India-based Neutrino Observatory (INO)...an indirect boost to CP sensitivity
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1 VietNus 2012: Towards CP Violation in Neutrino Oscillations Qui Nhon, December 2012 India-based Neutrino Observatory (INO)...an indirect boost to CP sensitivity Sushant Raut Physical Research Laboratory (PRL), Ahmedabad for the INO Collaboration
2 Outline Motivation: INO CP Violation Requirements for measuring CP INO: Details Physics aims Detector and simulations Current status INO: Physics potential Precision measurements Mass hierarchy measurement Octant measurement Towards CP measurement? Summary
3 Outline Motivation: INO CP Violation Requirements for measuring CP INO: Details Physics aims Detector and simulations Current status INO: Physics potential Precision measurements Mass hierarchy measurement Octant measurement Towards CP measurement? Summary
4 Q: Why should we discuss atmospheric neutrinos at a workshop on CP Violation?
5 Q: Why should we discuss atmospheric neutrinos at a workshop on CP Violation? Currently unknown oscillation parameters: Mass hierarchy d CP Octant of q 23 Hierarchy-d CP degeneracy: P(NH, d CP ) = P(IH, d CP )
6 Towards CPV discovery Q: What can we say about d CP, using data from existing/upcoming long baseline facilities? Huber, Lindner, Schwetz, Winter:
7 Measuring d CP Prakash, SR, Uma Sankar:
8 Measuring d CP Need to know the hierarchy first, in order to measure d CP! Prakash, SR, Uma Sankar:
9 Lifting the hierarchy-d CP degeneracy (with current/upcoming facilities) Current generation LBL Small matter effects
10 Lifting the hierarchy-d CP degeneracy (with current/upcoming facilities) Current generation LBL Small matter effects Combining data from various LBLs extensive literature...
11 Lifting the hierarchy-d CP degeneracy (with current/upcoming facilities) Current generation LBL Small matter effects Combining data from various LBLs Additional detector modules (hence higher statistics) extensive literature... Thomas: GLADE proposal; Agarwalla, Prakash, SR, Uma Sankar:
12 Lifting the hierarchy-d CP degeneracy (with current/upcoming facilities) Current generation LBL Atmospheric neutrinos Small matter effects Larger matter effects Combining data from various LBLs extensive literature... Additional detector modules (hence higher statistics) Wide range of L,E INO Thomas: GLADE proposal; Agarwalla, Prakash, SR, Uma Sankar: Gandhi et al: ; Blennow, Schwetz: ; Ghosh, Thakore, Choubey:
13 Outline Motivation: INO CP Violation Requirements for measuring CP INO: Details Physics aims Detector and simulations Current status INO: Physics potential Precision measurements Mass hierarchy measurement Octant measurement Towards CP measurement? Summary
14 INO: India-based Neutrino Observatory Ahmedabad: Physical Research Lab Aligarh: Aligarh Muslim Univ Allahabad: Harish-Chandra Research Inst Calicut: Univ of Calicut Chandigarh: Panjab Univ Chennai: IIT Madras, Inst of Mathematical Sciences Delhi: Univ of Delhi Guwahati: IIT Guwahati Hawaii: Univ of Hawaii Indore: IIT Indore Jammu: Univ of Jammu Kalpakkam: Indira Gandhi Centre for Atomic Research Kolkata: Ramakrishna Mission Vivekananda Univ, Saha Inst of Nuclear Physics, Variable Energy Cyclotron Centre, Univ of Calcutta Lucknow: Lucknow Univ Madurai: American College Mumbai: Bhabha Atomic Research Centre, IIT Bombay, Tata Inst of Fundamental Research Mysore: Univ of Mysore Sambalpur: Sambalpur Univ Srinagar: Univ of Kashmir Varanasi: Banaras Hindu Univ Collaborators are welcome!
15 Physics Aims of INO Detection of atmospheric neutrinos: wide range of L,E Iron Calorimeter (ICAL) with charge-id (magnetization), for nu-antinu separation Precision measurement of atmospheric parameters Mass hierarchy determination NSI, CPT violation, NDBD, ultra high energy muons, etc. Stage I: Atmospheric neutrino observatory Stage II: Detector for a future long baseline experiment??
16 Location of INO Bodi West Hills, Pottipuram village, Theni district, Tamil Nadu state ( 9 o 58 N, 77 o 16 E) 120 km west of Madurai town
17 The INO site Vertical cover :1289 m; all-round cover: ~1000 m Four caverns: Accessible through a 2 km tunnel Cavern 1: 50 kt ICAL (space for 100 kt) Caverns 2-4: Available for other experiments: NDBD, DM, etc. Underground cavern and tunnel, small surface lab at Pottipuram (outside the reserve forest boundary)
18 Construction updates INO project approved in principle by Indian funding agencies Environment and forest clearance obtained Tendering for site preparation in progress Pre-project works (approach roads, water supply, electricity connections) have begun
19 Detector factsheet
20 The ICAL Detector Iron plates (target mass) separated by glass RPCs (active detector): 150 layers Magnetization: Charge-id through bending of muons Directionality through tracking and timing (1 ns resolution) Modular structure, for ease of construction and modification Front end electronics chip developed at BARC Electronics Division
21 Detector updates Timing resolution, noise, tracking, etc of RPC being tested with cosmic muons RPC R&D almost complete. 2m x 2m RPCs being fabricated by the industry. 40 kt prototype tested in Kolkata. Both glass and bakelite RPCs tested. Electronics: Design and prototyping going on, ASIC front end being tested in RPC lab Magnetization: Prototype magnet running at VECC
22 Simulation framework
23 Simulation Updates Inhomogenous magnetic field map implemented Muon reconstruction: Energy and direction resolutions available, but efforts are on to improve them Hadron reconstruction: Energy resolutions available Neutrino energy resolution using muon and hadron momenta
24 Detector efficiency
25 Detector resolution
26 More work required Detector effects Improving sensitivity to electrons Improving angular resolution of neutrinos by more precise direction reconstruction for hadrons Lowering the energy threshold Improving resolution/efficiency for horizontal events Other systematic effects: Flux normalization uncertainty Flux tilt uncertainty Cross-section uncertainty
27 Outline Motivation: INO CP Violation Requirements for measuring CP INO: Details Physics aims Detector and simulations Current status INO: Physics potential Precision measurements Mass hierarchy measurement Octant measurement Towards CP measurement? Summary
28 Precision measurements (with projected priors on atmospheric parameters)
29 Mass hierarchy determination Impact of resolutions Gandhi et al: ; Also see Petcov, Schwetz: hep-ph/
30 Mass hierarchy timeline: INO
31 Mass hierarchy timeline: INO+others
32 Mass hierarchy determination Impact of systematics and priors 20-30% drop in sensitivity due to systematics Further 20-30% drop due to parameter uncertainties
33 Comparison & Combination INO 10 years data
34 Outline Motivation: INO CP Violation Requirements for measuring CP INO: Details Physics aims Detector and simulations Current status INO: Physics potential Precision measurements Mass hierarchy measurement Octant measurement Towards CP measurement? Summary
35 Q: Why should we discuss atmospheric neutrinos at a workshop on CP Violation?
36 Q: Why should we discuss atmospheric neutrinos at a workshop on CP Violation? Measuring d CP requires knowledge of the hierarchy With current LBL experiments, hierarchy sensitivity depends significantly on the value of d CP Atmospheric neutrino experiments (in particular INO) can determine hierarchy independently of d CP Combining with other experiments improves the sensitivity
37 Summary: INO Experiment Land acquired, civil construction to start soon RPC testing going on Improvements expected in energy and angular resolutions through simulations Data taking expected to start around 2017.
38 THANK YOU Thanks to Sandhya Choubey, Brajesh Choudhary, Amol Dighe, Anushree Ghosh, Pomita Ghoshal, Srubabati Goswami, Naba Mondal, M.V.N.Murthy and Tarak Thakore for their inputs.
39 BACKUP SLIDES
40 Atmospheric neutrino flux at Theni
41 INO Cavern Access tunnel Cavern 1 Cavern 2 Auxiliary tunnel
42 Mass hierarchy determination Impact of d CP Gandhi et al:
43 Mass hierarchy timeline: INO+others
44 RPC
45 Dighe: NuFact 2012
46 Testing RPCs using cosmic rays Timing resolution Pulse height resolution Tracking capability for muons and hadrons Noise rate
47 INO Timeline
Amol Dighe TIFR, Mumbai (On behalf of the INO Collaboration)
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Naba K Mondal, TIFR, Mumbai
ICAL ( conceptual) INO Peak at Bodi West Hills RPC Test stand at TIFR Prototype ICAL at VECC Naba K Mondal, TIFR, Mumbai 2mX2m RPC Test Stand at TIFR ASIC for RPC designed at BARC Ahmedabad: Physical Research
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