cosmic:dm_particle
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| cosmic:dm_particle [2020/12/02 13:10] – hughlippincott | cosmic:dm_particle [2020/12/11 11:22] (current) – [Big Questions White Papers] tongylin | ||
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| * For instructions how to join an Email list refer to [[https:// | * For instructions how to join an Email list refer to [[https:// | ||
| * Slack channel: [[https:// | * Slack channel: [[https:// | ||
| - | * Indico page with summer/ | + | * Indico page for all CF1 meetings, |
| ====== Description ====== | ====== Description ====== | ||
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| * Direct detection to the neutrino floor (theory motivation including EFT) | * Direct detection to the neutrino floor (theory motivation including EFT) | ||
| - | * Coordinators: | + | * Coordinators: |
| * Slack: # | * Slack: # | ||
| - | * multi-scale portfolio that includes a broad energy range and experiment cost. (Xe, Ar, CCDs, Bubble chamber, Solid State Detectors) | + | |
| - | * focus on ~>1 GeV nuclear recoils | + | |
| - | * reasonable to achieve on a G3 timescale (~10 yr including construction and operations). | + | |
| * The landscape of low threshold detection in the next decade (theory motivation included by theory of detectors including AMO, bandgaps, | * The landscape of low threshold detection in the next decade (theory motivation included by theory of detectors including AMO, bandgaps, | ||
| * Coordinators: | * Coordinators: | ||
| * Slack: # | * Slack: # | ||
| - | * Re-statement of parts of BRN/Cosmic Visions for low threshold detectors | + | |
| - | * Theory to motivate then a description of the new wave of experimental ideas. | + | |
| - | * How to handle experiments at different phases (e.g. SENSEI/ | + | |
| * Calibration/ | * Calibration/ | ||
| * Coordinators: | * Coordinators: | ||
| * Slack: # | * Slack: # | ||
| - | * What improvements do we need to make in understanding detector calibration and backgrounds to support/ | + | |
| - | * Discuss common needs/ | + | |
| - | * Endorsement of low energy NR sources wherever they are | + | |
| - | * Discussion of noise sources (electron emission, IR backgrounds, | + | |
| * Computing/ | * Computing/ | ||
| * Coordinators: | * Coordinators: | ||
| * Slack: # | * Slack: # | ||
| - | | + | |
| - | * Could cover effective theory techniques, common statistical frameworks, better simulations, | + | * The landscape of cosmic-ray and high-energy photon probes of particle dark matter |
| - | * Support theory | + | |
| + | * Slack: # | ||
| + | |||
| + | * Puzzling excesses and how we can resolve their origin/ | ||
| + | * Coordinators: | ||
| + | | ||
| + | |||
| + | * Synergies between DM searches | ||
| + | * Coordinators: | ||
| + | * Slack: # | ||
| + | |||
| + | * Ultraheavy particle dark matter / probing the heaviest particle dark matter candidates (envisaged to be a shorter paper than some others) | ||
| + | * Coordinators: | ||
| + | * # | ||
cosmic/dm_particle.1606936259.txt.gz · Last modified: 2020/12/02 13:10 by hughlippincott