About Hubble Radius (Radius of the Hubble sphere)

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SUMMARY

The Hubble Radius, defined as the distance from a fixed point to an object moving with cosmological expansion at the speed of light, is mathematically represented as R=c(a/da), where c is the speed of light and a(t) is the scale factor. Observers at different origins perceive distinct Hubble spheres due to the finite speed of light, leading to variations in the observed size of the Hubble Bubble. The Hubble sphere is equivalent to the particle horizon since the dust era, with a radius of approximately 13,700 million light-years (Mly), while the particle horizon is about 45,000 Mly. This discussion clarifies the theoretical nature of the Hubble Bubble and its implications for distance measurements in cosmology.

PREREQUISITES
  • Understanding of cosmological expansion and its effects on distance measurements
  • Familiarity with the concept of the scale factor a(t) in cosmology
  • Knowledge of the speed of light and its role in the universe
  • Basic grasp of the particle horizon and Hubble time τ=1/H(t)
NEXT STEPS
  • Research the mathematical derivation of the Hubble Radius and its implications in cosmology
  • Explore the relationship between the Hubble sphere and the particle horizon in greater detail
  • Study the effects of cosmological expansion on light travel time and observational astronomy
  • Investigate the concept of the Hubble Bubble and its significance in modern cosmological theories
USEFUL FOR

Astronomers, cosmologists, and physics students interested in understanding the implications of the Hubble Radius and its relevance to the structure of the universe.

Ricky2357
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I found the following definition for the Hubble Radius:

The radius of the Hubble sphere (Hubble radius) is defined to be the distance from a fixed point O (center of coordinate system) of an object moving with the cosmological expansion at the speed of light (with respect to O).

Mathematically, R=c(a/da) , c=speed of light , a=a(t) is the scale factor ,t is time.

How's this definition valid since the Hubble radius as defined depends on the moving object?
 
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It means that each observer (each origin O you choose to define) has a different 'Hubble sphere'.
 
True, but, they are time limited. The Hubble bubble looks smaller to distant observers [speed of light thing].
 
I'm not sure what you mean Chronos, the 'Hubble Bubble' doesn't 'look' like anything since it's just a theoretical construct, a useful term in distance measures, rather than a physical structure. I'm not sure what you are saying looks different to distant observers (or who they are distant from?) ?
 
I found out that the Hubble sphere can also be defined as the sphere of center 0 (observer) and radius the distance that light can travel within the characteristic expansion time, that is the Hubble time : τ=1/H(t).
So R=c*τ. From the moment we entered the dust era, the Hubble sphere is the same as the particle horizon.
 
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But what is your question?
 
Nothing, I believe it is clear now. Thanks for the help!
 
Looks like everyone skipped out Wallace! My intent was merely to point out the Hubble Bubble looks the same to all observers. It looks 'smaller' to distant observers because the universe was younger when 'they' sent us the picture we just received.
 
Ricky2357 said:
From the moment we entered the dust era, the Hubble sphere is the same as the particle horizon.
The Hubble sphere is much closer than the particle horizon. The Hubble sphere has a radius of about 13,700 Mly and the particle horizon is located at about 45,000 Mly. Both distances measured on the hypersurface of current time.
 

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