Published November 15, 1989
| Version v1
Journal article
Results of a laboratory search for cosmic axions and other weakly coupled light particles
Creators
- 1. Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627 (USA)
- 2. Brookhaven National Laboratory, Upton, New York 11973 (USA)
- 3. Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (USA)
Description
A microwave cavity experiment designed to search for the signal from cosmic axions converting in an external magnetic field covered the mass range (4.5--16.3)x10-6 eV, corresponding to the frequency range from 1.09 to 3.93 GHz. Upper limits on the coupling and abundance of nonrelativistic galactic axions have been measured; these limits yield a coupling which is 1--2 orders of magnitude higher than that predicted by the Dine-Fischler-Srednicki model. Also presented are limits on axions with a continuum spectrum, limits on the presence of a wide axion line at the frequency of the 21-cm hydrogen emission line, and limits on the production of pseudoscalar particles by photons in the cavity interacting with the magnetic field
Additional details
Publishing Information
- Journal Title
- Physical Review, D
- Journal Volume
- 40
- Journal Issue
- 10
- Series
- Phys. Rev., D.
- Journal Page Range
- 3153-3167
- ISSN
- 0556-2821
- CODEN
- PRVDA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21030076
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- AXIONS; COSMIC RADIATION; CP INVARIANCE; EMISSION SPECTRA; GALAXIES; HUBBLE EFFECT; HYDROGEN; MAGNETIC FIELDS; MASS; MICROWAVE EQUIPMENT; NONLUMINOUS MATTER; PARTICLE IDENTIFICATION; PHOTONS; QUANTUM CHROMODYNAMICS; UNIVERSE
- Descriptors DEC
- BOSONS; ELECTRONIC EQUIPMENT; ELEMENTARY PARTICLES; ELEMENTS; EQUIPMENT; FIELD THEORIES; GOLDSTONE BOSONS; INVARIANCE PRINCIPLES; IONIZING RADIATIONS; MASSLESS PARTICLES; MATTER; NONMETALS; POSTULATED PARTICLES; QUANTUM FIELD THEORY; RADIATIONS; SPECTRA