Do the Universe's Greatest Voids Challenge Hubble's Law?

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    Hubble's law Law
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Discussion Overview

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.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that Hubble's law would apply more strongly in voids due to the absence of strong gravitational wells, which dampen peculiar velocities over time.
  • One participant suggests that in an expanding universe, peculiar velocities tend to diminish, leading to a closer adherence to Hubble's law as expansion continues.
  • Another participant questions how the Hubble effect interacts with matter undergoing "cosmological constant" acceleration, pondering if peculiar velocities would still dampen without gravitational interactions.
  • A response indicates that the presence of a cosmological constant does not prevent the damping of peculiar velocities, although it may influence the rate at which this occurs.

Areas of Agreement / Disagreement

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.

Contextual Notes

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.

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?
 
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Loren Booda said:
Would the greatest voids in the universe support Hubble's law to a substantially lesser radius than the neighborhoods of galaxies?
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:

If you take an expanding universe that includes lots of stuff moving at various peculiar velocities, and ignore gravitational interaction, then over time those peculiar velocities tend to get damped by the expansion: as the universe expands, it more and more closely approaches Hubble's law.

Why is this? Well, it's easiest to think of it in terms of one-dimensional expansion. If we take this case, and consider an object receding at a bit faster than the expansion rate for its distance, then over time it will catch up with objects further away that are moving faster, until it finds itself at just the right location, just by coasting, as stuff that's moving as fast as it is. If it's moving a bit slower, then stuff closer-in will catch up with it, and it will eventually find itself again at the right distance to match the Hubble flow.

Gravitational interactions counteract this, of course, as when things fall into a gravitational well, they accelerate, and their orbits around gravitational wells are obviously non-Hubble motions. So in a void where there are fewer deep gravitational wells, I would tend to expect that the damping induced by the Hubble flow would indeed result in a Hubble law that holds more strongly. I can't say precisely what the magnitude of the effect would be without some calculations, of course, but it seems likely to be sound.
 
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)?
 
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)?
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.

Now, the existence of a cosmological constant affects the details, of course, and therefore affects how quickly it happens. But it doesn't affect the fact that it does happen.
 

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