B BA
AB
BAR
AR
Beam Background
Beam Background Simulation Simulation
Steven Robertson
2nd Hawaii Super B Factory Workshop April 21, 2005
B A B AR Beam Background Beam Background Simulation Simulation - - PowerPoint PPT Presentation
B A B AR B A B AR Beam Background Beam Background Simulation Simulation Steven Robertson 2 nd Hawaii Super B Factory Workshop April 21, 2005 Motivation Motivation EMC EMC y g r Beam background conditions result in Beam background
Steven Robertson
2nd Hawaii Super B Factory Workshop April 21, 2005
Apr 21, 2005 2 BABAR Beam Background Simulation Steven H. Robertson
Beam background conditions result in detector occupancy, radiation damage and detector occupancy, radiation damage and degradation of data quality degradation of data quality
Background characterization is based on dedicated beam background experiments dedicated beam background experiments
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single and two beam colliding/non-colliding, single and two beam colliding/non-colliding, trickle injection etc. trickle injection etc.
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permit extrapolation to future running conditions permit extrapolation to future running conditions (under assumptions about beam conditions) (under assumptions about beam conditions)
Simulation is needed in order to:
1) 1) Validate and aid interpretation of background data Validate and aid interpretation of background data 2) 2) Identify sources and underlying causes of Identify sources and underlying causes of background background 3) 3) Evaluate sensitivities to specific sources Evaluate sensitivities to specific sources (e.g. details of IR geometry) (e.g. details of IR geometry) 4) 4) Evaluate effects of future upgrades on bg rates Evaluate effects of future upgrades on bg rates
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Extrapolate to Super-B ? Extrapolate to Super-B ?
#
c r y s t a l s w i t h s i g n i f i c a n t e n e r g y
L L = 3.3x10
= 3.3x1034
34 cm
cm-2
s-1
Apr 21, 2005 3 BABAR Beam Background Simulation Steven H. Robertson
Recent effort to simulate two of the dominant contributions to observed subdetector background rates subdetector background rates
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“ “Lost-particle Lost-particle” single beam backgrounds produced by bremmstrahlung or Coulumb ” single beam backgrounds produced by bremmstrahlung or Coulumb scattering of primary beam particles from beam gas scattering of primary beam particles from beam gas
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“ “Luminosity Luminosity” backgrounds associated with small-angle radiative bhabha events in ” backgrounds associated with small-angle radiative bhabha events in which electron/positron strikes machine elements outside of nominal BABAR fiducial which electron/positron strikes machine elements outside of nominal BABAR fiducial acceptance acceptance
– machine lattice & apertures (TURTLE) - T. Feiguth, R. Barlow – Geant 4 IR geometry, materials model - M. Bonioli, G.Calderini – Geant 4 IR magnetic field model - G. Bower – small angle bhabha generators - B. Lockman, D. Strom, N. Blount – e/gamma – nuclear physics modeling - D. Wright – study and interpretation of results - subdetector groups
Apr 21, 2005 4 BABAR Beam Background Simulation Steven H. Robertson
Apr 21, 2005 5 BABAR Beam Background Simulation Steven H. Robertson
Magbends
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propagates charged particles through magnetic fields propagates charged particles through magnetic fields
Decay Turtle
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Transport of Coulomb and bremsstrahlung final state particles to vicinity of IR Transport of Coulomb and bremsstrahlung final state particles to vicinity of IR
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Modeling of beam phase space and beam tails Modeling of beam phase space and beam tails
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Knowledge of apertures and assumptions regarding vaccuum pressure profile Knowledge of apertures and assumptions regarding vaccuum pressure profile
Geant4
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Full modeling of materials and magnetic fields in vicinity of IR (+/- 8m) Full modeling of materials and magnetic fields in vicinity of IR (+/- 8m)
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Contains physics of particle interactions, detector materials and response Contains physics of particle interactions, detector materials and response
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Can be used as stand-alone simulation of physics processes (e.g. Bhabha) or Can be used as stand-alone simulation of physics processes (e.g. Bhabha) or using Turtle rays as input using Turtle rays as input
Data
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Impact of background occupancy in data “modeled” in BABAR physics Monte Impact of background occupancy in data “modeled” in BABAR physics Monte Carlo from cyclic triggers in data Carlo from cyclic triggers in data
Apr 21, 2005 6 BABAR Beam Background Simulation Steven H. Robertson
– Magbends model suggests that most radiative Bhabha daughters hit machine
elements further from the IP
– however, radiative Bhabha daughters still hit in the vicinity of Belle detector so still
surprising that NO lumi term is observed, particularily if neutrons contribute...
3 2.5 2 1.5 1 0.5
LER Radiative Bhabhas
2.5 5 7.5 10 20 30
m cm
3.1 GeV 3.1 GeV 9 GeV 9 GeV
Apr 21, 2005 7 BABAR Beam Background Simulation Steven H. Robertson
IP Normalized to:
IP
Coulomb scattering in Arcs (y- plane) e- Brems- strahlung in last 26 m (x-plane)
Vacuum pipe / mask apertures
Apr 21, 2005 8 BABAR Beam Background Simulation Steven H. Robertson
Most subdetector background occupancies are due to flux of low energy secondary particles rather than primary electrons/positrons energy secondary particles rather than primary electrons/positrons from bhabhas or beam particles from bhabhas or beam particles
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EM shower fragments or neutrons from primary particle hits in various EM shower fragments or neutrons from primary particle hits in various machine elements machine elements
Need full geometry+magnetic fields+materials+interactions for IR
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previously only B1 & Q1 geometry were modeled, but no magnetic fields previously only B1 & Q1 geometry were modeled, but no magnetic fields
Apr 21, 2005 9 BABAR Beam Background Simulation Steven H. Robertson
– Studies for BABAR TDR and predicted to be a possible background source – Observed in data in ~2000; currently a dominant background source – Recently, significant interest in simulation
Mike Sullivan
Apr 21, 2005 10 BABAR Beam Background Simulation Steven H. Robertson
In absence the of complete magnetic field model in GEANT4, TURTLE model has been used to simulate radiative bhabha backgrounds model has been used to simulate radiative bhabha backgrounds
Use magnetic field and machine aperture definitions from TURTLE decks
Yields information on primary particle impact point but no information on secondaries (i.e neutrons, EM showers) secondaries (i.e neutrons, EM showers)
photons electrons
HER radiative bhabhas
Achille Stochi & Patrick Roudeau
(bbbrem) to obtain particle trajectories and energy flux through beamline elements
– Results recently updated using new
HER/LER Turtle decks including BABAR solenoid
“Golden orbit”
Apr 21, 2005 11 BABAR Beam Background Simulation Steven H. Robertson
from “Magbends” accelerator magnetic field model
section and total energy flux through beamline elements:
3 2.5 2 1.5 1 0.5
LER Radiative Bhabhas
2.5 5 7.5 10 20 30
m cm
3 . 1 G e V 3 . 1 G e V 9 GeV 9 GeV
13.5 50 117 27.7 2.5 E x σ (mb GeV) 5.2 2.8<Z 20. 2.2<Z<2.8 56.7 1.4<Z<2.2 26.4 .8<Z<1.4 9.2 <.8 σ (mb) Z range (m)
Q1 Q2
Apr 21, 2005 12 BABAR Beam Background Simulation Steven H. Robertson
Off energy electrons Off energy positrons
(“BrmBbbrem”)
– Working on including BHLUMI generator as well
crossection info) yield results consistent with magbends/turtle:
Ben Campbell, McGill
Apr 21, 2005 13 BABAR Beam Background Simulation Steven H. Robertson
BF3 counter installed on forward Q4 magnet
but not single beam running
source believed to be due to radiative Bhabhas striking in vicinity of Q2 septum
– Do neutrons interact in detector?
– Can (in principle) be simulated using full
Geant4 with e/ - nuclear processes
– Neutron detectors added to Geant4
detector model
Apr 21, 2005 14 BABAR Beam Background Simulation Steven H. Robertson
physics processes included for the first time in BABAR simulation
– Results in production of additional
low-energy (0-20 MeV) particles
– Important for EMC (?)
in test releases for study of thermalized neutrons produced by beam backgrounds
– Will be included in future production
releases with enable/disable switch (off by default!)
Neutron kinetic energy (MeV) 1 ms Dennis Wright
Neutron TOF (0.025 eV cutoff)
Apr 21, 2005 15 BABAR Beam Background Simulation Steven H. Robertson
– Q2 septum geometry incomplete and Q5 magnets still missing – Magnetic fields believed to be correct
– Comparison of TURTLE/GEANT particle trajectories and impact positions – Large scale production of TURTLE lost-particle events
– Study of sources and rates
– Study of luminosity backgrounds
Apr 21, 2005 16 BABAR Beam Background Simulation Steven H. Robertson
– Well understood and not significant (by design!) in current IR
– Well characterized in data, simulated with Turtle – Also inelastic beam-gas / beam-wall contribution to L1 trigger rate
– Contribution to background rates not well understood
– Well measured, but not well understood (neutrons?)
– mechanism understood, measured in data
– Characterized from data and not currently problematic
Apr 21, 2005 17 BABAR Beam Background Simulation Steven H. Robertson
Synchrotron radiation
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Magbends studies for IR upgrades Magbends studies for IR upgrades
Beam-beam collimation
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affects orbit of outgoing beam particles; collimate downstream? affects orbit of outgoing beam particles; collimate downstream?
Beam gas Coulomb scattering and bremsstrahlung
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Turtle and Turtle/Geant4 Turtle and Turtle/Geant4
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similar to ~2000 era studies but with upgraded simulation tools similar to ~2000 era studies but with upgraded simulation tools
Radiative Bhabha (“luminosity”) background
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Separate Magbends, Turtle and Geant4 studies in progress Separate Magbends, Turtle and Geant4 studies in progress
use fields & apertures in Turtle to study trajectories of charged particles
(but need extended beamline geomerty!) (but need extended beamline geomerty!)
Questions:
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Where are primary particles produced and where do they go? Where are primary particles produced and where do they go?
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Secondaries, neutrons and potential for shielding? Secondaries, neutrons and potential for shielding?
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Effect of “2005 IR upgrade”, Super-B IR etc... Effect of “2005 IR upgrade”, Super-B IR etc...
Apr 21, 2005 18 BABAR Beam Background Simulation Steven H. Robertson
– No primary synchrotron radiation background seen in BABAR detector – Relevent for heating etc. of machine elements in the vicinity of IR
Apr 21, 2005 19 BABAR Beam Background Simulation Steven H. Robertson
Recently, a substantial effort has been made to expand Geant4 has been made to expand Geant4 simulation to include beamline geometry simulation to include beamline geometry
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Include also various background sensors Include also various background sensors (pin diodes, diamond, quartz and CsI) (pin diodes, diamond, quartz and CsI)
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Modeling of magnetic fields (incl. Solenoid) and validation Modeling of magnetic fields (incl. Solenoid) and validation against Magbends & Turtle against Magbends & Turtle
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Significant improvements in geometry and materials Significant improvements in geometry and materials modeling compared to old Geant3 version modeling compared to old Geant3 version
Proceeding concurrently with updating of HER & updating of HER & LER LER Turtle Turtle decks decks
Apr 21, 2005 20 BABAR Beam Background Simulation Steven H. Robertson
Challenging geometry! – problems with G4 representation (M. Bondioli and G. Calderini)
(M. Bondioli and G. Calderini)
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(Almost) complete model out to Q5 magnets (Almost) complete model out to Q5 magnets
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Final checks of geometry in progress (overlapping Geant volumes etc) Final checks of geometry in progress (overlapping Geant volumes etc)
Magnetic field modeling (G. Bower)
(G. Bower)
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Validated against Magbends/Turtle Validated against Magbends/Turtle
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Technical issues tracking particles through a varying field (“resolved”) Technical issues tracking particles through a varying field (“resolved”)
– extended model runs ~10x
slower than nominal detector model
– Sources outside of +/-10m? Do
we need additional beam elements?
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 21
X (mm)
Zone 1
X (mm)
Zone 2 Zone 3
X (mm)
Bremmsstrahlung in field-free region Bremmsstrahlung Bremmsstrahlung
“zones” are empirically defined based on observation that lost particles zones” are empirically defined based on observation that lost particles from different regions have differing characteristics: from different regions have differing characteristics:
LER Zone Range (m) 0 -4, 4 1 4, 10 2 10, 21 3 21, 36 4 36, 62 5 62, 2196 HER Zone Range (m) 0 -4, 4 1 -4, -26 2 -26, -42 3 -42, -66 4 -66, -2196
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 22
X (mm)
Zone 1 Zone 3
X (mm)
Bremmsstrahlung in field-free region Bremmsstrahlung
Simulates production and propagation of Bremsstrahlung and Coulomb scattered Bremsstrahlung and Coulomb scattered primary beam particles through PEP-II primary beam particles through PEP-II magnet lattice magnet lattice
gives rates and impact point of particles in vicinity of IR vicinity of IR
requires knowledge of vacuum profile in the rings (particularily incoming HER and LER rings (particularily incoming HER and LER straights near the IR) straights near the IR)
Effort in progress to update TURTLE magnet and aperture descriptions magnet and aperture descriptions
not updated since 1998 (commissioning run!)
LER optics done but apertures still to come
HER optics (essentially) done, aperture description is available but not yet description is available but not yet implemented implemented
T.Feiguth, R.Barlow
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 23
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 24
Updated HER deck to 2004 configuration
Aperture and orbit checks performed
LER deck update still in progress
Coulomb scattering in HER (2004 configuration):
Scattered e- impact point Scattered e- production zone
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 25
bremsstrahlung and Coulomb scatter events generated scatter events generated uniformly around ring assuming a uniformly around ring assuming a flat 1nTorr pressure profile flat 1nTorr pressure profile
Reweight to “known” profile to get absolute predictions absolute predictions
Record location, energy etc of primary particles hitting in vicinity primary particles hitting in vicinity
Useful information about impact regions and background sensitivities regions and background sensitivities to regions of the rings: to regions of the rings:
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 26
Used during commissioning phase and first few years of running
Modeled BABAR detector and beam line out to Q5 (+/- 8m from IR)
Turtle ray input to allow lost particle background studies
Some known issues with beamline geometry, fields and material model
“Replaced” by Geant4 detector simulation in ~2002 Replaced” by Geant4 detector simulation in ~2002
Beamline simulation only out to ~Q2 !
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 27
Chih-Hsiang Cheng
SVT pin-diode simulation studies SVT pin-diode simulation studies
G-hit based study using Turtle rays as input to Geant-3 pin-diode detector input to Geant-3 pin-diode detector model model
Used during initial PEP-II commissioning and early data taking phases of BABAR and early data taking phases of BABAR
Predictions for SVT background sensitivities to HER and LER zones sensitivities to HER and LER zones
Some diodes appeared to be better modeled than others, but overall modeled than others, but overall agreement with data to within a factor ~2.5 agreement with data to within a factor ~2.5
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 28
4-vectors of Turtle rays which strike apertures near IP are recorded at a point ~8m upstream, then passed to Geant upstream, then passed to Geant
Geant propagates particle into IR and simulates interactions in beampipe/detector material material
permits identification of turtle rays which produce activity (e.g. from secondary particles in specific detector elements particles in specific detector elements
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 29
Extrapolate simulated lost- particle induced detector particle induced detector
measured (or assumed) vacuum measured (or assumed) vacuum profile profile
Once appropriate backgrounds data was available, this was done data was available, this was done using data instead using data instead
Full detector response to backgrounds can be simulated backgrounds can be simulated to obtain “reconstructed” to obtain “reconstructed” information e.g. clusters, tracks information e.g. clusters, tracks and even triggers and even triggers
April 21, 2005 BBBTF Steven H. Robertson McGill University, Institute of Particle Physics 30
RadFET calorimeter radiation monitoring gives integrated dose in monitoring gives integrated dose in various regions of the EMC various regions of the EMC
Not necessarily representative of dose in individual crystals individual crystals
Total radiation dose estimated by integrating estimated flux rate from integrating estimated flux rate from simulation simulation
Assume pressure profile
Reasonable agreement with RadFET data (~30%) (~30%)
Interesting features!
simulation predicted region of reduced dose in forward barrel (naively expected dose in forward barrel (naively expected to be high dose) to be high dose)
RadFET Data