Parametric simulation
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==Talks== | ==Talks== | ||
| + | * Software meeting 2018-06-29, Friday, [[File:sctau_papas_v2_20180629.pdf]] by '''Georgiy Razuvaev''' | ||
| + | * Software meeting 2019-02-01 [[:Media:Sctau_papas_v3_20190201.pdf | Status of PAPAS]] by '''Georgiy Razuvaev''' | ||
| + | * Software meeting 2019-08-09 [[:Media:Sctparsim_20190809.pdf | Super c-τ parametric simulation: Status]] by '''Georgiy Razuvaev''' | ||
| + | * Software meeting 2019-12-27 [[:Media:SctParSim_status_20191127_Belozyorova.pdf | SctParSim: status and recent progress]] by '''Maria Belozyorova''' | ||
| + | * Workshop on future Super c-tau factories 2021-11-16 [https://indico.inp.nsk.su/event/62/contributions/2315/ Parametric simulation of the SCT detector] by '''Maria Belozyorova''' | ||
| − | == | + | = SctParSim (Aurora) = |
| + | A parametric simulation is a tool to receive a detector response without detailed description of interaction of particles with matter. The simulation is the part of the Aurora project, which is a software suit for SCTF. | ||
| + | Implemented detector subsystems: | ||
| + | * drift chamber | ||
| + | * FARICH PID system | ||
| + | * calorimeter | ||
| + | * muon system | ||
| − | == | + | The parametric simulation yields the detector response in the SCT EDM format thus allowing to analyze its result in the same manner as the result of the full simulation. The tracker and the calorimeter smear particle parameters according |
| + | to a Gaussian distribution, while the FARICH PID and the muon subsystem use for that purpose the results of a pre-conducted standalone full Geant4 simulations. | ||
| + | |||
| + | '''More information about parameterization''' is presented [[SctParSim (Aurora)|here]]. | ||
| + | |||
| + | '''How-to use the parametric simulation''' is demonstrated [https://ctd.inp.nsk.su/wiki/index.php/SCT_parametric_simulation here] | ||
| + | |||
| + | = SctParSim (Python) = | ||
| + | |||
| + | This version of the parametric simulation had written in the Python language. The main difference is that this version has the ability to draw events. | ||
| + | |||
| + | '''How to run and parameter description''' is [[SctParSim (python)|here]] | ||
| + | |||
| + | = PAPAS (Old) = | ||
| + | |||
| + | More details are [[SctparSim (PAPAS)|here]] | ||
Latest revision as of 15:03, 24 November 2021
Contents |
[edit] Talks
- Software meeting 2018-06-29, Friday, File:Sctau papas v2 20180629.pdf by Georgiy Razuvaev
- Software meeting 2019-02-01 Status of PAPAS by Georgiy Razuvaev
- Software meeting 2019-08-09 Super c-τ parametric simulation: Status by Georgiy Razuvaev
- Software meeting 2019-12-27 SctParSim: status and recent progress by Maria Belozyorova
- Workshop on future Super c-tau factories 2021-11-16 Parametric simulation of the SCT detector by Maria Belozyorova
[edit] SctParSim (Aurora)
A parametric simulation is a tool to receive a detector response without detailed description of interaction of particles with matter. The simulation is the part of the Aurora project, which is a software suit for SCTF.
Implemented detector subsystems:
- drift chamber
- FARICH PID system
- calorimeter
- muon system
The parametric simulation yields the detector response in the SCT EDM format thus allowing to analyze its result in the same manner as the result of the full simulation. The tracker and the calorimeter smear particle parameters according to a Gaussian distribution, while the FARICH PID and the muon subsystem use for that purpose the results of a pre-conducted standalone full Geant4 simulations.
More information about parameterization is presented here.
How-to use the parametric simulation is demonstrated here
[edit] SctParSim (Python)
This version of the parametric simulation had written in the Python language. The main difference is that this version has the ability to draw events.
How to run and parameter description is here
[edit] PAPAS (Old)
More details are here
