Tidal Suppression of Fuzzy Dark Matter Heating in Milky Way Satellite Galaxies
Many previous studies have imposed stringent constraints on the particle mass of fuzzy dark matter (FDM) by analyzing observations of Galactic satellite galaxies, which show no significant evidence of the heating effect predicted by FDM.
Yu-Ming Yang +3 more
doaj +1 more source
The detailed structure and the onset of galaxy formation in low-mass gaseous dark matter haloes [PDF]
Alejandro Benítez-Llambay +1 more
openalex +1 more source
For their ability to enhance performance, immune response, and robustness to environmental stressors in both fish and crustaceans, phytogenic compounds are receiving increasing attention from the aquaculture industry as alternatives to traditional feed additives.
Fabrizio Caruso +8 more
wiley +1 more source
Analysis of Galaxies at the Extremes: Failed Galaxy Progenitors in the MAGNETICUM Simulations
There is increasing observational evidence for a “failed galaxy” formation pathway for ultra-diffuse galaxies (UDGs) at low redshift however they currently lack simulated counterparts.
Jonah S. Gannon +7 more
doaj +1 more source
Heavy Metal Contamination in Chocolates and Candies: Sources, Health Risks, and Analytical Insights
The presence of heavy metals in chocolates and candies poses growing public health concerns, particularly for children who are frequent consumers. This review consolidates evidence on the occurrence, sources, toxicological impacts, and analytical monitoring of metals, including Pb, Cd, Hg, As, Cr, Ni, and Al, in confectionery products.
Mahmood Ahmed +12 more
wiley +1 more source
How to empirically model star formation in dark matter haloes – I. Inferences about central galaxies from numerical simulations [PDF]
Yangyao Chen +3 more
openalex +1 more source
Hydro-Gravitational Dynamics of Planets and Dark Energy
Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the 0.3 Myr ...
Carl H. Gibson, R.E, Schild
doaj
Halo Asymmetry in the Modeling of Galaxy Clustering
Conventional studies of galaxy clustering within the framework of halo models typically assume that the density profile of all dark matter halos can be approximated by the Navarro–Frenk–White (NFW) spherically symmetric profile.
Anna Durkalec +2 more
doaj +1 more source
DARK MATTER HALOS AND EVOLUTION OF BARS IN DISK GALAXIES: COLLISIONLESS MODELS REVISITED [PDF]
Jorge Villa-Vargas +2 more
openalex +1 more source
Massive Dark Matter Halos and Evolution of Early‐Type Galaxies toz≈ 1 [PDF]
Tommaso Treu, L. V. E. Koopmans
openalex +1 more source

