Cosmic: Difference between revisions
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(Created page with " == Cosmic Frontier == Contact profumo@ucsc.edu , diehl@fnal.gov to nominate conveners) Dark Matter Direct Detection Particles (WIMP-like) Waves (Axion/ALP...") |
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Contact profumo@ucsc.edu , diehl@fnal.gov to nominate conveners) | Contact profumo@ucsc.edu , diehl@fnal.gov to nominate conveners) | ||
Dark Matter Direct Detection | *Dark Matter Direct Detection | ||
**Particles (WIMP-like) | |||
**Waves (Axion/ALP-like) | |||
**Dark Sector Phenomenology and New Directions | |||
Indirect DM detection (gamma and cosmic ray signatures) | *Indirect DM detection (gamma and cosmic ray signatures) | ||
Astrophysical DM probes (galaxy halo substructure, clusters, large-scale structure) | *Astrophysical DM probes (galaxy halo substructure, clusters, large-scale structure) | ||
Dark Energy and Cosmic Expansion: | *Dark Energy and Cosmic Expansion: | ||
Growth of structure probes | *Growth of structure probes | ||
Expansion (H0) and expansion history probes | *Expansion (H0) and expansion history probes | ||
Inflation and the early universe: CMB, Other probes of the early universe | *Inflation and the early universe: CMB, Other probes of the early universe | ||
Probes/Tests of General Relativity | *Probes/Tests of General Relativity | ||
Gravitational waves as probes of cosmology and fundamental physics | *Gravitational waves as probes of cosmology and fundamental physics | ||
Multi-messenger astroparticle physics | *Multi-messenger astroparticle physics | ||
Cosmic Probes of Neutrino properties | *Cosmic Probes of Neutrino properties | ||
Cosmic Ray Physics | *Cosmic Ray Physics | ||
Cosmic Observatories/Facilities (CMB, O/IR, Radio, Gamma ray, Cosmic ray, grav. wave, etc.) | *Cosmic Observatories/Facilities (CMB, O/IR, Radio, Gamma ray, Cosmic ray, grav. wave, etc.) | ||
Revision as of 19:20, 21 October 2019
Cosmic Frontier
Contact profumo@ucsc.edu , diehl@fnal.gov to nominate conveners)
- Dark Matter Direct Detection
- Particles (WIMP-like)
- Waves (Axion/ALP-like)
- Dark Sector Phenomenology and New Directions
- Indirect DM detection (gamma and cosmic ray signatures)
- Astrophysical DM probes (galaxy halo substructure, clusters, large-scale structure)
- Dark Energy and Cosmic Expansion:
- Growth of structure probes
- Expansion (H0) and expansion history probes
- Inflation and the early universe: CMB, Other probes of the early universe
- Probes/Tests of General Relativity
- Gravitational waves as probes of cosmology and fundamental physics
- Multi-messenger astroparticle physics
- Cosmic Probes of Neutrino properties
- Cosmic Ray Physics
- Cosmic Observatories/Facilities (CMB, O/IR, Radio, Gamma ray, Cosmic ray, grav. wave, etc.)