Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)

The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths. The primary focus of this experiment is to explore the Earth matter...

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Veröffentlicht in:arXiv.org 2017-05
Hauptverfasser: The ICAL Collaboration, Ahmed, Shakeel, M Sajjad Athar, Rashid, Hasan, Salim, Mohammad, Singh, S K, Inbanathan, S S R, Singh, Venktesh, Subrahmanyam, V S, Shiba Prasad Behera, Chandratre, Vinay B, Dash, Nitali, Datar, Vivek M, Kashyap, V K S, Mohanty, Ajit K, Pant, Lalit M, Chatterjee, Animesh, Choubey, Sandhya, Gandhi, Raj, Ghosh, Anushree, Tiwari, Deepak, Ajmi, Ali, Sankar, S Uma, Behera, Prafulla, Chacko, Aleena, Jafer, Sadiq, Libby, James, Raveendrababu, K, Rebin, K R, Indumathi, D, Meghna, K, Lakshmi, S M, Murthy, M V N, Pal, Sumanta, Rajasekaran, G, Sinha, Nita, Agarwalla, Sanjib Kumar, Khatun, Amina, Mehta, Poonam, Bhatnagar, Vipin, Kanishka, R, Kumar, A, Shahi, J S, Singh, J B, Ghosh, Monojit, Ghoshal, Pomita, Goswami, Srubabati, Gupta, Chandan, Raut, Sushant, Bhattacharya, Sudeb, Bose, Suvendu, Ghosal, Ambar, Jash, Abhik, Kar, Kamalesh, Majumdar, Debasish, Majumdar, Nayana, Mukhopadhyay, Supratik, Saha, Satyajit, Acharya, B S, Banerjee, Sudeshna, Bhattacharya, Kolahal, Dasgupta, Sudeshna, Moon Moon Devi, Dighe, Amol, Majumder, Gobinda, Mondal, Naba K, Redij, Asmita, Samuel, Deepak, Satyanarayana, B, Thakore, Tarak, Ravikumar, C D, Vinodkumar, A M, Gangopadhyay, Gautam, Raychaudhuri, Amitava, Choudhary, Brajesh C, Gaur, Ankit, Kaur, Daljeet, Kumar, Ashok, Kumar, Sanjeev, Naimuddin, Md, Bari, Waseem, Malik, Manzoor A, Singh, Jyotsna, Krishnaveni, S, Ravikumar, H B, Ranganathaiah, C, Mahapatra, Swapna, Biswas, Saikat, Chattopadhyay, Subhasis, Ganai, Rajesh, Ghosh, Tapasi, Viyogi, Y P
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creator The ICAL Collaboration
Ahmed, Shakeel
M Sajjad Athar
Rashid, Hasan
Salim, Mohammad
Singh, S K
Inbanathan, S S R
Singh, Venktesh
Subrahmanyam, V S
Shiba Prasad Behera
Chandratre, Vinay B
Dash, Nitali
Datar, Vivek M
Kashyap, V K S
Mohanty, Ajit K
Pant, Lalit M
Chatterjee, Animesh
Choubey, Sandhya
Gandhi, Raj
Ghosh, Anushree
Tiwari, Deepak
Ajmi, Ali
Sankar, S Uma
Behera, Prafulla
Chacko, Aleena
Jafer, Sadiq
Libby, James
Raveendrababu, K
Rebin, K R
Indumathi, D
Meghna, K
Lakshmi, S M
Murthy, M V N
Pal, Sumanta
Rajasekaran, G
Sinha, Nita
Agarwalla, Sanjib Kumar
Khatun, Amina
Mehta, Poonam
Bhatnagar, Vipin
Kanishka, R
Kumar, A
Shahi, J S
Singh, J B
Ghosh, Monojit
Ghoshal, Pomita
Goswami, Srubabati
Gupta, Chandan
Raut, Sushant
Bhattacharya, Sudeb
Bose, Suvendu
Ghosal, Ambar
Jash, Abhik
Kar, Kamalesh
Majumdar, Debasish
Majumdar, Nayana
Mukhopadhyay, Supratik
Saha, Satyajit
Acharya, B S
Banerjee, Sudeshna
Bhattacharya, Kolahal
Dasgupta, Sudeshna
Moon Moon Devi
Dighe, Amol
Majumder, Gobinda
Mondal, Naba K
Redij, Asmita
Samuel, Deepak
Satyanarayana, B
Thakore, Tarak
Ravikumar, C D
Vinodkumar, A M
Gangopadhyay, Gautam
Raychaudhuri, Amitava
Choudhary, Brajesh C
Gaur, Ankit
Kaur, Daljeet
Kumar, Ashok
Kumar, Sanjeev
Naimuddin, Md
Bari, Waseem
Malik, Manzoor A
Singh, Jyotsna
Krishnaveni, S
Ravikumar, H B
Ranganathaiah, C
Mahapatra, Swapna
Biswas, Saikat
Chattopadhyay, Subhasis
Ganai, Rajesh
Ghosh, Tapasi
Viyogi, Y P
description The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths. The primary focus of this experiment is to explore the Earth matter effects by observing the energy and zenith angle dependence of the atmospheric neutrinos in the multi-GeV range. This study will be crucial to address some of the outstanding issues in neutrino oscillation physics, including the fundamental issue of neutrino mass hierarchy. In this document, we present the physics potential of the detector as obtained from realistic detector simulations. We describe the simulation framework, the neutrino interactions in the detector, and the expected response of the detector to particles traversing it. The ICAL detector can determine the energy and direction of the muons to a high precision, and in addition, its sensitivity to multi-GeV hadrons increases its physics reach substantially. Its charge identification capability, and hence its ability to distinguish neutrinos from antineutrinos, makes it an efficient detector for determining the neutrino mass hierarchy. In this report, we outline the analyses carried out for the determination of neutrino mass hierarchy and precision measurements of atmospheric neutrino mixing parameters at ICAL, and give the expected physics reach of the detector with 10 years of runtime. We also explore the potential of ICAL for probing new physics scenarios like CPT violation and the presence of magnetic monopoles.
doi_str_mv 10.48550/arxiv.1505.07380
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The primary focus of this experiment is to explore the Earth matter effects by observing the energy and zenith angle dependence of the atmospheric neutrinos in the multi-GeV range. This study will be crucial to address some of the outstanding issues in neutrino oscillation physics, including the fundamental issue of neutrino mass hierarchy. In this document, we present the physics potential of the detector as obtained from realistic detector simulations. We describe the simulation framework, the neutrino interactions in the detector, and the expected response of the detector to particles traversing it. The ICAL detector can determine the energy and direction of the muons to a high precision, and in addition, its sensitivity to multi-GeV hadrons increases its physics reach substantially. Its charge identification capability, and hence its ability to distinguish neutrinos from antineutrinos, makes it an efficient detector for determining the neutrino mass hierarchy. In this report, we outline the analyses carried out for the determination of neutrino mass hierarchy and precision measurements of atmospheric neutrino mixing parameters at ICAL, and give the expected physics reach of the detector with 10 years of runtime. We also explore the potential of ICAL for probing new physics scenarios like CPT violation and the presence of magnetic monopoles.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1505.07380</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Antineutrinos ; Dependence ; Hadrons ; Magnetic monopoles ; Muons ; Neutrinos ; Observatories ; Physics ; Physics - High Energy Physics - Experiment ; Physics - High Energy Physics - Phenomenology ; Physics - Instrumentation and Detectors ; Sensors</subject><ispartof>arXiv.org, 2017-05</ispartof><rights>2017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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Srubabati</creatorcontrib><creatorcontrib>Gupta, Chandan</creatorcontrib><creatorcontrib>Raut, Sushant</creatorcontrib><creatorcontrib>Bhattacharya, Sudeb</creatorcontrib><creatorcontrib>Bose, Suvendu</creatorcontrib><creatorcontrib>Ghosal, Ambar</creatorcontrib><creatorcontrib>Jash, Abhik</creatorcontrib><creatorcontrib>Kar, Kamalesh</creatorcontrib><creatorcontrib>Majumdar, Debasish</creatorcontrib><creatorcontrib>Majumdar, Nayana</creatorcontrib><creatorcontrib>Mukhopadhyay, Supratik</creatorcontrib><creatorcontrib>Saha, Satyajit</creatorcontrib><creatorcontrib>Acharya, B S</creatorcontrib><creatorcontrib>Banerjee, Sudeshna</creatorcontrib><creatorcontrib>Bhattacharya, Kolahal</creatorcontrib><creatorcontrib>Dasgupta, Sudeshna</creatorcontrib><creatorcontrib>Moon Moon Devi</creatorcontrib><creatorcontrib>Dighe, Amol</creatorcontrib><creatorcontrib>Majumder, Gobinda</creatorcontrib><creatorcontrib>Mondal, Naba K</creatorcontrib><creatorcontrib>Redij, Asmita</creatorcontrib><creatorcontrib>Samuel, Deepak</creatorcontrib><creatorcontrib>Satyanarayana, B</creatorcontrib><creatorcontrib>Thakore, Tarak</creatorcontrib><creatorcontrib>Ravikumar, C D</creatorcontrib><creatorcontrib>Vinodkumar, A M</creatorcontrib><creatorcontrib>Gangopadhyay, Gautam</creatorcontrib><creatorcontrib>Raychaudhuri, Amitava</creatorcontrib><creatorcontrib>Choudhary, Brajesh C</creatorcontrib><creatorcontrib>Gaur, Ankit</creatorcontrib><creatorcontrib>Kaur, Daljeet</creatorcontrib><creatorcontrib>Kumar, Ashok</creatorcontrib><creatorcontrib>Kumar, Sanjeev</creatorcontrib><creatorcontrib>Naimuddin, Md</creatorcontrib><creatorcontrib>Bari, Waseem</creatorcontrib><creatorcontrib>Malik, Manzoor A</creatorcontrib><creatorcontrib>Singh, Jyotsna</creatorcontrib><creatorcontrib>Krishnaveni, S</creatorcontrib><creatorcontrib>Ravikumar, H B</creatorcontrib><creatorcontrib>Ranganathaiah, C</creatorcontrib><creatorcontrib>Mahapatra, Swapna</creatorcontrib><creatorcontrib>Biswas, Saikat</creatorcontrib><creatorcontrib>Chattopadhyay, Subhasis</creatorcontrib><creatorcontrib>Ganai, Rajesh</creatorcontrib><creatorcontrib>Ghosh, Tapasi</creatorcontrib><creatorcontrib>Viyogi, Y P</creatorcontrib><title>Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)</title><title>arXiv.org</title><description>The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths. The primary focus of this experiment is to explore the Earth matter effects by observing the energy and zenith angle dependence of the atmospheric neutrinos in the multi-GeV range. This study will be crucial to address some of the outstanding issues in neutrino oscillation physics, including the fundamental issue of neutrino mass hierarchy. In this document, we present the physics potential of the detector as obtained from realistic detector simulations. We describe the simulation framework, the neutrino interactions in the detector, and the expected response of the detector to particles traversing it. The ICAL detector can determine the energy and direction of the muons to a high precision, and in addition, its sensitivity to multi-GeV hadrons increases its physics reach substantially. Its charge identification capability, and hence its ability to distinguish neutrinos from antineutrinos, makes it an efficient detector for determining the neutrino mass hierarchy. In this report, we outline the analyses carried out for the determination of neutrino mass hierarchy and precision measurements of atmospheric neutrino mixing parameters at ICAL, and give the expected physics reach of the detector with 10 years of runtime. We also explore the potential of ICAL for probing new physics scenarios like CPT violation and the presence of magnetic monopoles.</description><subject>Antineutrinos</subject><subject>Dependence</subject><subject>Hadrons</subject><subject>Magnetic monopoles</subject><subject>Muons</subject><subject>Neutrinos</subject><subject>Observatories</subject><subject>Physics</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Physics - Instrumentation and 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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><scope>GOX</scope></search><sort><creationdate>20170509</creationdate><title>Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)</title><author>The ICAL Collaboration ; Ahmed, Shakeel ; M Sajjad Athar ; Rashid, Hasan ; Salim, Mohammad ; Singh, S K ; Inbanathan, S S R ; Singh, Venktesh ; Subrahmanyam, V S ; Shiba Prasad Behera ; Chandratre, Vinay B ; Dash, Nitali ; Datar, Vivek M ; Kashyap, V K S ; Mohanty, Ajit K ; Pant, Lalit M ; Chatterjee, Animesh ; Choubey, Sandhya ; Gandhi, Raj ; Ghosh, Anushree ; Tiwari, Deepak ; Ajmi, Ali ; Sankar, S Uma ; Behera, Prafulla ; Chacko, Aleena ; Jafer, Sadiq ; Libby, James ; Raveendrababu, K ; Rebin, K R ; Indumathi, D ; Meghna, K ; Lakshmi, S M ; Murthy, M V N ; Pal, Sumanta ; Rajasekaran, G ; Sinha, Nita ; Agarwalla, Sanjib Kumar ; Khatun, Amina ; Mehta, Poonam ; Bhatnagar, Vipin ; Kanishka, R ; Kumar, A ; Shahi, J S ; Singh, J B ; Ghosh, Monojit ; Ghoshal, Pomita ; Goswami, Srubabati ; Gupta, Chandan ; Raut, Sushant ; Bhattacharya, Sudeb ; Bose, Suvendu ; Ghosal, Ambar ; Jash, Abhik ; Kar, Kamalesh ; Majumdar, Debasish ; Majumdar, Nayana ; Mukhopadhyay, Supratik ; Saha, Satyajit ; Acharya, B S ; Banerjee, Sudeshna ; Bhattacharya, Kolahal ; Dasgupta, Sudeshna ; Moon Moon Devi ; Dighe, Amol ; Majumder, Gobinda ; Mondal, Naba K ; Redij, Asmita ; Samuel, Deepak ; Satyanarayana, B ; Thakore, Tarak ; Ravikumar, C D ; Vinodkumar, A M ; Gangopadhyay, Gautam ; Raychaudhuri, Amitava ; Choudhary, Brajesh C ; Gaur, Ankit ; Kaur, Daljeet ; Kumar, Ashok ; Kumar, Sanjeev ; Naimuddin, Md ; Bari, Waseem ; Malik, Manzoor A ; Singh, Jyotsna ; Krishnaveni, S ; Ravikumar, H B ; Ranganathaiah, C ; Mahapatra, Swapna ; Biswas, Saikat ; Chattopadhyay, Subhasis ; Ganai, Rajesh ; Ghosh, Tapasi ; Viyogi, Y P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a528-80d535be8edc05c0607ccba9fdbd3a97ad31e7320dd4498c27af6c469d19605e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Antineutrinos</topic><topic>Dependence</topic><topic>Hadrons</topic><topic>Magnetic monopoles</topic><topic>Muons</topic><topic>Neutrinos</topic><topic>Observatories</topic><topic>Physics</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Physics - Instrumentation and Detectors</topic><topic>Sensors</topic><toplevel>online_resources</toplevel><creatorcontrib>The ICAL Collaboration</creatorcontrib><creatorcontrib>Ahmed, 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K</au><au>Pant, Lalit M</au><au>Chatterjee, Animesh</au><au>Choubey, Sandhya</au><au>Gandhi, Raj</au><au>Ghosh, Anushree</au><au>Tiwari, Deepak</au><au>Ajmi, Ali</au><au>Sankar, S Uma</au><au>Behera, Prafulla</au><au>Chacko, Aleena</au><au>Jafer, Sadiq</au><au>Libby, James</au><au>Raveendrababu, K</au><au>Rebin, K R</au><au>Indumathi, D</au><au>Meghna, K</au><au>Lakshmi, S M</au><au>Murthy, M V N</au><au>Pal, Sumanta</au><au>Rajasekaran, G</au><au>Sinha, Nita</au><au>Agarwalla, Sanjib Kumar</au><au>Khatun, Amina</au><au>Mehta, Poonam</au><au>Bhatnagar, Vipin</au><au>Kanishka, R</au><au>Kumar, A</au><au>Shahi, J S</au><au>Singh, J B</au><au>Ghosh, Monojit</au><au>Ghoshal, Pomita</au><au>Goswami, Srubabati</au><au>Gupta, Chandan</au><au>Raut, Sushant</au><au>Bhattacharya, Sudeb</au><au>Bose, Suvendu</au><au>Ghosal, Ambar</au><au>Jash, Abhik</au><au>Kar, Kamalesh</au><au>Majumdar, Debasish</au><au>Majumdar, Nayana</au><au>Mukhopadhyay, Supratik</au><au>Saha, Satyajit</au><au>Acharya, B S</au><au>Banerjee, Sudeshna</au><au>Bhattacharya, Kolahal</au><au>Dasgupta, Sudeshna</au><au>Moon Moon Devi</au><au>Dighe, Amol</au><au>Majumder, Gobinda</au><au>Mondal, Naba K</au><au>Redij, Asmita</au><au>Samuel, Deepak</au><au>Satyanarayana, B</au><au>Thakore, Tarak</au><au>Ravikumar, C D</au><au>Vinodkumar, A M</au><au>Gangopadhyay, Gautam</au><au>Raychaudhuri, Amitava</au><au>Choudhary, Brajesh C</au><au>Gaur, Ankit</au><au>Kaur, Daljeet</au><au>Kumar, Ashok</au><au>Kumar, Sanjeev</au><au>Naimuddin, Md</au><au>Bari, Waseem</au><au>Malik, Manzoor A</au><au>Singh, Jyotsna</au><au>Krishnaveni, S</au><au>Ravikumar, H B</au><au>Ranganathaiah, C</au><au>Mahapatra, Swapna</au><au>Biswas, Saikat</au><au>Chattopadhyay, Subhasis</au><au>Ganai, Rajesh</au><au>Ghosh, Tapasi</au><au>Viyogi, Y P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)</atitle><jtitle>arXiv.org</jtitle><date>2017-05-09</date><risdate>2017</risdate><eissn>2331-8422</eissn><abstract>The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths. The primary focus of this experiment is to explore the Earth matter effects by observing the energy and zenith angle dependence of the atmospheric neutrinos in the multi-GeV range. This study will be crucial to address some of the outstanding issues in neutrino oscillation physics, including the fundamental issue of neutrino mass hierarchy. In this document, we present the physics potential of the detector as obtained from realistic detector simulations. We describe the simulation framework, the neutrino interactions in the detector, and the expected response of the detector to particles traversing it. The ICAL detector can determine the energy and direction of the muons to a high precision, and in addition, its sensitivity to multi-GeV hadrons increases its physics reach substantially. Its charge identification capability, and hence its ability to distinguish neutrinos from antineutrinos, makes it an efficient detector for determining the neutrino mass hierarchy. In this report, we outline the analyses carried out for the determination of neutrino mass hierarchy and precision measurements of atmospheric neutrino mixing parameters at ICAL, and give the expected physics reach of the detector with 10 years of runtime. We also explore the potential of ICAL for probing new physics scenarios like CPT violation and the presence of magnetic monopoles.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1505.07380</doi><oa>free_for_read</oa></addata></record>
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subjects Antineutrinos
Dependence
Hadrons
Magnetic monopoles
Muons
Neutrinos
Observatories
Physics
Physics - High Energy Physics - Experiment
Physics - High Energy Physics - Phenomenology
Physics - Instrumentation and Detectors
Sensors
title Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO)
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