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Improving the Discovery Potential of Future Light-Shining-through-a-Wall Experiments

2010/09/08 by Paola Arias, Arias, Paola, Joerg Jaeckel +6
Engineering · Physics and Astronomy · #Advanced Optical Sensing Technologies #Atomic and Subatomic Physics Research #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Laser Design and Applications #Photocathodes and Microchannel Plates #Random lasers and scattering media #hep-ph

paper · pdf · doi:10.48550/arxiv.1009.1519

4 pages, 2 figures, contribution to 6th Patras Workshop on Axions, WIMPs and WISPs, Zurich University, Switzerland, 5-9 July 2010

arxiv created 2010/09/08 · openalex publication_date 2010/09/08 · arxiv updated 2010/09/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Planning for the next generation of light-shining-through-wall experiments has started. It is therefore timely to investigate possible ways to optimize their setups. The goals are to improve the sensitivity towards smaller couplings and increase the mass range to which the experiments are sensitive. We discuss possible magnet arrangements and the effects of the unavoidable gaps in the magnetic field profile. Furthermore, we discuss requirements on the diameter of the laser beam and aperture of the magnets in order to achieve high-quality cavities.

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