
Since the late 1970s, scientists have initiated discussions on neutrino astronomy experiments and put forward the proposal to construct DUMAND experiment. The 2002 Nobel Prize in Physics was jointly awarded in half to Raymond Davis Jr. and Masatoshi Koshiba "for their pioneering contributions to astrophysics, especially for the detection of cosmic neutrinos." In 2013, high - energy neutrinos from outside the solar system were detected for the first time in the IceCube experiment, which marked the beginning of a new era in high-energy neutrino astronomy.
Over the past half - century, remarkable progress has been achieved in neutrino astronomy experiments. Presently, a dynamic global research community has emerged, accompanied by an increasing interest from students and young scientists across the globe.
The advancement of this frontier requires international cooperation, state-of-the-art technologies, and the continuous efforts of successive generations of researchers. To promote knowledge exchange and expedite progress in neutrino astronomy, we are privileged to announce the inauguration of the China - Europe Neutrino Astronomy Summer School (CENA2026) in China.
CENA2026 is intended to assemble outstanding graduate students and early - career scientists from China and Europe to explore the latest advancements in neutrino physics and astrophysics. Participants will have the opportunity to learn directly from leading experts engaged in major global neutrino projects. The program provides intensive training in experimental techniques, data analysis, and scientific collaboration, while also facilitating students in establishing a long - lasting professional network for their future careers.
Owing to landmark achievements such as the PeV gamma - ray sources discovered by the Large High Altitude Air Shower Observatory (LHAASO) and similar experiments, as well as the successful deployment of large - scale underwater and ice - based detectors like KM3NeT, IceCube, and Baikal - GVD, we are now on the verge of a new era in high - energy astrophysics.
In this context, the Institute of High Energy Physics (IHEP) of the Chinese Academy of Sciences has proposed the High - energy Underwater Neutrino Telescope in Lake Baikal(Baikal-HUNT) — a next - generation underwater observatory with an effective volume of approximately 30 km³ or larger, designed for high - sensitivity observations of neutrino point sources in the Milky Way.
The summer school will span 10 days in Chengdu, the R&D base of the Baikal-HUNT project, offering in-depth technical exchanges and on-site visits to gain hands-on insight into the development of next generation neutrino detector.
And as the capital of Sichuan Province, Chengdu is a charming city celebrated for giant pandas, delicious Sichuan cuisine and a leisurely lifestyle. The Chengdu Research Base of Giant Panda Breeding lets visitors meet adorable pandas. Famous local food including spicy hotpot and mapo tofu brings unique numbing and spicy tastes. Locals love slow days: drinking tea in traditional teahouses and enjoying Sichuan opera. With a gentle pace, rich culture and friendly residents, Chengdu is an ideal place to experience authentic western China.
In addition, we will arrange a visit to the LHAASO site from the 22nd to the 23rd. And the visitors shall cover their own airfare and accommodation expenses.
Courses will cover a wide range of modern topics in neutrino physics, particle physics, and related interdisciplinary fields, bringing together frontier theories and experimental progress to provide participants with a comprehensive academic perspective.
Contact Information
For any inquiries or further information, please contact us at: Mr. Xicheng Liu.

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