the LHCSeptember 2008 incident at the LHC
Incident during poweringIncident during powering
The magnet circuits in the seven other sectors of the LHC had been fully commissioned to their nominal currents (corresponding to beam energy of 5.5 TeV) before the first beam injection on 10 September 2008. For the main dipole circuit, this meant a powering in stages up to a current of 9.3 kA. The dipole circuit of sector 3-4, the last one to be commissioned, had only been powered to 7 kA prior to 10 September 2008. After the successful injection and circulation of the first beams at 0.45 TeV, commissioning of this sector up to the 5.5 TeV beam energy level was resumed as planned and according to established procedures.
On 19 September 2008 morning, the current was being ramped up to 9.3 kA in the main dipole circuit at the nominal rate of 10 A/s, when at a value of 8.7 kA, a resistive zone developed in the electrical bus in the region between dipole C24 and quadrupole Q24. The first evidence was the appearance of a voltage of 300 mV detected in the circuit above the noise level: the time was 11:18:36 CEST. No resistive voltage appeared on the dipoles of the circuit, individually equipped with quench detectors with a detection sensitivity of 100 mV each, so that the quench of any magnet can be excluded as initial event. After 0.39 s, the resistive voltage had grown to 1 V and the power converter, unable to maintain the current ramp, tripped off at 0.46 s (slow discharge mode). The current started to decrease in the circuit and at 0.86 s, the energy discharge switch opened, inserting dump resistors in the circuit to produce a fast power abort. In this sequence of events, the quench detection, power converter and energy discharge systems behaved as expected.
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Interim Summary Report on the analysis of the 19th Interim Summary Report on the analysis of the 19th September 2008 incident at the LHCSeptember 2008 incident at the LHC
Sequence of events and consequencesSequence of events and consequences
Within the first second, an electrical arc developed and punctured the helium enclosure, leading to release of helium into the insulation vacuum of the cryostat.
The spring-loaded relief discs on the vacuum enclosure opened when the pressure exceeded atmospheric, thus relieving the helium to the tunnel. They were however unable to contain the pressure rise below the nominal 0.15 MPa absolute in the vacuum enclosures of subsector 23-25, thus resulting in large pressure forces acting on the vacuum barriers separating neighboring subsectors, which most probably damaged them. These forces displaced dipoles in the subsectors affected from their cold internal supports, and knocked the Short Straight Section cryostats housing the quadrupoles and vacuum barriers from their external support jacks at positions Q23, Q27 and Q31, in some locations breaking their anchors in the concrete floor of the tunnel. The displacement of the Short Straight Section cryostats also damaged the “jumper” connections to the cryogenic distribution line, but without rupture of the transverse vacuum barriers equipping these jumper connections, so that the insulation vacuum in the cryogenic line did not degrade.
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BusbarBusbar splicesplice
72
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QQBI.27R3QQBI.27R3
73
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Q27R3Q27R3
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