Steps in the Simulation
- NuMI beam simulation
- output: neutrino flux
- simulate the secondary particle generation
- WBB/NBB horn/Li-lens optics
- decay of secondaries in flight to produce neutrinos
- Neutrino event generator
- output: STDHEP(-like) particle list
- perform $\nu$ oscillations
- simulate the various cross-sections (CC, NC, QE, ...)
- fragmentation in the case of Deep Inelastic Scattering.
- GEANT - {\tt gminos}
- output: hits (true quantities)
- track input particles through defined volumes
- standard physics processes ($\Delta E \over \Delta x$,
interactions, etc)
- store important quantities ($\vec{x}$,E,$\vec{p}$,ipart,$\Delta E$)
for particles passing through active volumes.
- Active detector response
- output: ``data''
- convert true quantities into signals that one would see in
an actual detector by modelling the response of the
individual technologies (LiqScint, LST, RPC).
- Event analysis
- output: reconstructed events
- from ``digits'' calculate energies and angles
- perform tracking
- event classification (CC, NC, $\nu_e$, etc.)
- calculate $x$, $y$, $E_{\nu}$, ...
- Physics analysis
- output: physics
- use events to determine $\sin^2{(2\theta)}$, $\Delta m^2$
- other possible analyses (cf. Jorge's request for proposals)
- Online DAQ
- output: data
- read out the detector elements
- provide consistency checks, alarms for real-time monitoring
The cascade of distinct steps should be as decoupled as possible
as to allow each step to be performed based on the output of the
previous step. A standardized exchange format for each intermediate
file must be established.
hatcher@astro.indiana.edu
- updated 1996.01.11 -
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