Matches in SemOpenAlex for { <https://semopenalex.org/work/W4319591425> ?p ?o ?g. }
- W4319591425 endingPage "6" @default.
- W4319591425 startingPage "6" @default.
- W4319591425 abstract "Abstract The recent detection of a repeating fast radio burst (FRB) in an old globular cluster in M81 challenges traditional FRB formation mechanisms based on the magnetic activity of young neutron stars formed in core-collapse supernovae. Furthermore, the detection of this repeater in such a nearby galaxy implies a high local universe rate of similar events in globular clusters. Building off the properties inferred from the M81 FRB, we predict the number of FRB sources in nearby ( d ≲ 20 Mpc) galaxies with large globular cluster systems known. Incorporating the uncertain burst energy distribution, we estimate the rate of bursts detectable in these galaxies by radio instruments such as FAST and MeerKat. Of all local galaxies, we find M87 is the best candidate for FRB detections. We predict that M87's globular cluster system contains <?CDATA ${ mathcal O }(10)$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi mathvariant=italic></mml:mi> <mml:mo stretchy=false>(</mml:mo> <mml:mn>10</mml:mn> <mml:mo stretchy=false>)</mml:mo> </mml:math> FRB sources at present and that a dedicated radio survey (by either FAST or MeerKat) of <?CDATA ${ mathcal O }(10)$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mi mathvariant=italic></mml:mi> <mml:mo stretchy=false>(</mml:mo> <mml:mn>10</mml:mn> <mml:mo stretchy=false>)</mml:mo> </mml:math> hr has a 90% probability of detecting a globular cluster FRB in M87. The detection of even a handful of additional globular cluster FRBs would provide invaluable constraints on FRB mechanisms and population properties. Previous studies have demonstrated young neutron stars formed following the collapse of dynamically formed massive white dwarf binary mergers may provide the most natural mechanism for these bursts. We explore the white dwarf merger scenario using a suite of N -body cluster models, focusing in particular on such mergers in M87's clusters. We describe a number of outstanding features of this scenario that in principle may be testable with an ensemble of observed FRBs in nearby globular clusters." @default.
- W4319591425 created "2023-02-09" @default.
- W4319591425 creator A5037828745 @default.
- W4319591425 creator A5045415901 @default.
- W4319591425 creator A5045473616 @default.
- W4319591425 creator A5050742735 @default.
- W4319591425 creator A5071502706 @default.
- W4319591425 date "2023-02-01" @default.
- W4319591425 modified "2023-10-03" @default.
- W4319591425 title "Prospects for Detecting Fast Radio Bursts in the Globular Clusters of Nearby Galaxies" @default.
- W4319591425 cites W1526547736 @default.
- W4319591425 cites W1875172237 @default.
- W4319591425 cites W1926800210 @default.
- W4319591425 cites W1965805692 @default.
- W4319591425 cites W1965868948 @default.
- W4319591425 cites W1965941590 @default.
- W4319591425 cites W1967164129 @default.
- W4319591425 cites W1973041142 @default.
- W4319591425 cites W1973516488 @default.
- W4319591425 cites W1974765573 @default.
- W4319591425 cites W1977051691 @default.
- W4319591425 cites W1977525924 @default.
- W4319591425 cites W1979733958 @default.
- W4319591425 cites W1993244035 @default.
- W4319591425 cites W1993985662 @default.
- W4319591425 cites W1996040890 @default.
- W4319591425 cites W1996902696 @default.
- W4319591425 cites W2001883968 @default.
- W4319591425 cites W2004341830 @default.
- W4319591425 cites W2006933876 @default.
- W4319591425 cites W2014470520 @default.
- W4319591425 cites W2015437799 @default.
- W4319591425 cites W2017416565 @default.
- W4319591425 cites W2018462618 @default.
- W4319591425 cites W2020356115 @default.
- W4319591425 cites W2022558167 @default.
- W4319591425 cites W2024297548 @default.
- W4319591425 cites W2027649935 @default.
- W4319591425 cites W2032563997 @default.
- W4319591425 cites W2036423640 @default.
- W4319591425 cites W2038347333 @default.
- W4319591425 cites W2041313887 @default.
- W4319591425 cites W2045565446 @default.
- W4319591425 cites W2049416023 @default.
- W4319591425 cites W2060014682 @default.
- W4319591425 cites W2063790219 @default.
- W4319591425 cites W2066406099 @default.
- W4319591425 cites W2067239832 @default.
- W4319591425 cites W2070304421 @default.
- W4319591425 cites W2076480618 @default.
- W4319591425 cites W2078463662 @default.
- W4319591425 cites W2097082581 @default.
- W4319591425 cites W2102825905 @default.
- W4319591425 cites W2110223759 @default.
- W4319591425 cites W2115517418 @default.
- W4319591425 cites W2121480729 @default.
- W4319591425 cites W2121795427 @default.
- W4319591425 cites W2137957713 @default.
- W4319591425 cites W2143468430 @default.
- W4319591425 cites W2146335359 @default.
- W4319591425 cites W2148672165 @default.
- W4319591425 cites W2164393310 @default.
- W4319591425 cites W2165372548 @default.
- W4319591425 cites W2169863525 @default.
- W4319591425 cites W2223253074 @default.
- W4319591425 cites W2254470438 @default.
- W4319591425 cites W2270122817 @default.
- W4319591425 cites W2289905436 @default.
- W4319591425 cites W2343140613 @default.
- W4319591425 cites W2411081038 @default.
- W4319591425 cites W2482412227 @default.
- W4319591425 cites W2571196594 @default.
- W4319591425 cites W2577231583 @default.
- W4319591425 cites W2732921053 @default.
- W4319591425 cites W2755027818 @default.
- W4319591425 cites W2762139206 @default.
- W4319591425 cites W2765830426 @default.
- W4319591425 cites W2794558609 @default.
- W4319591425 cites W2801355237 @default.
- W4319591425 cites W2885692583 @default.
- W4319591425 cites W2889445544 @default.
- W4319591425 cites W2896012203 @default.
- W4319591425 cites W2896625698 @default.
- W4319591425 cites W2953952753 @default.
- W4319591425 cites W2963626393 @default.
- W4319591425 cites W2982829710 @default.
- W4319591425 cites W2986612101 @default.
- W4319591425 cites W3003668048 @default.
- W4319591425 cites W3012981439 @default.
- W4319591425 cites W3014188352 @default.
- W4319591425 cites W3023355781 @default.
- W4319591425 cites W3027686705 @default.
- W4319591425 cites W3029501268 @default.
- W4319591425 cites W3037896639 @default.
- W4319591425 cites W3047986031 @default.
- W4319591425 cites W3077911205 @default.
- W4319591425 cites W3094691047 @default.
- W4319591425 cites W3098013579 @default.