Difference between revisions of "MOLLER Simulations"
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* Detector simulations (Patrick Rogan ) | * Detector simulations (Patrick Rogan ) | ||
* Al backgrounds (Mark Pitt's student) | * Al backgrounds (Mark Pitt's student) | ||
| − | * Power deposited in collimator and coils ( | + | * Power deposited in collimator and coils (Damon Spayde's student) |
* Neutron backgrounds | * Neutron backgrounds | ||
<br><br> Return to [[MOLLER at 11 GeV E09-005]] | <br><br> Return to [[MOLLER at 11 GeV E09-005]] | ||
Revision as of 17:23, 10 June 2011
GEANT4 Simulations
TOSCA
Meetings
Simulation Teleconferences
The Simulation group is led by Klaus Grimm and Neven Simicevic, Louisiana Tech, and organized by Juliette Mammei, UMass, from Jefferson Lab. The group will meet regularly to discuss the progress of the MOLLER simulations.
Projects
Development
- Ongoing improvements to moller_sim (used to generate physics results for proposal)
- improving generators (Dustin)
- geometry specification (Juliette)
- batch submission (Juliette)
- Additional generators (pion production, including rare weak decays)
- Development of molgemc (using GEMC, developed in Hall B and used by CLAS)
- external generators (Dustin)
- read-in of two field maps (Juliette)
- Hit processing
- Output (EVIO->Root?)
- set up mysql database, add to svn, documentation
Simulation
- Collimator optimization (Sereres Johnston)
- Simulation of weak decays (Konrad Aniol's student)
- Detector simulations (Patrick Rogan )
- Al backgrounds (Mark Pitt's student)
- Power deposited in collimator and coils (Damon Spayde's student)
- Neutron backgrounds
Return to MOLLER at 11 GeV E09-005
