event analysis for the gamma-ray large area space telescope robin morris, riacs johann cohen-tanugi...
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![Page 1: Event Analysis for the Gamma-ray Large Area Space Telescope Robin Morris, RIACS Johann Cohen-Tanugi INFN, Pisa](https://reader036.vdocuments.net/reader036/viewer/2022062320/56649d785503460f94a5a448/html5/thumbnails/1.jpg)
Event Analysis for the Gamma-ray Large Area
Space Telescope
Robin Morris, RIACS
Johann Cohen-Tanugi INFN, Pisa
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Why study gamma-rays?• Gamma-rays are produced by some of the highest energy
events in the universe, events that are not yet fully understood.
• Study of these events is critical to understanding the origins and evolution of the universe.
• The distribution of gamma-rays (both across the sky and in terms of energy) can confirm theories about the early universe.
• The Large Area Telescope is designed to map the incidence of gamma-rays.
• We are developing a Bayesian methodology for the analysis of the instrument response.
(background - distribution of gamma-rays from EGRET)
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The Large Area Telescope (LAT)
• For each incident gamma ray photon, we want to know its incident direction and energy
• The LAT has three components:– Anticoincidence detector -
eliminates responses due to incident charged particles
– Array of conversion towers - the heart of the detector
– Imaging calorimeter - measures the residual energy in the particles generated by an incident gamma ray photon
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How the conversion towers work• Alternating conversion and
detection layers• Incident gamma rays are
converted into electron/positron pairs
• The electron and positron cascade through the detector– Undergo secondary scattering– Produce further electrons and
photons
• Each time they cross a detection layer, they trigger the silicon microstrip detectors, producing a readout
• The output from an event is a set of (x,y,z) positions of the silicon microstrips that were triggered (+ calorimeter response)
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Examples (from the GLEAM simulator)
200MeV photon• blue line - incident photon and
electron/positron• orange - microstrip detectors• blue cubes - calorimeter• green - anticoincidence detector
points to note:• inherent ambiguity in the number of
particles at each layer• significant secondary scattering• production of secondary electrons
(hits to left of main track)• anticoincidence detector fired by
secondary electrons• opening angle depends on energy
GLEAM - GLAST Event Analysis Machine
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Examples (from the GLEAM simulator)
100GeV photon
• secondary photons are suppressed in the figure (to enable the secondary electron tracks to be seen)
• very small opening angle• huge number of secondary
electrons (black “cloud”)• lots of firing from the secondary
electrons• firings well away from the main
track (from secondary photons converted into charged particles)
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Physics ProcessesPair production• conversion of gamma ray photons into
electron/positron pairs
multiple coulomb scattering• charged particles are deflected on interacting
with (primarily) atoms
positron anihilation• positron + electron => photons
ionisation• liberation of electrons from atoms by the transfer
of (at least) the binding energy from a particle to the electron
bremsstrahlung• radiation emitted by a charged particle undergoing acceleration (typically deceleration when passing through the field of atomic nuclei)
photoelectric effect• ejection of electrons from the surface of material by incident photons
compton scattering• transfer of energy from photons to electrons; may liberate bound electrons
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Pair Production - energy and angles
• The tungsten conversion foils are 0.105mm thick, resulting in a conversion probability of ~2% for photons of 1GeV
• The lowest 4 foils are 0.723mm thick (~10% conversion probability)
• Compromise between pair production and multiple scattering and other physics processes that hide the primary event
• The energy of the incident photon is divided between the electron and positron
• The electron/positron angle depends stochastically on the electron/positron energy
photonE
electron
Ee
positron
Ep
e
p
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Pair Production - energy and angles
• Distribution of energy split between electron and positron as a function of photon energy
• Distribution of electron/positron angle
where u is distributed as above
€
φ±=mec
2
E±
u
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Other electron/positron processes
Currently we include
multiple scattering ionisation bremsstrahlung
Using the Geant4 physics simulation toolkit, we simulate the interaction of electrons with the tungsten foils, and estimate the scattering distributions
Apart from the tails, the distribution can be approximated by a gamma distribution
We currently neglect other physics processes/particles
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Simplified Simulation
Using the physics distributions described so far, we implemented a simulation of the detector• uses the LAT geometry• only includes the primary electron and positron• doesn’t include energy deposition by particles as they pass through matter
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Over-simplified Simulation
• Reduce the detector to 2D• Keep the physical distributions
–conversion–energy distribution–opening angle–scattering distributions
- neglect all other physics processes
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Probabilistic event analysis
Incorporate data one layer at a time:
• p()
• p( | d1) p(d1 | )p()
• p( | d1,d2) p(d2 | )p(d1 | )p()
• p( | d1,d2,…dN)
p(dN | )p(dN-1 | ) … p(d2 | )p(d1 | )p()
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Probabilistic event analysis
Incorporate data one layer at a time:
• p()
• p( | d1) p(d1 | )p()
• p( | d1,d2) p(d2 | )p(d1 | )p()
• p( | d1,d2,…dN)
p(dN | )p(dN-1 | ) … p(d2 | )p(d1 | )p()
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Probabilistic event analysis
Likelihood:
• p(d | )
• This is zero-one - if the trajectory described by triggers all the detectors that fired, then p(d | )=1, else p(d | )=0
• This makes applying MCMC directly somewhat difficult.
• This is a simplification of the likelihood– some detectors fire spuriously– some particles pass through gaps between microstrips– information regarding the particles energy
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Computation• The basic idea:
– run the forward simulation a very large number of times, keeping those runs which triggered the same detectors that were triggered in the event we are analysing
– compute the mean, variance etc of the photon direction and energy from the runs that are retained
– clearly this is computationally infesable (and becomes more so the more physics processes we include)
• Instead:
– use ideas from sequential importance sampling to only generate runs that with high probability trigger the detectors that fired
– non-parametric representation of the distribution that allows for tracking of multiple hypotheses
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ComputationA combination of ideas from Particle Filters and MCMC
• represent p( | {d}) by a set of particles
• propagate the set of particles down the stack– use importance sampling distributions that generate trajectories
that intersect, with high probability, with the detectors that fired (0-1 likelihood)
– weight the particles by the ratio of the physics distribution to the importance sampling distribution
– re-sample the set of weighted particles
• apply mcmc steps to the particles after each layer– because the event has no dynamics between layers (the photon
angle does not change), “particle starvation” can be a problem
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Over-simplified simulation
• Only analyse the incident photon angle and position• Also estimate the “nuisance” variables - the vertex position (shown) and scattering angles at
each layer (not shown)• Assume the energy split between the electron and positron is known (see later)
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Over-simplified simulation
• The energy split is almost equal, so the “opening angle” is symmetric (107:93MeV)• Because the positron (blue) is scattered much less, a good fit to the data is a slightly offset
photon angle, with more even scattering down the two trajectories
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Over-simplified simulation
• Very small opening angle, so energy split is less important (actual split is 154:46MeV)• Estimate is unbiased, but the remaining uncertainty is larger
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Simplified Simulation
• Show the results for the estimate of the photon angles for the first four levels
(after that particle starvation became an issue)
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Future work• Add more physics
– add the analysis of the energy of the photon, and consider also the deposition of energy by the particles as they interact with the detector
– addition of the processes which produce secondary particles will complicate the analysis significantly
• the dimensionality of the particles will vary
• Improve the likelihood:
– currently we use a simple 1-0 likelihood
– model the physics of the silicon microstrip detectors• the microstrips give information about the quantity of charge deposited• the number of strips that fire depends on the energy of the incident
particles
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Future work• Analysis of the energy
– the angle distribution is highly dependent on the energy split between the electron and positron
photon200MeV
electron80MeV
positron120MeV
e
p
photon200MeV
electron190MeV
positron10MeV
e p
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Conclusion
“If you have to use statistics, go back and design the experiment properly”
Lord Rutherford
“If you have to use statistics, think about the statistics at the same time as you design the experiment”
Me