WIMP matter power spectra and small scale power generation
Dark Matter (DM) is generally assumed to be massive, cold and collisionless from the structure formation point of view. A more correct statement however is that DM indeed experiences collisional damping, but on a scale which is supposed to be too small to be relevant for structure formation. The aim...
المؤلفون الرئيسيون: | Boehm, C, Mathis, H, Devriendt, J, Silk, J |
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التنسيق: | Internet publication |
اللغة: | English |
منشور في: |
2003
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مواد مشابهة
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Non-linear evolution of suppressed dark matter primordial power spectra
حسب: Boehm, C, وآخرون
منشور في: (2005) -
Resummed photon spectra for WIMP annihilation
حسب: Baumgart, Matthew, وآخرون
منشور في: (2018) -
Planck-scale effects on WIMP dark matter
حسب: Sofiane M Boucenna, وآخرون
منشور في: (2014-01-01) -
Thermodynamic evolution of secluded vector dark matter: conventional WIMPs and nonconventional WIMPs
حسب: Kwei-Chou Yang
منشور في: (2019-11-01) -
Closing the window on WIMP Dark Matter
حسب: Salvatore Bottaro, وآخرون
منشور في: (2022-01-01)