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  1. 20 de jun. de 2024 · Gabriele Veneziano, a young theorist working at the European Organization for Nuclear Research , contributed a key breakthrough in 1968 with his realization that a 200-year-old formula, the Euler beta function, was capable of explaining much of the data on the strong force then being collected at various particle accelerators around ...

  2. 12 de jun. de 2024 · La respuesta en términos de participación, subrayó el padre Gabriele Gionti, cosmólogo jesuita, vicedirector del Observatorio Vaticano- fue entusiasta.

  3. 19 de jun. de 2024 · Gabriele Veneziano: Video If you experience any problem watching the video, click the download button below. Download Embed. Show n. of views. Mp4: Low (101 kbps) Medium (1029 kbps) High (3207 kbps) More.. 324 kbps: Copy-paste this code into your page:

  4. 28 de jun. de 2024 · En 1968, Gabriele Veneziano introduit une formule pour décrire les interactions hadroniques. Cependant, c'est au milieu des années 1970 que le concept de la théorie commence à prendre forme grâce aux contributions de John Schwarz et Joël Scherk, qui démontrent qu'une particule de spin 2 et de masse nulle, identifiée comme le ...

  5. 10 de jun. de 2024 · This is an informal celebration of our distinguished colleague and friend Alvaro de Rujula, turning 80 in 2024. The scientific program will consist of talks by Howard Georgi (Harvard)), Jose Bernabeu (Valencia), Sheldon Glashow (Boston University) and Alvaro himself, followed by contributions by other participants. The talks will be streamed on Zoom, which will also allow for remote ...

  6. 20 de jun. de 2024 · Oggi il modello di universi paralleli viene unito alla Teoria delle Stringhe, della quale si cominciò a parlare nel 1965 grazie al fisico Gabriele Veneziano. Questa teoria vede tutte le particelle come ottenute dalla vibrazione di oggetti unidimensionali, detti “Stringhe”, che vibrano sino a 26 dimensioni.

  7. 17 de jun. de 2024 · In this paper, we use the dispersion measure ( DM DM) of fast radio bursts (FRB) combined with type Ia supernovae (SNe) data to investigate a possible redshift evolution of the fine-structure constant ( \alpha α), considering the runaway dilaton scenario, which predicts \frac {\Delta \alpha} {\alpha} = - \gamma\ln { (1+z)} αΔα = −γln(1+z), where...