Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Bodo Schwabe"'
Publikováno v:
Zaguán. Repositorio Digital de la Universidad de Zaragoza
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The Universe may pass through an effectively matter-dominated epoch between inflation and Big Bang Nucleosynthesis during which gravitationally bound structures can form on subhorizon scales. In particular, the inflaton field can collapse into inflat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d27ca4ef73df3da3f10937c330f13335
http://zaguan.unizar.es/record/112519
http://zaguan.unizar.es/record/112519
Autor:
Bodo Schwabe, Jens C. Niemeyer
Fuzzy dark matter (FDM) made of ultra-light bosonic particles is a viable alternative to cold dark matter (CDM) with clearly distinguishable small-scale features in collapsed structures. On large scales, it behaves gravitationally like CDM deviating
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27b6a6f78514511a369db372870c88c0
http://arxiv.org/abs/2110.09145
http://arxiv.org/abs/2110.09145
Publikováno v:
Physical Review D. 102
The distinctive effects of fuzzy dark matter are most visible at nonlinear galactic scales. We present the first simulations of mixed fuzzy and cold dark matter, obtained with an extended version of the nyx code. Fuzzy (or ultralight or axionlike) da
Publikováno v:
Physical Review D. 98
We simulate the formation and evolution of ultralight bosonic dark matter halos from cosmological initial conditions. Using zoom-in techniques we are able to resolve the detailed interior structure of the halos. We observe the formation of solitonic
We study tidal stripping of fuzzy dark matter (FDM) subhalo cores using simulations of the Schr\"{o}dinger-Poisson equations and analyze the dynamics of tidal disruption, highlighting the differences with standard cold dark matter. Mass loss outside
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b02f05c5df91a765cfa3bfb48e802ea
Using three-dimensional simulations, we study the dynamics and final structure of merging solitonic cores predicted to form in ultra-light axion dark matter halos. The classical, Newtonian equations of motion of a self-gravitating scalar field are de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efb7bcc695a3ae914d2e7d4ebfe270e6
http://arxiv.org/abs/1606.05151
http://arxiv.org/abs/1606.05151
In the context of structure formation with ultralight axion dark matter, we offer an alternative explanation for the mass relation of solitonic cores and their host halos observed in numerical simulations. Our argument is based entirely on the mass g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a04f9c0a90cb1bcc099caf7d50e033b7
Autor:
Bodo Schwabe, Riccardo Catena
Publikováno v:
Journal of Cosmology and Astroparticle Physics
In the effective theory of isoscalar and isovector dark matter-nucleon interactions mediated by a heavy spin-1 or spin-0 particle, 8 isotope-dependent nuclear response functions can be generated in the dark matter scattering by nuclei. We compute the