La demostración, facilitada al autor en 2008 por Gloria Carvalho Kassar, se apoya en estudios de fenómenos opto electrónicos (propagación de ondas a través de fibra óptica).
La aplicación del teorema de Wiener–Khinchin a los resultados generaría, desde el punto de vista teórico, los valores correspondientes a toda la gama de radiaciones del espectro. A los efectos divulgativos de este espacio tampoco se ha considerado abundar en esos aspectos matemáticos, por lo que la aplicación de dicho teorema no se presenta.
Otro aspecto de la demostración que por razones obvias no es posible presentar es el relativo al factor de escala macroscópico. Se requeriría contar con un generador que produjera una onda del tamaño representativo (amplitud de la onda vs. tamaño de muestra del medio) al del ancho del universo a estudiar, y luego contar con detectores capaces de registrar con la debida precisión los datos, amén de que sería imprescindible tener un control lo más preciso posible de las anisotropías que caracterizaran la muestra del ancho del universo a estudiar.
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The interaction between the Media and the waves propagating through it is responsible to the wave’s frequency value diminution. In order to demonstrate it, the results of the studies of propagation of emissions through optical fibre are considered. Such results were taken and then extrapolate like a valid analogy to prove completely that the frequencies of waves are diminished by effect of the Medias that serve them to propagate.
The demonstration, a kind contribution in 2008 by PhD Gloria Carvalho Kassar, leans in Optoelectronics phenomena studies (wave’s propagation through optical fibre).
The Wiener-Khinchin theorem application to the results would generate, theoretically, the values corresponding to the whole range radiations Spectra. Is nor the scope of this site either consider to abound in those mathematical aspects, reason why the application of this theorem does not appear.
Another aspect of the demonstration that, for obvious reasons, is not possible to show is concerning to the macroscopic scale factor. It could be required to count on a generator producing representative amplitude waves compared to the Media size sample of the Universe to study, as well as to count on detectors able to register data precisely, in addition it would be essential to have properly characterized the Universe’s sample anisotropies to be studied.







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