The Planck Consortium has now published new analyses of data returned by the eponymous space telescope. The telescope on board of the Planck satellite has measured the distribution of the cosmic microwave background radiation (CMB), which, in essence, tells us what the Universe looked like about 400,000 years after the Big Bang. These latest findings are in complete agreement with the predictions of Mukhanov’s theory – for example, his calculation of the value of the so-called spectral index of the initial inhomogeneities. As Jean-Loup Puget, Principal Investigator for the HFI-instrument on the Planck satellite, stated: “The Planck data confirm the basic predictions that quantum fluctuations are at the origin of all structures in the Universe.” Mukhanov, who first published his model in 1981 and joined the Physics Faculty at LMU in 1997, says “I couldn’t hope for a better verification of my theory.”

For Mukhanov, the idea that quantum fluctuations must have played a role in the very earliest phase of the history of the Universe is implicit in Heisenberg’s Uncertainty Principle. Heisenberg showed that there is a specific limit to the precision with which the position and the momentum of a particle can be determined at any given moment. This in turn implies that the initial matter distribution will inevitably exhibit minute inhomogeneities in density. Mukhanov’s calculations first demonstrated that such quantum fluctuations could give rise to density differences in the early Universe, which in turn could serve as seeds for the galaxies and their clusters. Indeed, without quantum fluctuations, whose nature and magnitude Mukhanov quantitatively characterized, the observed distribution of matter in the Universe would be inexplicable.

The latest study of the Planck datasets is more detailed and more informative than the preliminary analysis published about 2 years ago. It reveals with unprecedented precision the patterns imprinted by primordial fluctuations on the distribution of radiation in the young Universe. Thus, instruments such as the Planck telescope can record these dispatches from an unimaginably remote past encoded in the microwave radiation that is still propagating through space – 13.8 billion years later. And from this information the Planck team can reconstruct a detailed picture of the distribution of matter at the birth of our Universe.

Furthermore, the Planck data show that a previously reported signal purportedly confirming the existence of so-called primordial gravitational waves can be largely attributed to dust in our own galaxy. The BICEP2 team is using a ground-based telescope in the Antarctic to search the CMB for signs of gravity waves produced immediately after the Big Bang. In March 2014, the team reported the detection of the long-sought pattern. However, doubts soon emerged regarding this interpretation. Now a joint analysis by the Planck and BICEP2 teams has concluded that the data do not actually provide observational evidence for gravitational waves. In the spring of 2014 Viatcheslav Mukhanov had already asserted that, if the theory is correct, then the BICEP2 and Planck teams could not both be right. Thus this latest Planck-BICEP2 analysis reassures us that the theoretical framework is well-founded. “Gravitational waves may well be there,” he said then, “but clearly our instruments are not yet sensitive enough to pick them up.” ­– Regardless of whether or not the search for primordial gravitational waves succeeds, he adds, no model that tries to capture the immediate aftermath of the Big Bang can now leave the quantum origin of the Universe’s structure out.

Quelle: LMU