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How To See The Invisible: Using The Dark Matter Distribution To Test Our Cosmological Model

How To See The Invisible: Using The Dark Matter Distribution To Test Our Cosmological Model
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How to see the invisible: Using the dark matter distribution to test our cosmological model

How to see the invisible: Using the dark matter distribution to test our cosmological model
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How to see the invisible: Using the dark matt

Astrophysicists led by Princeton University and the astronomical communities of Japan and Taiwan have measured a value for the “clumpiness” of the universe’s dark matter (known to cosmologists as “S8”) of 0.776, which does not align with the value derived from the Cosmic Microwave Background, which dates back to the universe’s origins. This has intriguing implications for the standard cosmological model.

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How to see the invisible: Using the dark matter distribution to test our cosmological model

A Princeton-led team of astrophysicists has measured a surprising value for the “clumpiness” of the universe’s dark matter.

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Chemist and astrophysicist team up to uncover spatial patterns in distribution of galaxies

"You can study the holes between the galaxies similarly to the way you would study the structure of materials,” says Princeton theoretical chemist Salvatore Torquato. His new paper with astrophysicist Oliver Philcox offers new tools for understanding complicated structures from the atomic level to the Universe itself. 

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