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

Abstract

Not provided.

Authors:
; ; ;
Publication Date:
Research Org.:
Univ. of California, Riverside, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1536554
DOE Contract Number:  
SC0008541
Resource Type:
Journal Article
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 119; Journal Issue: 11; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
Physics

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. https://doi.org/10.1103/physrevlett.119.111102
Kamada, Ayuki, Kaplinghat, Manoj, Pace, Andrew B., and Yu, Hai-Bo. Fri . "Self-Interacting Dark Matter Can Explain Diverse Galactic Rotation Curves". United States. https://doi.org/10.1103/physrevlett.119.111102.
@article{osti_1536554,
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 = {Not provided.},
doi = {10.1103/physrevlett.119.111102},
url = {https://www.osti.gov/biblio/1536554}, journal = {Physical Review Letters},
issn = {0031-9007},
number = 11,
volume = 119,
place = {United States},
year = {2017},
month = {9}
}

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