Density Gradient and Absorption Effects in Gas-Filled Magnetic Axion Helioscopes

Simple item page
dc.creatorCreswick, R. J.
dc.creatorNussinov, S.
dc.creatorAvignone III, F. T.
dc.date2008-05-14
dc.date.accessioned2026-07-07T11:33:49Z
dc.date.available2026-07-07T11:33:49Z
dc.descriptionThe effects of absorption in the gas, and of density variations on the sensitivity of gas-filled solar-axion helioscopes are theoretically investigated. It is concluded that the 10-meter long CAST helioscope, the most sensitive experiment to date is near the limit of sensitivity in axion mass. Increasing the length, gas density, or tilt angle all have negative influences, and will not improve the sensitivity.
dc.description8 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0805.2142
dc.identifierhttp://arxiv.org/abs/0805.2142
dc.identifierPhys.Rev.D78:017702,2008
dc.identifierdoi:10.1103/PhysRevD.78.017702
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198028
dc.subjectAstrophysics
dc.titleDensity Gradient and Absorption Effects in Gas-Filled Magnetic Axion Helioscopes
dc.typetext

Files

Collections

arXiv