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· 2019

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astro-ph.CO 1

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2019 1

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ACCEPT 1

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The Core-Cusp Problem Revisited: ULDM vs. CDM

astro-ph.CO · 2019-08-07 · accept · novelty 4.0

Including scatter in the ULDM core-halo mass relation can make ULDM halos less cuspy than NFW up to 10^12 M_sun, but SPARC rotation curves do not discriminate between ULDM and CDM.

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  • The Core-Cusp Problem Revisited: ULDM vs. CDM astro-ph.CO · 2019-08-07 · accept · none · ref 8

    Including scatter in the ULDM core-halo mass relation can make ULDM halos less cuspy than NFW up to 10^12 M_sun, but SPARC rotation curves do not discriminate between ULDM and CDM.