Exploring x-ray capillary optics for astrophysics
X-ray capillary optics are arrays of large numbers of curved and tapered hollow glass tubes that guide x-rays similarly to how optical fibers guide visible light. These optics typically have an entrance aperture of up to a square centimeter, a focal length of 10cm or less, and concentrate the x-rays to a focal spot with a diameter of a few hundred microns. Given the short focal length, a telescope using x-ray capillary optics would be a smaller and lighter alternative to currently existing technologies. Using the 100-meter beamline at NASA/GSFC, we have characterized two x-ray capillary optics with an imaging detector and a custom silicon detector specifically designed for use with these optics. Here we present the results of these measurements and discuss our outlook for a future x-ray telescope using capillary optics.
Authors
- Alexis Lane (ORCID: https://orcid.org/0000-0003-0626-2717)
- Clio Sleator (ORCID: https://orcid.org/0000-0003-4732-6174)
- Takashi Okajima (ORCID: https://orcid.org/0000-0002-6054-3432)
- Bernard F. Phlips
- Keisuke Tamura (ORCID: https://orcid.org/0000-0002-6677-3917)
Institutions
- United States Naval Research Laboratory (US)
- Goddard Space Flight Center (US)
- Technology Service Corporation (United States) (US)
- K Lab (United States) (US)
- University of Maryland, Baltimore County (US)
Publication Details
- Published
- 2025-09-18
- DOI
- https://doi.org/10.1117/12.3064580
- Primary Topic
- Astrophysical Phenomena and Observations
- Type
- article
- Field-Weighted Citation Impact
- 0.00