The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters

Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision o...
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Gespeichert in:

Autor*in:	Kaur, Daljeet [verfasserIn] Naimuddin, Md. [verfasserIn] Kumar, Sanjeev [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	Neutrino Oscillation Oscillation Parameter Atmospheric Neutrino Neutrino Energy Muon Energy

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 1998, 75(2015), 4 vom: 21. Apr.
Übergeordnetes Werk:	volume:75 ; year:2015 ; number:4 ; day:21 ; month:04

Links:	Volltext

DOI / URN:	10.1140/epjc/s10052-015-3374-0

Katalog-ID:	SPR00834390X

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Indexfelder

author_variant	d k dk m n mn s k sk
matchkey_str	article:14346052:2015----::hsniiiyfhiadtcoaidaaenurnosraoyoet
hierarchy_sort_str	2015
bklnumber	33.50
publishDate	2015
allfields	10.1140/epjc/s10052-015-3374-0 doi (DE-627)SPR00834390X (SPR)s10052-015-3374-0-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Kaur, Daljeet verfasserin aut The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure. Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213 Naimuddin, Md. verfasserin aut Kumar, Sanjeev verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 4 vom: 21. Apr. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:4 day:21 month:04 https://dx.doi.org/10.1140/epjc/s10052-015-3374-0 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 4 21 04
spelling	10.1140/epjc/s10052-015-3374-0 doi (DE-627)SPR00834390X (SPR)s10052-015-3374-0-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Kaur, Daljeet verfasserin aut The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure. Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213 Naimuddin, Md. verfasserin aut Kumar, Sanjeev verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 4 vom: 21. Apr. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:4 day:21 month:04 https://dx.doi.org/10.1140/epjc/s10052-015-3374-0 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 4 21 04
allfields_unstemmed	10.1140/epjc/s10052-015-3374-0 doi (DE-627)SPR00834390X (SPR)s10052-015-3374-0-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Kaur, Daljeet verfasserin aut The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure. Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213 Naimuddin, Md. verfasserin aut Kumar, Sanjeev verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 4 vom: 21. Apr. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:4 day:21 month:04 https://dx.doi.org/10.1140/epjc/s10052-015-3374-0 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 4 21 04
allfieldsGer	10.1140/epjc/s10052-015-3374-0 doi (DE-627)SPR00834390X (SPR)s10052-015-3374-0-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Kaur, Daljeet verfasserin aut The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure. Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213 Naimuddin, Md. verfasserin aut Kumar, Sanjeev verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 4 vom: 21. Apr. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:4 day:21 month:04 https://dx.doi.org/10.1140/epjc/s10052-015-3374-0 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 4 21 04
allfieldsSound	10.1140/epjc/s10052-015-3374-0 doi (DE-627)SPR00834390X (SPR)s10052-015-3374-0-e DE-627 ger DE-627 rakwb eng 530 ASE 33.50 bkl Kaur, Daljeet verfasserin aut The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure. Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213 Naimuddin, Md. verfasserin aut Kumar, Sanjeev verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 75(2015), 4 vom: 21. Apr. (DE-627)253722934 (DE-600)1459069-4 1434-6052 nnns volume:75 year:2015 number:4 day:21 month:04 https://dx.doi.org/10.1140/epjc/s10052-015-3374-0 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2031 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2061 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2113 GBV_ILN_2119 GBV_ILN_2190 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 33.50 ASE AR 75 2015 4 21 04
language	English
source	Enthalten in The European physical journal 75(2015), 4 vom: 21. Apr. volume:75 year:2015 number:4 day:21 month:04
sourceStr	Enthalten in The European physical journal 75(2015), 4 vom: 21. Apr. volume:75 year:2015 number:4 day:21 month:04
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Neutrino Oscillation Oscillation Parameter Atmospheric Neutrino Neutrino Energy Muon Energy
dewey-raw	530
isfreeaccess_bool	true
container_title	The European physical journal
authorswithroles_txt_mv	Kaur, Daljeet @@aut@@ Naimuddin, Md. @@aut@@ Kumar, Sanjeev @@aut@@
publishDateDaySort_date	2015-04-21T00:00:00Z
hierarchy_top_id	253722934
dewey-sort	3530
id	SPR00834390X
language_de	englisch
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author	Kaur, Daljeet
spellingShingle	Kaur, Daljeet ddc 530 bkl 33.50 misc Neutrino Oscillation misc Oscillation Parameter misc Atmospheric Neutrino misc Neutrino Energy misc Muon Energy The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters
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topic_title	530 ASE 33.50 bkl The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters Neutrino Oscillation (dpeaa)DE-He213 Oscillation Parameter (dpeaa)DE-He213 Atmospheric Neutrino (dpeaa)DE-He213 Neutrino Energy (dpeaa)DE-He213 Muon Energy (dpeaa)DE-He213
topic	ddc 530 bkl 33.50 misc Neutrino Oscillation misc Oscillation Parameter misc Atmospheric Neutrino misc Neutrino Energy misc Muon Energy
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title	The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters
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title_full	The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters
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author_browse	Kaur, Daljeet Naimuddin, Md. Kumar, Sanjeev
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title_sort	sensitivity of the ical detector at india-based neutrino observatory to neutrino oscillation parameters
title_auth	The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters
abstract	Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure.
abstractGer	Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure.
abstract_unstemmed	Abstract The India-based Neutrino Observatory will host a 50 kt magnetized iron calorimeter (ICAL) detector that will be able to detect muon tracks and hadron showers produced by charged-current muon neutrino interactions in the detector. The ICAL experiment will be able to determine the precision of atmospheric neutrino mixing parameters and neutrino mass hierarchy using atmospheric muon neutrinos through the earth matter effect. In this paper, we report on the sensitivity for the atmospheric neutrino mixing parameters (%$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$) and octant sensitivity for the ICAL detector using the reconstructed neutrino energy and muon direction as observables. We apply realistic resolutions and efficiencies obtained by the ICAL collaboration with a GEANT4-based simulation to reconstruct neutrino energy and muon direction. Our study shows that using neutrino energy and muon direction as observables for a %$\chi ^{2}%$ analysis, the ICAL detector can measure %$\sin ^{2}\theta _{23}%$ and %$\|\Delta m^{2}_{32}\|%$ with 13 % and 4 % uncertainties at 1%$\sigma %$ confidence level and can rule out the wrong octant of %$\theta _{23}%$ with 2%$\sigma %$ confidence level for 10 years of exposure.
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title_short	The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters
url	https://dx.doi.org/10.1140/epjc/s10052-015-3374-0
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up_date	2024-07-03T19:23:31.235Z
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The sensitivity of the ICAL detector at India-based Neutrino Observatory to neutrino oscillation parameters

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