dc.contributor.author | Reusch, Simeon ,et.al. | |
dc.contributor.author | Paliya, Vaidehi S. | |
dc.date.accessioned | 2024-05-09T07:01:21Z | |
dc.date.available | 2024-05-09T07:01:21Z | |
dc.date.issued | 2022-06 | |
dc.identifier.uri | https://doi.org/10.1103/PhysRevLett.128.221101 | |
dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/1581 | |
dc.description.abstract | The origins of the high-energy cosmic neutrino flux remain largely unknown. Recently, one high-energy neutrino was associated with a tidal disruption event (TDE). Here we present AT2019fdr, an exceptionally luminous TDE candidate, coincident with another high-energy neutrino. Our observations, including a bright dust echo and soft late-time x-ray emission, further support a TDE origin of this flare. The probability of finding two such bright events by chance is just 0.034%. We evaluate several models for neutrino production and show that AT2019fdr is capable of producing the observed high-energy neutrino, reinforcing the case for TDEs as neutrino sources | en_US |
dc.language.iso | en | en_US |
dc.publisher | Physical Review Letters | en_US |
dc.relation.ispartofseries | 1882;prl128-221101 | |
dc.subject | Tidal Disruption | en_US |
dc.subject | AT2019fdr | en_US |
dc.subject | High-Energy Neutrino | en_US |
dc.title | Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino | en_US |
dc.type | Article | en_US |