How Does the Quantum Structure of Electromagnetic Waves Describe Dark Matter?

Abstract

Dark matter is a kind of matter that we cannot see directly. Scientists have detected dark matter by analyzing the relationship between mass and velocity of the stars in galaxies. The higher speed of the stars implies more mass in the galaxies. However, they cannot describe it and its behavior clearly. Here we show that faster conversion of the dark matters spectrum to the Cosmic Microwave Background (CMB) is the reason why they are hidden. We found that observers out of the 72 light-years of dark matters do not receive their light. Hence, an emitter could be visible for nearby observers, while more distance observers might detect it as a dark matter.