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  • Naturally we have to consider universes outside the family of Robertson-Walker spaces, ie globally non-isotropic/non-homogeneous geometries.

    Against Bounces

  • As mentioned in the previous lecture, the above theory can be carried over fairly easily to non-isotropic settings, such as that given by the, which is holomorphically equivalent to the Siegel upper half-space

    What's new

  • The second term becomes for a non-isotropic polarizibility in three different, but fully equivalent, notations,

    Citizendium, the Citizens' Compendium - Recent changes [en]

  • On the other hand, Einstein encouraged Lemaître to look into the possibility of non-isotropic expansion models, so it’s clear he was not dismissive of the concept altogether.

    Egnor and ignorance - The Panda's Thumb

  • "Gives us more volume, better turbulence, but there's also a non-isotropic pressure drop, which cuts into our efficiency ....

    Gravity's Rainbow


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