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Pseudoscalar conversion and X-rays from the sun

1995/07/19 by Eric D. Carlson, Li-Sheng Tseng · 1 citation
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Solar and Space Plasma Dynamics #astro-ph #hep-ph

paper · pdf · doi:10.1016/0370-2693(95)01250-8

published as Phys.Lett. B365 (1996) 193 · 15 pages, RevTex file. Figures available upon request to [email protected]. (please include full mailing address in request). Submitted to Physics Letters B

arxiv created 1995/07/19 · openalex publication_date 1996/01/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We investigate the detection of a pseudoscalar ϕ that couples electromagnetically via an interaction 1\over4g ϕF F. In particular, we focus on the conversion of pseudoscalars produced in the sun's interior in the presence of the sun's external magnetic dipole field and sunspot-related magnetic fields. We find that the sunspot approach is superior. Measurements by the SXT on the Yohkoh satellite can measure the coupling constant down to g=0.5--1 × 10-10 \rm GeV-1, provided the pseudoscalar mass m < 7× 10-6 eV, which makes it competitive with other astrophysical approaches.

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