The discovery and significance of fast radio bursts
arXiv:2405.19106 · doi:10.1007/s10509-024-04322-6
Abstract
In 2007 we were part of a team that discovered the so-called ``Lorimer Burst'', the first example of a new class of objects now known as fast radio bursts (FRBs). These enigmatic events are only a few ms in duration and occur at random locations on the sky at a rate of a few thousand per day. Several thousand FRBs are currently known. While it is now well established that they have a cosmological origin, and about 10\% of all currently known sources have been seen to exhibit multiple bursts, the origins of these enigmatic sources are currently poorly understood. In this article, we review the discovery of FRBs and present some of the highlights from the vast body of work by an international community. Following a brief overview of the scale of the visible Universe in §1, we describe the key moments in radio astronomy (§2) that led up to the discovery of the Lorimer burst (§3). Early efforts to find more FRBs are described in §4 which led to the discovery of the first repeating source (§5). In §6, as we close out on the second decade of FRBs, we outline some of the many open questions in the field and look ahead to the coming years where many surprises are surely in store.
23 pages, 9 figures, accepted for publication in Astrophysics and Space Science; manuscript based on the 2023 Shaw Prize Lecture in Astronomy delivered by the authors
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- A search using GEO600 for gravitational waves coincident with fast radio bursts from SGR 1935+2154
- Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization
- Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
- A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010
- Prediction of Multi-Wavelength Afterglows Associated with FRB 20200120E and FRB 20201124A
- Fast radio bursts by stellar wind microlensing of a faint background source
- The Impact of Accretion on FRB Radiation Mechanisms in Binary Systems: Constraints and Implications