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The discovery and significance of fast radio bursts (2405.19106v3)

Published 29 May 2024 in astro-ph.HE and astro-ph.CO

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 \S 1, we describe the key moments in radio astronomy (\S 2) that led up to the discovery of the Lorimer burst (\S 3). Early efforts to find more FRBs are described in \S 4 which led to the discovery of the first repeating source (\S 5). In \S 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.

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References (15)
  1. \bibcommenthead
  2. Bailes M (2022) The discovery and scientific potential of fast radio bursts. Science 378(6620):abj3043. 10.1126/science.abj3043, arXiv:2211.06048 [astro-ph.HE]
  3. Benz AO, Paesold G (1998) A search for prompt radio emission of gamma-ray bursts. AAP 329:61–67
  4. Bondi H (1970) Astronomy of the Future. QJRAS 11:443
  5. Burns WR, Clark BG (1969) Pulsar Search Techniques. AAP 2:280–287
  6. Cavallo G, Jelley JV (1975) Why are no radio pulses associated with the bursts of celestial gamma-rays? ApJL 201:L113–L115. 10.1086/181954
  7. Cavallo G, Ventura A (1972) Restrictions on the Short Time Constant Astrophysics. Astrophys Sp Sci 19(2):431–439. 10.1007/BF00645726
  8. Colgate SA, Noerdlinger PD (1971) Coherent Emission from Expanding Supernova Shells. ApJ 165:509. 10.1086/150918
  9. Ginzburg VL (1973) Possibility of Determining Intergalactic Gas Density by Radio Observations of Flares of Remote Sources. Nature 246(5433):415. 10.1038/246415a0
  10. Huguenin GR, Moore EL (1974) A Search for Isolated Radiofrequency Pulses. ApJL 187:L57. 10.1086/181395
  11. Linscott IR, Erkes JW (1980) Discovery of millisecond radio bursts from M 87. ApJL 236:L109–L113. 10.1086/183209
  12. Palmer DM (1993) Radio Dispersion as a Diagnostic of Gamma-Ray Burst Distances. ApJL 417:L25. 10.1086/187085
  13. Phinney S, Taylor JH (1979) A sensitive search for radio pulses from primordial black holes and distant Supernovae. Nature 277(5692):117–118. 10.1038/277117a0
  14. Schmidt M (1963) 3C 273 : A Star-Like Object with Large Red-Shift. Nature 197(4872):1040. 10.1038/1971040a0
  15. Staelin DH, Reifenstein IEdward C. (1968) Pulsating Radio Sources near the Crab Nebula. Science 162(3861):1481–1483. 10.1126/science.162.3861.1481
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