Acceleration proportional to what?

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SUMMARY

The discussion centers on the relationship between acceleration and distance in the context of cosmic expansion, specifically addressing Hubble's law (V=HD). It establishes that while velocity is proportional to distance, acceleration is a time-dependent function that has shifted from negative to positive since the early universe. The scale factor is emphasized as a critical concept for understanding cosmic expansion, with implications for models of dark energy, including the Quintessence model and the cosmological constant. Accurate measurements of galaxy acceleration are necessary to validate these models.

PREREQUISITES
  • Understanding of Hubble's law and its implications for cosmic velocity.
  • Familiarity with the concept of the scale factor in cosmology.
  • Knowledge of dark energy models, particularly the cosmological constant and Quintessence.
  • Basic grasp of redshift calculations and their significance in observational cosmology.
NEXT STEPS
  • Research the mathematical formulation of the scale factor in cosmological models.
  • Study the implications of the Quintessence model of dark energy on cosmic acceleration.
  • Learn about the supernova cosmology project and its contributions to measuring cosmic expansion.
  • Investigate the methods for calculating redshift and its relation to galaxy distance and brightness.
USEFUL FOR

Astronomers, cosmologists, and astrophysics students interested in the dynamics of cosmic expansion and the nature of dark energy will benefit from this discussion.

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acceleration proportional to what??

Hello,

We know that according to Hubble's law V=HD that velocity of distant galaxies are proportional to distance from Earth but what about acceleration?? Is acceleration of space with distant galaxies proportional to distance from Earth and one another or different model works for it??
 
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Acceleration of space leads to deviations from Hubble's law.
The acceleration is a function of time. In the early universe, it was negative (so expansion slowed), now it is positive (so expansion is accelerating). Instead of the Hubble "constant" (which is not constant on cosmological timescales), it is better to interpret the evolution of the universe in terms of the scale factor. Without acceleration, the scale factor would increase with a constant derivative.

If you know the scale factor at the point where some light was emitted and the scale factor now (defined to be 1), you can calculate the redshift.
Example graph for the scale factor with various scenarios (red=accelerating) from NASA.
You can also calculate how bright those objects should appear to us, if you can estimate their true brightness. By comparing those observations with the model, you can measure the accelerated expansion. And this has been done with many measurements (from the supernova cosmology project)
 
But what about Quintessence model of dark energy?? If we measure acceleration of galaxies and if it is different for different galaxies which are currently at different distance from Earth than quintessence model is correct because it predict different dark energy density over place and over time otherwise cosmological constant model is true.
 
Even the cosmological constant model leads to a time-dependence of the acceleration, as the decreasing matter/radiation density leads to a acceleration of the acceleration (3rd derivative of the scale factor).
If the time-dependence deviates from this prediction, then a time-dependent cosmological constant might be an explanation. But that will need much more precise observations.
 

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