Bounding the Photon Mass with Solar Probes

Details Bounding the Photon Mass with Solar Probes Bounding the Photon Mass with Solar Probes

1993-04-13

arxiv.org/abs/hep-ph/9304250v1

Phys.Lett.B317:223-226,1993

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, LaTeX, Indiana University preprint IUHET 245 and Los Alamos Preprint LA-UR-93-1128

Scientific paper

10.1016/0370-2693(93)91597-G

Proposed close-encounter solar probes (Vulcan and Solar Probe) are planned to
have highly eccentric orbits, with a perihelion of about $4R_S$ and an
inclination close to $90^\circ$ out of the plane of the ecliptic. We show this
could allow at least an order-of-magnitude improvement in the present directly
measured limit on the photon mass.

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