Atmospheric results from Super-Kamiokande
Recent results from a 282 kiloton-year exposure of the Super-Kamiokande detector to atmospheric neutrinos are presented. The data when fit both by themselves and in conjunction with constraints from the T2K and reactor neutrino experiments show a weak, though insignificant, preference for the normal...
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description | Recent results from a 282 kiloton-year exposure of the Super-Kamiokande detector to atmospheric neutrinos are presented. The data when fit both by themselves and in conjunction with constraints from the T2K and reactor neutrino experiments show a weak, though insignificant, preference for the normal mass hierarchy at the level of~ 1σ. Searches for 2 evidence of oscillations into a sterile neutrino have resulted in limits on the parameters governing their mixing, |Uμ4|2 < 0.041 and |Uτ4|2 < 0.18 at 90% C.L. A similar search for an indication of Lorentz-invariance violating oscillations has yielded limits three to seven orders of magnitude more stringent than existing measurements. Additionally, analyses searching for an excess of neutrinos in the atmospheric data produced from the annihilation of dark matter particles in the galaxy and sun have placed tight limits on the cross sections governing their annihilation and scattering. |
doi_str_mv | 10.1063/1.4915569 |
format | Conference Proceeding |
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The data when fit both by themselves and in conjunction with constraints from the T2K and reactor neutrino experiments show a weak, though insignificant, preference for the normal mass hierarchy at the level of~ 1σ. Searches for 2 evidence of oscillations into a sterile neutrino have resulted in limits on the parameters governing their mixing, |Uμ4|2 < 0.041 and |Uτ4|2 < 0.18 at 90% C.L. A similar search for an indication of Lorentz-invariance violating oscillations has yielded limits three to seven orders of magnitude more stringent than existing measurements. 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The data when fit both by themselves and in conjunction with constraints from the T2K and reactor neutrino experiments show a weak, though insignificant, preference for the normal mass hierarchy at the level of~ 1σ. Searches for 2 evidence of oscillations into a sterile neutrino have resulted in limits on the parameters governing their mixing, |Uμ4|2 < 0.041 and |Uτ4|2 < 0.18 at 90% C.L. A similar search for an indication of Lorentz-invariance violating oscillations has yielded limits three to seven orders of magnitude more stringent than existing measurements. Additionally, analyses searching for an excess of neutrinos in the atmospheric data produced from the annihilation of dark matter particles in the galaxy and sun have placed tight limits on the cross sections governing their annihilation and scattering.</description><subject>ANNIHILATION</subject><subject>CROSS SECTIONS</subject><subject>Dark matter</subject><subject>Experiments</subject><subject>GALAXIES</subject><subject>LIMITING VALUES</subject><subject>LORENTZ INVARIANCE</subject><subject>MULTIPARTICLE SPECTROMETERS</subject><subject>NEUTRINO DETECTION</subject><subject>NEUTRINO OSCILLATION</subject><subject>NEUTRINOS</subject><subject>NONLUMINOUS MATTER</subject><subject>Oscillations</subject><subject>PARTICLE IDENTIFICATION</subject><subject>Particle physics</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>SCATTERING</subject><subject>SUN</subject><subject>WEINBERG ANGLE</subject><subject>YIELDS</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2015</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNpFjstKxDAUQIMoWEcX_kHBlYuM9yZpHsth8IUDLlRwV9JMwnScNjVJ_98BBVdnczgcQq4RlgiS3-FSGGwaaU5IdSRSJVGekgrACMoE_zwnFznvAZhRSlfkdlWGmKedT72rk8_zoeQ6pDjUb_PkE32xQx-_7Lj1l-Qs2EP2V39ckI-H-_f1E928Pj6vVxsamZCFSseYZcAZ10Gj0chdowMAD4IrpbwBDc6CRdVo37lgfMe3sgudkg6ajvMFufntxlz6Nru-eLdzcRy9Ky1jwoAU-t-aUvyefS7tPs5pPI61DJlA1EYB_wGUz00A</recordid><startdate>20150715</startdate><enddate>20150715</enddate><creator>Wendell, Roger</creator><general>American Institute of Physics</general><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20150715</creationdate><title>Atmospheric results from Super-Kamiokande</title><author>Wendell, Roger</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o246t-6c22a203238f819813c58f003f43777e9080ca0a1758ebcf9eb3d6bfb76c05b33</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2015</creationdate><topic>ANNIHILATION</topic><topic>CROSS SECTIONS</topic><topic>Dark matter</topic><topic>Experiments</topic><topic>GALAXIES</topic><topic>LIMITING VALUES</topic><topic>LORENTZ INVARIANCE</topic><topic>MULTIPARTICLE SPECTROMETERS</topic><topic>NEUTRINO DETECTION</topic><topic>NEUTRINO OSCILLATION</topic><topic>NEUTRINOS</topic><topic>NONLUMINOUS MATTER</topic><topic>Oscillations</topic><topic>PARTICLE IDENTIFICATION</topic><topic>Particle physics</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>SCATTERING</topic><topic>SUN</topic><topic>WEINBERG ANGLE</topic><topic>YIELDS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wendell, Roger</creatorcontrib><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wendell, Roger</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Atmospheric results from Super-Kamiokande</atitle><btitle>AIP conference proceedings</btitle><date>2015-07-15</date><risdate>2015</risdate><volume>1666</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>Recent results from a 282 kiloton-year exposure of the Super-Kamiokande detector to atmospheric neutrinos are presented. The data when fit both by themselves and in conjunction with constraints from the T2K and reactor neutrino experiments show a weak, though insignificant, preference for the normal mass hierarchy at the level of~ 1σ. Searches for 2 evidence of oscillations into a sterile neutrino have resulted in limits on the parameters governing their mixing, |Uμ4|2 < 0.041 and |Uτ4|2 < 0.18 at 90% C.L. A similar search for an indication of Lorentz-invariance violating oscillations has yielded limits three to seven orders of magnitude more stringent than existing measurements. Additionally, analyses searching for an excess of neutrinos in the atmospheric data produced from the annihilation of dark matter particles in the galaxy and sun have placed tight limits on the cross sections governing their annihilation and scattering.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4915569</doi><oa>free_for_read</oa></addata></record> |
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source | AIP Journals Complete |
subjects | ANNIHILATION CROSS SECTIONS Dark matter Experiments GALAXIES LIMITING VALUES LORENTZ INVARIANCE MULTIPARTICLE SPECTROMETERS NEUTRINO DETECTION NEUTRINO OSCILLATION NEUTRINOS NONLUMINOUS MATTER Oscillations PARTICLE IDENTIFICATION Particle physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS SCATTERING SUN WEINBERG ANGLE YIELDS |
title | Atmospheric results from Super-Kamiokande |
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