Growth of the nonbaryonic dark matter theory

Author(s): Peebles, P. James E.

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DC Field	Value	Language
dc.contributor.author	Peebles, P. James E.	-
dc.date.accessioned	2019-10-09T19:23:35Z	-
dc.date.available	2019-10-09T19:23:35Z	-
dc.date.issued	2017-03	en_US
dc.identifier.citation	Peebles, PJE. (2017). Growth of the nonbaryonic dark matter theory. NATURE ASTRONOMY, 1 (10.1038/s41550-017-0057	en_US
dc.identifier.issn	2397-3366	-
dc.identifier.uri	http://arks.princeton.edu/ark:/88435/pr1cq8s	-
dc.description.abstract	The evidence that has accumulated since the 1930s is that the mass of the Universe is dominated by an exotic nonbaryonic form of matter largely draped around the galaxies. This dark matter approximates an initially low-pressure gas of particles that interact only with gravity, but we know little more than that. Searches for detection thus must follow many difficult paths to a great discovery: what the Universe is made of.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartof	NATURE ASTRONOMY	en_US
dc.rights	Author's manuscript	en_US
dc.title	Growth of the nonbaryonic dark matter theory	en_US
dc.type	Journal Article	en_US
dc.identifier.doi	doi:10.1038/s41550-017-0057	-
dc.date.eissued	2017-03-02	en_US
pu.type.symplectic	http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article	en_US

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