Please download the first announcement for important details regarding the conference. ![]() More information can be found on the registration page of this website.įirst Announcement of the XXVII Conference on Neutrino Physics and Astrophysics (Neutrino 2016). Neutrino 2016 Second Announcement (PDF, 1MB) Registration open (February 2016) Please download the second announcement for further important details regarding the conference. Social programme and Professor Brian Cox public lecture event details announced. Second announcement (May 2016)įull programme information and current participant list available on website. Proceedings information can be found here, online submission will be available shortly. Group photograph (National Maritime Museum, 7 July 2016)ĭownload the delegate handbook for onsite information. Neutrino 2016 was an exciting event in which past achievements were celebrated and ground-breaking new results were discussed. Please submit full papers online by 30 September 2016. of 2016, experiments have shown that these masses are tiny in magnitude. The latest IceCube data suggest that the all-flavor cosmic neutrino flux may be as large. JPCS Volume 888 Paper submission (8 July 2016) A neutrino is a fermion that interacts only via the weak interaction and gravity. Proceedings from the Neutrino 2016 are available online at Latest news Proceedings (22 September 2017) The Nobel Prize in Physics 2015 Laureates: Takaaki Kajita, University of Tokyo, Japan and Arthur B McDonald, Queen's University, Canada The conference consists of invited plenary talks and contributed poster sessions. Its primary purpose is to review the status of the field of neutrino physics, the impact of neutrino physics on astronomy and cosmology, and the vision for the future development of these fields. This conference is held every other year. “The up-coming beam test at CERN also generated some excitement.The XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino 2016) will be held in London from Monday 4 July to Saturday 9 July 2016. “I had some very technical questions about the electronics, in particular the cold electronics and the signal chimney,” said Dawson. ![]() Jaime Dawson of APC-Paris, who presented a poster titled The ProtoDUNE large demonstrator of the Liquid Argon double phase TPC program at CERN, fielded quite a few questions, mostly about how the dual phase works and the difference between this technology and the single phase. ![]() “I think this highlights the increasing number of young scientists - students and postdocs - now working on DUNE, and the great progress being made in many different areas,” said Blake, who presented a poster on atmospheric neutrino studies planned for DUNE. Deadline for early-bird registration: 10 November 2016. In addition to the 11 posters presented on behalf of DUNE (listed in Urheim’s slides), several more were closely related to DUNE activities. Neutrinoless double beta decay Solar, atmospheric and supernova neutrinos Neutrino cosmology. “DUNE also had a great showing in the poster sessions at Neutrino 2016,” said Andy Blake of Lancaster University. Other speakers in the session addressed the statistical power of measuring the parameters describing the matter-antimatter asymmetry and described the proposed Hyper-Kamiokande program in Japan. In addition, postdoctoral fellows and graduate students are presenting their work at. He highlighted the unique physics capabilities of DUNE for solving the open questions in neutrino physics, searching for nucleon decay, and measuring the neutrinos from a galactic supernova. conferences, including Neutrino 2016 and the Lake Louise conference. In a session on future long-baseline neutrino experiments, Jon Urheim of Indiana University presented the status and physics case of the LBNF/DUNE program. Many of the 700 conference attendees were members of the DUNE collaboration. Neutrino physicists from around the world met in London at the XXVIIth International Conference on Neutrino Physics and Astrophysics in early July to discuss recent results and future prospects for understanding neutrinos.
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