Forty Years to the Artemovsk Scintillation Detector for Neutrinos
The current status of the ASD (Artemovsk scintillation detector) experiment aimed at search for a neutrino flux from gravitational collapses of stellar cores is presented. Experimental data obtained for 40 years of operation of the detector situated in a salt mine at a depth of 570 mwe are processed...
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| Veröffentlicht in: | Physics of atomic nuclei 2018-01, Vol.81 (1), p.88-94 |
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| creator | Antonenko, A. G. Borshchevsky, V. P. Enikeev, R. I. Ochkas, O. V. Ryazhskaya, O. G. Chernyshov, L. V. Yarosh, A. P. Iarosh, N. A. |
| description | The current status of the ASD (Artemovsk scintillation detector) experiment aimed at search for a neutrino flux from gravitational collapses of stellar cores is presented. Experimental data obtained for 40 years of operation of the detector situated in a salt mine at a depth of 570 mwe are processed. The results obtained by calculating the expected signal in the detector on the basis of two models of supernova explosion are described. No candidates for neutrino bursts from gravitational star collapses have been revealed: the limit on the frequency of gravitational collapses was found to be less than one event per 17.15 yr at a 90% confidence level (
f
col
< 0.058 yr
−1
). |
| doi_str_mv | 10.1134/S1063778818010040 |
| format | Article |
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f
col
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−1
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f
col
< 0.058 yr
−1
).</description><subject>Analysis</subject><subject>Astronomy</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Confidence intervals</subject><subject>DEPTH</subject><subject>Detection equipment</subject><subject>Elementary Particles and Fields Experiment</subject><subject>EXPLOSIONS</subject><subject>Gravitation</subject><subject>GRAVITATIONAL COLLAPSE</subject><subject>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</subject><subject>NEUTRINO DETECTION</subject><subject>NEUTRINOS</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Scintillation</subject><subject>SCINTILLATION COUNTERS</subject><subject>Sensors</subject><subject>Signal processing</subject><subject>SIGNALS</subject><subject>STARS</subject><subject>Stellar cores</subject><subject>SUPERNOVAE</subject><issn>1063-7788</issn><issn>1562-692X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kdtKAzEQhhdR8PgA3i145cVqJskmm8tSTwVRsAp6FdJ0tkbbTU1SsW9vpEIpIiHkMN83_DBFcQzkDIDx8yEQwaRsGmgIEMLJVrEHtaCVUPR5O99zufqp7xb7Mb4RAtDUZK_oXfmQluULmhDL5Mv0imUvJJz5z_heDq3rkptOTXK-Ky8woU0-lG3ed7hIwXU-HhY7rZlGPPo9D4qnq8vH_k11e3896PduK8tBpkoiA2HMCLloTVuLMVMN1BJHylJRA1XECsMsa4DDyOT3WFlJLSo0io8NYwfFyaqvj8npaF0O82p91-VMmlIpQNZqTc2D_1hgTPrNL0KXg2lKKJNcSdpk6mxFTcwUtetan4KxeY1x5nJPbF3-79WcUy5zoCycbgiZSfiVJmYRox4MHzZZWLE2-BgDtnoe3MyEpQaif4al_wwrO3TlxMx2Ewzr2P9L3zaQk1s</recordid><startdate>20180101</startdate><enddate>20180101</enddate><creator>Antonenko, A. G.</creator><creator>Borshchevsky, V. P.</creator><creator>Enikeev, R. I.</creator><creator>Ochkas, O. V.</creator><creator>Ryazhskaya, O. G.</creator><creator>Chernyshov, L. V.</creator><creator>Yarosh, A. P.</creator><creator>Iarosh, N. A.</creator><general>Pleiades Publishing</general><general>Springer</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>ISR</scope><scope>OTOTI</scope></search><sort><creationdate>20180101</creationdate><title>Forty Years to the Artemovsk Scintillation Detector for Neutrinos</title><author>Antonenko, A. G. ; Borshchevsky, V. P. ; Enikeev, R. I. ; Ochkas, O. V. ; Ryazhskaya, O. G. ; Chernyshov, L. V. ; Yarosh, A. P. ; Iarosh, N. 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G.</creatorcontrib><creatorcontrib>Borshchevsky, V. P.</creatorcontrib><creatorcontrib>Enikeev, R. I.</creatorcontrib><creatorcontrib>Ochkas, O. V.</creatorcontrib><creatorcontrib>Ryazhskaya, O. G.</creatorcontrib><creatorcontrib>Chernyshov, L. V.</creatorcontrib><creatorcontrib>Yarosh, A. P.</creatorcontrib><creatorcontrib>Iarosh, N. A.</creatorcontrib><collection>CrossRef</collection><collection>Gale In Context: Science</collection><collection>OSTI.GOV</collection><jtitle>Physics of atomic nuclei</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Antonenko, A. G.</au><au>Borshchevsky, V. P.</au><au>Enikeev, R. I.</au><au>Ochkas, O. V.</au><au>Ryazhskaya, O. G.</au><au>Chernyshov, L. V.</au><au>Yarosh, A. P.</au><au>Iarosh, N. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Forty Years to the Artemovsk Scintillation Detector for Neutrinos</atitle><jtitle>Physics of atomic nuclei</jtitle><stitle>Phys. Atom. Nuclei</stitle><date>2018-01-01</date><risdate>2018</risdate><volume>81</volume><issue>1</issue><spage>88</spage><epage>94</epage><pages>88-94</pages><issn>1063-7788</issn><eissn>1562-692X</eissn><abstract>The current status of the ASD (Artemovsk scintillation detector) experiment aimed at search for a neutrino flux from gravitational collapses of stellar cores is presented. Experimental data obtained for 40 years of operation of the detector situated in a salt mine at a depth of 570 mwe are processed. The results obtained by calculating the expected signal in the detector on the basis of two models of supernova explosion are described. No candidates for neutrino bursts from gravitational star collapses have been revealed: the limit on the frequency of gravitational collapses was found to be less than one event per 17.15 yr at a 90% confidence level (
f
col
< 0.058 yr
−1
).</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S1063778818010040</doi><tpages>7</tpages></addata></record> |
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| subjects | Analysis Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Confidence intervals DEPTH Detection equipment Elementary Particles and Fields Experiment EXPLOSIONS Gravitation GRAVITATIONAL COLLAPSE INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY NEUTRINO DETECTION NEUTRINOS Particle and Nuclear Physics Physics Physics and Astronomy Scintillation SCINTILLATION COUNTERS Sensors Signal processing SIGNALS STARS Stellar cores SUPERNOVAE |
| title | Forty Years to the Artemovsk Scintillation Detector for Neutrinos |
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