Detection of dark-matter-radiation of stars during visible sun eclipses

Abstract

Recently a so-far unknown form of quantized, cold dark matter was detected on a laboratory scale which shows a complementary structure as compared to known forms of matter. From the experiments results that the observed quanta of the new type of matter as integer multiples of the Planck mass (mp = n · h·c (2 · π · G) = n 0 21.77 μ g , with n = 1, 2, 3 etc.) exhibit a spatially extended “field-like” structure ranging over distances of centimetres or more, opposite to the “point-like” structure of the known elementary particles of the standard model. Association of quanta of the new form of “soft” (or subtle) matter to clusters was observed, as well as re-clustering after absorption. Thus, between such quanta a physical interaction must exist. In addition, the new form of matter shows at least two interactions with normal matter, a gravitational one due to its real mass content and a so-far unknown “topological”, i.e. form-specific, interaction at phase borders. Additional indications for a weak electromagnetic interaction exist. Furthermore, the experimental results reveal that some types of quanta of the new form of “field-like” matter exhibit positive mass, as normal matter, but others exhibit a negative mass content, both in the order of magnitude of the Planck mass. Memory effects in normal matter were detected after absorption of quanta of the new form of soft matter. In general, the findings characterize the quanta of “fieldlike” matter as WIMP candidates of a cosmic background radiation of cold dark matter (quanta with positive mass) as well as of a cosmic background radiation of dark energy (quanta with negative mass). During visible sun eclipses in 1989, 1996 and. 1999, as well as during full moon of 6 January 2001, a so-far unknown form of dark-matter-radiation (“dark radiation”) was detected. The quanta of this “dark radiation” travel with the speed of light, but reveal macroscopic real mass, with positive and with negative mass content. The presented method of experimentation offers a so-far unknown form of astrophysical observation, based on dark matter detection.