LHC : High Luminosity, UFOs and other surprises

143
LHC: High Luminosity, UFOs and other surprises Even before the drawing-board stage, the farsighted John Adams noted in 1977 that the tunnel for a future large electron–positron (LEP) collider should also be big enough to accommodate another ring of magnets. Rüdiger Schmidt, CERN 23 July 2012 Hadron Collider Summer School Introduction to the LHC accelerator Accelerator physics and LHC performance limitations Machine protection, collimation and UFOs Beam operation in 2012 Acknowledgements for slides from T.Baer, M.Lamont, R.Steinhagen, D.Wollmann and J.Wenninger

description

LHC : High Luminosity, UFOs and other surprises. Acknowledgements for slides from T.Baer , M.Lamont, R.Steinhagen , D.Wollmann and J.Wenninger. Rüdiger Schmidt, CERN 23 July 2012 Hadron Collider Summer School . Introduction to the LHC accelerator - PowerPoint PPT Presentation

Transcript of LHC : High Luminosity, UFOs and other surprises

Page 1: LHC :  High Luminosity, UFOs and other surprises

LHC: High Luminosity, UFOs and other surprises

Even before the drawing-board stage, the farsighted John Adams noted in 1977 that the tunnel for a future large electron–positron (LEP) collider

should also be big enough to accommodate another ring of magnets.

Rüdiger Schmidt, CERN23 July 2012

Hadron Collider Summer School

Introduction to the LHC acceleratorAccelerator physics and LHC performance limitationsMachine protection, collimation and UFOsBeam operation in 2012

Acknowledgements for slides from T.Baer, M.Lamont,

R.Steinhagen, D.Wollmann and J.Wenninger

Page 2: LHC :  High Luminosity, UFOs and other surprises

LHC: A long story starting in the distant past

First ideas to first protons: from 1984 to 2008 Tears of joy…. first beam in 2008 Tears of sadness…first (and hopefully last) accident in

2008

What doesn’t kill you makes you stronger The story of the champagne bottles

Page 3: LHC :  High Luminosity, UFOs and other surprises

Introduction to LHC Accelerator Physics Crash Course

• Why protons? Why superconducting magnets? Why “two” accelerators in one tunnel?

LHC layout and beam transport High Luminosity and the consequences High Energy and the consequences Wrapping up: LHC Parameters The CERN accelerator complex: injection and transfer LHC superconducting magnets Machine protection and collimation LHC operation Summary and conclusions

Outline

Page 4: LHC :  High Luminosity, UFOs and other surprises

Energy and Luminosity

Particle physics requires an accelerator colliding beams with a centre-of-mass energy substantially exceeding 1 TeV

In order to observe rare events, the luminosity should be in the order of 1034 [cm-2s-1] (challenge for the LHC accelerator)

Event rate:

Assuming a total cross section of about 100 mbarn for pp collisions, the event rate for this luminosity is in the order of 109 events/second (challenge for the LHC experiments)

Nuclear and particle physics require heavy ion collisions in the LHC (quark-gluon plasma .... )

][][ 212 cmscmLtN

Page 5: LHC :  High Luminosity, UFOs and other surprises

LHC pp and ions7 TeV/c 26.8 km Circumference

CERN Main Site

SwitzerlandLake Geneva

France

LHC Accelerator (100 m down)

SPS Accelerator

CERN-Prevessin

CMS, TOTEM

ALICE

LHCb

ATLAS

Page 6: LHC :  High Luminosity, UFOs and other surprises

The LHC: just another collider ?

Start Type Max proton energy [GeV]

Length [m]

B Field [Tesla]

Lumi [cm-2s-1]

Stored beam

energy [MJoule]

TEVATRONFermilab Illinois USA

1983

p-pbar 980 6300 4.5 4.3 1032 1.6 for protons

HERA DESY Hamburg

1992

p – e+p – e-

920 6300 5.5 5.1 1031 2.7 for protons

RHICBrookhavenLong Island

2000

Ion-Ionp-p

250 3834 4.3 1.5 1032 0.9 per proton beam

LHCCERN

2008

Ion-Ionp-p

7000 Now 4000

26800 8.3 1034

Now 6 1033

362 per Namebeam

Factor 7 4 2 50 100

Page 7: LHC :  High Luminosity, UFOs and other surprises

Accelerator Physics Crash Course

Page 8: LHC :  High Luminosity, UFOs and other surprises

The hierarchy in physics

DIE ZEIT 19/07/2012, citing Mike Lamont (Head of CERN accelerator operation):

Und unter den Physikern gebe es eine Hierarchie: »Ganz oben stehen die Theoretiker, dann kommen die Experimentalphysiker und dann wir, die Maschinenleute.«

Among physicists there is a hierarchy: » On top are the theorists, then the experimental physicist, then us, the machine people.«

Accelerator physicist

Experimental physicist

Theorist

Page 9: LHC :  High Luminosity, UFOs and other surprises

To accelerate a particle to high energy …

Particle energy about 10 kJoule

Page 10: LHC :  High Luminosity, UFOs and other surprises

To get to 7 TeV: Synchrotron – circular accelerator and many passages in RF cavities

LHC circular machine with energy gain per turn ~0.5 MeVacceleration from 450 GeV to 7 TeV will take about 20 minutes

Page 11: LHC :  High Luminosity, UFOs and other surprises

Lorentz Force

The force on a charged particle is proportional to the charge, the electric field, and the vector product of velocity and magnetic field:

For an electron or proton the charge is:

Acceleration (increase of energy) only by electrical fields – not by magnetic fields:

][. C106021eq 190

)( BvEF

q

EvBvvEv

Fv

qqdtdEdtdE

))((

2

1

s

sE sdF

Page 12: LHC :  High Luminosity, UFOs and other surprises

Particle deflection: superconducting magnets

The force on a charged particle is proportional to the charge, the electric field, and the vector product of velocity and magnetic field given by Lorentz Force:

)( BvEF

qRe

pB

0

z

x

s

v

B

F• Maximum momentum 7000 GeV/c• Radius 2805 m fixed by LEP tunnel• Magnetic field B = 8.33 Tesla• Iron magnets limited to 2 Tesla, therefore

superconducting magnets are required • Deflecting magnetic fields for two beams

in opposite directions

Page 13: LHC :  High Luminosity, UFOs and other surprises

Deflection by 1232 superconducing dipole magnets

Superconducting magnets in LHC tunnel

Page 14: LHC :  High Luminosity, UFOs and other surprises

Particle acceleration: accelerating protons to 7 TeV

Acceleration of the protons in an electrical field with 7 TV

But: no constant electrical

field above some Million Volt (break down)

no time dependent electrical field above some 10 Million Volt (about 30 MV/m)

1 MeV requires U = 1 MV

2s

1sU sdE

UqqEs

s

s

s

2

1

2

1sdEsdF

Page 15: LHC :  High Luminosity, UFOs and other surprises

LHC RF frequency 400 MHz

Revolution frequency 11246 Hz

Particle acceleration with RF cavity

)(tE

Time varying field

Maximum field about 20 MV/m

Beams are accelerated in bunches (no continuous beam)

Page 16: LHC :  High Luminosity, UFOs and other surprises

RF systems: 400 MHz

400 MHz system: 16 sc cavities (copper sputtered with niobium) for 16 MV/beam were built and assembled in four modules

Page 17: LHC :  High Luminosity, UFOs and other surprises

400 MHz RF buckets and bunches

E

time

RF Voltage

time

LHC bunch spacing = 25 ns = 10 buckets 7.5 m

2.5 ns

The particles are trapped in the RF voltage:this gives the bunch structure

RMS bunch length 11.2 cm 7.6 cmRMS energy spread 0.031% 0.011%

450 GeV 7 TeV

The particles oscillate back and forth in time/energy

RF bucket

2.5 ns

Page 18: LHC :  High Luminosity, UFOs and other surprises

Limitation of the energy

LEP was operating with electrons and positrons with an energy of 103 GeV / particle

As a factory for Higgs (?), operation at 120 GeV would be required (....assuming that ATLAS and CMS results are confirmed)

This was just a little above the LEP limit

There is a large interest in exceeding the LEP energy by one order of magnitude (LHC => 7 TeV)

The LHC provides proton – proton collisions

Page 19: LHC :  High Luminosity, UFOs and other surprises

Radius Lorenz Force = accelerating force

Particle trajectory Radiation field

charged particle

Figure from K.Wille

Power emitted for one particle: Ps=e0

2 c

6 0 m0 c2 4

E4

2

with E = energy, m0 = rest mass, e0 = charge, and = radius

Energy loss for charged particles by synchrotron radiation

Page 20: LHC :  High Luminosity, UFOs and other surprises

Energy loss for charged particles electrons / protons in LEP tunnel

Elep 100GeV Elhc 7000GeV

Energy loss for one particle per turn:

Ulep 3.844 109 eV Ulhc 8.121 103 eV

Total power of synchrotronradiation:

Number of electrons in LEP: Nlep 1012 Number of protons in LHC Nlhc 1014

Ptotal_lep Nlep Plep Ptotal_lhc Nlhc Plhc

Ptotal_lep 1.278 107 W Ptotal_lhc 2.699 103 W

The power of the synchrotronradiation emitted at the LHC is very small, but the radiation goes into the supraconducting magnets at 1.9 K ... 20 K

Page 21: LHC :  High Luminosity, UFOs and other surprises

LHC layout and beam transport

Page 22: LHC :  High Luminosity, UFOs and other surprises

LHC Layouteight arcs (sectors)eight long straight section (about 700 m long) IR4: RF + Beam

instrumentation

IR5:CMS

IR1: ATLAS

IR8: LHC-BIR2: ALICE

InjectionInjectionBeams from SPS

?? ??

??

Page 23: LHC :  High Luminosity, UFOs and other surprises

Beam transport

Need for getting protons on a circle: dipole magnets

Need for focusing the beams:

Particles with different injection parameters (angle, position) separate with time• Assuming an angle difference of 10-6 rad, two particles would

separate by 1 m after 106 m. At the LHC, with a length of 26860 m, this would be the case after 50 turns (5 ms !)

Particles would „drop“ due to gravitation The beam size must be well controlled

• At the collision point the beam size must be tiny Particles with (slightly) different energies should stay

together

Page 24: LHC :  High Luminosity, UFOs and other surprises

Magnets and beam stability

Dipole magnets• To make a circle around LHC

Quadrupol magnets• To keep beam particles together• Particle trajectory stable for particles with nominal momentum

Sextupole magnets• To correct the trajectories for off momentum particles • Particle trajectories stable for small amplitudes (about 10 mm)

Multipole-corrector magnets• Sextupole - and decapole corrector magnets at end of dipoles

Particle trajectories can become instable after many turns (even after, say, 106 turns)

Page 25: LHC :  High Luminosity, UFOs and other surprises

Focusing using lenses as for light beams

f1

x x

Quadrupolemagnet – B-field zero in centre, linear increase (as an optical lense)

Dipolemagnet – B-field in aperture constant

z z

Page 26: LHC :  High Luminosity, UFOs and other surprises

Assuming proton runs along s (=y), perpendicular to x and z

z

x

zconstzxconstx

x

z

)()(

BB

x

z

s

z

s

x Side viewfocusing

Looking along protontrajectory

Top viewdefocusing

From Maxwell equations:

Page 27: LHC :  High Luminosity, UFOs and other surprises

Focusing of a system of two lenses for both planes

d = 50 m

horizontal plane

vertical plane

f1 100m

f2 100 m

d 50m

F1f1

1f2

d

f1 f2

1

F 200 m

To focuse the beams in both planes, a succession of focusing and defocusing quadrupole magnets is required: FODO structure

Page 28: LHC :  High Luminosity, UFOs and other surprises

R.Schmidt

A (F0D0) cell in the LHC arcs

SSS

quadrupoleMQF

sextupole corrector(MCS)

decapoleoctupolecorrector(MCDO)

lattice sextupole

(MS)

lattice sextupole

(MS)

lattice sextupole

(MS)

orbit corrector

special corrector (MQS)

special corrector

(MO)

special corrector

(MO)

quadrupoleMQD

quadrupoleMQF

main dipole

MB

orbit corrector

orbit corrector

main dipole

MB

main dipole

MB

main dipole

MB

main dipole

MB

main dipole

MB

LHC Cell - Length about 110 m (schematic layout)

Vertical / Horizontal plane(QF / QD)

Quadrupole magnets controlling the beam size „to keep protons together“ (similar to optical lenses)

10000 magnets powered in 1700 electrical circuits

Page 29: LHC :  High Luminosity, UFOs and other surprises

Particle stability and superconducting magnets - Quadrupolar- and multipolar fields

LHC

Teilchenschwingungim Quadrupolfeld(kleine Amplitude)

Harmonische Schwingung(Koordinatentransformation)

Kreisbewegung im Phasenraum

z

y

y

y'

LHC

Teilchenschwingungbei nichlinearen Feldernund grosser Amplitude

Amplitude wächst bis zumTeilchenverlust

Keine Kreisbewegung im Phasenraum

z

y

y

y'

Particle oscillations in quadrupole field (small amplitude)

Harmonic oscillation after coordinate transformation

Circular movement in phase space

Particle oscillation assuming non-linear fields, large amplitude

Amplitude grows until particle is lost (touches aperture)

No circular movement in phasespace

Page 30: LHC :  High Luminosity, UFOs and other surprises

Relevant parameters to remember

Betatron tune: number of oscillations of a proton within one turn

Closed orbit: deviation of the centre of the bunch from the ideal path (approximately a circle)

Resonances: if the value of the betatron tune is equal to, say, n+0.5 or n+0.3333, the beam is lost

Page 31: LHC :  High Luminosity, UFOs and other surprises

Betatron tune measurement

Page 32: LHC :  High Luminosity, UFOs and other surprises

LHC superconducting magnets

Page 33: LHC :  High Luminosity, UFOs and other surprises

1232 Dipole magnetsLength about 15 m

Magnetic Field 8.3 T

Two beam tubes with an opening of 56 mm

plus many other magnets, to ensure beam stability (1700 main magnets and about 8000 corrector magnets)

Dipole magnets for the LHC

Page 34: LHC :  High Luminosity, UFOs and other surprises

Coils for Dipolmagnets

Page 35: LHC :  High Luminosity, UFOs and other surprises

The superconducting state only occurs in a limited domain of temperature, magnetic field and transport current density

Superconducting magnets produce high field with high current density

Lowering the temperature enables better usage of the superconductor, by broadening its working range

T [K]

B [T]

J [kA/mm2]

Operating temperature of superconductors (NbTi)

J [kA/mm2]

Page 36: LHC :  High Luminosity, UFOs and other surprises

Beam tubes

Supraconducting coil

Nonmagetic collars

Ferromagnetic iron

Steelcylinder for Helium

Insulationvacuum

Supports

Vacuumtank

Dipole magnet cross section16 mBar cooling tube

Quadrupolemagnet

Page 37: LHC :  High Luminosity, UFOs and other surprises

Operational margin of a superconducting magnet

Temperature [K]

App

lied

field

[T]

Superconductingstate

Normal state

Bc

Tc

9 K

Applied Magnetic Field [T]

Bc critical field

1.9 K

quench with fast loss of ~5 · 109 protons

quench with fast loss of ~5 · 106 protons

8.3 T

0.54 T

QUENCH

Tc critical temperature

Temperature [K]

Page 38: LHC :  High Luminosity, UFOs and other surprises

Movies dipole magnets

Page 39: LHC :  High Luminosity, UFOs and other surprises

High Luminosity: many protons in the collider

Page 40: LHC :  High Luminosity, UFOs and other surprises

High luminosity by colliding trains of bunches

Number of „New Particles“per unit of time:

The objective for the LHC as proton – proton collider is a luminosity of about 1034 [cm-2s-1]

• LEP (e+e-) : 3-4 1031 [cm-2s-1]• Tevatron (p-pbar) : some 1032 [cm-2s-1]• B-Factories : > 1034 [cm-2s-1]

212 cmscmLT

N

Page 41: LHC :  High Luminosity, UFOs and other surprises

Luminosity parameters

L = N … number of protons per bunch … revolution frequency … number of bunches per beam … beam dimensions at interaction point

Page 42: LHC :  High Luminosity, UFOs and other surprises

Beam beam interaction determines parameters

Beam size 16 m, for = 0.5 m ( is a function of the lattice)

Beam size given by injectors and by space in vacuum chamber

Number of protons per bunch limited to about 1-31011 due to the beam-beam interaction and beam instabilities

Beam size 16 m, for = 0.5 m ( is a function of the lattice)

f = 11246 Hz

with 2808 bunches (every 25 ns one bunch) L = 1034 [cm-2s-1]

L = for one bunch

Page 43: LHC :  High Luminosity, UFOs and other surprises

…smallest beam size at experiments

QuadrupoleQuadrupole Collision point in experiment

Large beam size in adjacent quadrupole magnets Separation between beams needed, about 10 Limitation with aperture in quadrupoles Limitation of β function at IP to 1 m (2011) and 0.6 m (2012)

Page 44: LHC :  High Luminosity, UFOs and other surprises

The 2 LHC beams are brought together to collide in a ‘common’ region Over ~260 m the beams circulate in one vacuum chamber with ‘parasitic’

encounters (when the spacing between bunches is small enough) Total crossing angle of about 300 rad

Experimental long straight sections

200 m

inner quadrupoletriplet

separationdipole (warm)

recombinationdipole

quadrupoleQ4

quadrupoleQ5

ATLAS or CMS

inner quadrupoletriplet

separationdipole

recombinationdipole

quadrupoleQ4

quadrupoleQ5

collision point

beam I

Example for an LHC insertion with ATLAS or CMS

24 m

beamdistance194 mm

beam II

Page 45: LHC :  High Luminosity, UFOs and other surprises

194 mm ATLAS IP

~ 260 m

Common vacuum chamber

Horizontal plane: the beams are combined and then separated

Vertical plane: the beams are deflected to produce a crossing angle at the IP to avoid undesired encounters in the region of the common vacuum chamber

a (rad)

ATLAS -145 / ver.

ALICE 90 / ver.

CMS 120 / hor

LHCb -220 /hor

~ 7 mm

Not to scale !

a

Separation and crossing: example of ATLAS

Page 46: LHC :  High Luminosity, UFOs and other surprises

LHC Main Parameters

Page 47: LHC :  High Luminosity, UFOs and other surprises

LHC ParameterNominal 2011 2012

Proton energy [TeV] 7.0 3.5 4.0Current in main dipoles [kA] 11.85 6.0 6.8

Stored energy, dipole circuit (154 dipoles)

[GJ] 1.07 ~0.28 ~0.35

Protons per bunch - 1.15 x 1011 ~1.5 x 1011 ~1.5 x 1011

Number of bunches - 2808 1380 1380Bunch spacing [ns] 25 50 50Normalized emittance [mm] 3.75 2.0 - 3.0 2.0 - 3.0β* in IP1 and IP5 [m] 0.55 1.5 / 1.0 0.6Stored energy / beam [MJ] 362 ~116 ~130

Peak luminosity for ATLAS and CMS

[cm-2s-1] 1.0 x 1034 0.36 x 1034 ~0.6 x 1034

Integrated luminosity for ATLAS and CMS

[fb-1] - 5.6 15

Page 48: LHC :  High Luminosity, UFOs and other surprises

LHC Parameter (energy)Nominal 2011 2012 (intended)

Proton energy [TeV] 7.0 3.5 4.0Current in main dipoles [kA] 11.85 6.0 6.8

Stored energy, dipole circuit (154 dipoles)

[GJ] 1.07 ~0.28 ~0.35

Protons per bunch - 1.15 x 1011 ~1.5 x 1011 ~1.5 x 1011

Number of bunches - 2808 1380 1380Bunch spacing [ns] 25 50 50Normalized emittance [mm] 3.75 2.0 - 3.0 2.0 - 3.0β* in IP1 and IP5 [m] 0.55 1.5 / 1.0 0.6Stored energy / beam [MJ] 362 ~116 ~130

Peak luminosity for ATLAS and CMS

[cm-2s-1] 1.0 x 1034 0.36 x 1034 ~0.6 x 1034

Integrated luminosity for ATLAS and CMS

[fb-1] - 5.6 15

Page 49: LHC :  High Luminosity, UFOs and other surprises

LHC Parameter (luminosity)Nominal 2011 2012

Proton energy [TeV] 7.0 3.5 4.0Current in main dipoles [kA] 11.85 6.0 6.8

Stored energy, dipole circuit (154 dipoles)

[GJ] 1.07 ~0.28 ~0.35

Protons per bunch - 1.15 x 1011 ~1.5 x 1011 ~1.5 x 1011

Number of bunches - 2808 1380 1380Bunch spacing [ns] 25 50 50Normalized emittance [mm] 3.75 2.0 - 3.0 2.0 - 3.0β* in IP1 and IP5 [m] 0.55 1.5 / 1.0 0.6Stored energy / beam [MJ] 362 ~116 ~130

Peak luminosity for ATLAS and CMS

[cm-2s-1] 1.0 x 1034 0.36 x 1034 ~0.6 x 1034

Integrated luminosity for ATLAS and CMS

[fb-1] - 5.6 15

Page 50: LHC :  High Luminosity, UFOs and other surprises

Very high beam luminosity: consequences

High energy stored in the beams Dumping the beam in a safe way Avoiding beam losses, in particular in the superconducting

magnets• Beam induced magnet quenching (when 10-8-10-7 of beam hits magnet at 7

TeV)• Beam cleaning (Betatron and momentum cleaning)

Radiation, in particular in experimental areas from beam collisions (beam lifetime is dominated by this effect)• Single event upset in the tunnel electronics

Beam instabilities due to impedance and beam–beam effects Photo electrons, generated by beam losses - accelerated by the

following bunches – lead to instabilities

Page 51: LHC :  High Luminosity, UFOs and other surprises

LHC Layouteight arcs (sectors)eight long straight section (about 700 m long) IR4: RF + Beam

instrumentation

IR5:CMS

IR1: ATLAS

IR8: LHC-BIR2: ALICE

InjectionInjection

IR6: Beam dumping system

IR3: Moment Beam Cleaning (warm)

IR7: Betatron Beam Cleaning (warm)

Beam dump blocks

Detection of beam losses with >3600

monitors around LHC

Signal to kicker magnet

Beams from SPS

Page 52: LHC :  High Luminosity, UFOs and other surprises

Machine Protection and Collimation

Page 53: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

Energy stored magnets and beam

0.01

0.10

1.00

10.00

100.00

1000.00

10000.00

1 10 100 1000 10000Momentum [GeV/c]

Ener

gy s

tore

d in

the

beam

[MJ] LHC 7 TeV

LHC at injection

ISR

SNSLEP2

HERA

TEVATRON

SPSppbar

SPS transfer to LHC

Factor~200

RHIC proton

LHC energy in magnets

LHC 3.5 TeV

SPS material test

Page 54: LHC :  High Luminosity, UFOs and other surprises

What does this mean?

360 MJoule: the energy stored in one LHC beam corresponds

approximately to…

• 90 kg of TNT

• 8 litres of gasoline

• 15 kg of chocolate

It’s how ease the energy is released that matters most !!

The energy of an 200 m long fast train at 155 km/hour corresponds to the energy of 360 MJoule stored in one LHC beam

Page 55: LHC :  High Luminosity, UFOs and other surprises

55

Controlled SPS experiment 81012 protons clear damage beam size σx/y = 1.1mm/0.6mmabove damage limit for copper stainless steel no damage 21012 protons below damage limit for copper

6 cm25 cm

• Damage limit ~200 kJoule• 0.1 % of the full LHC 7 TeV beams• factor of ~10 below the energy in a

bunch train injected into LHC

V.Kain et al

A B D C

SPS experiment: Beam damage with 450 GeV proton beam

Page 56: LHC :  High Luminosity, UFOs and other surprises

56

Beam losses

In accelerators, particles are lost due to a variety of reasons • End of a physics fill• Beam-gas interaction • Losses from collisions • Losses due to the beam halo touching the aperture• Losses due to instabilities

Continuous beam losses are inherent to the operation of accelerators• Taken into account during the design of the accelerator

Accidental beam losses are due to a multitude of failures mechanisms

The number of possible failures leading to accidental beam loss is (nearly) infinite

Page 57: LHC :  High Luminosity, UFOs and other surprises

Layout of beam dump system in IR6

Beam 2

Beam dump block

Kicker magnets to paint (dilute)

the beam

about 700 m

about 500 m

15 fast ‘kicker’ magnets deflect the beam to the

outside

When it is time to get rid of the beams (also in case of emergency!), the beams are ‘kicked’ out of the ring by a system of kicker magnetsd send into a dump block !

Septum magnets deflect the

extracted beam vertically

quadrupoles

The 3 s gap in the beam gives the kicker time to

reach full field.

Ultra-high reliability system !!

Page 58: LHC :  High Luminosity, UFOs and other surprises

Dump line in IR6

Page 59: LHC :  High Luminosity, UFOs and other surprises

Dump line

Page 60: LHC :  High Luminosity, UFOs and other surprises

Dump installation

CERN visit McEwen 60

Page 61: LHC :  High Luminosity, UFOs and other surprises

Beam dump with 1380 bunches

Beam spot at the end of the beam dumping line, just in front of the beam dump block

Page 62: LHC :  High Luminosity, UFOs and other surprises

62

Beam losses, machine protection and collimation

Continuous beam losses

Collimation prevents too high beam losses around the accelerator (beam cleaning)

A collimation system is a (very complex) system installed in the LHC to

capture mostly halo particles Such system is also called (beam) Cleaning System

Accidental beam losses

“Machine Protection” protects equipment from damage, activation and downtime

Machine protection includes a large variety of systems

Page 63: LHC :  High Luminosity, UFOs and other surprises

RF contacts for guiding image

currents

Beam spot

2 mm View of a two

sided collimator

about 100 collimators are

installed in LHC

Ralph Assmann, CERN

length about 120 cm

Page 64: LHC :  High Luminosity, UFOs and other surprises

Betatron beam cleaning

Cold aperture

Cleaning insertion Arc(s) IP

Circulating beam

Illustration drawing

Arc(s)

Primarycollimator

Secondarycollimators

Tertiary beam halo + hadronic showers

Shower absorbers

Tertiarycollimators

SCTriplet

Page 65: LHC :  High Luminosity, UFOs and other surprises

• Ionization chambers to detect beam losses:• Reaction time ~ ½ turn (40 s)• Very large dynamic range (> 106)

• There are ~3600 chambers distributed over the ring to detect abnormal beam losses and if necessary trigger a beam abort !

Beam Loss Monitors

Page 66: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Continuous beam losses during collisions

66CMS

ExperimentATLAS

ExperimentLHC

ExperimentALICE

ExperimentMomentumCleaning

RF and BI

Beamdump

Betatron Cleaning

Page 67: LHC :  High Luminosity, UFOs and other surprises

Measurement: 500kJ losses at primary collimators (loss rate: 9.1e11 p/s) – IR7

Daniel Wollmann

TCP: ~505 kJ

Q8L7: ~335 J

Q11L7: ~35 J

Q19L7: ~4.7 J

Q8L7:h ~ 6.7e-4

Lower limit:RqLdil ~ 1.22e9 p/s (with

cresp= 2 )

Lost energy over 1 s

Page 68: LHC :  High Luminosity, UFOs and other surprises

Strategy for protection and related systems

Avoid that a specific failure can happen

Detect failure at hardware level and stop beam operation Detect initial consequences of failure with beam

instrumentation ….before it is too late…

Stop beam operation• stop injection• extract beam into beam dump block• stop beam by beam absorber / collimator

Elements in the protection systems• hardware monitoring and beam monitoring• beam dump (fast kicker magnet and absorber block)• collimators and beam absorbers• beam interlock systems linking different systems

Page 69: LHC :  High Luminosity, UFOs and other surprises

Machine Protection at Injection

…throwing 3 MJ at LHC

Page 70: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

SPS, transfer line and LHC

1 km

Beam is accelerated in SPS to 450 GeV (stored energy of 3 MJ)Beam is transferred from SPS to LHCBeam is accelerated in LHC to 3.5 TeV (stored energy of 100 MJ)Scraping of beam in SPS before transfer to LHC

Transfer line 3km

LHC

SPS6911 m

450 GeV / 400 GeV3 MJ

Acceleration cycle of ~10 s

CNGS Target

IR8

Switching magnetFast extraction

kicker

Injection kicker

Transfer line

Injection kicker

IR2 Fast extraction kicker

Page 71: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

Protection at injection

LHC circulating beam

Circulating beam in LHC

LHC vacuum chamber

Transfer line vacuum chamber

Page 72: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

LHC circulating beam

Beam injected from SPS and transfer line

Protection at injection

Beam from SPS

Injection Kicker

LHC injected beam

Page 73: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

LHC circulating beam

Kicker failure (no kick)

Protection at injection

Beam from SPS

Injection Kicker

Page 74: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

LHC circulating beam

Beam absorbers take beam in case of kicker misfiringTransfer line collimators ensure that incoming beam trajectory is ok

Protection at injection

Beam from SPS

Injection Kicker Set of transfer line

collimators (TCDI) ~5σ

Injection absorber(TDI) ~7σ

phase advance 900

Page 75: LHC :  High Luminosity, UFOs and other surprises

HASCO 2012 Rüdiger Schmidt

LHC circulating beam

Beam absorbers take beam in case of kicker misfiring on circulating beam

Protection at injection

Injection Kicker

Injection absorber(TDI) ~7σ

Circulating beam – kicked out

phase advance 900

LHC circulating beam

Set of transfer line collimators (TCDI)

~5σ

Page 76: LHC :  High Luminosity, UFOs and other surprises

Understanding LHC operation• Filling• Ramp• Squeeze• Adjust• Stable beams• Pilot beam• Batches• Closed orbit • Beta function• Betatron tunes• Emittance• Impedance

Page 77: LHC :  High Luminosity, UFOs and other surprises

From first year to first fb-1

2008First beam in

LHC

2010First fb-1

Page 78: LHC :  High Luminosity, UFOs and other surprises

From 2010….

Page 79: LHC :  High Luminosity, UFOs and other surprises

…..to 2012

1 fb-1 6 fb-1

Page 80: LHC :  High Luminosity, UFOs and other surprises

Excellent fill 2195 in 2011

A nice long fill of about 18 hours……

Injection and

ramp

Stable beams

Beam dump

Page 81: LHC :  High Luminosity, UFOs and other surprises

Beam Intensities and Luminosity, 11-18/6/2012

Stable performance

Mixe

d ba

g

Stable performance

2×1014

6×1033

Page 82: LHC :  High Luminosity, UFOs and other surprises

LHC 8:30 meeting

Overview of fillsFill Duration Ibeam Lpeak

[e30 cm-2s-1]Lint [pb-1]

Dump

2723 2:26 2.03E+14 6406 46.06 Trip of ROD.A81B1, SEU?

2724 1:13 2.03E+14 6329 25.905 Electrical perturbation

2725 7:04 2.05E+14 6520 115.5 Trip of S81

2726 8:58 2.05E+14 6499 142.5Elecitrical perturbation, FMCM

2728 11:41 2.06E+14 6525 171.5 Operator dump

2729 3:28 2.06E+14 6502 67.7 BLM self trigger

2732 1:52 2.06E+14 6592.5 40 QPS trigger RQX.R1, SEU?

2733 12:34 2.06E+14 6674 183 Triplet RQX.L2 tripped.

2734 15:33 2.01E+14 6257.5 203.5 Operator dump

2736 17:29 2.02E+14 6465.5 233 Operator dump

2737 3:36 1.99E+14 6021 66.1 RF Trip 2B2

Total 51.1% 1301

51 % of time in stable beams; total of 1.3 fb-1 in one week !

Page 83: LHC :  High Luminosity, UFOs and other surprises

Good fill 2195 in 2011 – start of the fill

Start injection

End injection

Start energy ramp

End energy ramp

3.5 TeV

~1 hour

Page 84: LHC :  High Luminosity, UFOs and other surprises

Reference fill 2195 in 2011 – at 3.5 TeV

Start ramp to collisiong

Squeezing

Energy ramp to 3.5 TeV

Bringing beams into collision

Page 85: LHC :  High Luminosity, UFOs and other surprises

Luminosity increase

Page 86: LHC :  High Luminosity, UFOs and other surprises

Luminosity increase

Page 87: LHC :  High Luminosity, UFOs and other surprises

Luminosity increase

Page 88: LHC :  High Luminosity, UFOs and other surprises

Luminosity increase

To increase the luminosity, the beta function was reduced between 2011 and 2012 from 1.0 m to 0.6 m

This reduces the beam size in the experiments, and increases the beam size in the adjacent quadrupole magnets (inner triplets)

Page 89: LHC :  High Luminosity, UFOs and other surprises

…beam size at experiments in 2011

Collision point in experiment

Crossing angle to avoid parasitic beam-beam interaction Minimum separation in the order of 10 ( rms beam size)

Quadrupole Quadrupole

Page 90: LHC :  High Luminosity, UFOs and other surprises

…becoming smaller during more squeezing

Collision point in experiment

β function at IP down to 0.6 m in 2012 Larger beam size in quadrupole magnets Higher energy: emittance decreases for protons Separation needs to increase to keep 10 Problems with aperture in quadrupoles Collimators need to be set tighter

Quadrupole Quadrupole

Page 91: LHC :  High Luminosity, UFOs and other surprises

Record fill 2692 in 2012, max. integrated luminosity

Start energy ramp

End energy ramp4 TeV

Page 92: LHC :  High Luminosity, UFOs and other surprises

Fill 2701, typical fill in 2012

R.Schmidt 92

end squeeze and start

adjust end adjust

start squeeze

Page 93: LHC :  High Luminosity, UFOs and other surprises

Fill 2602, also a typical fill in 2012…….

R.Schmidt 93

21:41:24 start

squeeze

21:57:33 start

adjust 22:07:15end adjust

21:37:59 end ramp

Page 94: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

BLM system: beam losses before collisions

CMS Experiment

ATLAS Experiment

LHC Experiment

ALICE Experiment

MomentumCleaning

RF and BI

Beamdump

Betatron Cleaning

Page 95: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Continuous beam losses during collisions

95CMS

ExperimentATLAS

ExperimentLHC

ExperimentALICE

ExperimentMomentumCleaning

RF and BI

Beamdump

Betatron Cleaning

Page 96: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

2. An object falls into the beam

Page 97: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Continuous beam losses during collisions

97CMS

ExperimentATLAS

ExperimentLHC

ExperimentALICE

ExperimentMomentumCleaning

RF and BI

Beamdump

Betatron Cleaning

Page 98: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Accidental beam losses during collisions

98CMS

ExperimentATLAS

ExperimentLHC

ExperimentALICE

ExperimentMomentumCleaning

RF and BI

Beamdump

Betatron Cleaning

Page 99: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Zoom one monitor: beam loss as a function of time

1 ms

Page 100: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

UFOs at LHC

Page 101: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 102: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 103: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 104: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 105: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 106: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 107: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 108: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 109: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 110: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 111: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 112: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 113: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 114: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 115: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 116: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 117: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 118: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 119: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 120: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 121: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 122: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 123: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 124: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 125: LHC :  High Luminosity, UFOs and other surprises

Rüdiger Schmidt

Page 126: LHC :  High Luminosity, UFOs and other surprises

2012 Achieved vs. Target LuminosityEstimates from Moriand (Mike Lamont & Steve Myers)

Assumptions– 4 TeV, 50 ns, 1380 bunches, 1.6e11, 2.5 um, pile-up ~ 35– 150 days of proton physics (assuming similar efficiencies to 2011)

Initial slow recovery a technical stop, but eventually caught upPresently operating with ~1 fb-1/week

Page 127: LHC :  High Luminosity, UFOs and other surprises

What we learned….. Head-on beam-beam effect is not a limitation Long range beam-beam effect has to be taken seriously

• Need separation of 10 -12 σ (otherwise bad lifetime and beam loss) Small as possible emittances are good Established β* reach (aperture, collimation, optics) Luminosity levelling via offset tested – works fine in LHCb! High-intensity operation close to beam instability limits Instabilities were observed and are not fully understood

• for small IP beam offsets while going into collisions, ….• impedances (kicker, collimator heating), collective effects, ...

Availability• Single Event Upsets, vacuum pressure increase, UFOs,

cryogenics, magnet protection system, ..…) – • vigorous follow-up and consolidation

Page 128: LHC :  High Luminosity, UFOs and other surprises

LHC Operation after the shutdown 2013/14

Energy 6.5 TeV during 2015 Bunch spacing 25 ns (in case of problem fall back to 50 ns) Beta-function at experiments ~0.5 m Pile-up of events in the experiments– assume acceptable

• Depends on bunch spacing and squeeze beyond 0.5 m• Beta* luminosity-levelling to mitigate the initial large pile-up

Performance could be impacted by• UFOs at higher energy and with 25 ns buch spacing• Radiation to electronics – SEU’s• Electron cloud & high energy & at 25 ns• Long-range beam-beam & smaller crossing angle & at 25 ns• Single- and bunch-by-bunch beam instabilities (impedances...)

It should be possible to achieve nominal luminosity of 1034 [cm-2s-1] or more

Page 129: LHC :  High Luminosity, UFOs and other surprises

Summary

• In 2012 the peak luminosity exceeded 6x1033 cm-2s-1 in ATLAS and CMS with beams of 50 ns spacing• The stored energy of the beams exceeded by a factor ~50 that of

existing or previous machines• No beam induced magnet quench was observed with stored beams

• Operation in 2012 is at 4.0 TeV • Integrated luminosity for 2012 is in excess of 7 fm-1, hope to

reach 15-20 fm-1 until the end of the run in February 2013• The consolidation of the splices between magnet will be

done in 2013/14 to restart in 2015 at about 6.5 TeV• UFOs could become a limitation for the availability of LHC at

6.5 TeV

Page 130: LHC :  High Luminosity, UFOs and other surprises

Thanks for your attention

Page 131: LHC :  High Luminosity, UFOs and other surprises

Reserve slides

Page 132: LHC :  High Luminosity, UFOs and other surprises

LHC nominal energy is 7 TeV

Why 3.5 TeV in 2011 and 4 TeV in 2012 ?

Page 133: LHC :  High Luminosity, UFOs and other surprises

Accident in 2008

Commissioning of main dipole circuit in last LHC sector: ramp to 9.3 kA (5.5 TeV)

At 8.7 kA an electrical fault developed in a dipole bus bar interconnection between a quadrupole and dipole

Later correlated to a local resistance of ~220 nOhm – nominal value 0.35 nOhm

An electrical arc developed which punctured the helium enclosure and the beam vacuum tube

Secondary arcs developed along the sector Around 400 MJ from a total of 600 MJ were dissipated in

the cold-mass and in electrical arcs Large amounts of helium were released into the insulating

vacuum, in total 6 tons were released

Page 134: LHC :  High Luminosity, UFOs and other surprises

Rupture of high current cable between two magnets

12 kA cable

Page 135: LHC :  High Luminosity, UFOs and other surprises

Pressure inside the cryostats

PTQVQV QV QVQV SVSV

Cold-massVacuum vesselLine ECold support postWarm JackCompensator/BellowsVacuum barrier

Q D D QD D D QD D D QD D D QD

• Self actuating relief valves could not handle the pressure

• designed for 2 kg He/s, incident ~ 20 kg/s• Large forces exerted on the vacuum barriers (every 2

cells, 230 m)• designed for a pressure of 1.5 bar, incident ~ 10 bar• Several quadrupoles displaced by up to ~50 cm• Connections to the cryogenic line damaged in some

places

Page 136: LHC :  High Luminosity, UFOs and other surprises

Incident location

Dipole bus bar

Page 137: LHC :  High Luminosity, UFOs and other surprises

Quadrupole-dipole interconnection (27R3)

Quadrupole support

• 39 dipoles out of 154• 14 quadrupole short straight

sections (SSS) out of 52

…had to be moved to the surface for control, repair or replacement

Collateral damage : displacements

Page 138: LHC :  High Luminosity, UFOs and other surprises

Incident in 2008, caused by a bad splice

Page 139: LHC :  High Luminosity, UFOs and other surprises

4 TeV - limitation of energy

• To reach nominal energy of 7 TeV requires a consolidation campaign of the connections (will take more than one year, requires full warm up of LHC)

• In order to avoid any risk, it was decided to limit the current in the main magnets and therefore the energy to 3.5 TeV for 2010 and 2011, and to 4.0 TeV for 2011

• It turned out that there is still excellent physics at this energy, and it is planned to increase the energy to 6.5 TeV after the consolidation

Page 140: LHC :  High Luminosity, UFOs and other surprises

Risk during a quench of a main dipole

1 qu

ench

/mon

th

If during 2012 the number of high current quenches stays below 5-6 then we have the same probability of burn-out as during 3.5 TeV run in 2011 with 40 quenches

Page 141: LHC :  High Luminosity, UFOs and other surprises

Schematic of the main dipole circuit

Global protection of the busbar and joints between magnetsprotection threshold 1 V (160 V inductive voltage during ramp)

Local (quench) protection of each

magnet

Page 142: LHC :  High Luminosity, UFOs and other surprises

Long Shutdown LS1

2013 – 2014: LS1 consolidate LHC for 6.5 / 7TeV: Measure all splices and repair the defective Consolidate interconnects with new design (clamp, shunt) Finish installation of pressure release valves (DN200) Magnet consolidation Electronics relocation, redesign, etc. to further reduce

SINGLE EVENT EFFECTS on electronics Install collimators with integrated button BPMs (tertiary

collimators and a few secondary collimators)

Extensive parallel consolidation and upgrades of experiments

Page 143: LHC :  High Luminosity, UFOs and other surprises

DN200 – He blow-hole

LHC MB Circuit Splice Consolidation PlansClamping and Shielding