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Title: Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves

Authors:
; ; ;
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1389900
Grant/Contract Number:
SC0008541
Resource Type:
Journal Article: Publisher's Accepted Manuscript
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 119; Journal Issue: 11; Related Information: CHORUS Timestamp: 2017-09-13 10:34:51; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English

Citation Formats

Kamada, Ayuki, Kaplinghat, Manoj, Pace, Andrew B., and Yu, Hai-Bo. Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves. United States: N. p., 2017. Web. doi:10.1103/PhysRevLett.119.111102.
Kamada, Ayuki, Kaplinghat, Manoj, Pace, Andrew B., & Yu, Hai-Bo. Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves. United States. doi:10.1103/PhysRevLett.119.111102.
Kamada, Ayuki, Kaplinghat, Manoj, Pace, Andrew B., and Yu, Hai-Bo. 2017. "Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves". United States. doi:10.1103/PhysRevLett.119.111102.
@article{osti_1389900,
title = {Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves},
author = {Kamada, Ayuki and Kaplinghat, Manoj and Pace, Andrew B. and Yu, Hai-Bo},
abstractNote = {},
doi = {10.1103/PhysRevLett.119.111102},
journal = {Physical Review Letters},
number = 11,
volume = 119,
place = {United States},
year = 2017,
month = 9
}

Journal Article:
Free Publicly Available Full Text
This content will become publicly available on September 13, 2018
Publisher's Accepted Manuscript

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