Working Group Breakout Topics
This page is intended to help organize the breakout sessions. There are 3 primary categories, each with several subtopics. Note that there is natural overlap among the categories, and that cross-collaboration is encouraged.
There are two breakout sessions on Thursday and Friday afternoons and a combined session on Saturday intended for integration:
Mar 20 (Thu) 3:30-6:00 pm → Identify topics and tasks
Mar 21 (Fri) 4:00-6:00 pm → Prioritize topics and plan future work
Mar 22 (Sat) 10:30 am - 12:00 pm → Integration into proposals, Consortium planning, and new integrative initiatives
Simulation (Comitium)
coordinator: Anthony Villano
Specialized Detector Physics Simulation (Thu 3:30 - 5:00 pm)
How can specialized models be incorporated into simulation packages systematically, how can different detector packages be cross-compared systematically and continuously for new versions to be sure models behave correctly and new data is incorporated properly.
specialized detector physics
specific benchmarking with specialized geometry (e.g. Geant4/FLUKA comparison)
microscopic data for vetting specialized detector physics
Cross-Collaboration with Neutron Benchmarking (Thu 5:00 - 6:00 pm)
Identify the data which exists and where they can constrain the understanding of backgrounds. Specifically focus on exactly how some data sets can be used to constrain cosmogenic simulations.
Simulation Codes (Fri 4:00 - 5:00 pm)
Review of the existing packages for simulation and what processes exist and what the models are to add processes.
simulation packages for low background physics (Geant4, FLUKA, MCNP)
processes in each simulation package
model for adding to each package
relevant processes which exist in each package
specific models used by all these processes – and for different versions of the packages
Cross-collaboration with Radiogenics (Fri 5:00 - 6:00 pm)
cross sections data for microscopic (e.g. (alpha,n)) events
specific small scale cross section data (e.g. (alpha,n))
Radiogenics - One East (Natural Radioactivity in Shielding Materials and Detectors)
coordinators: Jodi Cooley and Chao Zhang
secretary: Silvia Scorza & Jeter Hall
minutes: docx
Assays Thu 3:30 - 4:30 pm
Community Assays Database
Facilities, access and needs (review of what has been done)
-
SNOWMASS 2013 data collected on world wide facilities
(wiki)
New Detector Developments?
Background Reduction Thu 4:30 - 5:30 pm
Calculations Fri 4:00 - 5:00
Cross Collaboration with Simulation Working Group Fri 5:00 - 6:00 pm
Nuclear cross sections and new experiments to improve nuclear data
Cross sections data for microscopic (e.g. (alpha,n)) events
Specific small scale cross section data (e.g. (alpha,n))
Studies of non-equilibrium decay
Neutron capture in materials
Implement physics model into GEANT4
Benchmarking (Curia II)
coordinator: Ray Bunker
Measurements — Thu 3:30-4:30 pm
Where are we now? (i.e., which neutron- and muon-related backgrounds are well measured?)
Muon-induced neutrons — summary papers:
Muon-Induced Background Study for Underground Laboratories
Muon-Induced neutron production and detection with Geant4 and FLUKA
Predicting Neutron Production from Cosmic-ray Muons
Detector-specific measurements:
Production of Radioactive Isotopes through Cosmic Muon Spallation in KamLAND
A detection system to measure muon-induced neutrons for direct Dark Matter searches
Measurement and simulation of the muon-induced neutron yield in lead
Cosmogenic Background in Borexino at 3800 m water-equivalent depth
Measurement of the muon-induced neutron yield in liquid scintillator and stainless steel at LNGS with the LVD experiment
LVD — Persiani
et al., AIP Conf. Proc.
1549 (2013) 235 —
LRT 2013
Spallation-source measurements:
Others?
Organization of measurements, publications, and constraints?
What remains to be done? (i.e., which backgrounds are still poorly constrained?)
High-energy neutron flux & energy spectrum vs. depth
Background from muon bundles
Long-lived isotopes from muon spallation & stopping muons
Radiogenic benchmarking
Others?
Data - Part I — Thu 4:30-5 pm
Cross-collaboration with Simulation — Thu 5-6 pm
Data - Part II — Fri 4-4:30 pm
Detector Technology — Fri 4:30-6 pm
Pros & cons of different neutron-detection technologies
Design/proposal of next-generation neutron detector/facility for underground measurements
Funding for underground benchmarking in general
Purpose of AARM
Coordination of Background Identification and Reduction
Prisca Cushman (3/18/2014)
Note that this outline is not organized with respect to the breakout session titles. Instead, it is organized by type of background and by AARM integration jobs.
Natural Radioactivity in Shielding Materials and Detectors
Simulation
Codes and frameworks
General Physics models and processes
Advances in specific detector physics (e.g. noble liquids, or photon physics)
Nuclear cross sections and new experiments to improve nuclear data
Databases (e.g. alpha-n etc)
Assay
Background Reduction
Cosmogenic Effects
Muon distributions
Parameterization and physics
Site-specific distributions, MUSUN
Cosmic Ray physics: bundles and modulation effects
Muon-induced neutrons
Cosmogenic Activation
Organization and Shared Resources
Shared User Facilities for screening
Populating and regulating the Materials Database
Simulation tools
Creating a community for shared resources and information - future of AARM