Slides 2 - Nanyang Technological University

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n e , n m , n t are different mixtures of n 1, n 2, n 3 • The emitted neutrino ( n e ) is actually a mixture of n 1 , n 2 & n 3 • n e , n m , n t are different soups all made from the same ingredients n 1, n 2, n 3 e Original n1, n2, n3 soup n e Neutrino Soup n1, n2, n3 parts of soup travel at different speeds because they have different masses Neutrino flavor change implies neutrino mass n m t New different n1, n2, n3 soup 18
SNO comes to the rescue • Charged Current:n e • Neutral Current: n e+n m+n t • 7.6s difference n m,t are coming from the Sun! n x e n x e n e d p p e n n x d x 19 p n
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: • For neutrinos weak eigenstates
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 and 30: INO-ICAL Detector
Page 31 and 32: Physics using atmospheric neutrinos
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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