Georgiy Zatsepin

Georgiy Zatsepin

Georgiy Timofeyevich Zatsepin ( _ru. Георгий Тимофеевич Зацепин) (born OldStyleDate|May 28|1917|May 15 in Moscow) - Soviet/Russian astrophysicist, known for his works in cosmic rays physics and neutrino astrophysics.

Zatsepin graduated from the Faculty of Physics of the Moscow State University in 1941 and worked for three years at an aircraft building plant in Moscow and later in Irkutsk. He entered aspirantura of the faculty in 1944 and six years later defended dissertation "Density spectrum of Extensive Air Showers" for Candidate of Sciences degree. Prior to this, in 1947-1949 he developed methods of studying and using experimental data discovered, that they are based on nuclear cascade process, with electron-photon processes being secondary. Since 1950 he works as senior research assistant at the Lebedev Physical Institute. In 1951 he was awarded the USSR State Prize for discovering the nuclear cascade process. He defended dissertation "Nuclear-cascade process and EAS" for Doctor of Sciences degree in 1954 and became professor in 1958.

In the 1960s Zatsepin predicted Greisen-Zatsepin-Kuzmin limit. In the same period he begin research of muons and neutrinos laying foundations of neutrino astronomy and neutrino astrophysics. At the neutrino laboratory created by him in Lebedev Physical Institute methods of solar neutrino detection were developed. He became Corresponding Member of the USSR Academy of Sciences in 1968 and Full Member in 1981. In 1982 Zatsepin was awarded Lenin Prize for creating Station of Cosmic Rays of the Yakut Scientific-Research Base of the USSR Academy of Sciences. For creating the Baksan Neutrino Observatory, and conducting experiments there he was awarded Russian State Prize in 1998.

Zatsepin was also awarded the Order of the Red Banner of Labour in 1975 and 1981, Order of the October Revolution in 1987. Until 2006 was the chairman of the Cosmic Rays and Space Physics Chair of the MSU Skobeltsyn Institute of Nuclear Physics.

ources

* [http://www.inr.ru/zatsepin/index.html Georgy Zatsepin] at the Institute for Nuclear Research of the Russian Academy of Sciences
*Great Soviet Encyclopedia article on [http://slovari.yandex.ru/dict/bse/article/00027/33400.htm Georgy Zatsepin]


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Greisen-Zatsepin-Kuzmin limit — The Greisen Zatsepin Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic rays from distant sources. Computation of the GZK limit This limit was computed in 1966 by Kenneth Greisencite journal |last=Greisen |first=Kenneth …   Wikipedia

  • Greisen–Zatsepin–Kuzmin limit — The Greisen–Zatsepin–Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic rays (high energy charged particles from space) coming from distant sources. The limit is 5×1019 eV, or about 8 joules. The limit is set by slowing …   Wikipedia

  • Greisen-Zatsepin-Kuzmin Beschränkung — GZK Cutoff ist die nach den Physikern Kenneth Greisen [1], Georgiy Zatsepin und Vadim Kuzmin[2] benannte Obergrenze (engl. cutoff) für die Energie kosmischer Strahlung weitentfernter Quellen. Diese Grenze wurde von ihnen im Jahre 1966 errechnet.… …   Deutsch Wikipedia

  • GZK-Cutoff — ist die nach den Physikern Kenneth Greisen [1], Georgiy Zatsepin und Vadim Kuzmin[2] benannte Obergrenze (engl. cutoff) für die Energie kosmischer Strahlung sehr weit entfernter Quellen. Diese Grenze wurde von ihnen im Jahre 1966 errechnet.… …   Deutsch Wikipedia

  • Gzk — Cutoff ist die nach den Physikern Kenneth Greisen [1], Georgiy Zatsepin und Vadim Kuzmin[2] benannte Obergrenze (engl. cutoff) für die Energie kosmischer Strahlung weitentfernter Quellen. Diese Grenze wurde von ihnen im Jahre 1966 errechnet.… …   Deutsch Wikipedia

  • Gzk cutoff — ist die nach den Physikern Kenneth Greisen [1], Georgiy Zatsepin und Vadim Kuzmin[2] benannte Obergrenze (engl. cutoff) für die Energie kosmischer Strahlung weitentfernter Quellen. Diese Grenze wurde von ihnen im Jahre 1966 errechnet. Teilchen,… …   Deutsch Wikipedia

  • Scientific phenomena named after people — This is a list of scientific phenomena and concepts named after people (eponymous phenomena). For other lists of eponyms, see eponym. NOTOC A* Abderhalden ninhydrin reaction Emil Abderhalden * Abney effect, Abney s law of additivity William de… …   Wikipedia

  • SAGE (Soviet-American Gallium Experiment) — SAGE (Soviet–American Gallium Experiment, or sometimes Russian American Gallium Experiment) is a collaborative experiment devised by several prominent Physicists to measure the solar neutrino flux.The ExperimentSAGE was devised to measure the… …   Wikipedia

  • Russian Young Physicists' Tournament — The Russian Young Physicists’ Tournament is a competition among secondary school students in their ability to solve complicated scientific problems, to present solutions to these problems and to defend them in scientific discussions called… …   Wikipedia

  • Deaths in March 2010 — Contents 1 March 2010 1.1 31 1.2 30 1.3 29 …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”