AstroParticule et Cosmologie (APC) | |
Type | Mixed Research Unit (UMR) |
---|---|
Established | 2005 |
Director | Antoine Kouchner |
Academic staff | 157 |
Administrative staff | 14 |
31 | |
Location | Paris , France |
Campus | Paris Rive Gauche (location) |
Affiliations | Paris Cité University, CNRS, CEA, Paris Observatory |
Website | www |
The Astroparticle and Cosmology (APC) laboratory in Paris gathers researchers (experimentalists, theorists and observers) working in different areas including high-energy astrophysics, cosmology, gravitation, and neutrino physics. [1]
The institute was founded in January 2005 [2] [3] and soon moved to new Great Mills campus of Paris Cité University in the Paris Rive Gauche area.
The laboratory is a "Mixed Research Unit" in French terminology, funded by Paris Diderot University, the Centre national de la recherche scientifique (represented by three of its Institutes: mainly IN2P3, but also INSU and INP), the Commissariat à l'énergie atomique et aux énergies alternatives, and the Paris Observatory.
The first director of the laboratory was Pierre Binétruy (2005-2013). From January 2014 until December 2017 the director was Stavros Katsanevas, followed by Sotiris Loucatos, and Antoine Kouchner (since July 2018).
This group, headed by Cyrille Rosset, includes two main areas of research:
Research carried out by this group, headed by Anne Lemière, aims at understanding the violent phenomena of the universe (mostly within compact stars, neutron stars, or black holes). The group is engaged in many international projects with telescopes or instruments detecting photons, cosmic rays, or neutrinos. For the observation of:
The research carried out by this group, headed by Davide Franco, is dedicated to understanding neutrino properties is one of the laboratories' main activities. Researchers are involved in studies of the phenomenon of oscillation (Borexino, Double Chooz) [17] [18] and on future projects addressing the measurement of the neutrino mass hierarchy with atmospheric neutrinos with the deep-sea water Cherenkov telescope Orca [19] and the long-baseline neutrino oscillation project Laguna-LBNO. [20]
This core research of this group led by Stanislav Babak is the direct detection of gravitational waves. The group is involved in both ground-based (Virgo interferometer) [21] and space-based (Laser Interferometer Space Antenna and its precursor LISA Pathfinder) instruments. [22]
This group, headed by Dmitri Semikoz, covers the research topics of the laboratory from a theoretical perspective. It also carries out work on other areas of fundamental physics.
The staff of the laboratory consists of 75 permanent researchers and over 60 engineers, technicians, and administrative personnel, plus about 125 non-permanent employees (PhD students, postdoctoral fellows, visitors). In addition, the Paris Center for Cosmological Physics directed by George Smoot is also part of the laboratory [23] and one of the three functional centres of the Astroparticle Physics European Consortium is based here. [24]
An "International Associated Laboratory" in astroparticle physics was launched in September 2007. It associates the APC laboratory with the Kavli Institute for Particle Astrophysics and Cosmology (Stanford University). [25]
The laboratory has been evaluated twice by the AERES: in 2008 [26] and in 2013. [1] In the latter evaluation, the lab won excellent scores (A or A+ in all criteria).
Astroparticle Physics European Consortium (APPEC) is a consortium of organizations from European countries that coordinate and fund research in astroparticle physics. [27]
DESY, short for Deutsches Elektronen-Synchrotron, is a national research centre for fundamental science located in Hamburg and Zeuthen near Berlin in Germany. It operates particle accelerators used to investigate the structure, dynamics and function of matter, and conducts a broad spectrum of interdisciplinary scientific research in four main areas: particle and high energy physics; photon science; astroparticle physics; and the development, construction and operation of particle accelerators. Its name refers to its first project, an electron synchrotron. DESY is publicly financed by the Federal Republic of Germany and the Federal States of Hamburg and Brandenburg and is a member of the Helmholtz Association.
The French National Institute of Nuclear and Particle Physics, also known as CNRS Nucléaire & Particules, is the coordinating body for nuclear and particle physics in France. It was established in 1971 as a division of the French National Centre for Scientific Research (CNRS). Its purpose is "to promote and unite research activities in the various fields of physics".
The Max-Planck-Institut für Kernphysik is a research institute in Heidelberg, Germany.
The Supernova Cosmology Project is one of two research teams that determined the likelihood of an accelerating universe and therefore a positive cosmological constant, using data from the redshift of Type Ia supernovae. The project is headed by Saul Perlmutter at Lawrence Berkeley National Laboratory, with members from Australia, Chile, France, Portugal, Spain, Sweden, the United Kingdom, and the United States.
ANTARES is a neutrino detector residing 2.5 km under the Mediterranean Sea off the coast of Toulon, France. It is designed to be used as a directional neutrino telescope to locate and observe neutrino flux from cosmic origins in the direction of the Southern Hemisphere of the Earth, a complement to the South Pole neutrino detector IceCube that detects neutrinos from both hemispheres. The experiment is a recognized CERN experiment (RE6). Other neutrino telescopes designed for use in the nearby area include the Greek NESTOR telescope and the Italian NEMO telescope, which are both in early design stages. The data taking of ANTARES was finished in February 2022, after 16 years of continuous operation.
Laboratori Nazionali del Gran Sasso (LNGS) is the largest underground research center in the world. Situated below Gran Sasso mountain in Italy, it is well known for particle physics research by the INFN. In addition to a surface portion of the laboratory, there are extensive underground facilities beneath the mountain. The nearest towns are L'Aquila and Teramo. The facility is located about 120 km from Rome.
Astroparticle physics, also called particle astrophysics, is a branch of particle physics that studies elementary particles of astrophysical 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.
The Cubic Kilometre Neutrino Telescope, or KM3NeT, is a European research infrastructure located at the bottom of the Mediterranean Sea. It hosts the next-generation neutrino telescope with water Cherenkov detectors.
ASPERA is a network of national government agencies responsible for coordinating and funding national research efforts in astroparticle physics.
José W. F. Valle is a Spanish physicist.
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.
The Canfranc Underground Laboratory is an underground scientific facility located in the former railway tunnel of Somport under Monte Tobazo (Pyrenees) in Canfranc. The laboratory, 780 m deep and protected from cosmic radiation, is mainly devoted to study rarely occurring natural phenomena such as the interactions of neutrinos of cosmic origin or dark matter with atomic nuclei.
The Laboratoire d'Annecy de physique des particules, usually abbreviated as LAPP, is a French experimental physics laboratory located in Annecy in the Haute-Savoie department of France. It is associated with both the French particle and nuclear physics institute IN2P3, a subdivision of the CNRS research council, and the Université Savoie Mont Blanc.
Large Apparatus studying Grand Unification and Neutrino Astrophysics or LAGUNA was a European project aimed to develop the next-generation, very large volume underground neutrino observatory. The detector was to be much bigger and more sensitive than any previous detector, and make new discoveries in the field of particle and astroparticle physics. The project involved 21 European institutions in 10 European countries, and brought together over 100 scientists.
Stavros Katsanevas was a Greek-French astrophysicist who was director of the European Gravitational Observatory, professor at the Université Paris Cité, former director of the AstroParticle and Cosmology (APC) laboratory and former chairman of the Astroparticle Physics European Consortium (APPEC). In 2000, he received for his work on supersymmetry the Physics Prize from the Academy of Athens. In 2011, he was awarded the Ordre National du Merite. He was an ordinary member of Academy of Europe, Earth and Cosmic Sciences since 2019.
Multi-messenger astronomy is the coordinated observation and interpretation of multiple signals received from the same astronomical event. Many types of cosmological events involve complex interactions between a variety of astrophysical processes, each of which may independently emit signals of a characteristic "messenger" type: electromagnetic radiation, gravitational waves, neutrinos, and cosmic rays. When received on Earth, identifying that disparate observations were generated by the same source can allow for improved reconstruction or a better understanding of the event, and reveals more information about the source.
Nicolao Fornengo is an Italian physicist. He is currently Full Professor at the University of Turin and he works on astroparticle physics, neutrino physics and cosmology.
Francis Louis Halzen is a Belgian particle physicist. He is the Hilldale and Gregory Breit Distinguished Professor at the University of Wisconsin–Madison and Director of its Institute for Elementary Particle Physics. Halzen is the Principal Investigator of the IceCube Neutrino Observatory at the Amundsen–Scott South Pole Station in Antarctica, the world's largest neutrino detector which has been operational since 2010.
Teresa Montaruli is an Italian astronomer specializing in neutrino astronomy, and in particular in the search for high-energy neutrinos from cosmic sources. She is a professor in the particle physics department at the University of Geneva.
Pierre Binétruy was a French theoretical physicist, known for his research on cosmology, gravitational waves, strong nuclear interactions, and supersymmetry.
Created the 1st January 2005, APC is managed, other than by the Paris Diderot University, by the CNRS 1, the CEA 2 and the Observatoire de Paris.
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