Neutrino mass hierarchy determination for theta{sub 13} = 0
We examine the possibility of determining the neutrino mass hierarchy in the limit theta{sub 13} = 0 using atmospheric neutrinos as the source. In this limit, theta{sub 13} driven matter effects are absent so independent measurements of DELTA{sub 31} and DELTA{sub 32} can, in principle, lead to hier...
Gespeichert in:
Veröffentlicht in: | AIP conference proceedings 2010-03, Vol.1222 (1) |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 1 |
container_start_page | |
container_title | AIP conference proceedings |
container_volume | 1222 |
creator | Gandhi, Raj Ghoshal, Pomita Goswami, Srubabati Sankar, S. Uma |
description | We examine the possibility of determining the neutrino mass hierarchy in the limit theta{sub 13} = 0 using atmospheric neutrinos as the source. In this limit, theta{sub 13} driven matter effects are absent so independent measurements of DELTA{sub 31} and DELTA{sub 32} can, in principle, lead to hierarchy determination. Since their difference is DELTA{sub 21}, one needs an experimental arrangement where DELTA{sub 21}L/E > or approx. 1 can be achieved. This can be satisfied by atmospheric neutrinos which have a large range of L and E. Still, we find that hierarchy determination in the theta{sub 13} = 0 limit with atmospheric neutrinos is not a realistic possibility, even in conjunction with a beam experiment like T2K or NOnuA. We discuss why, and also reiterate the general conditions for hierarchy determination if theta{sub 13} = 0. |
doi_str_mv | 10.1063/1.3399365 |
format | Article |
fullrecord | <record><control><sourceid>osti</sourceid><recordid>TN_cdi_osti_scitechconnect_21367128</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>21367128</sourcerecordid><originalsourceid>FETCH-LOGICAL-o148t-f4b6166dbb5665de6b3551c61a758464d7fb3702a59d8926b1ca826777265abf3</originalsourceid><addsrcrecordid>eNotzs1KAzEUQOEgCo7VhW8QcD01Nz83CeJCilWh6EbBXUkyGSZiE5ikCxHf3YKuzu7wEXIJbAkMxTUshbBWoDoiHSgFvUbAY9IxZmXPpXg_JWe1fjDGrdamIzfPcd_mlAvduVrplOLs5jB90SG2OO9Sdi2VTMcy0zbF5r7r3lMQP_SWsnNyMrrPGi_-uyBv6_vX1WO_eXl4Wt1t-gLStH6U_mDAwXuFqIaIXhxgAcFpZSTKQY9eaMadsoOxHD0EZzhqrTkq50exIFd_31Jb2taQWgxTKDnH0LYcBGrgRvwCc0tHHg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Neutrino mass hierarchy determination for theta{sub 13} = 0</title><source>AIP Journals Complete</source><creator>Gandhi, Raj ; Ghoshal, Pomita ; Goswami, Srubabati ; Sankar, S. Uma</creator><creatorcontrib>Gandhi, Raj ; Ghoshal, Pomita ; Goswami, Srubabati ; Sankar, S. Uma</creatorcontrib><description>We examine the possibility of determining the neutrino mass hierarchy in the limit theta{sub 13} = 0 using atmospheric neutrinos as the source. In this limit, theta{sub 13} driven matter effects are absent so independent measurements of DELTA{sub 31} and DELTA{sub 32} can, in principle, lead to hierarchy determination. Since their difference is DELTA{sub 21}, one needs an experimental arrangement where DELTA{sub 21}L/E > or approx. 1 can be achieved. This can be satisfied by atmospheric neutrinos which have a large range of L and E. Still, we find that hierarchy determination in the theta{sub 13} = 0 limit with atmospheric neutrinos is not a realistic possibility, even in conjunction with a beam experiment like T2K or NOnuA. We discuss why, and also reiterate the general conditions for hierarchy determination if theta{sub 13} = 0.</description><identifier>ISSN: 0094-243X</identifier><identifier>EISSN: 1551-7616</identifier><identifier>DOI: 10.1063/1.3399365</identifier><language>eng</language><publisher>United States</publisher><subject>CHERENKOV COUNTERS ; DETECTION ; ELEMENTARY PARTICLES ; FERMIONS ; LEPTON REACTIONS ; LEPTONS ; MASS ; MASSLESS PARTICLES ; MEASURING INSTRUMENTS ; NEUTRINO DETECTION ; NEUTRINO OSCILLATION ; NEUTRINO REACTIONS ; NEUTRINOS ; NUCLEAR REACTIONS ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; PROBABILITY ; RADIATION DETECTION ; RADIATION DETECTORS ; REST MASS ; WEINBERG ANGLE</subject><ispartof>AIP conference proceedings, 2010-03, Vol.1222 (1)</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27922,27923</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/21367128$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Gandhi, Raj</creatorcontrib><creatorcontrib>Ghoshal, Pomita</creatorcontrib><creatorcontrib>Goswami, Srubabati</creatorcontrib><creatorcontrib>Sankar, S. Uma</creatorcontrib><title>Neutrino mass hierarchy determination for theta{sub 13} = 0</title><title>AIP conference proceedings</title><description>We examine the possibility of determining the neutrino mass hierarchy in the limit theta{sub 13} = 0 using atmospheric neutrinos as the source. In this limit, theta{sub 13} driven matter effects are absent so independent measurements of DELTA{sub 31} and DELTA{sub 32} can, in principle, lead to hierarchy determination. Since their difference is DELTA{sub 21}, one needs an experimental arrangement where DELTA{sub 21}L/E > or approx. 1 can be achieved. This can be satisfied by atmospheric neutrinos which have a large range of L and E. Still, we find that hierarchy determination in the theta{sub 13} = 0 limit with atmospheric neutrinos is not a realistic possibility, even in conjunction with a beam experiment like T2K or NOnuA. We discuss why, and also reiterate the general conditions for hierarchy determination if theta{sub 13} = 0.</description><subject>CHERENKOV COUNTERS</subject><subject>DETECTION</subject><subject>ELEMENTARY PARTICLES</subject><subject>FERMIONS</subject><subject>LEPTON REACTIONS</subject><subject>LEPTONS</subject><subject>MASS</subject><subject>MASSLESS PARTICLES</subject><subject>MEASURING INSTRUMENTS</subject><subject>NEUTRINO DETECTION</subject><subject>NEUTRINO OSCILLATION</subject><subject>NEUTRINO REACTIONS</subject><subject>NEUTRINOS</subject><subject>NUCLEAR REACTIONS</subject><subject>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</subject><subject>PROBABILITY</subject><subject>RADIATION DETECTION</subject><subject>RADIATION DETECTORS</subject><subject>REST MASS</subject><subject>WEINBERG ANGLE</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNotzs1KAzEUQOEgCo7VhW8QcD01Nz83CeJCilWh6EbBXUkyGSZiE5ikCxHf3YKuzu7wEXIJbAkMxTUshbBWoDoiHSgFvUbAY9IxZmXPpXg_JWe1fjDGrdamIzfPcd_mlAvduVrplOLs5jB90SG2OO9Sdi2VTMcy0zbF5r7r3lMQP_SWsnNyMrrPGi_-uyBv6_vX1WO_eXl4Wt1t-gLStH6U_mDAwXuFqIaIXhxgAcFpZSTKQY9eaMadsoOxHD0EZzhqrTkq50exIFd_31Jb2taQWgxTKDnH0LYcBGrgRvwCc0tHHg</recordid><startdate>20100330</startdate><enddate>20100330</enddate><creator>Gandhi, Raj</creator><creator>Ghoshal, Pomita</creator><creator>Goswami, Srubabati</creator><creator>Sankar, S. Uma</creator><scope>OTOTI</scope></search><sort><creationdate>20100330</creationdate><title>Neutrino mass hierarchy determination for theta{sub 13} = 0</title><author>Gandhi, Raj ; Ghoshal, Pomita ; Goswami, Srubabati ; Sankar, S. Uma</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-o148t-f4b6166dbb5665de6b3551c61a758464d7fb3702a59d8926b1ca826777265abf3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>CHERENKOV COUNTERS</topic><topic>DETECTION</topic><topic>ELEMENTARY PARTICLES</topic><topic>FERMIONS</topic><topic>LEPTON REACTIONS</topic><topic>LEPTONS</topic><topic>MASS</topic><topic>MASSLESS PARTICLES</topic><topic>MEASURING INSTRUMENTS</topic><topic>NEUTRINO DETECTION</topic><topic>NEUTRINO OSCILLATION</topic><topic>NEUTRINO REACTIONS</topic><topic>NEUTRINOS</topic><topic>NUCLEAR REACTIONS</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>PROBABILITY</topic><topic>RADIATION DETECTION</topic><topic>RADIATION DETECTORS</topic><topic>REST MASS</topic><topic>WEINBERG ANGLE</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gandhi, Raj</creatorcontrib><creatorcontrib>Ghoshal, Pomita</creatorcontrib><creatorcontrib>Goswami, Srubabati</creatorcontrib><creatorcontrib>Sankar, S. Uma</creatorcontrib><collection>OSTI.GOV</collection><jtitle>AIP conference proceedings</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gandhi, Raj</au><au>Ghoshal, Pomita</au><au>Goswami, Srubabati</au><au>Sankar, S. Uma</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Neutrino mass hierarchy determination for theta{sub 13} = 0</atitle><jtitle>AIP conference proceedings</jtitle><date>2010-03-30</date><risdate>2010</risdate><volume>1222</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>We examine the possibility of determining the neutrino mass hierarchy in the limit theta{sub 13} = 0 using atmospheric neutrinos as the source. In this limit, theta{sub 13} driven matter effects are absent so independent measurements of DELTA{sub 31} and DELTA{sub 32} can, in principle, lead to hierarchy determination. Since their difference is DELTA{sub 21}, one needs an experimental arrangement where DELTA{sub 21}L/E > or approx. 1 can be achieved. This can be satisfied by atmospheric neutrinos which have a large range of L and E. Still, we find that hierarchy determination in the theta{sub 13} = 0 limit with atmospheric neutrinos is not a realistic possibility, even in conjunction with a beam experiment like T2K or NOnuA. We discuss why, and also reiterate the general conditions for hierarchy determination if theta{sub 13} = 0.</abstract><cop>United States</cop><doi>10.1063/1.3399365</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0094-243X |
ispartof | AIP conference proceedings, 2010-03, Vol.1222 (1) |
issn | 0094-243X 1551-7616 |
language | eng |
recordid | cdi_osti_scitechconnect_21367128 |
source | AIP Journals Complete |
subjects | CHERENKOV COUNTERS DETECTION ELEMENTARY PARTICLES FERMIONS LEPTON REACTIONS LEPTONS MASS MASSLESS PARTICLES MEASURING INSTRUMENTS NEUTRINO DETECTION NEUTRINO OSCILLATION NEUTRINO REACTIONS NEUTRINOS NUCLEAR REACTIONS PHYSICS OF ELEMENTARY PARTICLES AND FIELDS PROBABILITY RADIATION DETECTION RADIATION DETECTORS REST MASS WEINBERG ANGLE |
title | Neutrino mass hierarchy determination for theta{sub 13} = 0 |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-10T09%3A26%3A03IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-osti&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Neutrino%20mass%20hierarchy%20determination%20for%20theta%7Bsub%2013%7D%20=%200&rft.jtitle=AIP%20conference%20proceedings&rft.au=Gandhi,%20Raj&rft.date=2010-03-30&rft.volume=1222&rft.issue=1&rft.issn=0094-243X&rft.eissn=1551-7616&rft_id=info:doi/10.1063/1.3399365&rft_dat=%3Costi%3E21367128%3C/osti%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |