Published December 1, 2008
| Version v1
Journal article
Enhanced rare pion decays from a model of MeV dark matter
- 1. Northwestern University, Department of Physics and Astronomy, 2145 Sheridan Road, Evanston, Illinois 60208 (United States)
- 2. HEP Division, Argonne National Lab, Argonne, Illinois 60439 (United States)
Description
A model has been proposed in which neutral scalar particles χ, of mass 1-10 MeV, annihilate through the exchange of a light vector boson U, of mass 10-100 MeV, to produce the 511 keV line observed emanating from the center of the Galaxy. The χ interacts weakly with normal matter and is a viable dark matter candidate. If the U boson couples to quarks as well as to electrons, it could enhance the branching ratio for the rare decay π0→e+e-. A recent measurement by the KTeV Collaboration lies 3 standard deviations above a prediction by Dorokhov and Ivanov, and we relate this excess to the couplings of the U boson. The values are consistent with other constraints and considerations. We make some comments on possible improvements in the data.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.115002;
- arXiv
- arXiv:0712.0007v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 11
- Journal Page Range
- p. 115002-115002.4
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41002361
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BRANCHING RATIO; COUPLING; ELECTRONS; FORECASTING; GALAXY NUCLEI; INTERMEDIATE VECTOR BOSONS; KEV RANGE; MASS; MESONS; MEV RANGE; NONLUMINOUS MATTER; PARTICLE DECAY; PARTICLES; PIONS; PIONS NEUTRAL; POSITRONS; QUARKS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; BOSONS; DECAY; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRONS; INTERMEDIATE BOSONS; LEPTONS; MATTER; MESONS; PIONS; PSEUDOSCALAR MESONS
Optional Information
- Notes
- (c) 2008 The American Physical Society