Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors

ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrin...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Agarwalla, Sanjib Kumar [verfasserIn] Conrad, J. M. Shaevitz, M. H.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2011

Schlagwörter:	Neutrino Detectors Telescopes

Anmerkung:	© SISSA, Trieste, Italy 2011

Übergeordnetes Werk:	Enthalten in: Journal of high energy physics - Berlin : Springer, 1997, 2011(2011), 12 vom: 22. Dez.
Übergeordnetes Werk:	volume:2011 ; year:2011 ; number:12 ; day:22 ; month:12

Links:	Volltext

DOI / URN:	10.1007/JHEP12(2011)085

Katalog-ID:	SPR030393841

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allfields	10.1007/JHEP12(2011)085 doi (DE-627)SPR030393841 (SPR)JHEP12(2011)085-e DE-627 ger DE-627 rakwb eng Agarwalla, Sanjib Kumar verfasserin aut Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2011 ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. Neutrino Detectors (dpeaa)DE-He213 Telescopes (dpeaa)DE-He213 Conrad, J. M. aut Shaevitz, M. H. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2011(2011), 12 vom: 22. Dez. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2011 year:2011 number:12 day:22 month:12 https://dx.doi.org/10.1007/JHEP12(2011)085 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2011 2011 12 22 12
spelling	10.1007/JHEP12(2011)085 doi (DE-627)SPR030393841 (SPR)JHEP12(2011)085-e DE-627 ger DE-627 rakwb eng Agarwalla, Sanjib Kumar verfasserin aut Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2011 ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. Neutrino Detectors (dpeaa)DE-He213 Telescopes (dpeaa)DE-He213 Conrad, J. M. aut Shaevitz, M. H. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2011(2011), 12 vom: 22. Dez. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2011 year:2011 number:12 day:22 month:12 https://dx.doi.org/10.1007/JHEP12(2011)085 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2011 2011 12 22 12
allfields_unstemmed	10.1007/JHEP12(2011)085 doi (DE-627)SPR030393841 (SPR)JHEP12(2011)085-e DE-627 ger DE-627 rakwb eng Agarwalla, Sanjib Kumar verfasserin aut Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2011 ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. Neutrino Detectors (dpeaa)DE-He213 Telescopes (dpeaa)DE-He213 Conrad, J. M. aut Shaevitz, M. H. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2011(2011), 12 vom: 22. Dez. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2011 year:2011 number:12 day:22 month:12 https://dx.doi.org/10.1007/JHEP12(2011)085 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2011 2011 12 22 12
allfieldsGer	10.1007/JHEP12(2011)085 doi (DE-627)SPR030393841 (SPR)JHEP12(2011)085-e DE-627 ger DE-627 rakwb eng Agarwalla, Sanjib Kumar verfasserin aut Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2011 ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. Neutrino Detectors (dpeaa)DE-He213 Telescopes (dpeaa)DE-He213 Conrad, J. M. aut Shaevitz, M. H. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2011(2011), 12 vom: 22. Dez. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2011 year:2011 number:12 day:22 month:12 https://dx.doi.org/10.1007/JHEP12(2011)085 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2011 2011 12 22 12
allfieldsSound	10.1007/JHEP12(2011)085 doi (DE-627)SPR030393841 (SPR)JHEP12(2011)085-e DE-627 ger DE-627 rakwb eng Agarwalla, Sanjib Kumar verfasserin aut Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors 2011 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © SISSA, Trieste, Italy 2011 ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. Neutrino Detectors (dpeaa)DE-He213 Telescopes (dpeaa)DE-He213 Conrad, J. M. aut Shaevitz, M. H. aut Enthalten in Journal of high energy physics Berlin : Springer, 1997 2011(2011), 12 vom: 22. Dez. (DE-627)320910571 (DE-600)2027350-2 1029-8479 nnns volume:2011 year:2011 number:12 day:22 month:12 https://dx.doi.org/10.1007/JHEP12(2011)085 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_161 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2068 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4338 AR 2011 2011 12 22 12
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title	Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors
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title_full	Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors
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title_sort	short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors
title_auth	Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors
abstract	ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. © SISSA, Trieste, Italy 2011
abstractGer	ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. © SISSA, Trieste, Italy 2011
abstract_unstemmed	ABSTRACT Powerful new multi-kiloton liquid scintillator neutrino detectors, including NOνA and, possibly, LENA, will come on-line within the next decade. When coupled with a modest-power decay-at-rest (DAR) neutrino source at short-baseline, these detectors can decisively address signals for neutrino oscillations at high $ Δm^{2} $. Along the greater than 50 m length of the detector, the characteristic oscillation wave will be apparent, providing powerful verification of the oscillation phenomenon. LENA can simultaneously perform νμ → νe appearance and νe → νe disappearance searches while NOνA is likely limited to $ ν_{e} $ disappearance. For the appearance channel, a LENA-like detector could test the LSND and MiniBooNE signal regions at >5 σ with a fiducial volume of 5 kt and a 10 kW neutrino source. The LENA and NOνA $ ν_{e} $ disappearance sensitivities are complementary to the recent reactor anomaly indicating possible $ ν_{e} $ disappearance and would cover this possible oscillation signal at ~3 σ. © SISSA, Trieste, Italy 2011
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title_short	Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors
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Short-baseline neutrino oscillation waves in ultra-large liquid scintillator detectors

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