Dark Matter and Dark Energy as a Derivate from Cosmic Photon Radiation


  •  Guido Zbiral    

Abstract

For many decades now, intensive efforts have been undertaken by physicists and cosmologists around the world to investigate dark matter (DM), without noticeable success to date. This situation leads me to believe that one of the assumptions underlying the current doctrine in physics may well be erroneous or incomplete since a breakthrough in this field of physics and cosmology would otherwise surely have already taken place by now.

For this year (2015) and the following two years, the CERN Nuclear Research Centre has set itself the task of using the LHC (now upgraded to 13 TeV) to investigate the still completely mysterious phenomenon of dark matter. The researchers at CERN favour the assumption – shared by the majority of physicists and cosmologists – that DM consists of massive non-baryonic particles (so-called WIMPs, Weakly Interacting Massive Particles) hitherto completely unknown to us, which produce a non-baryonic, static gravitational field distributed throughout the entire cosmos.

I cast doubt on the above assumption that DM is massive in nature. As this paper will show, DM can be far better (and more simply) explained in terms of a non-massive gravitational derivate of those photons consumed in the expansion of cosmic space (by performing the work of expansion), those photons thereby being transformed into static physical quantities. This gravitational derivate creates a free gravitational field (decoupled from the other forces of nature) of non-baryonic, static nature, regionally varying in intensity, and this is known as dark matter.



This work is licensed under a Creative Commons Attribution 4.0 License.
  • Issn(Print): 1916-9639
  • Issn(Onlne): 1916-9647
  • Started: 2009
  • Frequency: bimonthly

Journal Metrics

Google-based Impact Factor (2017): 3.90
h-index (November 2017): 17
i10-index (November 2017): 33
h5-index (November 2017): 12
h5-median (November 2017): 19

Learn more

Contact