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http://arxiv.org/abs/0806.2179...
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Preprint . 2008
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Astrophysics and Space Science
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Shock waves in the large-scale structure of the Universe

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2008Embargo end date: 01 Jan 2008 English Publisher:Springer NetherlandsJournal:Astrophysics and Space Science, volume 322, pages 65-70 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: Ryu, Dongsu; Kang, Hyesung;

doi: 10.1007/978-90-481-9999-0_11 , 10.1007/s10509-008-9928-y , 10.48550/arxiv.0806.2179

arXiv: http://arxiv.org/abs/0806.2179

Shock waves in the large-scale structure of the Universe

Abstract

Cosmological shock waves are induced during hierarchical formation of large-scale structure in the universe. Like most astrophysical shocks, they are collisionless, since they form in the tenuous intergalactic medium through electromagnetic viscosities. The gravitational energy released during structure formation is transferred by these shocks to the intergalactic gas as heat, cosmic-rays, turbulence, and magnetic fields. Here we briefly describe the properties and consequences of the shock waves in the context of the large-scale structure of the universe.

Submitted to Astrophysics and Space Science (Special Issue for the proceedings of International Conference on HEDP/HEDLA-08). Pdf with full resolution Figure 1 can be downloaded from http://canopus.cnu.ac.kr/ryu/rk.pdf

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Keywords

Shock waves, Turbulence, Magnetic fields, Astrophysics (astro-ph), Large-scale structure of universe, FOS: Physical sciences, Cosmic-rays, Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
4
Average
Average
Average
Green
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