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arxiv: 1505.07380 · v2 · submitted 2015-05-27 · ⚛️ physics.ins-det · hep-ex· hep-ph

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

The ICAL Collaboration: Shakeel Ahmed , M. Sajjad Athar , Rashid Hasan , Mohammad Salim , S. K. Singh (Aligarh Muslim U.) , S. S. R. Inbanathan (The American College) , Venktesh Singh , V. S. Subrahmanyam (Banaras Hindu U.)
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Shiba Prasad Behera Vinay B. Chandratre Nitali Dash Vivek M. Datar V. K. S. Kashyap Ajit K. Mohanty Lalit M. Pant (Bhabha Atomic Res. Ctr.) Animesh Chatterjee Sandhya Choubey Raj Gandhi Anushree Ghosh Deepak Tiwari (HRI Allahabad) Ali Ajmi S. Uma Sankar (Indian Inst. Tech. Mumbai) Prafulla Behera Aleena Chacko Sadiq Jafer James Libby K. Raveendrababu K. R. Rebin (Indian Inst. Tech. Madras) D. Indumathi K. Meghna S. M. Lakshmi M. V. N. Murthy Sumanta Pal G. Rajasekaran Nita Sinha (IMSc Chennai) Sanjib Kumar Agarwalla Amina Khatun (Inst. Phys. Bhubaneswar) Poonam Mehta (Nehru U.) Vipin Bhatnagar R. Kanishka A. Kumar J. S. Shahi J. B. Singh (Panjab U. Chandigarh) Monojit Ghosh Pomita Ghoshal Srubabati Goswami Chandan Gupta Sushant Raut (PRL Ahmedabad) Sudeb Bhattacharya Suvendu Bose Ambar Ghosal Abhik Jash Kamalesh Kar Debasish Majumdar Nayana Majumdar Supratik Mukhopadhyay Satyajit Saha (Saha Inst. Nucl. Phys. Kolkata) B. S. Acharya Sudeshna Banerjee Kolahal Bhattacharya Sudeshna DasGupta Moon Moon Devi Amol Dighe Gobinda Majumder Naba K. Mondal Asmita Redij Deepak Samuel B. Satyanarayana Tarak Thakore (TIFR C. D. Ravikumar A. M. Vinodkumar (Calicut U.) Gautam Gangopadhyay Amitava Raychaudhuri (Calcutta U.) Brajesh C. Choudhary Ankit Gaur Daljeet Kaur Ashok Kumar Sanjeev Kumar Md. Naimuddin (Delhi U.) Waseem Bari Manzoor A. Malik (Kashmir U.) Jyotsna Singh (Lucknow U.) S. Krishnaveni H. B. Ravikumar C. Ranganathaiah (Mysore U.) Swapna Mahapatra (Utkal U.) Saikat Biswas Subhasis Chattopadhyay Rajesh Ganai Tapasi Ghosh Y. P. Viyogi (VECC Calcutta)
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classification ⚛️ physics.ins-det hep-exhep-ph
keywords detectorneutrinophysicsicalatmospherichierarchymassneutrinos
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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.

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