Astro Skipper-CCD Detector

O'Neil, Judah

doi:10.2172/1656629

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DOE OSTI · 1656629

Astro Skipper-CCD Detector

O'Neil, Judah

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Abstract

Cosmologists have determined that the majority of the universe is composed of dark energy and nonbaryonic (not made of atoms) dark matter. Dark energy is an unknown form of energy, hypothesized to be the cause of the accelerating expansion of the universe. Dark matter can not be detected electromagnetically, however cosmologists are confident it exists because of its gravitational effect on galaxies. In spiral galaxies, we observe stars that orbit at speeds that can not be accounted for by the gravitational force of visible matter. This puzzling result is contrary to standard Newtonian gravity, yet makes sense if one assumes the gravitational effects of an unseen mass[1]. Better, more sensitive detectors are required to perform detailed measurements of faint stars and galaxies that will allow us to further understand these phenomena.

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BibTeX RIS

O'Neil, Judah. 2020-08-17. Astro Skipper-CCD Detector. https://doi.org/10.2172/1656629

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