Precision: Difference between revisions
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*Low Energy Measurements (AMO) | *Low Energy Measurements (AMO) | ||
*Dark Matter and Dark Sector Production | *Dark Matter and Dark Sector Production | ||
*Accelerator-based searches for dark matter | *Accelerator-based searches for dark matter ''''(Moved from the Energy Frontier)'''' | ||
*Nano-gravity and Fifth Force, frame-dragging, Eotvos | *Nano-gravity and Fifth Force, frame-dragging, Eotvos | ||
Revision as of 21:32, 29 October 2019
Frontiers in Rare Processes and Precision Measurements
TOPICS
(Contact slstone@syr.edu, rhbob@fnal.gov to nominate conveners)
- Weak decays of b & c quarks
- Tests of Standard Model CP violation, CKM measurements
- Lepton flavor universality tests
- Rare phenomena, B(s)->mu+mu-, B->K(*)lepton+lepton-, Bs-> phi gamma,other SM tests
- Beyond the SM direct searches including dark photon, Majorana neutrinos, etc...
- CP violation at colliders
- CP violation at low energies (e.g. where CP violation is not bound by EDM measurements)
- Electric and magnetic dipole moments
- CLFV (mu to e conversion, rare muon and tau decays)
- Parity violation and fundamental symmetry tests
- Nucleon decay, n-n-bar mixing
- Low Energy Measurements (AMO)
- Dark Matter and Dark Sector Production
- Accelerator-based searches for dark matter '(Moved from the Energy Frontier)'
- Nano-gravity and Fifth Force, frame-dragging, Eotvos
Corrections and Comments
- Moving beam-related dark matter searches here to make a community
- Would like a better Frontier name to make this clear - use the SLACK channel to make suggestions