Results 171 to 180 of about 117,029 (345)
The globular cluster-dark matter halo connection. [PDF]
Mon Not R Astron Soc, 2017 Boylan-Kolchin M.
europepmc +1 more source
Exploring the halo occupation of AGN using dark-matter cosmological simulations
, 2018 A. Georgakakis +5 more
openalex +1 more source
The Shape of Dark Matter Halos
, 1999 Techniques for inferring the radial and geometric form of dark matter halos and the results they have produced to date are reviewed. Dark halos appear to extend to at least ~50 kpc with total enclosed masses that rise linearly with radius R. Whether this behavior can be extrapolated to distances as large as 200 kpc and beyond is controversial; results ...
openaire +3 more sources
Dark energy and dark matter in galaxy halos
Physics Letters B, 2006 7 pages, 1 figure, references added and discussion ...
openaire +3 more sources
Unusual Swelling Behavior of Hydrogels Modified with Spiropyran as Appendage or Crosslinker
Advanced Functional Materials, EarlyView.Not so innocent after all—spiropyran crosslinkers in methylenebisacrylamide‐crosslinked poly(acrylamide‐co‐acrylic acid) hydrogels increase crosslinking density, but also, counterintuitively, increase swelling. Charge complexation, cooperative chemo‐mechanical effects, and aggregation may explain these observations.
Michael M. Lerch +7 more
wiley +1 more source
European Physical Journal C: Particles and FieldsIn this work, we present an exact solution describing a static, spherically symmetric black hole immersed in a cored Navarro–Frenk–White (NFW) dark matter halo.
David Senjaya
doaj +1 more source
First law and black hole thermodynamics of black hole in Dehnen (1,4,12) dark matter environment
Nuclear Physics BIn this work, we present a comprehensive thermodynamic analysis of a static, spherically symmetric black hole embedded in a Dehnen (1,4,12) dark matter halo.
David Senjaya
doaj +1 more source
Diverse dark matter haloes in two-field fuzzy dark matter
Physical Review DFuzzy dark matter (FDM) is a compelling candidate for dark matter, offering a natural explanation for the structure of diffuse low-mass haloes. However, the canonical FDM model with a mass of $10^{-22}~{\rm eV}$ encounters challenges in reproducing the observed diversity of dwarf galaxies, except for possibly scenarios where strong galactic feedback is
Hoang Nhan Luu +10 more
openaire +2 more sources