- Abstract:
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We present the first high-resolution N-body simulations of the fragmentation of dark matter filaments. Such fragmentation occurs in top-down scenarios of structure formation, when the dark matter is warm instead of cold. In a previous paper, we showed that warm dark matter (WDM) differs from the standard cold dark matter (CDM) mainly in the formation history and large-scale distribution of low-mass haloes, which form later and tend to be more clustered in WDM than in CDM universe...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Version of record
- Files:
-
-
(pdf, 159.7KB)
-
- Publisher copy:
- 10.1046/j.1365-2966.2003.07044.x
-
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- Publisher:
- Oxford University Press (OUP) Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 345
- Issue:
- 4
- Pages:
- 1285–1290
- Publication date:
- 2003-11-11
- Acceptance date:
- 2003-07-24
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
- URN:
-
uuid:5f77c963-12e2-4a9d-8080-cd1b7c559418
- Source identifiers:
-
205763
- Local pid:
- pubs:205763
- Copyright holder:
- RAS
- Copyright date:
- 2003
- Notes:
-
This is the version of record of the article. The final version is
available online from Oxford University Press (OUP) at: https://doi.org/10.1046/j.1365-2966.2003.07044.x
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2003 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Journal article
Top-down fragmentation of a warm dark matter filament
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