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By Dixon D. O., Bland R. P.

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Einstein propugnó en 1917 una nueva deducción de la fórmula de radiación de Planck 86 , en la que el concepto clásico de intensidad de la radiación era sustituido por el concepto estadístico de probabilidad de transición de un estado estacionario a otro, que significó un importante progreso en el desarrollo de la teoría cuántica 87 .  Su debilidad reside en el hecho de que, de un lado, no nos ofrece conexión más estrecha con los conceptos ondulatorios, y de otro, deja SÁNCHEZ RON, José Manuel: Historia de la física cuántica.

NORTH, John David: The Measure of the Universe, Oxford, Clarendon Press, 1965, Dover, 1990. A. SCHILPP, P. A. ), op. , pp. 439­456. : "The origin of the chemical elements", Physical Review (letters), vol. 73, 1948.  DICKE, R. ; PEEBLES, P. J. ; ROLL, P. , y WILKINSON, D.  Y HERMAN, R. : “Physical Conditions in the Initial Stages of the Expanding Universe”, Physical Review, 92, 1953, pp.  WEINBERG, Steven: Los tres primeros minutos del Universo, Madrid, Alianza, 1982, (1ª ed. : Agujeros negros y pequeños universos.

Zeitschrift für Physik, 35, 1926, p. 557 y ss.  104.  121. 91 PAULI, Wolfgang: Zeitschrift für Physik, vol. 36, 1926, p. 336.  106. La situación en el otoño de 1925 no podía dejar de ser más confusa. Por una parte, el desarrollo de la nueva mecánica cuántica por Heisenberg, Born y Jordan ofrecía una teoría que resolvía matemáticamente los problemas que habían aquejado a la primera teoría cuántica, mediante la formulación de una nueva mecánica que cuestionaba profundamente los fundamentos de la mecánica clásica; pero, y esto es importante, la nueva teoría se basaba en la consideración corpuscular del electrón, obviando su posible comportamiento ondulatorio.

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A Bayes solution for the problem of ranking Poisson parameters by Dixon D. O., Bland R. P.


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