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• W2801909691 endingPage "5452" @default.
• W2801909691 startingPage "5437" @default.
• W2801909691 abstract "Self-interacting dark matter provides a promising alternative for the cold dark matter paradigm to solve potential small-scale galaxy formation problems. Nearly all self-interacting dark matter simulations so far have considered only elastic collisions. Here we present simulations of a galactic halo within a generic inelastic model using a novel numerical implementation in the arepo code to study arbitrary multistate inelastic dark matter scenarios. For this model we find that inelastic self-interactions can: (i) create larger subhalo density cores compared to elastic models for the same cross-section normalization; (ii) lower the abundance of satellites without the need for a power spectrum cut-off; (iii) reduce the total halo mass by about |$10{{ rm per cent}}$|⁠; (iv) inject the energy equivalent of |$mathcal {O}(100)$| million Type II supernovae in galactic haloes through level de-excitation; (v) avoid the gravothermal catastrophe due to removal of particles from halo centres. We conclude that a ∼5 times larger elastic cross-section is required to achieve the same central density reduction as the inelastic model. This implies that well-established constraints on self-interacting cross-sections have to be revised if inelastic collisions are the dominant mode. In this case significantly smaller cross-sections can achieve the same core density reduction thereby increasing the parameter space of allowed models considerably." @default.
• W2801909691 created "2018-05-17" @default.
• W2801909691 creator A5005759342 @default.
• W2801909691 creator A5043394386 @default.
• W2801909691 creator A5047206136 @default.
• W2801909691 creator A5057537951 @default.
• W2801909691 date "2019-02-06" @default.
• W2801909691 modified "2023-10-13" @default.
• W2801909691 title "Evaporating the Milky Way halo and its satellites with inelastic self-interacting dark matter" @default.
• W2801909691 cites W1652376898 @default.
• W2801909691 cites W1711623178 @default.
• W2801909691 cites W1746626963 @default.
• W2801909691 cites W1758810109 @default.
• W2801909691 cites W1845642430 @default.
• W2801909691 cites W1850315173 @default.
• W2801909691 cites W1894488274 @default.
• W2801909691 cites W1908110434 @default.
• W2801909691 cites W1916386386 @default.
• W2801909691 cites W1969043344 @default.
• W2801909691 cites W1969586490 @default.
• W2801909691 cites W1971308472 @default.
• W2801909691 cites W1972284556 @default.
• W2801909691 cites W1996418221 @default.
• W2801909691 cites W1998252144 @default.
• W2801909691 cites W2004181471 @default.
• W2801909691 cites W2004460547 @default.
• W2801909691 cites W2010581546 @default.
• W2801909691 cites W2015754151 @default.
• W2801909691 cites W2019317906 @default.
• W2801909691 cites W2020266225 @default.
• W2801909691 cites W2022211932 @default.
• W2801909691 cites W2037341140 @default.
• W2801909691 cites W2041542911 @default.
• W2801909691 cites W2042561599 @default.
• W2801909691 cites W2046075055 @default.
• W2801909691 cites W2050990527 @default.
• W2801909691 cites W2055640540 @default.
• W2801909691 cites W2059302115 @default.
• W2801909691 cites W2060729394 @default.
• W2801909691 cites W2068725239 @default.
• W2801909691 cites W2070132648 @default.
• W2801909691 cites W2073424199 @default.
• W2801909691 cites W2078981992 @default.
• W2801909691 cites W2080189336 @default.
• W2801909691 cites W2083034637 @default.
• W2801909691 cites W2088813665 @default.
• W2801909691 cites W2088827965 @default.
• W2801909691 cites W2095792194 @default.
• W2801909691 cites W2097774535 @default.
• W2801909691 cites W2098995349 @default.
• W2801909691 cites W2099875176 @default.
• W2801909691 cites W2105056179 @default.
• W2801909691 cites W2110562740 @default.
• W2801909691 cites W2119131940 @default.
• W2801909691 cites W2121091041 @default.
• W2801909691 cites W2122765019 @default.
• W2801909691 cites W2137008363 @default.
• W2801909691 cites W2138029281 @default.
• W2801909691 cites W2139031955 @default.
• W2801909691 cites W2139937287 @default.
• W2801909691 cites W2141709306 @default.
• W2801909691 cites W2143389160 @default.
• W2801909691 cites W2146651836 @default.
• W2801909691 cites W2148581094 @default.
• W2801909691 cites W2150635298 @default.
• W2801909691 cites W2158802981 @default.
• W2801909691 cites W2161153073 @default.
• W2801909691 cites W2161457020 @default.
• W2801909691 cites W2164261957 @default.
• W2801909691 cites W2170918249 @default.
• W2801909691 cites W2181586707 @default.
• W2801909691 cites W2200301779 @default.
• W2801909691 cites W2204815181 @default.
• W2801909691 cites W2220218074 @default.
• W2801909691 cites W2227319875 @default.
• W2801909691 cites W2240695018 @default.
• W2801909691 cites W2313485937 @default.
• W2801909691 cites W2410976049 @default.
• W2801909691 cites W2524790098 @default.
• W2801909691 cites W2565322915 @default.
• W2801909691 cites W2565755431 @default.
• W2801909691 cites W2585531409 @default.
• W2801909691 cites W2594055979 @default.
• W2801909691 cites W2611348040 @default.
• W2801909691 cites W2612559938 @default.
• W2801909691 cites W2626681581 @default.
• W2801909691 cites W2735395126 @default.
• W2801909691 cites W2773362704 @default.
• W2801909691 cites W2774299677 @default.
• W2801909691 cites W2774598525 @default.
• W2801909691 cites W2775328404 @default.
• W2801909691 cites W2786978312 @default.
• W2801909691 cites W2951306382 @default.
• W2801909691 cites W2953228579 @default.
• W2801909691 cites W2963602939 @default.
• W2801909691 cites W3005079263 @default.
• W2801909691 cites W3098976132 @default.
• W2801909691 cites W3099996199 @default.

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