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We devise a method to constrain self-interacting dark matter (SIDM) from observations of quadruply-imaged quasars, and apply it to five self-interaction potentials with a long-range dark force.
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H. Sugai, A. Kawai, A. Shimono, T. Hattori, G. Kosugi, N. Kashikawa, K. T. Inoue, and M. Chiba, Integral Field Spectroscopy of the Quadruply Lensed Quasar 1RXS J1131-1231: New Light on Lens Substructures, ApJ 660
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M. R. Buckley and P. J. Fox, Dark matter self-interactions and light force carriers, PhysRevD 81
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C. Loken, D. Gruner, L. Groer, R. Peltier, N. Bunn, M. Craig, T. Henriques, J. Dempsey, C.-H. Yu, J. Chen, L. J. Dursi, J. Chong, S. Northrup, J. Pinto, N. Knecht, and R. Van Zon, SciNet: Lessons Learned from Building a Power-efficient Top-20 System and Data Centre, in Journal of Physics Conference Series , Journal of Physics Conference Series, Vol. 256 (2010) p. 012026
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2019
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B. Diemer and M. Joyce, An Accurate Physical Model for Halo Concentrations, ApJ 871
2019
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N. Banik and J. Bovy, On N-body simulations of globular cluster streams, MNRAS 504
2021
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A. Nierenberg, V. N. Bennert, A. Benson, S. Birrer, S. G. Djorgovski, X. Du, C. Fassnacht, D. Gilman, S. F. Hoenig, A. Kusenko, M. A. Malkan, V. Motta, L. A. Moustakas, D. Sluse, D. K. Stern, and T. L. Treu, A definitive test of the dark matter paradigm on small scales, JWST Proposal. Cycle 1, ID. #2046 (2021)
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