Sökning: WFRF:(Olivo A.) > Searching for soft ...
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000 | 13542naa a2203577 4500 | |
001 | oai:DiVA.org:uu-175862 | |
003 | SwePub | |
008 | 120613s2012 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-74258 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1758622 URI |
024 | 7 | a https://doi.org/10.1051/0004-6361/2011180712 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-742582 URI |
040 | a (SwePub)uud (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Abbasi, R.4 aut |
245 | 1 0 | a Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program |
264 | c 2012-02-24 | |
264 | 1 | b EDP Sciences,c 2012 |
338 | a print2 rdacarrier | |
500 | a Publikationen har totalt 263 författare, R. Abbasi et al. | |
520 | a Context. Transient neutrino sources such as gamma-ray bursts (GRBs) and supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of less than or similar to 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. Aims. 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. Methods. If a neutrino multiplet, i.e. 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. Results. No statistically significant excess in the rate of neutrino multiplets has been observed and furthermore no coincidence with an optical counterpart was found. Conclusions. The search allows, for the first time, to set stringent limits on current models predicting a high-energy neutrino flux from soft relativistic hadronic jets in core-collapse SNe. We conclude that a sub-population of SNe with typical Lorentz boost factor and jet energy of 10 and 3 x 1051 erg, respectively, does not exceed 4.2% at 90% confidence. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
653 | a neutrinos | |
653 | a supernovae: general | |
653 | a gamma-ray burst: general | |
653 | a Physics | |
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773 | 0 | t Astronomy and Astrophysicsd : EDP Sciencesg 539, s. A60-q 539<A60-x 0004-6361x 1432-0746 |
856 | 4 | u https://www.aanda.org/articles/aa/pdf/2012/03/aa18071-11.pdf |
856 | 4 | u https://doi.org/10.1051/0004-6361/201118071y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-175862 |
856 | 4 8 | u https://doi.org/10.1051/0004-6361/201118071 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-74258 |
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