International Conference on Neutrino Physics and Astrophysics

Last updated

The International Conference on Neutrino Physics and Astrophysics is a significant international conference series in the field of neutrino physics, during which talks detailing notable progress in theoretical and experimental work are given. In addition, the conference reviews the status of proposed research in neutrino physics and astrophysics. Held every two years, the conference programs consist of plenary sessions with invited speakers, poster sessions and short evening talks. The shorthand designator for a particular conference is "Neutrino" followed by its year, e.g. Neutrino 2011. [1]

The first conference was held in Balatonfüred in 1972; however, three preceding conferences are often referenced with respect to the history of the Neutrino series. These meetings include the 1965 Informal Conference on Experimental Neutrino Physics at CERN; a 1968 conference in Moscow sponsored by the Academy of the USSR, which was organized just after certain cosmic ray neutrino events were seen in the gold mines of India, South Africa and Utah; and a 1970 meeting in Cortona. [2]

Each conference is supervised by a changing International Advisory Committee as well as the permanent International Neutrino Commission. The latter is assembled from the chairs of former conferences.

The 28th meeting, Neutrino 2018, concluded June 9, 2018 in Heidelberg after featuring presentations encompassing many different branches of neutrino physics. [3] It was recently announced that Neutrino 2024 will be held in Milano, following the 2020 conference in Chicago and the 2022 conference in Seoul. [4]

Related Research Articles

The tau, also called the tau lepton, tau particle, tauon or tau electron, is an elementary particle similar to the electron, with negative electric charge and a spin of 1/2. Like the electron, the muon, and the three neutrinos, the tau is a lepton, and like all elementary particles with half-integer spin, the tau has a corresponding antiparticle of opposite charge but equal mass and spin. In the tau's case, this is the "antitau". Tau particles are denoted by the symbol
τ
and the antitaus by 
τ+
.

<span class="mw-page-title-main">Max Planck Society</span> Association of German research institutes

The Max Planck Society for the Advancement of Science is a formally independent non-governmental and non-profit association of German research institutes. Founded in 1911 as the Kaiser Wilhelm Society, it was renamed to the Max Planck Society in 1948 in honor of its former president, theoretical physicist Max Planck. The society is funded by the federal and state governments of Germany.

The Max Planck Institute for Extraterrestrial Physics is part of the Max Planck Society, located in Garching, near Munich, Germany. In 1991 the Max Planck Institute for Physics and Astrophysics split up into the Max Planck Institute for Extraterrestrial Physics, the Max Planck Institute for Physics and the Max Planck Institute for Astrophysics. The Max Planck Institute for Extraterrestrial Physics was founded as sub-institute in 1963. The scientific activities of the institute are mostly devoted to astrophysics with telescopes orbiting in space. A large amount of the resources are spent for studying black holes in the galaxy and in the remote universe.

<span class="mw-page-title-main">Max Planck Institute for Astronomy</span> Research institute of the Max Planck Society, Germany

The Max-Planck-Institut für Astronomie is a research institute of the Max Planck Society (MPG). It is located in Heidelberg, Baden-Württemberg, Germany near the top of the Königstuhl, adjacent to the historic Landessternwarte Heidelberg-Königstuhl astronomical observatory. The institute primarily conducts basic research in the natural sciences in the field of astronomy.

<span class="mw-page-title-main">SNOLAB</span> Canadian neutrino laboratory

SNOLAB is a Canadian underground science laboratory specializing in neutrino and dark matter physics. Located 2 km below the surface in Vale's Creighton nickel mine near Sudbury, Ontario, SNOLAB is an expansion of the existing facilities constructed for the original Sudbury Neutrino Observatory (SNO) solar neutrino experiment.

Astroparticle physics, also called particle astrophysics, is a branch of particle physics that studies elementary particles of astronomical origin and their relation to astrophysics and cosmology. It is a relatively new field of research emerging at the intersection of particle physics, astronomy, astrophysics, detector physics, relativity, solid state physics, and cosmology. Partly motivated by the discovery of neutrino oscillation, the field has undergone rapid development, both theoretically and experimentally, since the early 2000s.

<span class="mw-page-title-main">KM3NeT</span> European undersea neutrino detector

The Cubic Kilometre Neutrino Telescope, or KM3NeT, is a future European research infrastructure that will be located at the bottom of the Mediterranean Sea. It will host the next-generation neutrino telescope in the form of a water Cherenkov detector with an instrumented volume of several cubic kilometres distributed over three locations in the Mediterranean: KM3NeT-Fr, KM3NeT-It and KM3NeT-Gr. The KM3NeT project continues work done under the ANTARES, NEMO and NESTOR neutrino telescope projects.

The Max Planck Institute of Microstructure Physics in Halle (Saale) is a research institute in Germany in the field of materials research. It was founded in 1992 by Hellmut Fischmeister and is a follow-up to the German Academy of Sciences Institute of Solid State Physics and Electron Microscopy. The institute moved into new buildings from 1997 till 1999. It is one of 84 institutes in the Max Planck Society (Max-Planck-Gesellschaft).

<span class="mw-page-title-main">V420 Aurigae</span> Star in the constellation Auriga

V420 Aurigae is a high-mass star with an inferred compact companion. Closely orbiting each other every 0.8 days, they are a source of X-ray emission.

The International Cosmic Ray Conference, or ICRC, is a physics conference organized biennially by the Commission C4 of the International Union of Pure and Applied Physics (IUPAP) since 1947, where physicists from the whole world present the results of their research in Astroparticle Physics. The main topics of Astroparticle Physics are

<span class="mw-page-title-main">ICRANet</span>

ICRANet, the International Center for Relativistic Astrophysics Network, is an international organization which promotes research activities in relativistic astrophysics and related areas. Its members are four countries and three Universities and Research Centers: Armenia, the Federative Republic of Brazil, Italian Republic, the Vatican City State, the University of Arizona (USA), Stanford University (USA) and ICRA.

<span class="mw-page-title-main">NA61 experiment</span>

NA61/SHINE is a particle physics experiment at the Super Proton Synchrotron (SPS) at the European Organization for Nuclear Research (CERN). The experiment studies the hadronic final states produced in interactions of various beam particles with a variety of fixed nuclear targets at the SPS energies.

The Baikal Deep Underwater Neutrino Telescope (BDUNT) is a neutrino detector conducting research below the surface of Lake Baikal (Russia) since 2003. The first detector was started in 1990 and completed in 1998. It was upgraded in 2005 and again starting in 2015 to build the Baikal Gigaton Volume Detector (Baikal-GVD.) BDUNT has studied neutrinos coming through the Earth with results on atmospheric muon flux. BDUNT picks up many atmospheric neutrinos created by cosmic rays interacting with the atmosphere – as opposed to cosmic neutrinos which give clues to cosmic events and are therefore of greater interest to physicists.

Manfred Lindner is a German physicist and director at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. He conducts basic research in particle and astro-particle physics.

The Nucifer Experiment is a proposed test of equipment and methodologies for using neutrino detection for the monitoring of nuclear reactor activity and the assessment of the isotopic composition of reactor fuels for non-proliferation treaty compliance monitoring. Based upon an idea proposed by L.A. Mikaélyan in 1977, the Nucifer Experiment was proposed to the IAEA in October 2008.

<span class="mw-page-title-main">Astroparticle and Cosmology Laboratory</span>

The Astroparticle and Cosmology (APC) laboratory in Paris gathers researchers working in different areas including high-energy astrophysics, cosmology, gravitation, and neutrino physics.

ICRA, the International Center for Relativistic Astrophysics is an international research institute for relativistic astrophysics and related areas. Its members are seven Universities and four organizations. The center is located in Rome, Italy.

Probir Roy is an Indian particle physicist and a former professor at Tata Institute of Fundamental Research. He is also a senior scientist of the Indian National Science Academy at Bose Institute and a former Raja Ramanna fellow of Department of Atomic Energy at Saha Institute of Nuclear Physics.

Laura Baudis (1969) is a Romanian-born Swiss particle astrophysicist. She is employed as a full professor by the University of Zurich, Switzerland. Her research focuses on dark matter and neutrino physics. She is a member of the science strategy team for XENON as well as the CERN Scientific Policy Committee (2016–18) and the PSI Research Committee for Particle Physics.

References

  1. Frenkel, A.; Marx, G. (1975), Neutrino'75 IUPAP Conference Balatonfüred Hungary, 12-17 June 1975 proceedings, vol. 1, Budapest: Hungarian Phys. Soc, p. 1
  2. Schneps, J. (2015), Brief history of ‘Neutrino’, the International Conference on Neutrino Physics and Astrophysics, vol. 1666, 190002, doi: 10.1063/1.4915603, AIP Conference Proceedings, p. 2
  3. "Neutrino 2018". mpi-hd.mpg.de. Retrieved 2019-07-29.
  4. "INC Report (Neutrino 2018)" (PDF). mpi-hd.mpg.de. 2018-06-09. Retrieved 2019-07-29.