Major mergers between dark matter haloes – II. Profile and concentration changes-Reference-Cited by-同舟云学术

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Major mergers between dark matter haloes – II. Profile and concentration changes

Published:2019-05-11 Issue:1 Volume:487 Page:1008-1024
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Drakos Nicole E¹²^ORCID,Taylor James E¹²^ORCID,Berrouet Anael²,Robotham Aaron S G³^ORCID,Power Chris³^ORCID

Affiliation:

1. Waterloo Centre for Astrophysics, University of Waterloo, 200 University Avenue West, Waterloo, ON N2L 3G1, Canada

2. Department of Physics and Astronomy, University of Waterloo, 200 University Avenue West, Waterloo, ON N2L 3G1, Canada

3. ICRAR, University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia

Funder

Natural Sciences and Engineering Research Council of Canada

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1307/28601508/stz1307.pdf

Reference42 articles.

1. Dark Matter Properties and Halo Central Densities

2. Major mergers of galaxy haloes: cuspy or cored inner density profile?

3. Profiles of dark haloes: evolution, scatter and environment

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1. Toward more realistic mass functions for ultradense dark matter halos;Physics of the Dark Universe;2024-12

2. A differentiable model of the evolution of dark matter halo concentration;Monthly Notices of the Royal Astronomical Society;2023-09-20

3. How an era of kination impacts substructure and the dark matter annihilation rate;Physical Review D;2023-07-27

4. Lensing constraints on ultradense dark matter halos;Physical Review D;2023-04-06

5. Ultradense dark matter haloes accompany primordial black holes;Monthly Notices of the Royal Astronomical Society;2023-02-01

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