Physics III: Cuts, Decay and Optical Physics Geant4 Tutorial at Jefferson Lab 10 July 2012 Dennis Wright (SLAC) Geant4 9.6 beta.

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Presentation transcript:

Physics III: Cuts, Decay and Optical Physics Geant4 Tutorial at Jefferson Lab 10 July 2012 Dennis Wright (SLAC) Geant4 9.6 beta

Outline Production Thresholds (aka cuts) Cuts per Region The Decay Process – applicability – available decay modes Optical Photons – available processes 2

Threshold for Secondary Production Every simulation developer must answer the question: how low can you go? – at what energy do I stop tracking particles? This is a balancing act: – need to go low enough to get the physics you’re interested in – can’t go too low because some processes have infrared divergence causing CPU to skyrocket The traditional Monte Carlo solution is to impose an absolute cutoff in energy – particles are stopped when this energy is reached – remaining energy is dumped at that point 3

Threshold for Secondary Production But, such a cut may cause imprecise stopping location and deposition of energy There is also a particle dependence – range of a 10 keV  in Si is a few cm – range of a 10 keV e- in Si is a few microns And a material dependence – suppose you have a detector made of alternating sheets of Pb and plastic scintillator – if the cutoff is OK for Pb it will likely be wrong for the scintillator which does the actual energy measurement 4

Threshold for Secondary Production Geant4 solution: impose a production threshold this threshold is a distance, not an energy default = 1 mm the primary particle loses energy by producing secondary electrons or gammas if primary no longer has enough energy to produce secondaries which travel at least 1 mm, two things happen: discrete energy loss ceases (no more secondaries produced) the primary is tracked down to zero energy using continuous energy loss Stopping location is therefore correct Only one value of production threshold distance is needed for all materials because it corresponds to different energies depending on material 5

Production Threshold vs. Energy Cut Example: 500 MeV p in LAr-Pb Sampling Calorimeter Geant3 (and others) Geant4 Production range = 1.5 mm 6

Threshold for Secondary Production Geant4 recommends the default value of 1 mm – user needs to decide the best value – this will depend on the size and sensitive elements within the simulated detector, and on available CPU This value is set in the SetCuts() method of your physics list Instead of “secondary production threshold distance” it is more convenient to simply say “cuts” – but please remember that this does not mean that any particle is actually stopped before it runs out of energy 7

Cuts per Region In a complex detector there may be many different types of sub-detectors involving – finely segmented volumes – very sensitive materials – large, undivided volumes – inert materials The same value of the secondary production threshold may not be appropriate for all of these – user must define regions of similar sensitivity and granularity and assign a different set of production thresholds (cuts) for each Warning: this feature is for users who are simulating the most complex detectors experienced at simulating EM showers in matter 8

Cuts per Region A default region is created automatically for the world volume – it has the cuts which you set in SetCuts() in your physics list – these will be used everywhere except for user-defined regions To define a special region with different cuts, user must – create a G4ProductionCuts object – initialize it with the the new cuts – assign it to a region which has already been created 9

Cuts per Region void BeamTestPhysicsList::SetCuts() { SetCutValue(defaultCutValue, “gamma”); // same for e-, e+, p // Get the region G4Region* aRegion = G4RegionStore::GetInstance()->GetRegion(“RegionA”); // Define cuts object for the new region and set values G4ProductionCuts* cuts = new G4ProductionCuts(); cuts->SetProductionCut(0.01*mm); // here, same for all // Assign cuts to region aRegion-> SetProductionCuts(cuts); } 10

The Decay Process Derived from G4VRestDiscreteProcess decay can happen in-flight or at rest Should be applied to all unstable, long-lived particles Different from other physical processes: mean free path for most processes: = N   /A for decay in flight: =   c  Same decay process is used for all eligible particles decay process retrieves branching ratios and decay modes from decay table stored for each particle type 11

Available Decay Modes Phase space: 2-body:  0    3-body: K 0 L   0  +  - many body Dalitz: P 0   l + l - Muon and tau decay V – A, no radiative corrections, mono-energetic neutrinos Semi-leptonic K decay K   l 12

Pre-assigned Decays Geant4 provides decay modes for long-lived particles user can re-define decay channels if necessary But decay modes for short-lived (e.g. heavy flavor) particles not provided by Geant4 user must “pre-assign” to particle: proper lifetime decay modes decay products decay process can invoke decay handler from external generator must use G4ExtDecayer interface Take care the pre-assigned decays from generators do not overlap with those defined by Geant4 (K 0 S, , e.g.) 13

Specialized Decay Processes G4DecayWithSpin produces Michel electron/positron spectrum with 1 st order radiative corrections initial muon spin is required propagates spin in magnetic field (precession) over remainder of muon lifetime G4UnknownDecay only for not yet discovered particles (Higgs, SUSY, etc.) discrete process – only in-flight decays allowed pre-assigned decay channels must be supplied by user or generator 14

Optical Photons Technically, should belong to electromagnetic category, but: optical photon wavelength is >> atomic spacing treated as waves  no smooth transition between optical and gamma particle classes Optical photons are produced by the following Geant4 processes: G4Cerenkov G4Scintillation G4TransitionRadiation Warning: these processes generate optical photons without energy conservation 15

Optical Photons Optical photons undergo: Rayleigh scattering refraction and reflection at medium boundaries bulk absorption wavelength shifting Geant4 keeps track of polarization but not overall phase  no interference Optical properties can be specified in G4Material reflectivity, transmission efficiency, dielectric constants, surface properties Photon spectrum properties also defined in G4Material scintillation yield, time structure (fast, slow components) 16

Optical Photons Geant4 demands particle- like behavior for tracking: thus, no “splitting” event with both refraction and reflection must be simulated by at least two events 17

Wavelength Shifting Handled by G4OpWLS initial photon is killed, one with new wavelength is created builds its own physics table for mean free path User must supply: absorption length as function of photon energy emission spectra parameters as function of energy time delay between absorption and re-emission 18

Boundary Interactions Handled by G4OpBoundaryProcess refraction reflection User must supply surface properties using G4OpticalSurfaceModel Boundary properties: – dielectric-dielectris – dielectric-metal – dielectric-black material Surface properties: – polished – ground – front- or back-painted, … 19

Absorption and Rayleigh Scattering G4OpAbsorption uses photon attenuation length from material properties to get mean free path photon is simply killed after a selected path length G4OpRayleigh elastic scattering including polarization of initial and final photons builds its own physics table (for mean free path) using G4MaterialTable may only be used for optical photons (a different process provided for gammas) 20

Summary The precision of particle stopping and the production of secondary particles are determined by a secondary production threshold For complex detectors with different types of sensitive volumes, different production thresholds may be defined for different regions within the detector These is only one decay process for all long-lived, unstable particles Optical processes handle the reflection, refraction, absorption and wavelength shifting of long-wavelength photons 21