We propose a variation, based on very low energy and extremely intense photon sources, on the well established technique of Light-Shining-through-Wall (LSW) experiments for axion-like particle searches. With radiation sources at 30 GHz, we compute that present laboratory exclusion limits on axion-like particles might be improved by at least four orders of magnitude, for masses ma≲0.01 meV. This could motivate research and development programs on dedicated single-photon sub-THz detectors.

Axion-like particle searches with sub-THz photons / Capparelli, LUDOVICO MARK; Cavoto, Gianluca; Ferretti, Jacopo; Giazotto, F.; Polosa, ANTONIO DAVIDE; Spagnolo, P.. - In: PHYSICS OF THE DARK UNIVERSE. - ISSN 2212-6864. - STAMPA. - 12:(2016), pp. 37-44. [10.1016/j.dark.2016.01.003]

Axion-like particle searches with sub-THz photons

CAPPARELLI, LUDOVICO MARK;CAVOTO, Gianluca;FERRETTI, JACOPO;POLOSA, ANTONIO DAVIDE;
2016

Abstract

We propose a variation, based on very low energy and extremely intense photon sources, on the well established technique of Light-Shining-through-Wall (LSW) experiments for axion-like particle searches. With radiation sources at 30 GHz, we compute that present laboratory exclusion limits on axion-like particles might be improved by at least four orders of magnitude, for masses ma≲0.01 meV. This could motivate research and development programs on dedicated single-photon sub-THz detectors.
2016
Axion-like particles; Chameleons; Dark-matter constituents; Light-Shining-through-Wall experiments; Paraphotons; Astronomy and Astrophysics; Space and Planetary Science
01 Pubblicazione su rivista::01a Articolo in rivista
Axion-like particle searches with sub-THz photons / Capparelli, LUDOVICO MARK; Cavoto, Gianluca; Ferretti, Jacopo; Giazotto, F.; Polosa, ANTONIO DAVIDE; Spagnolo, P.. - In: PHYSICS OF THE DARK UNIVERSE. - ISSN 2212-6864. - STAMPA. - 12:(2016), pp. 37-44. [10.1016/j.dark.2016.01.003]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/904684
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