Modeling the core-halo mass relation in fuzzy dark matter halos-Reference-Cited by-同舟云学术

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Modeling the core-halo mass relation in fuzzy dark matter halos

Published:2024-07-15 Issue:2 Volume:110 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Kawai Hiroki¹²³^ORCID,Kamada Ayuki⁴⁵¹⁶^ORCID,Kamada Kohei⁷⁸¹^ORCID,Yoshida Naoki¹⁵¹¹^ORCID

Affiliation:

1. The University of Tokyo

2. Chiba University

3. INAF—Osservatorio Astronomico di Bologna

4. University of Warsaw

5. Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI)

6. Institute for Basic Science (IBS)

7. University of Chinese Academy of Sciences

8. International Centre for Theoretical Physics Asia-Pacific (ICTP-AP)

Funder

Japan Society for the Promotion of Science

Istituto Nazionale di Astrofisica

Narodowe Centrum Nauki

National Natural Science Foundation of China

Norwegian Financial Mechanism

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.110.023519/fulltext

Reference45 articles.

1. The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey

2. Matter power spectrum: from Ly α forest to CMB scales

3. Small-Scale Challenges to the ΛCDM Paradigm

4. Evidence against dissipation-less dark matter from observations of galaxy haloes

5. Dark Matter Substructure within Galactic Halos

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