Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program
Transient neutrino sources such as gamma-ray bursts (GRB) and supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of ...100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stal...
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| Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2012-03, Vol.539, p.1-1 |
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| creator | Abbasi, R Abdou, Y Abu-Zayyad, T Ackermann, M Adams, J Aguilar, J A Ahlers, M Allen, M M Altmann, D Andeen, K Hanson, K Heinen, D Helbing, K Hellauer, R Herquet, P Hickford, S Hill, G C Hoffman, K D Hoffmann, B Homeier, A Auffenberg, J Hoshina, K Huelsnitz, W Huel beta, J-P Hulth, P O Hultqvist, K Hussain, S Ishihara, A Jacobi, E Jacobsen, J Japaridze, G S Bai, X Johansson, H Kampert, K-H Kappes, A Karg, T Karle, A Kenny, P Kiryluk, J Kislat, F Klein, S R Kohne, J-H Baker, M Kohnen, G Kolanoski, H Kopke, L Kopper, S Koskinen, D J Kowalski, M Kowarik, T et. al |
| description | Transient neutrino sources such as gamma-ray bursts (GRB) and supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of ...100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. To increase the sensitivity to these neutrinos and identify their sources, a low-threshold optical follow-up program for neutrino multiplets detected with the IceCube observatory has been implemented. If a neutrino multiplet, ie two or more neutrinos from the same direction within 100 s, is found by IceCube a trigger is sent to the Robotic Optical Transient Search Experiment (ROTSE). The 4 ROTSE telescopes immediately start an observation program of the corresponding region of the sky in order to detect an optical counterpart to the neutrino events. No statistically significant excess in the rate of neutrino multiplets has been observed and furthermore no coincidence with an optical counterpart was found. (ProQuest: ... denotes formulae/symbols omitted.) |
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While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. To increase the sensitivity to these neutrinos and identify their sources, a low-threshold optical follow-up program for neutrino multiplets detected with the IceCube observatory has been implemented. If a neutrino multiplet, ie two or more neutrinos from the same direction within 100 s, is found by IceCube a trigger is sent to the Robotic Optical Transient Search Experiment (ROTSE). The 4 ROTSE telescopes immediately start an observation program of the corresponding region of the sky in order to detect an optical counterpart to the neutrino events. No statistically significant excess in the rate of neutrino multiplets has been observed and furthermore no coincidence with an optical counterpart was found. 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While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. To increase the sensitivity to these neutrinos and identify their sources, a low-threshold optical follow-up program for neutrino multiplets detected with the IceCube observatory has been implemented. If a neutrino multiplet, ie two or more neutrinos from the same direction within 100 s, is found by IceCube a trigger is sent to the Robotic Optical Transient Search Experiment (ROTSE). The 4 ROTSE telescopes immediately start an observation program of the corresponding region of the sky in order to detect an optical counterpart to the neutrino events. No statistically significant excess in the rate of neutrino multiplets has been observed and furthermore no coincidence with an optical counterpart was found. 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follow-up program</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2012-03-01</date><risdate>2012</risdate><volume>539</volume><spage>1</spage><epage>1</epage><pages>1-1</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><abstract>Transient neutrino sources such as gamma-ray bursts (GRB) and supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of ...100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. To increase the sensitivity to these neutrinos and identify their sources, a low-threshold optical follow-up program for neutrino multiplets detected with the IceCube observatory has been implemented. If a neutrino multiplet, ie two or more neutrinos from the same direction within 100 s, is found by IceCube a trigger is sent to the Robotic Optical Transient Search Experiment (ROTSE). The 4 ROTSE telescopes immediately start an observation program of the corresponding region of the sky in order to detect an optical counterpart to the neutrino events. No statistically significant excess in the rate of neutrino multiplets has been observed and furthermore no coincidence with an optical counterpart was found. (ProQuest: ... denotes formulae/symbols omitted.)</abstract></addata></record> |
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| title | Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program |
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