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  1. en.wikipedia.org › wiki › Niels_BohrNiels Bohr - Wikipedia

    Hace 3 días · Niels Henrik David Bohr ( Danish: [ˈne̝ls ˈpoɐ̯ˀ]; 7 October 1885 – 18 November 1962) was a Danish physicist who made foundational contributions to understanding atomic structure and quantum theory, for which he received the Nobel Prize in Physics in 1922. Bohr was also a philosopher and a promoter of scientific research.

  2. Hace 5 días · Contribuciones posteriores y el Instituto Niels Bohr. Después de la publicación de su modelo atómico, Bohr continuó realizando importantes contribuciones a la física teórica. En 1922, recibió el Premio Nobel de Física por su trabajo sobre la estructura de los átomos y la radiación emitida por ellos.

  3. Hace 3 días · Heisenberg and Bohr developed the Copenhagen interpretation amidst the blossoming of new quantum theories in the first half of the twentieth century. In 1927, Heisenberg announced his important uncertainty principle : at the quantum level, certain pairs of quantities, such as momentum and position, cannot be simultaneously measured to any desired degree of precision.

  4. Hace 1 día · The views of Niels Bohr, Werner Heisenberg and other physicists are often grouped together as the "Copenhagen interpretation". [53] [54] According to these views, the probabilistic nature of quantum mechanics is not a temporary feature which will eventually be replaced by a deterministic theory, but is instead a final renunciation of the classical idea of "causality".

  5. Hace 5 días · The seventh edition of the Initial Stages (IS) international conference was organized by the Niels Bohr Institute High Energy Heavy ion Group in Copenhagen, 19–23 June 2023.The IS2023 (https://indi...

  6. Hace 1 día · And it’s in our Niels Bohr Institute DNA that we, of course, have to get it to work. Even though it is also a complex matter.« The pendulum is 25 metres long and hangs in the rotunda used by Geocenter Denmark and the Gefion Gymnasium.

  7. Hace 4 días · Anisotropies in the distance-redshift relation of cosmological sources are expected due to large-scale inhomogeneities in the local Universe. When the observed sources are tracing a large-scale matter flow in a general spacetime geometry, the distance-redshift relation with its anisotropies can be described with a geometrical prediction that generalises the well-known Friedmann-Lemaître ...

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