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simulations/results: Synchrotron Radiation and Muons • Motivation and History • Tracking results • Synchrotron Radiation • Tracking of Halo • Muons • News from EUROTeV • Future plans/Summary Grahame Blair Royal Holloway, Univ of London MDI Workshop SLAC January 6 th 2005

BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

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Page 1: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

BDSIM simulations/results: Synchrotron Radiation and Muons

• Motivation and History• Tracking results• Synchrotron Radiation• Tracking of Halo• Muons• News from EUROTeV• Future plans/Summary

Grahame BlairRoyal Holloway, Univ of London

MDI Workshop SLAC

January 6th 2005

Page 2: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

BDS Simulation

~km

CollimationPrecision DiagnosticsDesign

MuonsHaloNeutronsSRLaser-wires …

Full simulations

Page 3: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Motivation and History

• Work dates back several years.• Grew out of initial plans to include Geant processes in Merlin.• Then “fast” tracking incorporated into Geant4.• Now a stand-alone approach and an alternative tracking code.• All Geant4 processes included automatically

Multiple scatteringBremsstrahlung …

• New processes modified (eg new SR, muons, laser-wire ).

Team at RHUL:Ilya Agapov - Optics design, beam diagnosticsJohn Carter - SR, beam diagnostics, IR layoutGB - Collimation, muons, backgroundsChafik Driouichi - Laser-wire design

Page 4: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Overview of Approach

Beam-lines are built up out ofmodular accelerator components

Full simulationof em showers

All secondariestracked

Page 5: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Synchrotron Radiation

Generator of H. BurkhardtImplemented for all componentsBased on local curvatureIndividual photons from individual parents

Primaries and secondaries tracked

Page 6: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

SR within beampipe

Axes scales are m

•J. Carter currently building IR model and simulation.•Interface to Guinea-Pig format for SR of disrupted beam (track reflections back to IR)•Implements low-energy G4 package

Page 7: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

IR

Add any detector IR as a BDSIM object

Ideal for MDI studiesFor various detectors

Page 8: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

SR Absorption along ILC BDSG

eV/m

Exit of Linac IPz (m)

Page 9: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

ILC Beam HaloG

eV/m

z (m)

Collimation efficiencystudies are easy.

Page 10: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Muon ShowersIncrease statistics for Bethe-Heitler by forcing The muons are in addition to the electrons(doesn’t conserve energy)correct spectra via track weighting:

Page 11: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

250 GeV electron on 1m iron

500 GeV electron on 1m iron

e ’s

Page 12: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

TESLA: Muon Trajectories

BDS

Concrete tunnel 2m radius

No offset from centre

View from top

Page 13: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

ILC: Muons at IP

Assume: 10-3 Halo bunch; ie 2.107 halo e’s per bunch Nμ per e ~ 1.4 10-5 , for 500 GeV e- (Bethe-Heitler only)

Adding a cut on initial energy >100 GeV (reduces number of tracked muons by a factor of ~30 withoutaffecting greatly the final results - preliminary)

Muon spoilers have now been implemented in BDSIM as iron cylinders. An optional toroidal magnetic field is also included

Including no spoilers and muon creation at z=1532,Gives approximately 144 muons per bunch at IR.

(Assuming Concrete tunnel of 2m radius.)

Page 14: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Muon Rates at IP

Linac IP624 15329m 18m

Initial z (m) Sp1 (Field/T) Sp2 (Field/T) Rel Flux

1532 1.0

1532 0 0.7

1532 1 0.7

624 0.5

624 0 0 0.2

624 1 1 0.2

624 1 -1 0.1

1981

Muon spoilers

Sp1 Sp2

Page 15: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Halo and Tail Generation (HTGEN)Part of Workpackage WP6 on Integrated Luminosity Performance Studies

• study of potential sources of halo and tail generation• development of analytic models of halo where appropriate• estimation of halo population• development of code modules for halo and tail generation• simulation studies of halo and tail generation• explore possibilities for benchmarking

For H. Burkhardt (CERN)

Page 16: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

There is some (limited) experience from other machines :• halo / tails can be a serious performance limitation• whenever seriously attempted : halo / tails can be quantitatively understood and their production or effects be minimizedFirst steps :• establish a list of all possible candidate processes• collect all existing information and codes• work plan : priorities, what is missing, which framework(s)• up-do-date web based list of processes, literature and code referencesas a very first attempt see

http://hbu.home.cern.ch/hbu/HTGEN.html

close collaboration with related activities and in particular COLSIM and the whole of WP6 (Integrated Luminosity Performance Studies)

Page 17: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Candidate Processes• Particle processes

Beam Gas elastic scatteringinelastic scattering, bremsstrahlungIon or electron-cloud effectsIntrabeam scatteringTouschek scatteringSynchrotron radiation (coherent and incoherent)Scattering off thermal photons

• Optics relatedMismatchCouplingDispersionNon-linearities

• Various, equipment related, collectiveNoise and vibrationDark currentsSpace charge effects close to sourceWake-fields

Page 18: BDSIM simulations/results: Synchrotron Radiation and Muons Motivation and History Tracking results Synchrotron Radiation Tracking of Halo Muons News from

Summary/Future Plans• Accurate accelerator tracking within Geant4 achieved.• Some optimisation still possible.• Code management and public release planned (I. Agapov).

• The code is already at the status of an alternative tracking code.• New processes: SR, Laser-wire, Muon generation• Serious studies of collimation efficiency are now underway• Neutron studies will need some work to gain efficiency

• G4 studies will set the scale for detailed BDS/MDI design.• Need to ensure accurate physics models – low energy gammas,

neutrons, multiple reflections of SR etc. • Will need to improve weighting models etc. for efficiency• BDIR simulation is a significant part of EUROTeV.