WebJan 27, 2024 · The team used the assumption that the only force acting on Dark Matter is gravity, and calculated that Dark Matter particles must have a mass between 10-3 eV and 10 7 eV. WebWe revisit constraints on decaying very heavy dark matter (VHDM) using the latest ultrahigh-energy cosmic-ray (UHECR; E ≳ 10 18 eV) data and ultrahigh-energy (UHE) γ-ray flux upper limits, measured by the Pierre Auger Observatory.We present updated limits on the VHDM lifetime (τ χ) for masses up to ∼ 10 15 ~GeV, considering decay into quarks, leptons, and …
WMAP- Content of the Universe - NASA
WebWelcome to Matter, your gateway to a virtual world that exists alongside the physical. Everything you need to start building new worlds. Connecting people, real locations & virtual content. ... The developer, Hot Dark Matter Ltd, indicated that the app’s privacy practices may include handling of data as described below. For more ... WebOct 15, 2024 · The main reason that dark matter has been favored over MOND is that dark matter is consistent with a much larger range of astrophysical observations. For example, dark matter can explain galaxies’ bending of light from distant sources (gravitational lensing), whereas MOND in its initial form could not. newtermquery
Cosmic Optical Background Excess, Dark Matter, and Line …
WebNov 29, 2024 · Dark Matter Could Cause Excess Optical Background Published 29 November 2024 Axions that decay into photons could account for visible light that exceeds what’s expected to come from all known galaxies. See more in Physics Authors & Affiliations José Luis Bernal, Gabriela Sato-Polito, and Marc Kamionkowski WebMar 8, 2024 · Dark matter that is really that simple behaves in a way that is possible to describe analytically (rather than just with N-body simulation models) and it is pretty strongly disfavored by observations because inferred dark matter halos are the wrong shape and because dark matter distributions are too tightly correlated with distributions of ... WebThe dark matter scenario for the Galactic center γ-ray excess is in tension with the FAST observation for reasonable choices of astrophysical factors {}. { But considering the large uncertainty on astrophysical parameters, such as the magnetic field, the diffusion coefficient, and the diffusion radius, and on DM halo parameters, the dark ... midview youth baseball