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What sets the splashback radius of dark matter haloes: accretion history or other properties?

What sets the splashback radius of dark matter haloes: accretion history or other properties?

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2729289165

What sets the splashback radius of dark matter haloes: accretion history or other properties?

About this item

Full title

What sets the splashback radius of dark matter haloes: accretion history or other properties?

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2022-10

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The density profiles of dark matter haloes contain rich information about their growth history and physical properties. One particularly interesting region is the splashback radius, \(R_{\rm sp}\), which marks the transition between particles orbiting in the halo and particles undergoing first infall. While the dependence of \(R_{\rm sp}\) on the r...

Alternative Titles

Full title

What sets the splashback radius of dark matter haloes: accretion history or other properties?

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2729289165

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2729289165

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2210.14262

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