Search for neutrino-induced particle showers with IceCube-40
We report on the search for neutrino-induced particle-showers, so-called cascades, in the IceCube-40 detector. The data for this search was collected between April 2008 and May 2009 when the first 40 IceCube strings were deployed and operational. Three complementary searches were performed, each opt...
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| Format: | Journal article |
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American Physical Society
2014
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| _version_ | 1797087649464320000 |
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| author | Aartsen, MG Sarkar, S |
| author_facet | Aartsen, MG Sarkar, S |
| author_sort | Aartsen, MG |
| collection | OXFORD |
| description | We report on the search for neutrino-induced particle-showers, so-called cascades, in the IceCube-40 detector. The data for this search was collected between April 2008 and May 2009 when the first 40 IceCube strings were deployed and operational. Three complementary searches were performed, each optimized for different energy regimes. The analysis with the lowest energy threshold (2 TeV) targeted atmospheric neutrinos. A total of 67 events were found, consistent with the expectation of 41 atmospheric muons and 30 atmospheric neutrino events. The two other analyses targeted a harder, astrophysical neutrino flux. The analysis with an intermediate threshold of 25 TeV lead to the observation of 14 cascade-like events, again consistent with the prediction of 3.0 atmospheric neutrino and 7.7 atmospheric muon events. We hence set an upper limit of $E^2 \Phi_{lim} \leq 7.46\times10^{-8}\,\mathrm{GeV sr^{-1} s^{-1} cm^{-2}}$ (90% C.L.) on the diffuse flux from astrophysical neutrinos of all neutrino flavors, applicable to the energy range 25 TeV to 5 PeV, assuming an $E_{\nu}^{-2}$ spectrum and a neutrino flavor ratio of 1:1:1 at the Earth. The third analysis utilized a larger and optimized sample of atmospheric muon background simulation, leading to a higher energy threshold of 100 TeV. Three events were found over a background prediction of 0.04 atmospheric muon events and 0.21 events from the flux of conventional and prompt atmospheric neutrinos. Including systematic errors this corresponds to a $2.7\sigma$ excess with respect to the background-only hypothesis. Our observation of neutrino event candidates above 100 TeV complements IceCube's recently observed evidence for high-energy astrophysical neutrinos. |
| first_indexed | 2024-03-07T02:38:41Z |
| format | Journal article |
| id | oxford-uuid:a9ae8f46-33e6-4953-bef5-b94ccaee9778 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T02:38:41Z |
| publishDate | 2014 |
| publisher | American Physical Society |
| record_format | dspace |
| spelling | oxford-uuid:a9ae8f46-33e6-4953-bef5-b94ccaee97782022-03-27T03:10:03ZSearch for neutrino-induced particle showers with IceCube-40Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:a9ae8f46-33e6-4953-bef5-b94ccaee9778Symplectic Elements at OxfordAmerican Physical Society2014Aartsen, MGSarkar, SWe report on the search for neutrino-induced particle-showers, so-called cascades, in the IceCube-40 detector. The data for this search was collected between April 2008 and May 2009 when the first 40 IceCube strings were deployed and operational. Three complementary searches were performed, each optimized for different energy regimes. The analysis with the lowest energy threshold (2 TeV) targeted atmospheric neutrinos. A total of 67 events were found, consistent with the expectation of 41 atmospheric muons and 30 atmospheric neutrino events. The two other analyses targeted a harder, astrophysical neutrino flux. The analysis with an intermediate threshold of 25 TeV lead to the observation of 14 cascade-like events, again consistent with the prediction of 3.0 atmospheric neutrino and 7.7 atmospheric muon events. We hence set an upper limit of $E^2 \Phi_{lim} \leq 7.46\times10^{-8}\,\mathrm{GeV sr^{-1} s^{-1} cm^{-2}}$ (90% C.L.) on the diffuse flux from astrophysical neutrinos of all neutrino flavors, applicable to the energy range 25 TeV to 5 PeV, assuming an $E_{\nu}^{-2}$ spectrum and a neutrino flavor ratio of 1:1:1 at the Earth. The third analysis utilized a larger and optimized sample of atmospheric muon background simulation, leading to a higher energy threshold of 100 TeV. Three events were found over a background prediction of 0.04 atmospheric muon events and 0.21 events from the flux of conventional and prompt atmospheric neutrinos. Including systematic errors this corresponds to a $2.7\sigma$ excess with respect to the background-only hypothesis. Our observation of neutrino event candidates above 100 TeV complements IceCube's recently observed evidence for high-energy astrophysical neutrinos. |
| spellingShingle | Aartsen, MG Sarkar, S Search for neutrino-induced particle showers with IceCube-40 |
| title | Search for neutrino-induced particle showers with IceCube-40 |
| title_full | Search for neutrino-induced particle showers with IceCube-40 |
| title_fullStr | Search for neutrino-induced particle showers with IceCube-40 |
| title_full_unstemmed | Search for neutrino-induced particle showers with IceCube-40 |
| title_short | Search for neutrino-induced particle showers with IceCube-40 |
| title_sort | search for neutrino induced particle showers with icecube 40 |
| work_keys_str_mv | AT aartsenmg searchforneutrinoinducedparticleshowerswithicecube40 AT sarkars searchforneutrinoinducedparticleshowerswithicecube40 |