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arXiv:astro-ph/0608407astro-ph

A direct empirical proof of the existence of dark matter

Douglas Clowe, Marusa Bradac, Anthony H. Gonzalez, Maxim Markevitch, Scott W. Randall, Christine Jones, Dennis Zaritsky

Abstract

We present new weak lensing observations of 1E0657-558 (z=0.296), a unique cluster merger, that enable a direct detection of dark matter, independent of assumptions regarding the nature of the gravitational force law. Due to the collision of two clusters, the dissipationless stellar component and the fluid-like X-ray emitting plasma are spatially segregated. By using both wide-field ground based images and HST/ACS images of the cluster cores, we create gravitational lensing maps which show that the gravitational potential does not trace the plasma distribution, the dominant baryonic mass component, but rather approximately traces the distribution of galaxies. An 8-sigma significance spatial offset of the center of the total mass from the center of the baryonic mass peaks cannot be explained with an alteration of the gravitational force law, and thus proves that the majority of the matter in the system is unseen.

arXiv comments
Accepted for publication in ApJL
Journal reference
Astrophys.J.648:L109-L113,2006
DOI
doi:10.1086/508162
Subjects
astro-phAstrophysics

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Linked by 2 identifiable commenters in 2 comments across 2 threads, from Apr 2019 to Aug 2020. Found in 1 HN submission from Aug 2022 to Aug 2022. Open submission discussions.

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Discussed in comments2 threads

    • No, it doesn't help. Brown dwarfs as dark matter was a somewhat mainstream theory in the late 90s under the name MACHOs ("MAssive Compact Halo Objects"), but a seminal 2006 study of colliding galaxy dynamics in the "Bullet Cluster" definitively ruled out that possibility…

      AprilArcusView on HNParent context

    • It's referred to as plasma in the primary literature: https://arxiv.org/abs/astro-ph/0608407 Many people use hot/ionised gas and plasma interchangeably though. For example: https://academic.oup.com/mnras/article/389/2/967/974617

      joshvmView on HNParent context

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