A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

© 2020. The American Astronomical Society. All rights reserved. During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy upgoing air...

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Format: Article in Journal/Newspaper
Language:English
Published: American Astronomical Society 2020
Subjects:
Online Access:https://hdl.handle.net/1721.1/132208
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spelling ftmit:oai:dspace.mit.edu:1721.1/132208 2023-06-11T04:06:15+02:00 A Search for IceCube Events in the Direction of ANITA Neutrino Candidates 2020-09-24T17:09:07Z application/pdf https://hdl.handle.net/1721.1/132208 en eng American Astronomical Society 10.3847/1538-4357/ab791d Astrophysical Journal https://hdl.handle.net/1721.1/132208 Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The American Astronomical Society Article http://purl.org/eprint/type/JournalArticle 2020 ftmit 2023-05-29T08:55:19Z © 2020. The American Astronomical Society. All rights reserved. During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy upgoing air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here we test the hypothesis that these events are astrophysical in origin, possibly caused by a point source in the reconstructed direction. Given that any ultra-high-energy tau neutrino flux traversing the Earth should be accompanied by a secondary flux in the TeV-PeV range, we search for these secondary counterparts in 7 yr of IceCube data using three complementary approaches. In the absence of any significant detection, we set upper limits on the neutrino flux from potential point sources. We compare these limits to ANITA's sensitivity in the same direction and show that an astrophysical explanation of these anomalous events under standard model assumptions is severely constrained regardless of source spectrum. Article in Journal/Newspaper Antarc* Antarctic DSpace@MIT (Massachusetts Institute of Technology) Antarctic The Antarctic
institution Open Polar
collection DSpace@MIT (Massachusetts Institute of Technology)
op_collection_id ftmit
language English
description © 2020. The American Astronomical Society. All rights reserved. During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy upgoing air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here we test the hypothesis that these events are astrophysical in origin, possibly caused by a point source in the reconstructed direction. Given that any ultra-high-energy tau neutrino flux traversing the Earth should be accompanied by a secondary flux in the TeV-PeV range, we search for these secondary counterparts in 7 yr of IceCube data using three complementary approaches. In the absence of any significant detection, we set upper limits on the neutrino flux from potential point sources. We compare these limits to ANITA's sensitivity in the same direction and show that an astrophysical explanation of these anomalous events under standard model assumptions is severely constrained regardless of source spectrum.
format Article in Journal/Newspaper
title A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
spellingShingle A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
title_short A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
title_full A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
title_fullStr A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
title_full_unstemmed A Search for IceCube Events in the Direction of ANITA Neutrino Candidates
title_sort search for icecube events in the direction of anita neutrino candidates
publisher American Astronomical Society
publishDate 2020
url https://hdl.handle.net/1721.1/132208
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source The American Astronomical Society
op_relation 10.3847/1538-4357/ab791d
Astrophysical Journal
https://hdl.handle.net/1721.1/132208
op_rights Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
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