International Neutrino Commission Report & Neutrino 2018
Stephen Parke - INC chair [email protected] F⌫AL
Unitarity is U †U = UU† = 1
– Typeset by FoilTEX – 1 to be called NEUTRINO ’72. It was organized by George Marx who also became Chair of the International Neutrino Commission (INC), formed to oversee the continuation of the series and establish rules for the format of the meetings. The numerology and the formal name of the series underwent various changes in the early years. From 1972 through 1979 the conferences were called NEUTRINO ‘XX (or a very close variation). In 1980 the formal name “Nth Conference on Neutrino Physics and Astrophysics” was adopted, with NEUTRINO XXXX continuing to be used as a short form nickname. The value of N also underwent changes. NEUTRINO ’72 was first denoted as the 4th conference (following CERN ’65, Moscow ’68, and Cortona ’70). In 1981 in Hawaii a transition occurred: at the opening talk NEUTRINO ’81 was described as the 11th in the series, but in the closing talk it was defined to be the 9th. The INC had met in between and decided to define NEUTRINO ’72 as the 1st, and the earlier CERN, Moscow and Cortona conferences as preludes. From 1972 to 1982 the conferences took place annually (except for 1973), but as experiments became larger and new results emerged more slowly, the decision was made to go to biannual meetings in even years, and to support the Weak Interaction and Neutrino (WIN) Workshops in the odd years. At about that time the membership of the INC was defined to consist of the chairs of the organizing committees of all previous NEUTRINO conferences (or substitutes) plus the overseer of WIN (Herbert Pietschmann). George Marx served as chair of the Commission from 1972 to 2002. He was our guiding spirit for 30 years, and passed away in 2002. Jacob Schneps carried on from 2002 to 2014, and Stephen Parke assumes the position in 2014.
In a way, this Conference took on a life of its own. As the field developed, the mysteries of neutrinos became more intriguing, theories more tantalizing, experiments more varied and larger, the number of physicists involved growing. NEUTRINO became the time and place where we all get together – to see where we are, where neutrinos are leading us, and to inspire each other. In between, of course, we have our smaller meetings to help us on our way – WIN, NuFact,Previous NuINT, etc., and poke Neutrino our noses into some bigger Conferences: ones too – ICHEP, Lepton-Photon. Conference Listing
Conference Location Chair No. Participants
1. NEUTRINO 1972 Balaton, Hungary George Marx* 139 2. NEUTRINO 1974 Philadelphia,PA, USA Sidney Bludman ~100 3. NEUTRINO 1975 Balaton, Hungary George Marx * 171 4. NEUTRINO 1976 Aachen, Germany Helmut Faissner* 267 5. NEUTRINO 1977 Elbrus, USSR M. Markov*, A.Tavkhelidze*, G. Zatsepin* 209 6. NEUTRINO 1978 Lafayette, IN, USA Earle Fowler* 264 7. NEUTRINO 1979 Bergen, Norway Cecilia Jarlskog 252 George 8. NEUTRINO 1980 Erice, Italy Ettore Fiorini ~100 9. NEUTRINO 1981 Maui,Hawaii,USA Vincent Peterson * 191 10. NEUTRINO 1982 Balaton, Hungary Deszo Kiss*, George Marx* 199 Marx 11. NEUTRINO 1984 Nordkirchen Germany Konrad Kleinknecht 232 12. NEUTRINO 1986 Sendai, Japan Toshio Kitagaki 230 13. NEUTRINO 1988 Boston, MA, USA Jacob Schneps 334 14. NEUTRINO 1990 Geneva, Switzerland Klaus Winter 339 15. NEUTRINO 1992 Granada, Spain Angel Morales* 261 16. NEUTRINO 1994 Eilat, Israel Arnon Dar 288 17. NEUTRINO 1996 Helsinki, Finland Matts Roos 308 18. NEUTRINO 1998 Takayama, Japan Yoichiro Suzuki, Yoji Totsuka* 339 19. NEUTRINO 2000 Sudbury, Canada Art McDonald 395 20. NEUTRINO 2002 Munich, Germany Franz v. Feilitzsch, Norbert Schmitz 410 21. NEUTRINO 2004 Paris, France François Vannucci, Daniel Vignaud 520 22. NEUTRINO 2006 Santa Fe, NM, USA Thomas Bowles ~450 23. NEUTRINO 2008 Christchurch, N. Zealand J. Adams, F. Halzen, S. Parke 294 24. NEUTRINO 2010 Athens, Greece George Tzanakos* 455 25. NEUTRINO 2012 Kyoto, Japan T. Kobayashi, M. Nakahata, T.Nakaya, 599 26. NEUTRINO 2014 Boston, MA, USA Gary Feldman, Ed Kearns 551 27. NEUTRINO 2016 London, U.K. Kenneth Long 28. NEUTRINO 2018 Heidelberg, Germany Manfred Lindner, Guido Drexlin 29. NEUTRINO 2020 Chicago, IL, USA Marvin Marshak, Jorge Morfin * deceased
190002-2 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions IP: 212.219.1.40 On: Fri, 08 Jul 2016 07:59:05 to be called NEUTRINO ’72. It was organized by George Marx who also became Chair of the International Neutrino Commission (INC), formed to oversee the continuation of the series and establish rules for the format of the meetings. The numerology and the formal name of the series underwent various changes in the early years. From 1972 through 1979 the conferences were called NEUTRINO ‘XX (or a very close variation). In 1980 the formal name “Nth Conference on Neutrino Physics and Astrophysics” was adopted, with NEUTRINO XXXX continuing to be used as a short form nickname. The value of N also underwent changes. NEUTRINO ’72 was first denoted as the 4th conference (following CERN ’65, Moscow ’68, and Cortona ’70). In 1981 in Hawaii a transition occurred: at the opening talk NEUTRINO ’81 was described as the 11th in the series, but in the closing talk it was defined to be the 9th. The INC had met in between and decided to define NEUTRINO ’72 as the 1st, and the earlier CERN, Moscow and Cortona conferences as preludes. From 1972 to 1982 the conferences took place annually (except for 1973), but as experiments became larger and new results emerged more slowly, the decision was made to go to biannual meetings in even years, and to support the Weak Interaction and Neutrino (WIN) Workshops in the odd years. At about that time the membership of the INC was defined to consist of the chairs of the organizing committees of all previous NEUTRINO conferences (or substitutes) plus the overseer of WIN (Herbert Pietschmann). George Marx served as chair of the Commission from 1972 to 2002. He was our guiding spirit for 30 years, and passed away in 2002. Jacob Schneps carried on from 2002 to 2014, and Stephen Parke assumes the position in 2014.
In a way, this Conference took on a life of its own. As the field developed, the mysteries of neutrinos became more intriguing, theories more tantalizing, experiments more varied and larger, the number of physicists involved growing. NEUTRINO became the time and place where we all get together – to see where we are, where neutrinos are leading us, and to inspire each other. In between, of course, we have our smaller meetings to help us on our way – WIN, NuFact,Previous NuINT, etc., and poke Neutrino our noses into some bigger Conferences: ones too – ICHEP, Lepton-Photon. Conference Listing
Conference Location Chair No. Participants
1. NEUTRINO 1972 Balaton, Hungary George Marx* 139 2. NEUTRINO 1974 Philadelphia,PA, USA Sidney Bludman ~100 3. NEUTRINO 1975 Balaton, Hungary George Marx * 171 4. NEUTRINO 1976 Aachen, Germany Helmut Faissner* 267 5. NEUTRINO 1977 Elbrus, USSR M. Markov*, A.Tavkhelidze*, G. Zatsepin* 209 6. NEUTRINO 1978 Lafayette, IN, USA Earle Fowler* 264 7. NEUTRINO 1979 Bergen, Norway Cecilia Jarlskog 252 George 8. NEUTRINO 1980 Erice, Italy Ettore Fiorini ~100 9. NEUTRINO 1981 Maui,Hawaii,USA Vincent Peterson * 191 10. NEUTRINO 1982 Balaton, Hungary Deszo Kiss*, George Marx* 199 Marx 11. NEUTRINO 1984 Nordkirchen Germany Konrad Kleinknecht 232 12. NEUTRINO 1986 Sendai, Japan Toshio Kitagaki 230 13. NEUTRINO 1988 Boston, MA, USA Jacob Schneps 334 14. NEUTRINO 1990 Geneva, Switzerland Klaus Winter 339 15. NEUTRINO 1992 Granada, Spain Angel Morales* 261 16. NEUTRINO 1994 Eilat, Israel Arnon Dar 288 17. NEUTRINO 1996 Helsinki, Finland Matts Roos 308 18. NEUTRINO 1998 Takayama, Japan Yoichiro Suzuki, Yoji Totsuka* 339 19. NEUTRINO 2000 Sudbury, Canada Art McDonald 395 20. NEUTRINO 2002 Munich, Germany Franz v. Feilitzsch, Norbert Schmitz 410 21. NEUTRINO 2004 Paris, France François Vannucci, Daniel Vignaud 520 22. NEUTRINO 2006 Santa Fe, NM, USA Thomas Bowles ~450 23. NEUTRINO 2008 Christchurch, N. Zealand J. Adams, F. Halzen, S. Parke 294 24. NEUTRINO 2010 Athens, Greece George Tzanakos* 455 25. NEUTRINO 2012 Kyoto, Japan T. Kobayashi, M. Nakahata, T.Nakaya, 599 26. NEUTRINO 2014 Boston, MA, USA Gary Feldman, Ed Kearns 551 27. NEUTRINO 2016 London, U.K. Kenneth Long 28. NEUTRINO 2018 Heidelberg, Germany Manfred Lindner, Guido Drexlin 29. NEUTRINO 2020 Chicago, IL, USA Marvin Marshak, Jorge Morfin * deceased
190002-2 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions IP: 212.219.1.40 On: Fri, 08 Jul 2016 07:59:05 to be called NEUTRINO ’72. It was organized by George Marx who also became Chair of the International Neutrino Commission (INC), formed to oversee the continuation of the series and establish rules for the format of the meetings. The numerology and the formal name of the series underwent various changes in the early years. From 1972 through 1979 the conferences were called NEUTRINO ‘XX (or a very close variation). In 1980 the formal name “Nth Conference on Neutrino Physics and Astrophysics” was adopted, with NEUTRINO XXXX continuing to be used as a short form nickname. The value of N also underwent changes. NEUTRINO ’72 was first denoted as the 4th conference (following CERN ’65, Moscow ’68, and Cortona ’70). In 1981 in Hawaii a transition occurred: at the opening talk NEUTRINO ’81 was described as the 11th in the series, but in the closing talk it was defined to be the 9th. The INC had met in between and decided to define NEUTRINO ’72 as the 1st, and the earlier CERN, Moscow and Cortona conferences as preludes. From 1972 to 1982 the conferences took place annually (except for 1973), but as experiments became larger and new results emerged more slowly, the decision was made to go to biannual meetings in even years, and to support the Weak Interaction and Neutrino (WIN) Workshops in the odd years. At about that time the membership of the INC was defined to consist of the chairs of the organizing committees of all previous NEUTRINO conferences (or substitutes) plus the overseer of WIN (Herbert Pietschmann). George Marx served as chair of the Commission from 1972 to 2002. He was our guiding spirit for 30 years, and passed away in 2002. Jacob Schneps carried on from 2002 to 2014, and Stephen Parke assumes the position in 2014.
In a way, this Conference took on a life of its own. As the field developed, the mysteries of neutrinos became more intriguing, theories more tantalizing, experiments more varied and larger, the number of physicists involved growing. NEUTRINO became the time and place where we all get together – to see where we are, where neutrinos are leading us, and to inspire each other. In between, of course, we have our smaller meetings to help us on our way – WIN, NuFact,Previous NuINT, etc., and poke Neutrino our noses into some bigger Conferences: ones too – ICHEP, Lepton-Photon. Conference Listing
Conference Location Chair No. Participants
1. NEUTRINO 1972 Balaton, Hungary George Marx* 139 2. NEUTRINO 1974 Philadelphia,PA, USA Sidney Bludman ~100 3. NEUTRINO 1975 Balaton, Hungary George Marx * 171 4. NEUTRINO 1976 Aachen, Germany Helmut Faissner* 267 5. NEUTRINO 1977 Elbrus, USSR M. Markov*, A.Tavkhelidze*, G. Zatsepin* 209 6. NEUTRINO 1978 Lafayette, IN, USA Earle Fowler* 264 7. NEUTRINO 1979 Bergen, Norway Cecilia Jarlskog 252 George 8. NEUTRINO 1980 Erice, Italy Ettore Fiorini ~100 9. NEUTRINO 1981 Maui,Hawaii,USA Vincent Peterson * 191 Marx 10. NEUTRINO 1982 Balaton, Hungary Deszo Kiss*, George Marx* 199 11. NEUTRINO 1984 Nordkirchen Germany Konrad Kleinknecht 232 Jack 12. NEUTRINO 1986 Sendai, Japan Toshio Kitagaki 230 13. NEUTRINO 1988 Boston, MA, USA Jacob Schneps 334 14. NEUTRINO 1990 Geneva, Switzerland Klaus Winter 339 Schneps 15. NEUTRINO 1992 Granada, Spain Angel Morales* 261 16. NEUTRINO 1994 Eilat, Israel Arnon Dar 288 17. NEUTRINO 1996 Helsinki, Finland Matts Roos 308 18. NEUTRINO 1998 Takayama, Japan Yoichiro Suzuki, Yoji Totsuka* 339 19. NEUTRINO 2000 Sudbury, Canada Art McDonald 395 20. NEUTRINO 2002 Munich, Germany Franz v. Feilitzsch, Norbert Schmitz 410 21. NEUTRINO 2004 Paris, France François Vannucci, Daniel Vignaud 520 22. NEUTRINO 2006 Santa Fe, NM, USA Thomas Bowles ~450 23. NEUTRINO 2008 Christchurch, N. Zealand J. Adams, F. Halzen, S. Parke 294 24. NEUTRINO 2010 Athens, Greece George Tzanakos* 455 25. NEUTRINO 2012 Kyoto, Japan T. Kobayashi, M. Nakahata, T.Nakaya, 599 26. NEUTRINO 2014 Boston, MA, USA Gary Feldman, Ed Kearns 551 27. NEUTRINO 2016 London, U.K. Kenneth Long 28. NEUTRINO 2018 Heidelberg, Germany Manfred Lindner, Guido Drexlin 29. NEUTRINO 2020 Chicago, IL, USA Marvin Marshak, Jorge Morfin * deceased
190002-2 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions IP: 212.219.1.40 On: Fri, 08 Jul 2016 07:59:05 Nu 2014
http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4915603
Brief History of ‘Neutrino’, The International Conference on Neutrino Physics and Astrophysics
Jacob Schneps 1,a)
1) Department of Physics and Astronomy Tufts University Medford, MA 02155
Abstract. We briefly review the history of the NEUTRINO conferences that began in 1972, with preludes taking place starting in 1965. We touch upon highlights, some un-highlights, various individuals, and the topics of interest.
Neutrinos are prolific, they are everywhere, but oh so elusive! In the times after Pauli’s 1930 hypothesis and Fermi’s 1934 theory the neutrino allowed us to understand beta decay and the production of energy in the sun, but directly observing neutrinos seemed hopeless. This changed with the development of nuclear reactors during World War II. Using the enormous flux of neutrinos from the Savannah River reactor Reines and Cowan, in the years 1953-1956, achieved the first direct detection of neutrino interactions. Within six years, in 1962, the first accelerator neutrino beam was built at Brookhaven and the muon neutrino was discovered. The possibility of detecting solar neutrinos, as a test of solar models, was being seriously considered. The idea that neutrino studies might lead to a deeper understanding of fundamental particle physics was in the air, and this led to the suggestion of a conference devoted primarily to neutrino physics. It took place at CERN, 20-22 January 1965, and was called “Informal Conference on Experimental Neutrino Physics”. The Proceedings are on the web and make fascinating reading [1]. It is worth quoting some excerpts from the opening speech of Victor Weisskopf, then Director General of CERN.
“This conference is an historic event. According to my recollection, I do not think there was ever a conference on neutrinos, so let us be conscious of something new in this world. This is the first conference on neutrinos which we are now assisting……..This will be a very small and very intimate discussion among friends from all parts and continents, to find out how best we proceed in this most exciting field of fundamental physics.”
There were twelve sessions dealing with high energy accelerator experiments, low energy reactor and double beta- decay experiments, cosmic and solar experiments, future proposals, and aspects of theory. Summary talks were by Maurice Goldhaber and T.D. Lee. Here are a couple of quotes – from Goldhaber, referring to a proposal for an undersea Cerenkov detector to observe atmospheric neutrinos: “ Uberall has suggested using deep caves filled with water to avoid being disturbed by swimming fish” - from Lee: “In two years the hardware used in neutrino physics increased more than a factor of 10 in its weight, and you can easily extrapolate to the possibility that in about forty years it may require the total mass of the earth”. Thinking about matter effects with up-going atmospheric neutrinos, we see he was not so far off (if you are willing to consider the Earth as part of the hardware, and why not).
The total attendance at the CERN meeting was 86. It was followed by small meetings in Moscow in 1968 [2] and Cortona, Italy [3] in 1970, more specifically devoted to neutrinos in astrophysics. After these meetings it was decided to formally make the neutrino conferences a continuing series, and the next was set for Balaton in Hungary,
XXVI International Conference on Neutrino Physics and Astrophysics AIP Conf. Proc. 1666, 190002-1–190002-10; doi: 10.1063/1.4915603 © 2015 AIP Publishing LLC 978-0-7354-1313-9/$30.00 190002-1 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions IP: 212.219.1.40 On: Fri, 08 Jul 2016 07:59:05 27. NEUTRINO 2016 London, UK Ken Long, Silvia Pascoli ~700 27. NEUTRINO 2016 London, UK Ken Long, Silvia Pascoli ~700 27. NEUTRINO 2016 London, UK Ken Long, Silvia Pascoli ~700
1000 Registrants by the 100th Birthday (2030) !!! International Neutrino Commission: (all passed chairs) meet Wednesday, July 6, 13:00-15:00
Members at Meeting: Ettore Fiorini (1980), INFN - Sezione di Milano Bicocca Jacob Schneps (1988), Tufts University Art McDonald (2000), Queen's University Francois Vannucci (2002), University of Paris VII Jenni Adams (2008), University of Canterbury Stephen Parke (2008, WIN) [Chair], FermiLab Masayuki Nakahata (2012), ICRR, University of Tokyo Tsuyoshi Nakaya (2012), Kyoto University Gary Feldman (2014), Harvard University Ed Kearns (2014), Boston University Ken Long (2016), Imperial College Silvia Pascoli (2016), Durham University Vittorio Palladino (WIN), INFN - Sezione di Napoli International Neutrino Commission: (all passed chairs) meet Wednesday, July 6, 13:00-15:00
Agenda for 2016 Meeting:
Members at Meeting: Open Section: Ettore Fiorini (1980), INFN - Sezione di Milano Bicocca Report of Nu2016 - London (10 mins) Update for Nu2018 - Heidelberg (5 mins) Jacob Schneps (1988), Tufts University Update for Nu2020 - ChicagoLand (5 mins) Art McDonald (2000), Queen's University Francois Vannucci (2002), University of Paris VII Proposals for 2022 in Asia: Jenni Adams (2008), University of Canterbury China (15 mins) Korea (15 mins) Stephen Parke (2008, WIN) [Chair], FermiLab Masayuki Nakahata (2012), ICRR, University of Tokyo Expressions of Interest for 2024 and beyond: Tsuyoshi Nakaya (2012), Kyoto University (< 5 mins each): Gary Feldman (2014), Harvard University Europe: Milano-Italy, Valencia-Spain, Ed Kearns (2014), Boston University Americas: Rio-Brazil, Irvine-USA, Virginia-USA Ken Long (2016), Imperial College Silvia Pascoli (2016), Durham University Closed Session: Decision on 2022. Vittorio Palladino (WIN), INFN - Sezione di Napoli Discussion on Geographic region for 2024.
Any other business
Future Neutrino Conferences: Future Neutrino Conferences:
• 2018 Heidelberg Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago
• 2022 Seoul Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago
• 2022 Seoul
• 2024 Europe Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago
• 2022 Seoul
• 2024 Europe
• 2026 Americas Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago
• 2022 Seoul
• 2024 Europe
• 2026 Americas
• 2028 Asia Future Neutrino Conferences:
• 2018 Heidelberg
• 2020 Chicago
• 2022 Seoul
• 2024 Europe
• 2026 Americas
• 2028 Asia
• 2030 Zurich, ETH ! Neutrino 2018 - Heidelberg June 4-9, 2018 Manfred Lindner & Guido Drexlin
https://www.mpi-hd.mpg.de/nu2018/6/8/16, 4:52 PM
. Preliminary web pages of NEUTRINO 2018 June 4-9, 2018, Heidelberg, Germany
Chair of the local organization committee: Manfred Lindner Max Planck Institut für Kernphysik Heidelberg, Germany http://www.mpi-hd.mpg.de/lin/
Co-Chair of the local organization committee: Guido Drexlin KIT - Karlsruhe Institute of Technology Karlsruhe, Germany then 2020 Chicago, 2022 Seoul https://neutrino.ikp.kit.edu/personal/drexlin/Home
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Images may be subject to copyright. Send feedback Something to Think about ! PMNS matrix Ue1 = cos ✓13 cos ✓12
500 km/GeV Ue2 = cos ✓13 sin ✓12 PMNS15,000 matrix: km/GeV i Ue3 = sin ✓13 e ⌫e Ue1 Ue2 Ue3 ⌫1 Uµ3 = cos ✓13 sin ✓23 ⌫ = U U U ⌫ U(1)⌧3 = cos ✓13 cos ✓13 0 µ 1 0 µ1 µ2 µ3 1 0 2 1 ⌫⌧ U⌧1 U⌧2 U⌧3 ⌫3 U 2 > U 2 > U 2 | e1| | e2| | e3| Mass 2 2 2 @ A @ flavor 2 A @2 A sin ✓13 0.02, sin ✓12 0.3 and sin ✓23 0.5 m31 30 m21 > 0Eigenstates SNO 2 2 • | | ⇡ m31 30 ⇡ m21 > 0 SNO ⇡ ⇡ states | | ⇡ Why do we label the mixing angles of the2 PMNS2 2 matrix as Normal2 2 Ordering:2 m2 (cos2 ✓ = cos2 ✓ 0.99) e3 13 ⇡ – Typeset by FoilTEX – 8 PMNS matrix Ue1 = cos ✓13 cos ✓12 500 km/GeV Ue2 = cos ✓13 sin ✓12 PMNS15,000 matrix: km/GeV i Ue3 = sin ✓13 e ⌫e Ue1 Ue2 Ue3 ⌫1 Uµ3 = cos ✓13 sin ✓23 ⌫ = U U U ⌫ U(1)⌧3 = cos ✓13 cos ✓13 0 µ 1 0 µ1 µ2 µ3 1 0 2 1 ⌫⌧ U⌧1 U⌧2 U⌧3 ⌫3 U 2 > U 2 > U 2 | e1| | e2| | e3| Mass 2 2 2 @ A @ flavor 2 A @2 A sin ✓13 0.02, sin ✓12 0.3 and sin ✓23 0.5 m31 30 m21 > 0Eigenstates SNO 2 2 • | | ⇡ m31 30 ⇡ m21 > 0 SNO ⇡ ⇡ states | | ⇡ WhyWhy do do we we label label the the mixing mixing angles angles of of the the2 PMNS PMNS2 2 matrix matrix as as Normal2 2 Ordering:2 m2 2 2 (cos(cos2 ✓ ✓e=3 = cos cos2 ✓ ✓13 0.99)0.99) e3 13 ⇡⇡ – Typeset by FoilTEX – 8 – Typeset by FoilTEX – 8 PMNS matrix Ue1 = cos ✓13 cos ✓12 500 km/GeV Ue2 = cos ✓13 sin ✓12 PMNS15,000 matrix: km/GeV i Ue3 = sin ✓13 e ⌫e Ue1 Ue2 Ue3 ⌫1 Uµ3 = cos ✓13 sin ✓23 ⌫ = U U U ⌫ U(1)⌧3 = cos ✓13 cos ✓13 0 µ 1 0 µ1 µ2 µ3 1 0 2 1 ⌫⌧ U⌧1 U⌧2 U⌧3 ⌫3 U 2 > U 2 > U 2 | e1| | e2| | e3| Mass 2 2 2 @ AWhy@ do weflavor label the mixing angles2 A @ of2 the PMNSA sin matrix✓13 as0.02, sin ✓12 0.3 and sin ✓23 0.5 m31 30 m21 > 0Eigenstates SNO 2 2 • | | ⇡ m31 30 ⇡ m21 > 0 SNO ⇡ ⇡ states | | ⇡ WhyWhy do do we we label label the the mixing mixing angles angles of of the the2 PMNS PMNS2 2 matrix matrix as as Normal2 2 Ordering:2 m2 • Poster Presenters (~400) • You the Participants (~700) • Poster Presenters (~400) • Scientific Speakers (~80) International Advisory Committees: XXVII International Conference on Neutrino Physics and Astrophysics 7/8/16, 3:57 AM International Advisory Committees: International Neutrino Commission The InternationalINC Neutrino Commission is the custodian of the International Conference on Neutrino Physics and Astrophysics. Jenni Adams, University of Canterbury Sidney Bludman, University of Maryland Thomas Bowles, Los Alamos National Laboratory Arnon Dar, Technion Israel Institute of Technology Franz von Feilitzsch, TU München Gary Feldman, Harvard University Ettore Fiorini, INFN - Sezione di Milano Bicocca Francis Halzen, University of Wisconsin-Madison Cecilia Jarlskog, Lund University Ed Kearns, Boston University Toshio Kitagaki, Tohoku University Konrad Kleinknecht, Johannes Gutenberg-Universität Mainz Takashi Kobayashi, High Energy Accelerator Research Organization (KEK) John Learned, University of Hawaii, Manoa William Louis, Los Alamos National Laboratory Arthur B McDonald, Queen's University, Canada Masayuki Nakahata, University of Tokyo Institute for Cosmic Ray Research Tsuyoshi Nakaya, Kyoto University Vittorio Palladino, INFN - Sezione di Napoli Stephen Parke (Chair), Fermi National Accelerator Laboratory Herbert Pietschmann, University of Vienna Matts Roos, University of Helsinki Norbert Schmitz, Max Planck Institute for Physics Jacob Schneps, Tufts University Yoichiro Suzuki, University of Tokyo Francois Vannucci, University of Paris VII Daniel Vignaud, University of Paris VII Supporting organisations IOP Conferences Conferences Calendar Subscribe Follow us Our current and archive events programme Subscribe to our weekly email #physicsconference Terms & Conditions Refund policy Send Feedback http://neutrino2016.iopconfs.org/advisory_committee Page 2 of 2 XXVII International Conference on Neutrino Physics and Astrophysics 7/8/16, 4:00 AM Key dates Public lecture ballot ticket entry deadline: 17 June 2016 Registration deadline (waiting list): 17 June 2016 #Neutrino2016 Documents Second announcement (PDF, 1MB) First announcement (PDF, 1MB) A3 conference poster (PDF, 1MB) XXVII International Conference on Neutrino Physics and Astrophysics 7/8/16, 3:57 AM A4 conference leaflet (PDF, 1.2MB) International AdvisoryInternational Committees: Committees International Neutrino Commission International2016 Advisory Committee IAC The International Neutrino Commission is the custodian of the International Conference on Neutrino Physics and Astrophysics. INC Laura Baudis, University of Zurich Jun Cao, Institute of High Energy Physics (IHEP), Chinese Academy of Sciences Jenni Adams, University of Canterbury Doug Cowen, The Pennsylvania State University Sidney Bludman, University of Maryland Scott Dodelson, Fermi National Accelerator Laboratory / University of Chicago Thomas Bowles, Los Alamos National Laboratory Yasaman Farzan, Institute for Research in Fundamental Sciences (IPM) Bonnie Fleming, Yale University Arnon Dar, Technion Israel Institute of Technology Katherine Freese, Nordic Institute for Theoretical Physics Franz von Feilitzsch, TU München Maury Goodman, Argonne National Laboratory Gary Feldman, Harvard University Giorgio Gratta, Stanford University Ettore Fiorini, INFN - Sezione di Milano Bicocca Yoshinari Hayato, The University of Tokyo Institute for Cosmic Ray Research Francis Halzen, University of Wisconsin-Madison Atsuko Ichikawa, Kyoto University Cecilia Jarlskog, Lund University Kunio Inoue, Tohoku University Ed Kearns, Boston University Stavros Katsanevas, Paris Diderot University Toshio Kitagaki, Tohoku University Soo-Bong Kim, Seoul National University Yoshi Kuno, Osaka University Konrad Kleinknecht, Johannes Gutenberg-Universität Mainz Thierry Lasserre, CEA Takashi Kobayashi, High Energy Accelerator Research OrganizationManfred (KEK) Lindner, Max Planck Institute for Nuclear Physics John Learned, University of Hawaii, Manoa Francesca Di Lodovico, Queen Mary, University of London William Louis, Los Alamos National Laboratory Antonio Masiero, Istituto Nazionale di Fisica Nucleare Sezione di Padova Arthur B McDonald, Queen's University, Canada Mauro Mezzetto, Istituto Nazionale di Fisica Nucleare Sezione di Padova Masayuki Nakahata, University of Tokyo Institute for Cosmic RayHisakazu Research Minakata, Tokyo Metropolitan University / Universidade de São Paulo Tsuyoshi Nakaya, Kyoto University Naba K Mondal, Tata Institute of Fundamental Research Vittorio Palladino, INFN - Sezione di Napoli Ann Nelson, University of Washington Stephen Parke (Chair), Fermi National Accelerator LaboratoryHamish Robertson, University of Washington Alexei Yu Smirnov, Max Planck Institute for Nuclear Physics / International Centre for Theoretical Physics (ICTP) Herbert Pietschmann, University of Vienna Nigel Smith, SNOLAB Matts Roos, University of Helsinki Jan Sobczyk, University of Wroclaw Norbert Schmitz, Max Planck Institute for Physics Hirohisa Tanaka, University of British Columbia Jacob Schneps, Tufts University Morimitsu Tanimoto, Niigata University Yoichiro Suzuki, University of Tokyo Jenny Thomas, University College London Francois Vannucci, University of Paris VII Licia Verde, ICREA / ICCUB / Harvard University / Oslo University Daniel Vignaud, University of Paris VII Raymond Volkas, University of Melbourne Yifang Wang , Institute of High Energy Physics (IHEP), Chinese Academy of Sciences Yvonne Wong, University of New South Wales Sam Zeller, Fermi National Accelerator Laboratory Supporting organisations International Neutrino Commission The International Neutrino Commission is the custodian of the International Conference on Neutrino Physics and Astrophysics. Jenni Adams, University of Canterbury Sidney Bludman, University of Maryland Thomas Bowles, Los Alamos National Laboratory Arnon Dar, Technion Israel Institute of Technology Franz von Feilitzsch, TU München http://neutrino2016.iopconfs.org/advisory_committee Page 1 of 2 IOP Conferences Conferences Calendar Subscribe Follow us Our current and archive events programme Subscribe to our weekly email #physicsconference Terms & Conditions Refund policy Send Feedback http://neutrino2016.iopconfs.org/advisory_committee Page 2 of 2 XXVII International Conference on Neutrino Physics and Astrophysics 7/8/16, 4:06 AM Key dates Public lecture ballot ticket entry deadline: 17 June 2016 Registration deadline (waiting list): 17 June 2016 #Neutrino2016 Documents Second announcement (PDF, 1MB) First announcement (PDF, 1MB) A3 conference poster (PDF, 1MB) A4 conference leaflet (PDF, 1.2MB) LocalLocal Organizing Organising Committee: Committee Henrique Araujo, Imperial College London David Colling, Imperial College London Carlo Contaldi, Imperial College London Peter Dornan, Imperial College London Andrey Golutvin, Imperial College London Steve F King, University of Southampton Kenneth Long (Co-chair), Imperial College London/STFC Silvia Pascoli (Co-chair), Durham University/Institute for Particle Physics Phenomenology Jaroslaw Pasternak, Imperial College London/RAL Jürgen Pozimski, Imperial College London/RAL Pat Scott, Imperial College London Julia K Sedgbeer, Imperial College London Yoshi Uchida, Imperial College London David Wark, University of Oxford/RAL Morgan Wascko, Imperial College London Supporting organisations http://neutrino2016.iopconfs.org/committee Page 1 of 2 XXVII International Conference on Neutrino Physics and Astrophysics 7/8/16, 4:06 AM Key dates Public lecture ballot ticket entry deadline: 17 June 2016 Registration deadline (waiting list): 17 June 2016 #Neutrino2016 Documents Second announcement (PDF, 1MB) First announcement (PDF, 1MB) A3 conference poster (PDF, 1MB) A4 conference leaflet (PDF, 1.2MB) LocalLocal Organizing Organising Committee: Committee Henrique Araujo, Imperial College London David Colling, Imperial College London Carlo Contaldi, Imperial College London Peter Dornan, Imperial College London Andrey Golutvin, Imperial College London Steve F King, University of Southampton Kenneth Long (Co-chair), Imperial College London/STFC Silvia Pascoli (Co-chair), Durham University/Institute for Particle Physics Phenomenology Jaroslaw Pasternak, Imperial College London/RAL Jürgen Pozimski, Imperial College London/RAL Pat Scott, Imperial College London Julia K Sedgbeer, Imperial College London Yoshi Uchida, Imperial College London David Wark, University of Oxford/RAL Morgan Wascko, Imperial College London Supporting organisations http://neutrino2016.iopconfs.org/committee Page 1 of 2 Co-Chairs Silvia Pascoli & Ken Long