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The Joint Institute for Nuclear Astrophysics (JINA) is a multi-institutional Physics Frontiers Center funded by the US National Science Foundation. JINA is a collaboration between Michigan State University, the University of Notre Dame, the University of Chicago, and a number of associated institutions, centers, and national laboratories in the US and across the world, with the goal bring together nuclear experimentalists, nuclear theorists, astrophysical modelers, astrophysics theorists, and observational astronomers to address the open scientific questions at the intersection of nuclear physics and astrophysics. JINA serves as an intellectual center and focal point for the rapidly growing and diversifying field of nuclear astrophysics, and enables and stimulates scientific work and exchange of data and information across field boundaries within its collaboration, and for the field as a whole though workshops, schools, and web-based tools and data bases. The JINA director is Michael Wiescher from the University of Notre Dame. Principal investigators are Hendrik Schatz (serving as co-director and science coordinator), Timothy Beers and Jim Truran.〔(【引用サイトリンク】url=http://www.jinaweb.org/html/people.html#pis )〕 The interdisciplinary nature of JINA enables it to address open questions at the frontiers of nuclear astrophysics: How did nature create the elements that we find today on earth? How do stars explode? What is the nature of neutron stars which are basically giant nuclei floating through space? Nuclear physics is at the heart of these phenomena. However, because of the extreme nature of the stellar conditions, the understanding of the underlying nuclear processes poses an enormous challenge to astrophysicists, nuclear theorists, and experimentalists. Advances in observational techniques allow astronomers to "see" farther into the history of our universe, and piece together a “fossil record” of chemical evolution of our Galaxy. Advances in supercomputing allow theorists to model stars and stellar explosions with much more realism. Advances in experimental nuclear astrophysics allow physicists to investigate many stellar processes in the laboratory using a wide range of techniques and facilities. They include innovative methods to measure the extremely slow reactions in the interiors of stars, as well as new facilities to produce the very same exotic, short-lived nuclei that come to existence in the extreme environments of stellar explosions and are thought to be the precursors of the stable elements found in nature. Most JINA nuclear physics experiments are carried out at the Nuclear Science Laboratory at the University of Notre Dame, the National Superconducting Cyclotron Laboratory at Michigan State University and the ATLAS/CARIBOU facility at Argonne National Laboratory. JINA is heavily involved in observations with the Apache Point Observatory within the framework of extensions to the Sloan Digital Sky Survey, LAMOST in China, SkyMapper in Australia, and the Hubble Space Telescope. Among many other observational data, JINA also uses heavily X-ray observational data from BeppoSAX, RXTE, Chandra, XMM-Newton, and INTEGRAL. JINA has stimulated the development of similar centers in other countries, and collaborates with a number of multi-institutional nuclear astrophysics centers in Germany, including NAVI, EMMI and the Universe Cluster in Munich. ==REACLIB Database== One of the many projects of JINA is the maintenance of an up to date nuclear reaction rate library called REACLIB.〔http://groups.nscl.msu.edu/jina/reaclib/db/〕 REACLIB contains over 75,000 thermonuclear reaction rates. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Joint Institute for Nuclear Astrophysics」の詳細全文を読む スポンサード リンク
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