LIMITS: SPACE CHARGE Dr. Cristhian Alfonso Valerio Lizrraga - - PowerPoint PPT Presentation

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LIMITS: SPACE CHARGE Dr. Cristhian Alfonso Valerio Lizrraga - - PowerPoint PPT Presentation

1 11/6/15 XV Mexican Workshop on Particles and Fields XV MEXICAN WORKSHOP ON PARTICLES AND FIELDS RING INJECTORS LUMINOSITY LIMITS: SPACE CHARGE Dr. Cristhian Alfonso Valerio Lizrraga Facultad de ciencias Fsico matemticas Universidad


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SLIDE 1

RING INJECTORS LUMINOSITY LIMITS: SPACE CHARGE

  • Dr. Cristhian Alfonso Valerio Lizárraga

Facultad de ciencias Físico matemáticas Universidad Autónoma de Sinaloa Mazatlán, México.

11/6/15 XV Mexican Workshop on Particles and Fields

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XV MEXICAN WORKSHOP ON PARTICLES AND FIELDS

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SLIDE 2

L = Nb

2kbγ f

4πβ

*εn

F

Beam parameters

The luminosity is a famous parameter in detectors …

11/6/15 XV Mexican Workshop on Particles and Fields

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Nb Number of particles per bunch Kb Number of bunches per beam β* Beta function γ Relativistic factor εn Normalized emittance BR Branching Ratio f collision frequency LHC Luminosity from 1033 to 1034 cm-2 s-1 Tevatron Max Luminosity 1032 cm-2 s-1

Ldel = t < L > barn

−1

Nevent = BRσ Ldel

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SLIDE 3

L = Nb

2kbγ f

4πβ

*εn

F

Beam parameters

The luminosity is a famous parameter in detectors …

11/6/15 XV Mexican Workshop on Particles and Fields

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LHC Luminosity from 1033 to 1034 cm-2 s-1 Tevatron Max Luminosity 1032 cm-2 s-1

Ldel = t < L > barn

−1

Nevent = BRσ Ldel

  • A good luminosity is the difference between wait 1 o 10 years!

There is a group in Guanajuato working in this parameter Two Mexicans working here

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SLIDE 4

Electron cloud issues in the LHC

Humberto Maury – Universidad de Guanajuato Gerardo Guillermo - CINVESTAV

  • Electron cloud: a set of electrons created inside the LHC

vacuum chamber by ionization of the residual gas or by photoemission due to beam-induced synchrotron

  • radiation. It can affect the accelerator performance and
  • r degraded beam quality.
  • Effects:
  • pressure increase by several orders of magnitude.
  • Beam instabilities
  • Additional heat load to the cryogenic system.

L = Nb

2kbγ f

4πβ

*εn

F

XV Mexican Workshop on Particles and Fields

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SLIDE 5

Space charge

Ø Coulomb´s force separate the same charge particles from

each other

Ø High intensity beams suffer from instabilities due severe

space charge problems

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I = qeNb t

L = Nb

2kbγ f

4πβ

*εn

F

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SLIDE 6

Beam space charge

11/6/15 XV Mexican Workshop on Particles and Fields

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) ( B v E q F × + =

F = q(E − vβE c )

= q(E − β 2E) = q E γ 2

Er = ρr 2ε0

Consider a longitudinally cylindrical beam with constant charge density ρ and current I. The magnetic field creates an

  • pposite force to the electric field

J = I πa2 Bθ = µ0Jr 2 = µ0Ir 2πa2 = βEr c

I ρ

Energy γ (protons) γ (electrons) 45Kev 1.00004 1.088 50 Mev 1.05328 98.084 160 MeV 1.17052 314.112 1 Gev 2.06574 1957.145 1 TeV 1066.7889 1956952.375

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SLIDE 7

Emittance

  • The region in phase space that the particles in a beam
  • ccupy is called the beam emittance
  • Mm.mrad? mrad from px/pz
  • The goal in every accelerator is to have the lower beam

emittance achievable

11/6/15 XV Mexican Workshop on Particles and Fields

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ε = r 2c kT m ∝T1/2

Brighness∝ 1 εyεx

The emittance always get worse(only by losing particles can get better)

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SLIDE 8

Fermilab Accelerator Complex

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[1] http://www.fnal.gov/

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SLIDE 9

Cern Accelerator complex

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Lina nac 4 4

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SLIDE 10

Why we need Linacs before the Rings?

  • The space charge

limits the beam intensity inside the ring

11/6/15 XV Mexican Workshop on Particles and Fields

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ΔQ ∝ Nb εnβγ 2

[1] CERN Courier, Sep 2012.

PS BOOSTER Tune shift using Linac2.

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SLIDE 11

Linac 4 vs Linac2

11/6/15 XV Mexican Workshop on Particles and Fields

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u H- Beam u 160 Mev u Lower Emittance than Linac2

Linac 4 Linac 2

Ions H- P Energy 160 MeV 50 MeV Emittance 0.4 mm mrad 1 mm mrad Frequency 352.2 MHz 202.56 MHz Beam Current 40 mA 170 mA. Pulse Lenght 400 us 100 us

Source LEBT

ΔQ ∝ Nb εnβγ 2

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SLIDE 12

Why H-?

  • Because the

Space charge repulsion is easier to insert a negative beam inside a positive beam

  • In therory the

efficiency will be 99% in transform the H- in to protons

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[1] CERN Courier, Sep 2012.

Schematic of H- injection into a circular machine.

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SLIDE 13

PSB Emittance

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0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 100 200 300 400 1-s norm. emittance [mm mrad]

PSB bunch intensity [E10]

  • LHC beams

Brightness out

  • f the PSB are

mainly determined by space charge during the injection process

  • G. Romulo Space charge meeting CERN, 19 March, 2015

By inject H- the emittance after the injection will be reduced by half

Present PSB performance for LHC beam production (measurements) PSB performance with Linac4 for LHC beam production

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SLIDE 14

Where the particles are created?

Ø The maximum Nb will be at

the beam source output

Ø After been created the

value C will be almost constant

Ø As we get closer to the ion

source more physics need to be included in simulations to predict results

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C ∝ Nb εn

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SLIDE 15

Source and Beam Extraction

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The beam energy is calculated by the diference of potential

) (

ground source

V V q E − =

The beam is formed by the particles in the plasma taken by the extractor Plasma extraction potential (meniscus) Child–Langmuir law

A plasma or discharge chamber Material input Power to create a plasma / discharge A hole to let the ions out! An extraction system

Ion Beam Plasma Ground Extracto r Potential lines(green) Electrodes (blue) Ions (Red)

j = 4ε0 9 2e m V 3/2 d 2

XV Mexican Workshop on Particles and Fields

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SLIDE 16

Beam transport under Space charge

  • The envelope of a cylindrically symmetric beam (r)

transported along the z-axis can be described by the differential equation:

Ø ko is the focusing strength Ø K0 is the space charge term

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ko1 k02 k03

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SLIDE 17

Beam transport simulations

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u Envelope code where a set of matrix represent

the magnets in the accelerator

u They are really fast(to obtain the solution it

takes a few seconds), and can cover all the accelerator chain in a normal computer without problem

X = RY = R(n)...R(2)R(1)Y

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SLIDE 18

Ray tracing codes

  • 250
  • 200
  • 150
  • 100
  • 50

0.5 1 1.5 Beam Potential (volts) (m) Solve ∇2φ=0

Calculate trajectories and Beam Charge Density ρB

Solve ∇2φ=ρ

Converge

No yes

Stop

u Is more accurate but the simulation time and resource

consumption is higher

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SLIDE 19

Space charge compensation

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Full space charge beam transport 80% compensation Beam Direction Ø The vacuum is not perfect inside the beam pipe Ø Range of pressure from 5x10-7 mbar 1x10-5 mbar Ø The beam ionizes residual gas atoms Ø The ionized particles from opposite charge are trapped by the beam potential and same charge particles are expelled to the walls Ions(Red) Potential lines (Green)

ρ = ρbeam −ρsecondary

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SLIDE 20

Compensation time

  • The space charge

compensation is time dependent

  • Beam pulse 500 µs
  • Baseline 1x10-6 mbar

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The beam properties are not constant in time and is necessary to use advanced codes to simulate this effect.

τ = 1 vb(σ H 2(E)nH 2 +σ x(E)nx)

20 40 60 80 100 200 400 600 RFQ Transmission %

Time(µs)

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Linac4 Low energy beam Transport (LEBT)

Ø Source Ø Multi step

extraction system

Ø LEBT Ø RFQ

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SLIDE 22

Linac4 LEBT elements

The system include:

  • 2XSolenoid
  • Beam focusing
  • Matching
  • 4XSteerers
  • Correct beam center alignment
  • Gas Injection
  • Controlling space charge

compensation degree

  • Faraday Cup
  • Beam current measurement
  • The beam is unbunched in this

stage.

  • Solenoid Effect in the beam

0 0.5 1.0 Z(m) 1.5 2.0 0.05 0.05

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Ions (red) Conductors (blue)

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SLIDE 23

Linac4 Ion Source and extraction system

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  • Electrons (yellow) are extracted along with negative ions (red).

0kV 20kV 10kV 45kV

  • Plasma is created using 2MHz RF in a

solenoid coil.

  • The H- is produced in the plasma

volume and surfaces

  • A surface near the extraction is coated

with cesium, evaporated from an oven at the back of the source.

  • The plasma ions strike the cesium

surface and H- are emitted.

35kV

Oystein middtun

0kV

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SLIDE 24

Linac4 source simulation using Ray tracing code

Ø Beam Current 35 mA Simulation Measurements

  • 30 -15 0 15 30

X(mm) Emittance mm.mrad 1 rms (norm) : 0.29 0.55 The absolute value of the emittance is almost 200% bigger in measurements

XV Mexican Workshop on Particles and Fields

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SLIDE 25

Particle in Cell codes (PIC)

Secondary ions density Beam density

u The interaction between the beam and the residual

gas inside the vacuum pipe generates secondary ions

u The secondary ions play a major role in the beam

transport

u To simulate 1 meter the simulation time goes from 1

day to 3 months

XV Mexican Workshop on Particles and Fields

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SLIDE 26

Space Charge compensation using H2

Ø Pressure 1.2X10-6 mbar Ø Current 35 mA Simulation Measurements

X(mm)

  • 30 -15 0 15 30
  • 30 -15 0 15 30
  • 30 -15 0 15 30

x’(mrad) x’(mrad) x’(mrad) X(mm) 100 µs 260 µs 400 µs

  • 30 -15 0 15 30
  • 30 -15 0 15 30
  • 30 -15 0 15 30

XV Mexican Workshop on Particles and Fields

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Compensation using different gases

Ø H2 N2 and Kr Ø Several pressures were used Simulation Measurements

X(mm)

  • 30 -15 0 15 30
  • 30 -15 0 15 30
  • 30 -15 0 15 30

x’(mrad) x’(mrad) x’(mrad) X(mm) H2

  • 30 -15 0 15

30

  • 30 -15 0 15 30
  • 30 -15 0 15

30

Kr N2

XV Mexican Workshop on Particles and Fields

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SLIDE 28

Summary

The beam space charge in the injectors is one of the biggest challenge to reach a higher luminosity in beam colliders At CERN, Linac4 is under construction to mitigate this problem and duplicate the Luminosity. The goal of produce 80 mA in the Linac4 source continue to be a problem A new method to take into account secondary ions created by the beam has been developed The simulation results from the Linac4 beam source agree with the measurements like not other code available today. Some improvements has been made to the beam source at linac4 thanks to the results of the simulations

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SLIDE 29

Thank you!

Disfruten la playa

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Acknowledgement Richard Scrivens Ildefonso León Guillermo Contreras

CONACYT

And the Linac4 collaboration