2012/01/31 by O. K. Baker, Baker, O. K., A. Lindner +9
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Pulsars and Gravitational Waves Research #astro-ph.IM
paper · pdf · doi:10.48550/arxiv.1201.6508
7 pages, 1 figure
arxiv created 2012/01/31 · openalex publication_date 2012/01/31 · arxiv updated 2012/02/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
The radiation pressure due to reflected chameleons is suggested for their detection. Sensitive photon radiation pressure or force measuring techniques could become the new antennas for chameleons or other particles with similar properties, with gravitational waves antennas being also of potential interest. This is eventually only at first sight a Gedankenexperiment. Also chameleon-through-a-wall experiments, in particular when equipped with a Fabry-Perot resonator, could apply the suggested techniques.