Loading…

Can lepton flavor violating interactions explain the atmospheric neutrino problem?

We investigate whether flavor changing neutrino interactions (FCNIs) can be sufficiently large to provide a viable solution to the atmospheric neutrino problem. Effective operators induced by heavy boson exchange that allow for flavor changing neutrino scattering off quarks or electrons are related...

Full description

Saved in:
Bibliographic Details
Published in:Physical review. D, Particles and fields Particles and fields, 2000-03, Vol.61 (5), Article 053005
Main Authors: Bergmann, Sven, Grossman, Yuval, Pierce, Damien M.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983
cites cdi_FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983
container_end_page
container_issue 5
container_start_page
container_title Physical review. D, Particles and fields
container_volume 61
creator Bergmann, Sven
Grossman, Yuval
Pierce, Damien M.
description We investigate whether flavor changing neutrino interactions (FCNIs) can be sufficiently large to provide a viable solution to the atmospheric neutrino problem. Effective operators induced by heavy boson exchange that allow for flavor changing neutrino scattering off quarks or electrons are related by an SU(2){sub L} rotation to operators that induce anomalous tau decays. Since SU(2){sub L} violation is small for new physics at or above the weak scale, one can use the upper bounds on lepton flavor violating tau decays or on lepton universality violation to put severe, model-independent bounds on the relevant non-standard neutrino interactions. Also Z-induced flavor changing neutral currents, due to heavy singlet neutrinos, are too small to be relevant for the atmospheric neutrino anomaly. We conclude that the FCNI solution to the atmospheric neutrino problem is ruled out. (c) 2000 The American Physical Society.
doi_str_mv 10.1103/PhysRevD.61.053005
format article
fullrecord <record><control><sourceid>crossref_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_20215918</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>10_1103_PhysRevD_61_053005</sourcerecordid><originalsourceid>FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983</originalsourceid><addsrcrecordid>eNo1kE1LAzEURYMoWKt_wFXA9dT3kiYzsxKpn1BQSvchSTNOZJoMSSz231up3s3dHC7cQ8g1wgwR-O17v88rt3uYSZyB4ADihEwQmraat9ickgkIISvWMDwnFzl_wiFM8glZLXSggxtLDLQb9C4muvNx0MWHD-pDcUnb4mPI1H2Pg_aBlt5RXbYxj71L3tLgvkryIdIxRTO47d0lOev0kN3VX0_J-ulxvXiplm_Pr4v7ZWVZLUpVM8PYhnHewVyLGqzkojbAeNtsDDcNohYgpNGCC2i1MUwKM7dYcxTYNnxKbo6zMRevsvXF2d7GEJwtigFDcXh-oNiRsinmnFynxuS3Ou0VgvpVp_7VKYnqqI7_ACkaY3k</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Can lepton flavor violating interactions explain the atmospheric neutrino problem?</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Bergmann, Sven ; Grossman, Yuval ; Pierce, Damien M.</creator><creatorcontrib>Bergmann, Sven ; Grossman, Yuval ; Pierce, Damien M.</creatorcontrib><description>We investigate whether flavor changing neutrino interactions (FCNIs) can be sufficiently large to provide a viable solution to the atmospheric neutrino problem. Effective operators induced by heavy boson exchange that allow for flavor changing neutrino scattering off quarks or electrons are related by an SU(2){sub L} rotation to operators that induce anomalous tau decays. Since SU(2){sub L} violation is small for new physics at or above the weak scale, one can use the upper bounds on lepton flavor violating tau decays or on lepton universality violation to put severe, model-independent bounds on the relevant non-standard neutrino interactions. Also Z-induced flavor changing neutral currents, due to heavy singlet neutrinos, are too small to be relevant for the atmospheric neutrino anomaly. We conclude that the FCNI solution to the atmospheric neutrino problem is ruled out. (c) 2000 The American Physical Society.</description><identifier>ISSN: 0556-2821</identifier><identifier>EISSN: 1089-4918</identifier><identifier>DOI: 10.1103/PhysRevD.61.053005</identifier><language>eng</language><publisher>United States</publisher><subject>COSMIC NEUTRINOS ; EARTH ATMOSPHERE ; ELECTRON NEUTRINOS ; MUON NEUTRINOS ; NEUTRINO-ELECTRON INTERACTIONS ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; SU-2 GROUPS ; TAU NEUTRINOS ; TAU PARTICLES ; THEORETICAL DATA</subject><ispartof>Physical review. D, Particles and fields, 2000-03, Vol.61 (5), Article 053005</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983</citedby><cites>FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/20215918$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Bergmann, Sven</creatorcontrib><creatorcontrib>Grossman, Yuval</creatorcontrib><creatorcontrib>Pierce, Damien M.</creatorcontrib><title>Can lepton flavor violating interactions explain the atmospheric neutrino problem?</title><title>Physical review. D, Particles and fields</title><description>We investigate whether flavor changing neutrino interactions (FCNIs) can be sufficiently large to provide a viable solution to the atmospheric neutrino problem. Effective operators induced by heavy boson exchange that allow for flavor changing neutrino scattering off quarks or electrons are related by an SU(2){sub L} rotation to operators that induce anomalous tau decays. Since SU(2){sub L} violation is small for new physics at or above the weak scale, one can use the upper bounds on lepton flavor violating tau decays or on lepton universality violation to put severe, model-independent bounds on the relevant non-standard neutrino interactions. Also Z-induced flavor changing neutral currents, due to heavy singlet neutrinos, are too small to be relevant for the atmospheric neutrino anomaly. We conclude that the FCNI solution to the atmospheric neutrino problem is ruled out. (c) 2000 The American Physical Society.</description><subject>COSMIC NEUTRINOS</subject><subject>EARTH ATMOSPHERE</subject><subject>ELECTRON NEUTRINOS</subject><subject>MUON NEUTRINOS</subject><subject>NEUTRINO-ELECTRON INTERACTIONS</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>SU-2 GROUPS</subject><subject>TAU NEUTRINOS</subject><subject>TAU PARTICLES</subject><subject>THEORETICAL DATA</subject><issn>0556-2821</issn><issn>1089-4918</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><recordid>eNo1kE1LAzEURYMoWKt_wFXA9dT3kiYzsxKpn1BQSvchSTNOZJoMSSz231up3s3dHC7cQ8g1wgwR-O17v88rt3uYSZyB4ADihEwQmraat9ickgkIISvWMDwnFzl_wiFM8glZLXSggxtLDLQb9C4muvNx0MWHD-pDcUnb4mPI1H2Pg_aBlt5RXbYxj71L3tLgvkryIdIxRTO47d0lOev0kN3VX0_J-ulxvXiplm_Pr4v7ZWVZLUpVM8PYhnHewVyLGqzkojbAeNtsDDcNohYgpNGCC2i1MUwKM7dYcxTYNnxKbo6zMRevsvXF2d7GEJwtigFDcXh-oNiRsinmnFynxuS3Ou0VgvpVp_7VKYnqqI7_ACkaY3k</recordid><startdate>20000301</startdate><enddate>20000301</enddate><creator>Bergmann, Sven</creator><creator>Grossman, Yuval</creator><creator>Pierce, Damien M.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20000301</creationdate><title>Can lepton flavor violating interactions explain the atmospheric neutrino problem?</title><author>Bergmann, Sven ; Grossman, Yuval ; Pierce, Damien M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>COSMIC NEUTRINOS</topic><topic>EARTH ATMOSPHERE</topic><topic>ELECTRON NEUTRINOS</topic><topic>MUON NEUTRINOS</topic><topic>NEUTRINO-ELECTRON INTERACTIONS</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>SU-2 GROUPS</topic><topic>TAU NEUTRINOS</topic><topic>TAU PARTICLES</topic><topic>THEORETICAL DATA</topic><toplevel>online_resources</toplevel><creatorcontrib>Bergmann, Sven</creatorcontrib><creatorcontrib>Grossman, Yuval</creatorcontrib><creatorcontrib>Pierce, Damien M.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bergmann, Sven</au><au>Grossman, Yuval</au><au>Pierce, Damien M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Can lepton flavor violating interactions explain the atmospheric neutrino problem?</atitle><jtitle>Physical review. D, Particles and fields</jtitle><date>2000-03-01</date><risdate>2000</risdate><volume>61</volume><issue>5</issue><artnum>053005</artnum><issn>0556-2821</issn><eissn>1089-4918</eissn><abstract>We investigate whether flavor changing neutrino interactions (FCNIs) can be sufficiently large to provide a viable solution to the atmospheric neutrino problem. Effective operators induced by heavy boson exchange that allow for flavor changing neutrino scattering off quarks or electrons are related by an SU(2){sub L} rotation to operators that induce anomalous tau decays. Since SU(2){sub L} violation is small for new physics at or above the weak scale, one can use the upper bounds on lepton flavor violating tau decays or on lepton universality violation to put severe, model-independent bounds on the relevant non-standard neutrino interactions. Also Z-induced flavor changing neutral currents, due to heavy singlet neutrinos, are too small to be relevant for the atmospheric neutrino anomaly. We conclude that the FCNI solution to the atmospheric neutrino problem is ruled out. (c) 2000 The American Physical Society.</abstract><cop>United States</cop><doi>10.1103/PhysRevD.61.053005</doi></addata></record>
fulltext fulltext
identifier ISSN: 0556-2821
ispartof Physical review. D, Particles and fields, 2000-03, Vol.61 (5), Article 053005
issn 0556-2821
1089-4918
language eng
recordid cdi_osti_scitechconnect_20215918
source American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)
subjects COSMIC NEUTRINOS
EARTH ATMOSPHERE
ELECTRON NEUTRINOS
MUON NEUTRINOS
NEUTRINO-ELECTRON INTERACTIONS
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
SU-2 GROUPS
TAU NEUTRINOS
TAU PARTICLES
THEORETICAL DATA
title Can lepton flavor violating interactions explain the atmospheric neutrino problem?
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T04%3A45%3A00IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-crossref_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Can%20lepton%20flavor%20violating%20interactions%20explain%20the%20atmospheric%20neutrino%20problem?&rft.jtitle=Physical%20review.%20D,%20Particles%20and%20fields&rft.au=Bergmann,%20Sven&rft.date=2000-03-01&rft.volume=61&rft.issue=5&rft.artnum=053005&rft.issn=0556-2821&rft.eissn=1089-4918&rft_id=info:doi/10.1103/PhysRevD.61.053005&rft_dat=%3Ccrossref_osti_%3E10_1103_PhysRevD_61_053005%3C/crossref_osti_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c275t-72b22d233f04a570c6357b02398db3b811a5056ba53509abb265b4c173151983%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true