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  1. 31 de mai. de 2024 · Mais tarde, os dados colhidos pelo satélite Cosmic Background Explorer (COBE) e analisados por John Mather e George Smoot e os resultados do Wilkinson Microwave Anisotropy Project (WMAP) revelaram que esta radiação, hoje conhecida como radiação cósmica de fundo, corresponde de perto à emissão de um corpo negro a uma temperatura de 2,725 ...

  2. ncatlab.org › nlab › showFRW model in nLab

    7 de jun. de 2024 · The Friedmann– Lemaître –Robertson– Walker models (often FRW-models) are class of models in cosmology. These are solutions to Einstein's equations describing a spatially homogeneous and isotropic expanding or contracting spacetime. Hence these are solutions used as models in cosmology.

  3. Há 1 dia · Hart had previously worked with Nobel Prize-winning astrophysicist George Smoot to translate into music for human ears Smoot’s converted light wave traces from the Big Bang.

  4. 29 de mai. de 2024 · Cosmologist George Smoot, who later won the Nobel Prize with John Mather for his work leading the COBE mission, in a fit of hyperbole, described the result as ‘like seeing the face of God.’ Well, maybe. But simulations since have gone on to underline the importance of these tiny fluctuations.

  5. 26 de mai. de 2024 · The great cosmologist George Smoot walked us through the history of cosmological thought and the known parameters of the cosmos. Michel Mayor, discoverer of the first exoplanet orbiting a sunlike star, describes the paradigm change we are undergoing in discovering vast numbers of planetary systems.

  6. 7 de jun. de 2024 · George Smoot is an astrophysicist and cosmologist who won the Nobel Prize in Physics in 2006 for his work on the Cosmic Microwave Background Radiation, providing insight into the early universe.

  7. 2 de jun. de 2024 · George F. Smoot: George Smoot is an astrophysicist who won the Nobel Prize in Physics in 2006, along with John Mather, for their work on the Cosmic Background Explorer (COBE) satellite, which provided crucial measurements of the CMB’s spectrum and anisotropies.