Abstract
The challenge for search of dark matter reached a new stage and the theorists and experimentalists in the field are still struggling to find an absolute signature of the dark matter candidates of any species by direct or indirect methods of detection. Many mathematical formulations and ideas were proposed but till today the results are negative. Various experimentalist groups and theorist groups of the field are making ceaseless efforts to take the research to its high level but there is something missing in their work. In the present paper we examine why any of dark matter candidates are not detectable in the detectors either by direct or indirect techniques and what will be the most suitable candidates to be detected in near future on the machines. Rindler’s coordinates are also examined to understand dynamics of normal matter with coexistence of dark matter. The Cosmic Microwave Background (CMB) simulator is also produced here in suggestion for existence of dark matter in our universe.
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