First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data
Since the discovery of a flux of high-energy astrophysical neutrinos, searches for their origins have focused primarily at TeV-PeV energies. Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross section, improved angular resolution on the neutrino directio...
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| Veröffentlicht in: | Journal of cosmology and astroparticle physics 2022-01, Vol.2022 (1), p.27 |
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| creator | Andeen, K. Anton, G. Bai, X. Barbano, A. Bay, R. Beatty, J.J. Bellenghi, C. Bradascio, F. Clark, B.A. Clark, K. Correa, P. Cowen, D.F. Dembinski, H. Dvorak, E. Evenson, P.A. Filimonov, K. Fischer, L. Franckowiak, A. Fritz, A. Fürst, P. Gallagher, J. Gerhardt, L. Goldschmidt, A. Gonzalez, J.G. Grant, D. Grégoire, T. Griffith, Z. Griswold, S. Gündüz, M. Halliday, R. Halve, L. Ha Minh, M. Hardin, J. Haungs, A. Helbing, K. Hoffman, K.D. In, S. Ishihara, A. Japaridze, G.S. Jeong, M. Joppe, R. Kappes, A. Kappesser, D. Karl, M. Karle, A. Kellermann, M. Kim, J. Kopper, C. Koskinen, D.J. Kurahashi, N. Kyriacou, A. Lanfranchi, J.L. Larson, M.J. Lauber, F. Leonard, K. Lucarelli, F. Meagher, K. Mockler, D. Naab, R. Nowicki, S.C. Olivas, A. O'Sullivan, E. Parker, G.K. Paudel, E.N. Pérez de los Heros, C. Pieloth, D. Porcelli, A. Przybylski, G.T. Raab, C. Rehman, A. Renschler, M. Reusch, S. Rhode, W. Richman, M. Rott, C. Sandroos, J. Sarkar, S. Sarkar, S. Schlunder, P. Schumacher, L. Seunarine, S. Silva, M. Soldin, D. Steuer, A. Tischbein, F. Tollefson, K. Toscano, S. Tosi, D. Tselengidou, M. Twagirayezu, J.P. Unland Elorrieta, M.A. Vandenbroucke, J. Verpoest, S. Walck, C. Watson, T.B. Weaver, C. Weldert, J. Wiebusch, C.H. Woschnagg, K. Wulff, J. |
| description | Since the discovery of a flux of high-energy astrophysical neutrinos, searches for their origins have focused primarily at TeV-PeV energies. Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross section, improved angular resolution on the neutrino direction, and a reduced background from atmospheric neutrinos and muons. However, the focus on high energy does not preclude the existence of sub-TeV neutrino emission where IceCube retains sensitivity. Here we present the first all-flavor search from IceCube for transient emission of low-energy neutrinos, focusing on the energy region of 5.6-100 GeV using three years of data obtained with the IceCube-DeepCore detector. We find no evidence of transient neutrino emission in the data, thus leading to a constraint on the volumetric rate of astrophysical transient sources in the range of ∼ 705-2301 Gpc
-3
yr
-1
for sources following a subphotospheric energy spectrum with a mean energy of 100 GeV and a bolometric energy of 10
52
erg. |
| doi_str_mv | 10.1088/1475-7516/2022/01/027 |
| format | Article |
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Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross section, improved angular resolution on the neutrino direction, and a reduced background from atmospheric neutrinos and muons. However, the focus on high energy does not preclude the existence of sub-TeV neutrino emission where IceCube retains sensitivity. Here we present the first all-flavor search from IceCube for transient emission of low-energy neutrinos, focusing on the energy region of 5.6-100 GeV using three years of data obtained with the IceCube-DeepCore detector. We find no evidence of transient neutrino emission in the data, thus leading to a constraint on the volumetric rate of astrophysical transient sources in the range of ∼ 705-2301 Gpc
-3
yr
-1
for sources following a subphotospheric energy spectrum with a mean energy of 100 GeV and a bolometric energy of 10
52
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A.</creatorcontrib><creatorcontrib>Fritz, A.</creatorcontrib><creatorcontrib>Fürst, P.</creatorcontrib><creatorcontrib>Gallagher, J.</creatorcontrib><creatorcontrib>Gerhardt, L.</creatorcontrib><creatorcontrib>Goldschmidt, A.</creatorcontrib><creatorcontrib>Gonzalez, J.G.</creatorcontrib><creatorcontrib>Grant, D.</creatorcontrib><creatorcontrib>Grégoire, T.</creatorcontrib><creatorcontrib>Griffith, Z.</creatorcontrib><creatorcontrib>Griswold, S.</creatorcontrib><creatorcontrib>Gündüz, M.</creatorcontrib><creatorcontrib>Halliday, R.</creatorcontrib><creatorcontrib>Halve, L.</creatorcontrib><creatorcontrib>Ha Minh, M.</creatorcontrib><creatorcontrib>Hardin, J.</creatorcontrib><creatorcontrib>Haungs, A.</creatorcontrib><creatorcontrib>Helbing, K.</creatorcontrib><creatorcontrib>Hoffman, K.D.</creatorcontrib><creatorcontrib>In, S.</creatorcontrib><creatorcontrib>Ishihara, A.</creatorcontrib><creatorcontrib>Japaridze, G.S.</creatorcontrib><creatorcontrib>Jeong, M.</creatorcontrib><creatorcontrib>Joppe, R.</creatorcontrib><creatorcontrib>Kappes, A.</creatorcontrib><creatorcontrib>Kappesser, D.</creatorcontrib><creatorcontrib>Karl, M.</creatorcontrib><creatorcontrib>Karle, A.</creatorcontrib><creatorcontrib>Kellermann, M.</creatorcontrib><creatorcontrib>Kim, J.</creatorcontrib><creatorcontrib>Kopper, C.</creatorcontrib><creatorcontrib>Koskinen, D.J.</creatorcontrib><creatorcontrib>Kurahashi, N.</creatorcontrib><creatorcontrib>Kyriacou, A.</creatorcontrib><creatorcontrib>Lanfranchi, J.L.</creatorcontrib><creatorcontrib>Larson, M.J.</creatorcontrib><creatorcontrib>Lauber, F.</creatorcontrib><creatorcontrib>Leonard, K.</creatorcontrib><creatorcontrib>Lucarelli, F.</creatorcontrib><creatorcontrib>Meagher, K.</creatorcontrib><creatorcontrib>Mockler, D.</creatorcontrib><creatorcontrib>Naab, R.</creatorcontrib><creatorcontrib>Nowicki, S.C.</creatorcontrib><creatorcontrib>Olivas, A.</creatorcontrib><creatorcontrib>O'Sullivan, E.</creatorcontrib><creatorcontrib>Parker, G.K.</creatorcontrib><creatorcontrib>Paudel, E.N.</creatorcontrib><creatorcontrib>Pérez de los Heros, C.</creatorcontrib><creatorcontrib>Pieloth, D.</creatorcontrib><creatorcontrib>Porcelli, A.</creatorcontrib><creatorcontrib>Przybylski, G.T.</creatorcontrib><creatorcontrib>Raab, C.</creatorcontrib><creatorcontrib>Rehman, A.</creatorcontrib><creatorcontrib>Renschler, M.</creatorcontrib><creatorcontrib>Reusch, S.</creatorcontrib><creatorcontrib>Rhode, W.</creatorcontrib><creatorcontrib>Richman, M.</creatorcontrib><creatorcontrib>Rott, C.</creatorcontrib><creatorcontrib>Sandroos, J.</creatorcontrib><creatorcontrib>Sarkar, S.</creatorcontrib><creatorcontrib>Sarkar, S.</creatorcontrib><creatorcontrib>Schlunder, P.</creatorcontrib><creatorcontrib>Schumacher, L.</creatorcontrib><creatorcontrib>Seunarine, S.</creatorcontrib><creatorcontrib>Silva, M.</creatorcontrib><creatorcontrib>Soldin, D.</creatorcontrib><creatorcontrib>Steuer, A.</creatorcontrib><creatorcontrib>Tischbein, F.</creatorcontrib><creatorcontrib>Tollefson, K.</creatorcontrib><creatorcontrib>Toscano, S.</creatorcontrib><creatorcontrib>Tosi, D.</creatorcontrib><creatorcontrib>Tselengidou, M.</creatorcontrib><creatorcontrib>Twagirayezu, J.P.</creatorcontrib><creatorcontrib>Unland Elorrieta, M.A.</creatorcontrib><creatorcontrib>Vandenbroucke, J.</creatorcontrib><creatorcontrib>Verpoest, S.</creatorcontrib><creatorcontrib>Walck, C.</creatorcontrib><creatorcontrib>Watson, T.B.</creatorcontrib><creatorcontrib>Weaver, C.</creatorcontrib><creatorcontrib>Weldert, J.</creatorcontrib><creatorcontrib>Wiebusch, C.H.</creatorcontrib><creatorcontrib>Woschnagg, K.</creatorcontrib><creatorcontrib>Wulff, J.</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</creatorcontrib><title>First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data</title><title>Journal of cosmology and astroparticle physics</title><addtitle>J. Cosmol. Astropart. Phys</addtitle><description>Since the discovery of a flux of high-energy astrophysical neutrinos, searches for their origins have focused primarily at TeV-PeV energies. Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross section, improved angular resolution on the neutrino direction, and a reduced background from atmospheric neutrinos and muons. However, the focus on high energy does not preclude the existence of sub-TeV neutrino emission where IceCube retains sensitivity. Here we present the first all-flavor search from IceCube for transient emission of low-energy neutrinos, focusing on the energy region of 5.6-100 GeV using three years of data obtained with the IceCube-DeepCore detector. We find no evidence of transient neutrino emission in the data, thus leading to a constraint on the volumetric rate of astrophysical transient sources in the range of ∼ 705-2301 Gpc
-3
yr
-1
for sources following a subphotospheric energy spectrum with a mean energy of 100 GeV and a bolometric energy of 10
52
erg.</description><subject>Angular resolution</subject><subject>Emission</subject><subject>Emissions</subject><subject>Energy</subject><subject>Energy spectra</subject><subject>Flavors</subject><subject>gamma ray burst experiments</subject><subject>Muons</subject><subject>neutrino astronomy</subject><subject>neutrino experiments</subject><subject>Neutrinos</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND 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(IOP)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OIOZB</scope><scope>OTOTI</scope><scope>ADTPV</scope><scope>AOWAS</scope><scope>DG7</scope><scope>DF2</scope></search><sort><creationdate>20220101</creationdate><title>First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data</title><author>Andeen, K. ; Anton, G. ; Bai, X. ; Barbano, A. ; Bay, R. ; Beatty, J.J. ; Bellenghi, C. ; Bradascio, F. ; Clark, B.A. ; Clark, K. ; Correa, P. ; Cowen, D.F. ; Dembinski, H. ; Dvorak, E. ; Evenson, P.A. ; Filimonov, K. ; Fischer, L. ; Franckowiak, A. ; Fritz, A. ; Fürst, P. ; Gallagher, J. ; Gerhardt, L. ; Goldschmidt, A. ; Gonzalez, J.G. ; Grant, D. ; Grégoire, T. ; Griffith, Z. ; Griswold, S. ; Gündüz, M. ; Halliday, R. ; Halve, L. ; Ha Minh, M. ; Hardin, J. ; Haungs, A. ; Helbing, K. ; Hoffman, K.D. ; In, S. ; Ishihara, A. ; Japaridze, G.S. ; Jeong, M. ; Joppe, R. ; Kappes, A. ; Kappesser, D. ; Karl, M. ; Karle, A. ; Kellermann, M. ; Kim, J. ; Kopper, C. ; Koskinen, D.J. ; Kurahashi, N. ; Kyriacou, A. ; Lanfranchi, J.L. ; Larson, M.J. ; Lauber, F. ; Leonard, K. ; Lucarelli, F. ; Meagher, K. ; Mockler, D. ; Naab, R. ; Nowicki, S.C. ; Olivas, A. ; O'Sullivan, E. ; Parker, G.K. ; Paudel, E.N. ; Pérez de los Heros, C. ; Pieloth, D. ; Porcelli, A. ; Przybylski, G.T. ; Raab, C. ; Rehman, A. ; Renschler, M. ; Reusch, S. ; Rhode, W. ; Richman, M. ; Rott, C. ; Sandroos, J. ; Sarkar, S. ; Sarkar, S. ; Schlunder, P. ; Schumacher, L. ; Seunarine, S. ; Silva, M. ; Soldin, D. ; Steuer, A. ; Tischbein, F. ; Tollefson, K. ; Toscano, S. ; Tosi, D. ; Tselengidou, M. ; Twagirayezu, J.P. ; Unland Elorrieta, M.A. ; Vandenbroucke, J. ; Verpoest, S. ; Walck, C. ; Watson, T.B. ; Weaver, C. ; Weldert, J. ; Wiebusch, C.H. ; Woschnagg, K. ; Wulff, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c490t-a12fccaaa73cd877f6c7e3cf6efd870ea62fe5b078b4723d8d32afe6b624803a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Angular resolution</topic><topic>Emission</topic><topic>Emissions</topic><topic>Energy</topic><topic>Energy spectra</topic><topic>Flavors</topic><topic>gamma ray burst experiments</topic><topic>Muons</topic><topic>neutrino astronomy</topic><topic>neutrino experiments</topic><topic>Neutrinos</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>Searching</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Andeen, K.</creatorcontrib><creatorcontrib>Anton, G.</creatorcontrib><creatorcontrib>Bai, X.</creatorcontrib><creatorcontrib>Barbano, A.</creatorcontrib><creatorcontrib>Bay, R.</creatorcontrib><creatorcontrib>Beatty, 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S.</creatorcontrib><creatorcontrib>Rhode, W.</creatorcontrib><creatorcontrib>Richman, M.</creatorcontrib><creatorcontrib>Rott, C.</creatorcontrib><creatorcontrib>Sandroos, J.</creatorcontrib><creatorcontrib>Sarkar, S.</creatorcontrib><creatorcontrib>Sarkar, S.</creatorcontrib><creatorcontrib>Schlunder, P.</creatorcontrib><creatorcontrib>Schumacher, L.</creatorcontrib><creatorcontrib>Seunarine, S.</creatorcontrib><creatorcontrib>Silva, M.</creatorcontrib><creatorcontrib>Soldin, D.</creatorcontrib><creatorcontrib>Steuer, A.</creatorcontrib><creatorcontrib>Tischbein, F.</creatorcontrib><creatorcontrib>Tollefson, K.</creatorcontrib><creatorcontrib>Toscano, S.</creatorcontrib><creatorcontrib>Tosi, D.</creatorcontrib><creatorcontrib>Tselengidou, M.</creatorcontrib><creatorcontrib>Twagirayezu, J.P.</creatorcontrib><creatorcontrib>Unland Elorrieta, M.A.</creatorcontrib><creatorcontrib>Vandenbroucke, J.</creatorcontrib><creatorcontrib>Verpoest, S.</creatorcontrib><creatorcontrib>Walck, C.</creatorcontrib><creatorcontrib>Watson, T.B.</creatorcontrib><creatorcontrib>Weaver, C.</creatorcontrib><creatorcontrib>Weldert, J.</creatorcontrib><creatorcontrib>Wiebusch, C.H.</creatorcontrib><creatorcontrib>Woschnagg, K.</creatorcontrib><creatorcontrib>Wulff, J.</creatorcontrib><creatorcontrib>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><collection>SwePub</collection><collection>SwePub Articles</collection><collection>SWEPUB Stockholms universitet</collection><collection>SWEPUB Uppsala universitet</collection><jtitle>Journal of cosmology and astroparticle physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Andeen, K.</au><au>Anton, G.</au><au>Bai, X.</au><au>Barbano, A.</au><au>Bay, R.</au><au>Beatty, J.J.</au><au>Bellenghi, C.</au><au>Bradascio, F.</au><au>Clark, B.A.</au><au>Clark, K.</au><au>Correa, P.</au><au>Cowen, D.F.</au><au>Dembinski, H.</au><au>Dvorak, E.</au><au>Evenson, P.A.</au><au>Filimonov, K.</au><au>Fischer, L.</au><au>Franckowiak, A.</au><au>Fritz, A.</au><au>Fürst, P.</au><au>Gallagher, J.</au><au>Gerhardt, L.</au><au>Goldschmidt, A.</au><au>Gonzalez, J.G.</au><au>Grant, D.</au><au>Grégoire, T.</au><au>Griffith, Z.</au><au>Griswold, S.</au><au>Gündüz, M.</au><au>Halliday, R.</au><au>Halve, L.</au><au>Ha Minh, M.</au><au>Hardin, J.</au><au>Haungs, A.</au><au>Helbing, K.</au><au>Hoffman, K.D.</au><au>In, S.</au><au>Ishihara, A.</au><au>Japaridze, G.S.</au><au>Jeong, M.</au><au>Joppe, R.</au><au>Kappes, A.</au><au>Kappesser, D.</au><au>Karl, M.</au><au>Karle, A.</au><au>Kellermann, M.</au><au>Kim, J.</au><au>Kopper, C.</au><au>Koskinen, D.J.</au><au>Kurahashi, N.</au><au>Kyriacou, A.</au><au>Lanfranchi, J.L.</au><au>Larson, M.J.</au><au>Lauber, F.</au><au>Leonard, K.</au><au>Lucarelli, F.</au><au>Meagher, K.</au><au>Mockler, D.</au><au>Naab, R.</au><au>Nowicki, S.C.</au><au>Olivas, A.</au><au>O'Sullivan, E.</au><au>Parker, G.K.</au><au>Paudel, E.N.</au><au>Pérez de los Heros, C.</au><au>Pieloth, D.</au><au>Porcelli, A.</au><au>Przybylski, G.T.</au><au>Raab, C.</au><au>Rehman, A.</au><au>Renschler, M.</au><au>Reusch, S.</au><au>Rhode, W.</au><au>Richman, M.</au><au>Rott, C.</au><au>Sandroos, J.</au><au>Sarkar, S.</au><au>Sarkar, S.</au><au>Schlunder, P.</au><au>Schumacher, L.</au><au>Seunarine, S.</au><au>Silva, M.</au><au>Soldin, D.</au><au>Steuer, A.</au><au>Tischbein, F.</au><au>Tollefson, K.</au><au>Toscano, S.</au><au>Tosi, D.</au><au>Tselengidou, M.</au><au>Twagirayezu, J.P.</au><au>Unland Elorrieta, M.A.</au><au>Vandenbroucke, J.</au><au>Verpoest, S.</au><au>Walck, C.</au><au>Watson, T.B.</au><au>Weaver, C.</au><au>Weldert, J.</au><au>Wiebusch, C.H.</au><au>Woschnagg, K.</au><au>Wulff, J.</au><aucorp>Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data</atitle><jtitle>Journal of cosmology and astroparticle physics</jtitle><addtitle>J. Cosmol. Astropart. Phys</addtitle><date>2022-01-01</date><risdate>2022</risdate><volume>2022</volume><issue>1</issue><spage>27</spage><pages>27-</pages><issn>1475-7516</issn><eissn>1475-7516</eissn><abstract>Since the discovery of a flux of high-energy astrophysical neutrinos, searches for their origins have focused primarily at TeV-PeV energies. Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross section, improved angular resolution on the neutrino direction, and a reduced background from atmospheric neutrinos and muons. However, the focus on high energy does not preclude the existence of sub-TeV neutrino emission where IceCube retains sensitivity. Here we present the first all-flavor search from IceCube for transient emission of low-energy neutrinos, focusing on the energy region of 5.6-100 GeV using three years of data obtained with the IceCube-DeepCore detector. We find no evidence of transient neutrino emission in the data, thus leading to a constraint on the volumetric rate of astrophysical transient sources in the range of ∼ 705-2301 Gpc
-3
yr
-1
for sources following a subphotospheric energy spectrum with a mean energy of 100 GeV and a bolometric energy of 10
52
erg.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1475-7516/2022/01/027</doi><tpages>21</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1475-7516 |
| ispartof | Journal of cosmology and astroparticle physics, 2022-01, Vol.2022 (1), p.27 |
| issn | 1475-7516 1475-7516 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1859718 |
| source | IOP Publishing Journals; Institute of Physics (IOP) Journals - HEAL-Link |
| subjects | Angular resolution Emission Emissions Energy Energy spectra Flavors gamma ray burst experiments Muons neutrino astronomy neutrino experiments Neutrinos PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Searching |
| title | First all-flavor search for transient neutrino emission using 3-years of IceCube DeepCore data |
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