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  2. Shadowdark - Wikipedia

    en.wikipedia.org/wiki/Shadowdark

    Shadowdark is a dark fantasy tabletop role-playing game created by Kelsey Dionne and published in 2023 after raising 1.4 million dollars on kickstarter. As part of the Old School Renaissance, it focuses primarily on dungeon crawling.

  3. Bolshoi cosmological simulation - Wikipedia

    en.wikipedia.org/wiki/Bolshoi_Cosmological...

    A successful large-scale simulation of the evolution of galaxies, with results consistent with what is actually seen by astronomers in the night sky, provides evidence that the theoretical underpinnings of the models employed, i.e., the supercomputer implementations ΛCDM, are sound bases for understanding galactic dynamics and the history of the universe, and opens avenues to further research.

  4. Mixed dark matter - Wikipedia

    en.wikipedia.org/wiki/Mixed_dark_matter

    Mixed dark matter (MDM) is a dark matter (DM) model proposed during the late 1990s. [1]Mixed dark matter is also called hot + cold dark matter. The most abundant form of dark matter is cold dark matter, almost one fourth of the energy contents of the Universe.

  5. Dungeon Masters Screen - Wikipedia

    en.wikipedia.org/wiki/Dungeon_Masters_Screen

    A Dungeon Master Screen was published in 2000, developed and assembled by Dale Donovan and Kim Mohan, and featuring cover art by Jeff Easley.A Dungeon Master Screen was also published for the Forgotten Realms campaign, which included a booklet titled "Encounters in Faerûn" designed by Skip Williams and Duane Maxwell, and featuring cover art by Justin Sweet.

  6. Lambda-CDM model - Wikipedia

    en.wikipedia.org/wiki/Lambda-CDM_model

    For the Lambda-CDM model with a positive cosmological constant (as observed), the universe is predicted to expand forever regardless of whether the total density is slightly above or below the critical density; though other outcomes are possible in extended models where the dark energy is not constant but actually time-dependent. [citation needed]

  7. images.huffingtonpost.com

    images.huffingtonpost.com/2012-03-30-Parker...

    %PDF-1.5 %âãÏÓ 191 0 obj > endobj xref 191 25 0000000016 00000 n 0000001437 00000 n 0000001560 00000 n 0000001882 00000 n 0000002862 00000 n 0000003042 00000 n 0000003184 00000 n 0000003359 00000 n 0000003594 00000 n 0000004073 00000 n 0000004242 00000 n 0000081823 00000 n 0000082060 00000 n 0000082215 00000 n 0000107550 00000 n 0000107790 00000 n 0000108080 00000 n 0000142116 00000 n ...

  8. Navarro–Frenk–White profile - Wikipedia

    en.wikipedia.org/wiki/Navarro–Frenk–White...

    The Navarro–Frenk–White (NFW) profile is a spatial mass distribution of dark matter fitted to dark matter halos identified in N-body simulations by Julio Navarro, Carlos Frenk and Simon White. [ 1 ] [ 2 ] The NFW profile is one of the most commonly used model profiles for dark matter halos. [ 3 ]

  9. Scalar field dark matter - Wikipedia

    en.wikipedia.org/wiki/Scalar_field_dark_matter

    The universe may be accelerating, fueled perhaps by a cosmological constant or some other field possessing long range 'repulsive' effects. A model must predict the correct form for the large scale clustering spectrum, [3] account for cosmic microwave background anisotropies on large and intermediate angular scales, and provide agreement with the luminosity distance relation obtained from ...

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