Talk detail

Participant	Ostermann, Peter
Institution	independent research - valpichlerstr. 150 - munich - bayern - Germany

Session	CM2-3	Accepted		Order	Time
Talk	Poster abstract	Title	The PLANCK 2015 Mismatch of Sunyaev-Zeldovich Cluster Counts and a Universal Microwave Background Composed of Redshifted Radiation from 'Dark' Matter
Coauthors
Abstract	The PLANCK 2015 model predictions do not match the observed Sunyaev-Zeldovich cluster counts well. The discrepancy suggests that the data favour a steeper slope. The question is whether this behaviour might be in better agreement with a Planck microwave background as mathematically composed of redshifted radiation emitted from 'dark' matter within a stationary universe. This alternative has been recently derived for the first time. According to SUM (Stationary Universe Model) the SZ amplitude would be continuously weakened and vanishing at z >> 1, even its profile might be disturbed and slightly shifted to lower frequencies.
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Session	DM1	Accepted		Order	Time
Talk	Oral abstract	Title	Homogeneously distributed dark matter of second kind as an alternative to 'dark energy'
Coauthors
Abstract	A vast isothermal main part of nearly homogeneously distributed dark matter (HDM) might exist instead of the 'dark energy' assumed today. The known smaller inhomogeneous part (DM) is commonly accepted to be gravitationally bound to galaxies, clusters, separate halos, or larger structures. The macroscopically non-lensing HDM can fill the gap between observable matter and critical density, the latter required by flat space solutions of Einstein's original gravitational equations without cosmological constant. In the framework of a stationary universe model (SUM) – and in accordance with the universal Supernova Ia data deduced there – an alternative Planck microwave background is mathematically shown to be composable of redshifted radiation emitted within the universe. Thus 'dark' matter gets rid of its mysterious lack of physical interaction.
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