Slides 2 - Nanyang Technological University

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Construction of the ICAL detector 30
Physics using atmospheric neutrinos during Phase I • Reconfirm atmospheric neutrino oscillation • Improved measurement of oscillation parameters • Search for potential matter effect in neutrino oscillation • Determining the sign of m 2 23 using matter effect • Measuring deviation from maximal mixing for 23 • Probing CP and CPT violation • Constraining long range leptonic forces • Ultra high energy neutrinos and muons 31
Page 1 and 2: India-based Neutrino Observatory Na
Page 3 and 4: a, b, g Rays
Page 5 and 6: Project Poltergeist Reines 1956 o n
Page 7 and 8: Where do neutrinos come from? • N
Page 9 and 10: Close Encounter with Neutrinos •
Page 11 and 12: Neutrinos from sun- Beginning of ne
Page 13 and 14: Homestake results 13
Page 15 and 16: Image of the sun as seen through ne
Page 17 and 18: • For neutrinos weak eigenstates
Page 19 and 20: SNO comes to the rescue • Charged
Page 21 and 22: Atmospheric Neutrinos 21
Page 23 and 24: Neutrino Masses and Mixing: Three G
Page 25 and 26: ICAL ( conceptual) RPC Test stand a
Page 27 and 28: INO site : Bodi West Hills Contact
Page 29: INO-ICAL Detector
Page 33 and 34: Neutrino Factory 7000 KM 33
Page 35 and 36: RPC building blocks 35
Page 37 and 38: Fabrication of 1m x 1m RPCs 37
Page 39 and 40: Prototype RPC Stack at TIFR trackin
Page 41 and 42: Some interesting cosmic ray tracks
Page 43 and 44: ICAL Front End Electronics chip dev
Page 45 and 46: Octant sensitivity Thakore et al, I
Page 47 and 48: Impact of d CP on mass hierarchy Si

Slides 2 - Nanyang Technological University

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