Closed Universe? Local H0 Measurements & Relativistic Corrections

In summary, the paper discusses the potential miscalculation of cosmological distance due to the accumulation of lensing effects and its impact on the tension between local and cosmological measurements of the Hubble constant. It also suggests that this could mean the universe is closed. The conversation further explores the impact of density perturbations on the CMB temperature and shape, and how photons experience a net blue-shift due to the shallowing of gravitational wells during expansion. The expansion of the universe makes the wells shallower, resulting in a wider and steeper well on the way in and a narrower and shallower well on the way out. This effect can accumulate as photons pass through gravitational lenses.
  • #1
Chronos
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In this paper; http://arxiv.org/abs/1405.7860, What is the distance to the CMB? How relativistic corrections remove the tension with local H0 measurements, it is suggested cosmological distance may be miscalculated due to failure to take into account systematic accumulation of lensing effects. The authors go on to suggest this may explain the tension between local and cosmological measurements of the Hubble constant and could mean the universe may, in fact, be closed.
 
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  • #2
Interesting. Thanks, Chronos.
 
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Thanks Chronos. I had wondered myself what percentage of the CMB photons make it to Earth without interacting with matter along the way and how much this distorts the CMB temperature and black body shape?
 
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I view this as consistent with Rees & Sciama [http://adsabs.harvard.edu/full/1968ApJ...153L...1R], who noted that large density perturbations interposed between the CMB surface and an observer can have an effect if the fluctuations change while photons traverse them. They experience more blue-shift infalling than when climbing out because expansion makes the wells shallower, giving rise to a net blue-shift of CMB photons. A similar effect can accumulate as photons pass through interposing gravitational lenses.
 
  • #5
Chronos said:
... expansion makes the wells shallower ...

Can you elabort on how expansion makes a well shallower? (Wider I get, and steeper on the way in than on the way out, I understand.)

Thanks in advance.
 

Related to Closed Universe? Local H0 Measurements & Relativistic Corrections

1. What is a closed universe?

A closed universe is a cosmological model in which the universe is finite and has a finite volume. This means that the universe has a boundary and everything within that boundary is contained within the universe.

2. How is the H0 measurement used in cosmology?

The H0 measurement, also known as the Hubble constant, is used in cosmology to determine the rate at which the universe is expanding. It is used to calculate the age of the universe and to understand the overall structure and evolution of the universe.

3. What are relativistic corrections in cosmology?

Relativistic corrections are adjustments made to cosmological equations to account for the effects of relativity, specifically the theory of general relativity. These corrections take into account the curvature of spacetime and the influence of gravity on the expansion of the universe.

4. How are local H0 measurements obtained?

Local H0 measurements are obtained by observing the motion of objects within the nearby universe and using the Hubble law to calculate their distances. This method is known as the "cosmic distance ladder" and involves using increasingly distant objects as reference points to estimate the Hubble constant.

5. Why are relativistic corrections important in closed universe models?

In closed universe models, relativistic corrections are important because they take into account the effects of gravity, which can significantly impact the expansion rate and overall dynamics of the universe. Without these corrections, the model would not accurately reflect the observed behavior of the universe.

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