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Title: Laboratory Constraints on Chameleon Dark Energy and Power-Law Fields

Abstract

We report results from a search for chameleon particles created via photon-chameleon oscillations within a magnetic field. This experiment is sensitive to a wide class of unexplored chameleon power-law and dark energy models. These results exclude 5 orders of magnitude in the coupling of chameleons to photons covering a range of 4 orders of magnitude in chameleon effective mass and, for individual models, exclude between 4 and 12 orders of magnitude in chameleon couplings to matter.

Authors:
; ; ; ; ;  [1];  [2];  [3]
  1. Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, Illinois 60510 (United States)
  2. Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637 (United States)
  3. Astrophysics, Cosmology and Gravity Centre, University of Cape Town, Rondebosch, Private Bag, 7700 (South Africa)
Publication Date:
OSTI Identifier:
21554495
Resource Type:
Journal Article
Resource Relation:
Journal Name: Physical Review Letters; Journal Volume: 105; Journal Issue: 26; Other Information: DOI: 10.1103/PhysRevLett.105.261803; (c) 2010 American Institute of Physics
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; COUPLING; EFFECTIVE MASS; MAGNETIC FIELDS; NONLUMINOUS MATTER; OSCILLATIONS; PHOTONS; BOSONS; ELEMENTARY PARTICLES; MASS; MASSLESS PARTICLES; MATTER

Citation Formats

Steffen, J. H., Baumbaugh, A., Chou, A. S., Mazur, P. O., Tomlin, R., Wester, W., Upadhye, A., and Weltman, A. Laboratory Constraints on Chameleon Dark Energy and Power-Law Fields. United States: N. p., 2010. Web. doi:10.1103/PHYSREVLETT.105.261803.
Steffen, J. H., Baumbaugh, A., Chou, A. S., Mazur, P. O., Tomlin, R., Wester, W., Upadhye, A., & Weltman, A. Laboratory Constraints on Chameleon Dark Energy and Power-Law Fields. United States. doi:10.1103/PHYSREVLETT.105.261803.
Steffen, J. H., Baumbaugh, A., Chou, A. S., Mazur, P. O., Tomlin, R., Wester, W., Upadhye, A., and Weltman, A. Fri . "Laboratory Constraints on Chameleon Dark Energy and Power-Law Fields". United States. doi:10.1103/PHYSREVLETT.105.261803.
@article{osti_21554495,
title = {Laboratory Constraints on Chameleon Dark Energy and Power-Law Fields},
author = {Steffen, J. H. and Baumbaugh, A. and Chou, A. S. and Mazur, P. O. and Tomlin, R. and Wester, W. and Upadhye, A. and Weltman, A.},
abstractNote = {We report results from a search for chameleon particles created via photon-chameleon oscillations within a magnetic field. This experiment is sensitive to a wide class of unexplored chameleon power-law and dark energy models. These results exclude 5 orders of magnitude in the coupling of chameleons to photons covering a range of 4 orders of magnitude in chameleon effective mass and, for individual models, exclude between 4 and 12 orders of magnitude in chameleon couplings to matter.},
doi = {10.1103/PHYSREVLETT.105.261803},
journal = {Physical Review Letters},
number = 26,
volume = 105,
place = {United States},
year = {Fri Dec 31 00:00:00 EST 2010},
month = {Fri Dec 31 00:00:00 EST 2010}
}
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