Invited review: 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: | Pramāṇa 2017-05, Vol.88 (5), p.1-72, Article 79 |
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creator | Kumar, A Vinod Kumar, A M Jash, Abhik Mohanty, Ajit K Chacko, Aleena Ajmi, Ali Ghosal, Ambar Khatun, Amina Raychaudhuri, Amitava Dighe, Amol Chatterjee, Animesh Gaur, Ankit Ghosh, Anushree Kumar, Ashok Redij, Asmita Satyanarayana, B Acharya, B S Choudhary, Brajesh C Ranganathaiah, C Ravikumar, C D Gupta, Chandan Indumathi, D Kaur, Daljeet Majumdar, Debasish Samuel, Deepak Tiwari, Deepak Rajasekaran, G Gangopadhyay, Gautam Majumder, Gobinda Ravikumar, H B Singh, J B Shahi, J S Libby, James Singh, Jyotsna Raveendrababu, K Meghna, K K Rebin, K R Kar, Kamalesh Bhattacharya, Kolahal Pant, Lalit M Athar, M Sajjad N Murthy, M V Malik, Manzoor A Naimuddin, Md Salim, Mohammad Ghosh, Monojit Devi, Moon Moon Mondal, Naba K Majumdar, Nayana Sinha, Nita Dash, Nitali Ghoshal, Pomita Mehta, Poonam Behera, Prafulla Kanishka, R Gandhi, Raj Ganai, Rajesh Hasan, Rashid Krishnaveni, S Lakshmi, S M Singh, S K R Inbanathan, S S Sankar, S Uma Jafer, Sadiq Biswas, Saikat Kumar, Sanjeev Agarwalla, Sanjib Kumar Choubey, Sandhya Saha, Satyajit Ahmed, Shakeel Behera, Shiba Prasad Goswami, Srubabati Chattopadhyay, Subhasis Bhattacharya, Sudeb Banerjee, Sudeshna Dasgupta, Sudeshna Pal, Sumanta Mukhopadhyay, Supratik Raut, Sushant Bose, Suvendu Mahapatra, Swapna Ghosh, Tapasi Thakore, Tarak S Kashyap, V K Subrahmanyam, V S Singh, Venktesh Chandratre, Vinay B Bhatnagar, Vipin Datar, Vivek M Bari, Waseem 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 | 10.1007/s12043-017-1373-4 |
format | Article |
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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>ISSN: 0304-4289</identifier><identifier>EISSN: 0973-7111</identifier><identifier>DOI: 10.1007/s12043-017-1373-4</identifier><language>eng</language><publisher>New Delhi: Springer India</publisher><subject>Antineutrinos ; Astronomy ; Astrophysics and Astroparticles ; Directional sensitivity ; Hadrons ; Magnetic monopoles ; Muons ; Neutrinos ; Observations and Techniques ; Parameter identification ; Parameter sensitivity ; Physics ; Physics and Astronomy</subject><ispartof>Pramāṇa, 2017-05, Vol.88 (5), p.1-72, Article 79</ispartof><rights>Indian Academy of Sciences 2017</rights><rights>Copyright Springer Science & Business Media 2017</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c382t-64d38655dc886aa28d961ba2e92253708f73e82bceca619606f0393289c3e2093</citedby><cites>FETCH-LOGICAL-c382t-64d38655dc886aa28d961ba2e92253708f73e82bceca619606f0393289c3e2093</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s12043-017-1373-4$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s12043-017-1373-4$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Kumar, A</creatorcontrib><creatorcontrib>Vinod Kumar, A M</creatorcontrib><creatorcontrib>Jash, Abhik</creatorcontrib><creatorcontrib>Mohanty, Ajit K</creatorcontrib><creatorcontrib>Chacko, Aleena</creatorcontrib><creatorcontrib>Ajmi, Ali</creatorcontrib><creatorcontrib>Ghosal, Ambar</creatorcontrib><creatorcontrib>Khatun, Amina</creatorcontrib><creatorcontrib>Raychaudhuri, Amitava</creatorcontrib><creatorcontrib>Dighe, Amol</creatorcontrib><creatorcontrib>Chatterjee, Animesh</creatorcontrib><creatorcontrib>Gaur, Ankit</creatorcontrib><creatorcontrib>Ghosh, Anushree</creatorcontrib><creatorcontrib>Kumar, Ashok</creatorcontrib><creatorcontrib>Redij, Asmita</creatorcontrib><creatorcontrib>Satyanarayana, B</creatorcontrib><creatorcontrib>Acharya, B S</creatorcontrib><creatorcontrib>Choudhary, Brajesh C</creatorcontrib><creatorcontrib>Ranganathaiah, C</creatorcontrib><creatorcontrib>Ravikumar, C D</creatorcontrib><creatorcontrib>Gupta, Chandan</creatorcontrib><creatorcontrib>Indumathi, D</creatorcontrib><creatorcontrib>Kaur, Daljeet</creatorcontrib><creatorcontrib>Majumdar, Debasish</creatorcontrib><creatorcontrib>Samuel, Deepak</creatorcontrib><creatorcontrib>Tiwari, Deepak</creatorcontrib><creatorcontrib>Rajasekaran, G</creatorcontrib><creatorcontrib>Gangopadhyay, Gautam</creatorcontrib><creatorcontrib>Majumder, Gobinda</creatorcontrib><creatorcontrib>Ravikumar, H B</creatorcontrib><creatorcontrib>Singh, J B</creatorcontrib><creatorcontrib>Shahi, J S</creatorcontrib><creatorcontrib>Libby, James</creatorcontrib><creatorcontrib>Singh, Jyotsna</creatorcontrib><creatorcontrib>Raveendrababu, K</creatorcontrib><creatorcontrib>Meghna, K K</creatorcontrib><creatorcontrib>Rebin, K R</creatorcontrib><creatorcontrib>Kar, Kamalesh</creatorcontrib><creatorcontrib>Bhattacharya, Kolahal</creatorcontrib><creatorcontrib>Pant, Lalit M</creatorcontrib><creatorcontrib>Athar, M Sajjad</creatorcontrib><creatorcontrib>N Murthy, M V</creatorcontrib><creatorcontrib>Malik, Manzoor A</creatorcontrib><creatorcontrib>Naimuddin, Md</creatorcontrib><creatorcontrib>Salim, Mohammad</creatorcontrib><creatorcontrib>Ghosh, Monojit</creatorcontrib><creatorcontrib>Devi, Moon Moon</creatorcontrib><creatorcontrib>Mondal, Naba K</creatorcontrib><creatorcontrib>Majumdar, Nayana</creatorcontrib><creatorcontrib>Sinha, Nita</creatorcontrib><creatorcontrib>Dash, Nitali</creatorcontrib><creatorcontrib>Ghoshal, Pomita</creatorcontrib><creatorcontrib>Mehta, Poonam</creatorcontrib><creatorcontrib>Behera, Prafulla</creatorcontrib><creatorcontrib>Kanishka, R</creatorcontrib><creatorcontrib>Gandhi, Raj</creatorcontrib><creatorcontrib>Ganai, Rajesh</creatorcontrib><creatorcontrib>Hasan, Rashid</creatorcontrib><creatorcontrib>Krishnaveni, S</creatorcontrib><creatorcontrib>Lakshmi, S M</creatorcontrib><creatorcontrib>Singh, S K</creatorcontrib><creatorcontrib>R Inbanathan, S S</creatorcontrib><creatorcontrib>Sankar, S Uma</creatorcontrib><creatorcontrib>Jafer, Sadiq</creatorcontrib><creatorcontrib>Biswas, Saikat</creatorcontrib><creatorcontrib>Kumar, Sanjeev</creatorcontrib><creatorcontrib>Agarwalla, Sanjib Kumar</creatorcontrib><creatorcontrib>Choubey, Sandhya</creatorcontrib><creatorcontrib>Saha, Satyajit</creatorcontrib><creatorcontrib>Ahmed, Shakeel</creatorcontrib><creatorcontrib>Behera, Shiba Prasad</creatorcontrib><creatorcontrib>Goswami, Srubabati</creatorcontrib><creatorcontrib>Chattopadhyay, Subhasis</creatorcontrib><creatorcontrib>Bhattacharya, Sudeb</creatorcontrib><creatorcontrib>Banerjee, Sudeshna</creatorcontrib><creatorcontrib>Dasgupta, Sudeshna</creatorcontrib><creatorcontrib>Pal, Sumanta</creatorcontrib><creatorcontrib>Mukhopadhyay, Supratik</creatorcontrib><creatorcontrib>Raut, Sushant</creatorcontrib><creatorcontrib>Bose, Suvendu</creatorcontrib><creatorcontrib>Mahapatra, Swapna</creatorcontrib><creatorcontrib>Ghosh, Tapasi</creatorcontrib><creatorcontrib>Thakore, Tarak</creatorcontrib><creatorcontrib>S Kashyap, V K</creatorcontrib><creatorcontrib>Subrahmanyam, V S</creatorcontrib><creatorcontrib>Singh, Venktesh</creatorcontrib><creatorcontrib>Chandratre, Vinay B</creatorcontrib><creatorcontrib>Bhatnagar, Vipin</creatorcontrib><creatorcontrib>Datar, Vivek M</creatorcontrib><creatorcontrib>Bari, Waseem</creatorcontrib><creatorcontrib>Viyogi, Y P</creatorcontrib><title>Invited review: Physics potential of the ICAL detector at the India-based Neutrino Observatory (INO)</title><title>Pramāṇa</title><addtitle>Pramana - J Phys</addtitle><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>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Directional sensitivity</subject><subject>Hadrons</subject><subject>Magnetic monopoles</subject><subject>Muons</subject><subject>Neutrinos</subject><subject>Observations and Techniques</subject><subject>Parameter identification</subject><subject>Parameter sensitivity</subject><subject>Physics</subject><subject>Physics and 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Neutrino Observatory (INO)</title><author>Kumar, A ; Vinod Kumar, A M ; Jash, Abhik ; Mohanty, Ajit K ; Chacko, Aleena ; Ajmi, Ali ; Ghosal, Ambar ; Khatun, Amina ; Raychaudhuri, Amitava ; Dighe, Amol ; Chatterjee, Animesh ; Gaur, Ankit ; Ghosh, Anushree ; Kumar, Ashok ; Redij, Asmita ; Satyanarayana, B ; Acharya, B S ; Choudhary, Brajesh C ; Ranganathaiah, C ; Ravikumar, C D ; Gupta, Chandan ; Indumathi, D ; Kaur, Daljeet ; Majumdar, Debasish ; Samuel, Deepak ; Tiwari, Deepak ; Rajasekaran, G ; Gangopadhyay, Gautam ; Majumder, Gobinda ; Ravikumar, H B ; Singh, J B ; Shahi, J S ; Libby, James ; Singh, Jyotsna ; Raveendrababu, K ; Meghna, K K ; Rebin, K R ; Kar, Kamalesh ; Bhattacharya, Kolahal ; Pant, Lalit M ; Athar, M Sajjad ; N Murthy, M V ; Malik, Manzoor A ; Naimuddin, Md ; Salim, Mohammad ; Ghosh, Monojit ; Devi, Moon Moon ; Mondal, Naba K ; Majumdar, Nayana ; Sinha, Nita ; Dash, Nitali ; Ghoshal, Pomita ; Mehta, Poonam ; Behera, Prafulla ; Kanishka, R ; Gandhi, Raj ; Ganai, Rajesh ; Hasan, Rashid ; Krishnaveni, S ; Lakshmi, S M ; Singh, S K ; R Inbanathan, S S ; Sankar, S Uma ; Jafer, Sadiq ; Biswas, Saikat ; Kumar, Sanjeev ; Agarwalla, Sanjib Kumar ; Choubey, Sandhya ; Saha, Satyajit ; Ahmed, Shakeel ; Behera, Shiba Prasad ; Goswami, Srubabati ; Chattopadhyay, Subhasis ; Bhattacharya, Sudeb ; Banerjee, Sudeshna ; Dasgupta, Sudeshna ; Pal, Sumanta ; Mukhopadhyay, Supratik ; Raut, Sushant ; Bose, Suvendu ; Mahapatra, Swapna ; Ghosh, Tapasi ; Thakore, Tarak ; S Kashyap, V K ; Subrahmanyam, V S ; Singh, Venktesh ; Chandratre, Vinay B ; Bhatnagar, Vipin ; Datar, Vivek M ; Bari, Waseem ; Viyogi, Y P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c382t-64d38655dc886aa28d961ba2e92253708f73e82bceca619606f0393289c3e2093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Antineutrinos</topic><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Directional sensitivity</topic><topic>Hadrons</topic><topic>Magnetic monopoles</topic><topic>Muons</topic><topic>Neutrinos</topic><topic>Observations and Techniques</topic><topic>Parameter identification</topic><topic>Parameter sensitivity</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kumar, A</creatorcontrib><creatorcontrib>Vinod Kumar, A M</creatorcontrib><creatorcontrib>Jash, Abhik</creatorcontrib><creatorcontrib>Mohanty, Ajit K</creatorcontrib><creatorcontrib>Chacko, Aleena</creatorcontrib><creatorcontrib>Ajmi, Ali</creatorcontrib><creatorcontrib>Ghosal, Ambar</creatorcontrib><creatorcontrib>Khatun, Amina</creatorcontrib><creatorcontrib>Raychaudhuri, Amitava</creatorcontrib><creatorcontrib>Dighe, Amol</creatorcontrib><creatorcontrib>Chatterjee, Animesh</creatorcontrib><creatorcontrib>Gaur, Ankit</creatorcontrib><creatorcontrib>Ghosh, Anushree</creatorcontrib><creatorcontrib>Kumar, Ashok</creatorcontrib><creatorcontrib>Redij, Asmita</creatorcontrib><creatorcontrib>Satyanarayana, B</creatorcontrib><creatorcontrib>Acharya, B S</creatorcontrib><creatorcontrib>Choudhary, Brajesh C</creatorcontrib><creatorcontrib>Ranganathaiah, C</creatorcontrib><creatorcontrib>Ravikumar, C D</creatorcontrib><creatorcontrib>Gupta, Chandan</creatorcontrib><creatorcontrib>Indumathi, D</creatorcontrib><creatorcontrib>Kaur, Daljeet</creatorcontrib><creatorcontrib>Majumdar, Debasish</creatorcontrib><creatorcontrib>Samuel, Deepak</creatorcontrib><creatorcontrib>Tiwari, Deepak</creatorcontrib><creatorcontrib>Rajasekaran, G</creatorcontrib><creatorcontrib>Gangopadhyay, Gautam</creatorcontrib><creatorcontrib>Majumder, Gobinda</creatorcontrib><creatorcontrib>Ravikumar, H B</creatorcontrib><creatorcontrib>Singh, J B</creatorcontrib><creatorcontrib>Shahi, J S</creatorcontrib><creatorcontrib>Libby, James</creatorcontrib><creatorcontrib>Singh, Jyotsna</creatorcontrib><creatorcontrib>Raveendrababu, K</creatorcontrib><creatorcontrib>Meghna, K K</creatorcontrib><creatorcontrib>Rebin, K R</creatorcontrib><creatorcontrib>Kar, Kamalesh</creatorcontrib><creatorcontrib>Bhattacharya, Kolahal</creatorcontrib><creatorcontrib>Pant, Lalit M</creatorcontrib><creatorcontrib>Athar, M Sajjad</creatorcontrib><creatorcontrib>N Murthy, M V</creatorcontrib><creatorcontrib>Malik, Manzoor A</creatorcontrib><creatorcontrib>Naimuddin, Md</creatorcontrib><creatorcontrib>Salim, Mohammad</creatorcontrib><creatorcontrib>Ghosh, Monojit</creatorcontrib><creatorcontrib>Devi, Moon Moon</creatorcontrib><creatorcontrib>Mondal, Naba K</creatorcontrib><creatorcontrib>Majumdar, Nayana</creatorcontrib><creatorcontrib>Sinha, Nita</creatorcontrib><creatorcontrib>Dash, Nitali</creatorcontrib><creatorcontrib>Ghoshal, Pomita</creatorcontrib><creatorcontrib>Mehta, Poonam</creatorcontrib><creatorcontrib>Behera, Prafulla</creatorcontrib><creatorcontrib>Kanishka, R</creatorcontrib><creatorcontrib>Gandhi, Raj</creatorcontrib><creatorcontrib>Ganai, Rajesh</creatorcontrib><creatorcontrib>Hasan, Rashid</creatorcontrib><creatorcontrib>Krishnaveni, S</creatorcontrib><creatorcontrib>Lakshmi, S M</creatorcontrib><creatorcontrib>Singh, S K</creatorcontrib><creatorcontrib>R Inbanathan, S S</creatorcontrib><creatorcontrib>Sankar, S Uma</creatorcontrib><creatorcontrib>Jafer, Sadiq</creatorcontrib><creatorcontrib>Biswas, Saikat</creatorcontrib><creatorcontrib>Kumar, Sanjeev</creatorcontrib><creatorcontrib>Agarwalla, Sanjib Kumar</creatorcontrib><creatorcontrib>Choubey, Sandhya</creatorcontrib><creatorcontrib>Saha, Satyajit</creatorcontrib><creatorcontrib>Ahmed, Shakeel</creatorcontrib><creatorcontrib>Behera, Shiba Prasad</creatorcontrib><creatorcontrib>Goswami, Srubabati</creatorcontrib><creatorcontrib>Chattopadhyay, Subhasis</creatorcontrib><creatorcontrib>Bhattacharya, Sudeb</creatorcontrib><creatorcontrib>Banerjee, Sudeshna</creatorcontrib><creatorcontrib>Dasgupta, Sudeshna</creatorcontrib><creatorcontrib>Pal, Sumanta</creatorcontrib><creatorcontrib>Mukhopadhyay, Supratik</creatorcontrib><creatorcontrib>Raut, Sushant</creatorcontrib><creatorcontrib>Bose, Suvendu</creatorcontrib><creatorcontrib>Mahapatra, Swapna</creatorcontrib><creatorcontrib>Ghosh, Tapasi</creatorcontrib><creatorcontrib>Thakore, Tarak</creatorcontrib><creatorcontrib>S Kashyap, V K</creatorcontrib><creatorcontrib>Subrahmanyam, V S</creatorcontrib><creatorcontrib>Singh, Venktesh</creatorcontrib><creatorcontrib>Chandratre, Vinay B</creatorcontrib><creatorcontrib>Bhatnagar, Vipin</creatorcontrib><creatorcontrib>Datar, Vivek M</creatorcontrib><creatorcontrib>Bari, Waseem</creatorcontrib><creatorcontrib>Viyogi, Y P</creatorcontrib><collection>CrossRef</collection><jtitle>Pramāṇa</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kumar, A</au><au>Vinod Kumar, A M</au><au>Jash, Abhik</au><au>Mohanty, Ajit K</au><au>Chacko, Aleena</au><au>Ajmi, Ali</au><au>Ghosal, Ambar</au><au>Khatun, Amina</au><au>Raychaudhuri, Amitava</au><au>Dighe, Amol</au><au>Chatterjee, Animesh</au><au>Gaur, Ankit</au><au>Ghosh, Anushree</au><au>Kumar, Ashok</au><au>Redij, Asmita</au><au>Satyanarayana, B</au><au>Acharya, B S</au><au>Choudhary, Brajesh C</au><au>Ranganathaiah, C</au><au>Ravikumar, C D</au><au>Gupta, Chandan</au><au>Indumathi, D</au><au>Kaur, Daljeet</au><au>Majumdar, Debasish</au><au>Samuel, Deepak</au><au>Tiwari, Deepak</au><au>Rajasekaran, G</au><au>Gangopadhyay, Gautam</au><au>Majumder, Gobinda</au><au>Ravikumar, H B</au><au>Singh, J B</au><au>Shahi, J S</au><au>Libby, James</au><au>Singh, Jyotsna</au><au>Raveendrababu, K</au><au>Meghna, K K</au><au>Rebin, K R</au><au>Kar, Kamalesh</au><au>Bhattacharya, Kolahal</au><au>Pant, Lalit M</au><au>Athar, M Sajjad</au><au>N Murthy, M V</au><au>Malik, Manzoor A</au><au>Naimuddin, Md</au><au>Salim, Mohammad</au><au>Ghosh, Monojit</au><au>Devi, Moon Moon</au><au>Mondal, Naba K</au><au>Majumdar, Nayana</au><au>Sinha, Nita</au><au>Dash, Nitali</au><au>Ghoshal, Pomita</au><au>Mehta, Poonam</au><au>Behera, Prafulla</au><au>Kanishka, R</au><au>Gandhi, Raj</au><au>Ganai, Rajesh</au><au>Hasan, Rashid</au><au>Krishnaveni, S</au><au>Lakshmi, S M</au><au>Singh, S K</au><au>R Inbanathan, S S</au><au>Sankar, S Uma</au><au>Jafer, Sadiq</au><au>Biswas, Saikat</au><au>Kumar, Sanjeev</au><au>Agarwalla, Sanjib Kumar</au><au>Choubey, Sandhya</au><au>Saha, Satyajit</au><au>Ahmed, Shakeel</au><au>Behera, Shiba Prasad</au><au>Goswami, Srubabati</au><au>Chattopadhyay, Subhasis</au><au>Bhattacharya, Sudeb</au><au>Banerjee, Sudeshna</au><au>Dasgupta, Sudeshna</au><au>Pal, Sumanta</au><au>Mukhopadhyay, Supratik</au><au>Raut, Sushant</au><au>Bose, Suvendu</au><au>Mahapatra, Swapna</au><au>Ghosh, Tapasi</au><au>Thakore, Tarak</au><au>S Kashyap, V K</au><au>Subrahmanyam, V S</au><au>Singh, Venktesh</au><au>Chandratre, Vinay B</au><au>Bhatnagar, Vipin</au><au>Datar, Vivek M</au><au>Bari, Waseem</au><au>Viyogi, Y P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Invited review: Physics potential of the ICAL detector at the India-based Neutrino Observatory (INO)</atitle><jtitle>Pramāṇa</jtitle><stitle>Pramana - J Phys</stitle><date>2017-05-01</date><risdate>2017</risdate><volume>88</volume><issue>5</issue><spage>1</spage><epage>72</epage><pages>1-72</pages><artnum>79</artnum><issn>0304-4289</issn><eissn>0973-7111</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>New Delhi</cop><pub>Springer India</pub><doi>10.1007/s12043-017-1373-4</doi><tpages>72</tpages></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0304-4289 |
ispartof | Pramāṇa, 2017-05, Vol.88 (5), p.1-72, Article 79 |
issn | 0304-4289 0973-7111 |
language | eng |
recordid | cdi_proquest_journals_1892388894 |
source | Indian Academy of Sciences; SpringerLink Journals - AutoHoldings |
subjects | Antineutrinos Astronomy Astrophysics and Astroparticles Directional sensitivity Hadrons Magnetic monopoles Muons Neutrinos Observations and Techniques Parameter identification Parameter sensitivity Physics Physics and Astronomy |
title | Invited review: Physics potential of the ICAL detector at the India-based Neutrino Observatory (INO) |
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