Loren Booda
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Would the greatest voids in the universe support Hubble's law to a substantially lesser radius than the neighborhoods of galaxies?
The discussion revolves around the applicability of Hubble's law in the context of the universe's greatest voids, particularly whether Hubble's law holds at smaller distances in these regions compared to areas with dense galaxy neighborhoods. Participants explore the implications of gravitational interactions and cosmological constants on the behavior of peculiar velocities in an expanding universe.
Participants express differing views on the influence of gravitational interactions and cosmological constants on Hubble's law, indicating that multiple competing perspectives remain without a consensus on the specifics of these interactions.
Participants acknowledge that the details of how gravitational interactions and cosmological constants affect the application of Hubble's law are complex and not fully resolved in the discussion.
Well, yes, I would tend to think that Hubble's law would apply at smaller distances in the absence of strong gravitational wells. My reasoning is thus:Loren Booda said:Would the greatest voids in the universe support Hubble's law to a substantially lesser radius than the neighborhoods of galaxies?
It doesn't really matter how the universe expands, as long as it expands, and the peculiar velocities tend to damp themselves out. So yes, it works in the presence of a cosmological constant. Or without one.Loren Booda said:Chalnoth,
What would the Hubble effect have on damping matter which undergoes "cosmological constant" acceleration? Without gravitational interaction, would large z bodies still tend towards damping's "self-fulfilling prophesy" of eradicating peculiar velocities (or perhaps peculiar accelerations)?