WIMPs Search require new track
Journal Title: IOSR Journal of Applied Physics (IOSR-JAP) - Year 2018, Vol 10, Issue 6
Abstract
Weakly interacting massive particles (WIMPs) are believe to be most promising dark matter candidates by various groups of theorists and experimentalists working in the field. Search for dark matter become debatable as till today no direct evidence is available of any dark matter candidate from various group. Recent investigations of Large Underground Xenon (LUX) experiment and Particle and Astrophysical Xenon Detector-II (PandaX-II) got null result though LUX and PandaX-II experiments are sensitive to a wide range of WIMP candidates from approximately 5–1000 GeV/c2 [1,2]. In the present paper a brief investigation of reasons of not detecting Wimps at any experiment is presented. The analysis will help the experimentalist and theorists to make necessary up gradation in their work in designing the advance detectors of Wimps search.
Authors and Affiliations
Rakesh Sharma
Keywords
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- EP ID EP431998
- DOI 10.9790/4861-1006022023
- Views 61
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