Document Type

Article

Publication Date

12-6-2024

Department

Department of Physics

Abstract

Finding Dyson rings around distant pulsars may involve identifying light-curve features that have not been previously identified. Previous studies covered the detection of a ring structure uniformly brightened by the central pulsar, mostly in infrared light. Here, more complex light curves are explored, which arise inherently from the pulsar beam spot’s commonly predicted superluminal speed. These speeds may cause multiple images of the pulsar’s spot on the Dyson ring to appear simultaneously to a distant observer, and so feature bright creation and annihilation events. Therefore, it is possible that even if Dyson ring structures had been observed previously, they might have remained unnoticed. Similar light-curve features may appear on naturally occurring dust rings around pulsars that reflect detectable pulsar radiation.

Publisher's Statement

© 2024 The Author(s). Publisher’s version of record: https://doi.org/10.1093/mnras/stae2701

Publication Title

Monthly Notices of the Royal Astronomical Society

Creative Commons License

Creative Commons Attribution 4.0 International License
This work is licensed under a Creative Commons Attribution 4.0 International License.

Version

Publisher's PDF

Download

Included in

Physics Commons

Share

COinS