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arXiv:1006.2483hep-ph

Dark Matter: A Primer

Katherine Garrett, Gintaras Duda

Abstract

Dark matter is one of the greatest unsolved mysteries in cosmology at the present time. About 80% of the universe's gravitating matter is non-luminous, and its nature and distribution are for the most part unknown. In this paper, we will outline the history, astrophysical evidence, candidates, and detection methods of dark matter, with the goal to give the reader an accessible but rigorous introduction to the puzzle of dark matter. This review targets advanced students and researchers new to the field of dark matter, and includes an extensive list of references for further study.

arXiv comments
26 pages, 6 figures
Journal reference
Adv.Astron.2011:968283,2011
DOI
doi:10.1155/2011/968283
Subjects
hep-phHigh Energy Physics, Phenomenology astro-ph.COCosmology and Nongalactic Astrophysics

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    • That's right. Those are called massive compact halo objects (MACHOs). From "Dark Matter: A Primer" (https://arxiv.org/abs/1006.2483): To hunt for these objects two collaborations, the MACHO Collaboration and the EROS-2 Survey, searched for gravitational microlensing (the…

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