Degeneracies between self-interacting dark matter and supernova feedback as cusp-core transformation mechanisms
Abstract We present a suite of 16 high-resolution hydrodynamic simulations of an isolated dwarf galaxy (gaseous and stellar disk plus a stellar bulge) within an initially cuspy dark matter (DM) halo, including self-interactions between the DM particles (SIDM); as well as stochastic star formation a...
| প্রধান লেখক: | , , , , , |
|---|---|
| বিন্যাস: | প্রবন্ধ |
| ভাষা: | English |
| প্রকাশিত: |
Oxford University Press (OUP)
2022
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| অনলাইন ব্যবহার করুন: | https://hdl.handle.net/1721.1/142385 |