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Viatcheslav Fyodorovich Mukhanov (Russian: Вячесла́в Фёдорович Муха́нов; born October 2, 1956) is a Soviet/Russian born German theoretical physicist and cosmologist. He is best known for the theory of Quantum Origin of the Universe Structure. Working in 1980-1981 with Gennady Chibisov in the Lebedev Physical Institute in Moscow he predicted the spectrum of inhomogeneities in the Universe, which are originated from the initial quantum fluctuations. The numerous experiments in which there were measured the temperature fluctuations of the Cosmic Microwave Background Radiation are in excellent agreement with this theoretical prediction, thus confirming that the galaxies and their clusters originated from the initial quantum fluctuations. Later on Mukhanov proved that the results he obtained wi

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  • Wjatscheslaw Fjodorowitsch Muchanow (de)
  • Viacheslav Mujánov (es)
  • Viatcheslav Moukhanov (fr)
  • Муханов, Вячеслав Фёдорович (ru)
  • Viatcheslav Mukhanov (pt)
  • Viatcheslav Mukhanov (en)
  • 维亚切斯拉夫·穆哈诺夫 (zh)
rdfs:comment
  • Wjatscheslaw Fjodorowitsch Muchanow (russisch Вячеслав Фёдорович Муханов; engl. Transkription Vyacheslav Fyodorovich Mukhanov, auch Viatcheslav Fyodorovich Mukhanov; wiss. Transliteration Vjačeslav Fëdorovič Muchanov; * 2. Oktober 1956 in Kanasch, Tschuwaschien) ist ein russischstämmiger Astrophysiker, Kosmologe und Hochschullehrer. (de)
  • Viatcheslav Mukhanov, né le 2 octobre 1956, est un cosmologiste d'origine russe actuellement en poste à l'université de Munich (Allemagne). (fr)
  • Viatcheslav F. Mukhanov (em russo: Вячеслав Фёдорович Муханов, Wjatscheslaw Fjodorowitsch Muchanow; , Chuváchia, 2 de outubro de 1956) é um astrofísico e cosmologista russo. (pt)
  • Вячеслав Фёдорович Муханов (род. 2 октября 1956, Канаш, Чувашская АССР, РСФСР) — германский (до 1991 — советский) физик-теоретик, космолог, один из авторов доказательства инфляционной теории развития Вселенной. Профессор Мюнхенского университета, в котором с 1997 года руководит кафедрой физики астрочастиц и космологии физического факультета. (ru)
  • 维亚切斯拉夫·费奥多罗维奇·穆哈诺夫(俄語:Вячесла́в Фёдорович Муха́нов,1956年10月2日-),苏联/俄罗斯理论物理学家和宇宙学家。他最知名于宇宙结构的量子起源理论。1980年至1981年,在莫斯科列別捷夫物理研究所工作时,他与根纳季·奇比索夫预言了起源于原初量子涨落的宇宙的不均匀性谱。 宇宙微波背景辐射(CMB)温度涨落的实验测量结果与穆哈诺夫的理论预言符合得极好,从而证实了星系和星系团确实起源于原初量子涨落。 后来,穆哈诺夫进一步发展了广义的量子宇宙微扰理论。 (zh)
  • Viacheslav Fiódorovich Mujánov (en ruso, Вячесла́в Фёдорович Муха́нов); es un físico teórico ruso y cosmólogo. Es conocido por predecir el origen cuántico de la estructura del Universo. Entonces pasó a formar parte del Instituto de investigación nuclear también en Moscú, desde 1982 a 1991. Tras la caída de la Unión Soviética, desde 1992 a 1997 estuvo en el ETH Zúrich (Instituto Federal Suizo de Tecnología). Y en diciembre de 1997 pasó a formar parte del Universidad de Múnich. Ha recibido multitud de premios de los más destacados en sus campos de estudio. (es)
  • Viatcheslav Fyodorovich Mukhanov (Russian: Вячесла́в Фёдорович Муха́нов; born October 2, 1956) is a Soviet/Russian born German theoretical physicist and cosmologist. He is best known for the theory of Quantum Origin of the Universe Structure. Working in 1980-1981 with Gennady Chibisov in the Lebedev Physical Institute in Moscow he predicted the spectrum of inhomogeneities in the Universe, which are originated from the initial quantum fluctuations. The numerous experiments in which there were measured the temperature fluctuations of the Cosmic Microwave Background Radiation are in excellent agreement with this theoretical prediction, thus confirming that the galaxies and their clusters originated from the initial quantum fluctuations. Later on Mukhanov proved that the results he obtained wi (en)
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  • Viatcheslav Mukhanov (en)
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  • Viatcheslav Mukhanov (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/SlavaMukhanov.jpg
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