Loading…
MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program
Nearly-sterile neutrinos with masses in the MeV range and below would be produced in the beam of the Short-Baseline Neutrino (SBN) program at Fermilab. In this article, we study the potential for SBN to discover these particles through their subsequent decays in its detectors. We discuss the decays...
Saved in:
Published in: | arXiv.org 2016-10 |
---|---|
Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | |
container_end_page | |
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Ballett, Peter Pascoli, Silvia Ross-Lonergan, Mark |
description | Nearly-sterile neutrinos with masses in the MeV range and below would be produced in the beam of the Short-Baseline Neutrino (SBN) program at Fermilab. In this article, we study the potential for SBN to discover these particles through their subsequent decays in its detectors. We discuss the decays which will be visible at SBN in a minimal and non-minimal extension of the Standard Model, and perform simulations to compute the parameter space constraints which could be placed in the absence of a signal. We demonstrate that the SBN program can extend existing bounds on well constrained channels such as \(N \rightarrow \nu l^+ l^-\) and \(N \rightarrow l^\pm \pi^\mp\) while, thanks to the strong particle identification capabilities of liquid-Argon technology, also place bounds on often neglected channels such as \(N \rightarrow \nu\gamma\) and \(N \rightarrow \nu \pi^0\). Furthermore, we consider the phenomenological impact of improved event timing information at the three detectors. As well as considering its role in background reduction, we note that if the light-detection systems in SBND and ICARUS can achieve nanosecond timing resolution, the effect of finite sterile neutrino mass could be directly observable, providing a smoking-gun signature for this class of models. We stress throughout that the search for heavy nearly-sterile neutrinos is a complementary new physics analysis to the search for eV-scale oscillations, and would extend the BSM program of SBN while requiring no beam or detector modifications. |
doi_str_mv | 10.48550/arxiv.1610.08512 |
format | article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2075949319</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2075949319</sourcerecordid><originalsourceid>FETCH-LOGICAL-a529-d07f406d6f79e5fa1e96f1ea41ce98397b1030f2799900b262b8aca2049964b23</originalsourceid><addsrcrecordid>eNo1jd1Kw0AQRhdBsFQfwLsFr1NnZ3-SudRiVaiKWLwtk3RiU9JEd1PRtzegXh34-DhHqXMDM1d4D5ccv5rPmQnjAIU3eKQmaK3JCod4os5S2gEAhhy9txP1_CCvWaq4FZ0Gic3ITg5DbLpeb6Ti76R50MNW9ELivmm51C_bPg7ZNSdpm0704__9PfZvkfen6rjmNsnZH6dqtbhZze-y5dPt_fxqmbFHyjaQ1w7CJtQ5ia_ZCIXaCDtTCRWW8tKAhRpzIgIoMWBZcMUIjii4Eu1UXfxqx-zHQdKw3vWH2I3FNULuyZE1ZH8AOtBQUA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2075949319</pqid></control><display><type>article</type><title>MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program</title><source>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</source><creator>Ballett, Peter ; Pascoli, Silvia ; Ross-Lonergan, Mark</creator><creatorcontrib>Ballett, Peter ; Pascoli, Silvia ; Ross-Lonergan, Mark</creatorcontrib><description>Nearly-sterile neutrinos with masses in the MeV range and below would be produced in the beam of the Short-Baseline Neutrino (SBN) program at Fermilab. In this article, we study the potential for SBN to discover these particles through their subsequent decays in its detectors. We discuss the decays which will be visible at SBN in a minimal and non-minimal extension of the Standard Model, and perform simulations to compute the parameter space constraints which could be placed in the absence of a signal. We demonstrate that the SBN program can extend existing bounds on well constrained channels such as \(N \rightarrow \nu l^+ l^-\) and \(N \rightarrow l^\pm \pi^\mp\) while, thanks to the strong particle identification capabilities of liquid-Argon technology, also place bounds on often neglected channels such as \(N \rightarrow \nu\gamma\) and \(N \rightarrow \nu \pi^0\). Furthermore, we consider the phenomenological impact of improved event timing information at the three detectors. As well as considering its role in background reduction, we note that if the light-detection systems in SBND and ICARUS can achieve nanosecond timing resolution, the effect of finite sterile neutrino mass could be directly observable, providing a smoking-gun signature for this class of models. We stress throughout that the search for heavy nearly-sterile neutrinos is a complementary new physics analysis to the search for eV-scale oscillations, and would extend the BSM program of SBN while requiring no beam or detector modifications.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1610.08512</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Argon ; Channels ; Computer simulation ; Detectors ; Neutrinos ; Particle decay ; Standard model (particle physics)</subject><ispartof>arXiv.org, 2016-10</ispartof><rights>2016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2075949319?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25752,27924,37011,44589</link.rule.ids></links><search><creatorcontrib>Ballett, Peter</creatorcontrib><creatorcontrib>Pascoli, Silvia</creatorcontrib><creatorcontrib>Ross-Lonergan, Mark</creatorcontrib><title>MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program</title><title>arXiv.org</title><description>Nearly-sterile neutrinos with masses in the MeV range and below would be produced in the beam of the Short-Baseline Neutrino (SBN) program at Fermilab. In this article, we study the potential for SBN to discover these particles through their subsequent decays in its detectors. We discuss the decays which will be visible at SBN in a minimal and non-minimal extension of the Standard Model, and perform simulations to compute the parameter space constraints which could be placed in the absence of a signal. We demonstrate that the SBN program can extend existing bounds on well constrained channels such as \(N \rightarrow \nu l^+ l^-\) and \(N \rightarrow l^\pm \pi^\mp\) while, thanks to the strong particle identification capabilities of liquid-Argon technology, also place bounds on often neglected channels such as \(N \rightarrow \nu\gamma\) and \(N \rightarrow \nu \pi^0\). Furthermore, we consider the phenomenological impact of improved event timing information at the three detectors. As well as considering its role in background reduction, we note that if the light-detection systems in SBND and ICARUS can achieve nanosecond timing resolution, the effect of finite sterile neutrino mass could be directly observable, providing a smoking-gun signature for this class of models. We stress throughout that the search for heavy nearly-sterile neutrinos is a complementary new physics analysis to the search for eV-scale oscillations, and would extend the BSM program of SBN while requiring no beam or detector modifications.</description><subject>Argon</subject><subject>Channels</subject><subject>Computer simulation</subject><subject>Detectors</subject><subject>Neutrinos</subject><subject>Particle decay</subject><subject>Standard model (particle physics)</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNo1jd1Kw0AQRhdBsFQfwLsFr1NnZ3-SudRiVaiKWLwtk3RiU9JEd1PRtzegXh34-DhHqXMDM1d4D5ccv5rPmQnjAIU3eKQmaK3JCod4os5S2gEAhhy9txP1_CCvWaq4FZ0Gic3ITg5DbLpeb6Ti76R50MNW9ELivmm51C_bPg7ZNSdpm0704__9PfZvkfen6rjmNsnZH6dqtbhZze-y5dPt_fxqmbFHyjaQ1w7CJtQ5ia_ZCIXaCDtTCRWW8tKAhRpzIgIoMWBZcMUIjii4Eu1UXfxqx-zHQdKw3vWH2I3FNULuyZE1ZH8AOtBQUA</recordid><startdate>20161026</startdate><enddate>20161026</enddate><creator>Ballett, Peter</creator><creator>Pascoli, Silvia</creator><creator>Ross-Lonergan, Mark</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20161026</creationdate><title>MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program</title><author>Ballett, Peter ; Pascoli, Silvia ; Ross-Lonergan, Mark</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a529-d07f406d6f79e5fa1e96f1ea41ce98397b1030f2799900b262b8aca2049964b23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Argon</topic><topic>Channels</topic><topic>Computer simulation</topic><topic>Detectors</topic><topic>Neutrinos</topic><topic>Particle decay</topic><topic>Standard model (particle physics)</topic><toplevel>online_resources</toplevel><creatorcontrib>Ballett, Peter</creatorcontrib><creatorcontrib>Pascoli, Silvia</creatorcontrib><creatorcontrib>Ross-Lonergan, Mark</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ballett, Peter</au><au>Pascoli, Silvia</au><au>Ross-Lonergan, Mark</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program</atitle><jtitle>arXiv.org</jtitle><date>2016-10-26</date><risdate>2016</risdate><eissn>2331-8422</eissn><abstract>Nearly-sterile neutrinos with masses in the MeV range and below would be produced in the beam of the Short-Baseline Neutrino (SBN) program at Fermilab. In this article, we study the potential for SBN to discover these particles through their subsequent decays in its detectors. We discuss the decays which will be visible at SBN in a minimal and non-minimal extension of the Standard Model, and perform simulations to compute the parameter space constraints which could be placed in the absence of a signal. We demonstrate that the SBN program can extend existing bounds on well constrained channels such as \(N \rightarrow \nu l^+ l^-\) and \(N \rightarrow l^\pm \pi^\mp\) while, thanks to the strong particle identification capabilities of liquid-Argon technology, also place bounds on often neglected channels such as \(N \rightarrow \nu\gamma\) and \(N \rightarrow \nu \pi^0\). Furthermore, we consider the phenomenological impact of improved event timing information at the three detectors. As well as considering its role in background reduction, we note that if the light-detection systems in SBND and ICARUS can achieve nanosecond timing resolution, the effect of finite sterile neutrino mass could be directly observable, providing a smoking-gun signature for this class of models. We stress throughout that the search for heavy nearly-sterile neutrinos is a complementary new physics analysis to the search for eV-scale oscillations, and would extend the BSM program of SBN while requiring no beam or detector modifications.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1610.08512</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2016-10 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2075949319 |
source | Publicly Available Content Database (Proquest) (PQ_SDU_P3) |
subjects | Argon Channels Computer simulation Detectors Neutrinos Particle decay Standard model (particle physics) |
title | MeV-scale sterile neutrino decays at the Fermilab Short-Baseline Neutrino program |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-08T15%3A04%3A40IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=MeV-scale%20sterile%20neutrino%20decays%20at%20the%20Fermilab%20Short-Baseline%20Neutrino%20program&rft.jtitle=arXiv.org&rft.au=Ballett,%20Peter&rft.date=2016-10-26&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1610.08512&rft_dat=%3Cproquest%3E2075949319%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a529-d07f406d6f79e5fa1e96f1ea41ce98397b1030f2799900b262b8aca2049964b23%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2075949319&rft_id=info:pmid/&rfr_iscdi=true |