Part of the Hubble discrepancy can be explained by local underdensity

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Discussion Overview

The discussion centers on a paper suggesting that a local underdensity in the universe may account for part of the discrepancy in the Hubble constant measurements. Participants explore the implications of this underdensity on local measurements compared to cosmic microwave background (CMB) measurements, with a focus on the potential for systematic errors and the overall impact on cosmological parameters.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants highlight that the paper claims a local underdensity could explain up to 5.5% of the Hubble constant discrepancy, suggesting that adjusting local measurements by this amount brings them within experimental errors.
  • Others question whether this 5.5% adjustment should already be considered part of the uncertainties in measurements, noting that it applies primarily to local measurements and not to more distant supernova observations.
  • A participant argues that while the underdensity could shift cosmological parameters, including the Hubble constant, it is difficult to account for such systematic errors in practice.
  • Some participants express skepticism about the sufficiency of the 5.5% adjustment, referencing a larger discrepancy of 9.6% that exceeds combined errors and suggesting that additional systematic effects may need to be considered.
  • There is a mention of a conference where Adam Riess stated that we do not live in a "giant" local void, which may challenge the assumptions made in the paper.
  • One participant reiterates that if the local underdensity accounts for 5.5%, the remaining discrepancy could be attributed to statistical errors, suggesting that the overall situation remains complex and unresolved.

Areas of Agreement / Disagreement

Participants express differing views on the significance of the 5.5% adjustment and its implications for the Hubble constant discrepancy. There is no consensus on whether this adjustment sufficiently accounts for the observed discrepancies or if additional factors must be considered.

Contextual Notes

Participants note that the discussion involves uncertainties related to systematic errors and the assumptions about local density distributions. The complexity of the Hubble constant measurements and the potential for overlooked systematic effects are acknowledged.

phyzguy
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TL;DR
The fact that we live in a local underdensity of matter (just by chance) can explain most of the discrepancy in the Hubble constant.
Interesting paper on the arXiv today. The authors claim that there is observational evidence that we live in a region with slightly lower density than the universe average, just by chance. Taking this into account can explain as much as 5.5% of the discrepancy in the Hubble constant between the local measurements and the CMB measurement. If you shift the local measurements to lower values by 5.5% (about 3.8 km/sec/Mpc), then the discrepancy is within the experimental errors.
 
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Interesting article thanks for sharing, the article has an interesting argument.
 
Shouldn't this be part of the uncertainties already?
phyzguy said:
If you shift the local measurements to lower values by 5.5% (about 3.8 km/sec/Mpc), then the discrepancy is within the experimental errors.
The 5.5% are only for quite local measurements, not for the more distant supernova measurements.
 
mfb said:
Shouldn't this be part of the uncertainties already?
In an ideal world, sure. In practice it's difficult to account for this type of systematic error.

The basic way to understand this is that if we are in, say, a 2-##\sigma## underdensity, then it stands to reason that estimates which assume our local density is drawn from a random ensemble of possible local densities will be biased. If the underdensity was less severe, say 1-##\sigma##, then the random sampling of local densities should average to provide the correct result, since 1-##\sigma## is the expected deviation in such an ensemble.

If the magnitude of the local density can be determined and definitively shown to be below the average in the observable universe, then it would shift a lot of cosmological parameter measurements quite a bit. There'd probably be less dark energy, for instance. Such an underdensity might cause estimates of spatial curvature to be off. And yes, the Hubble constant would be different.
 
In the conferance videos that mfb shared ( about the Hubble discrepancy), Adam Riess stated that we do not live in a "giant" local void.

https://arxiv.org/abs/1810.03526
1564954657499.png


İf you want to listen start from the 19:00

http://online.kitp.ucsb.edu/online/enervac-c19/riess/
 
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phyzguy said:
Summary: The fact that we live in a local underdensity of matter (just by chance) can explain most of the discrepancy in the Hubble constant.

Interesting paper on the arXiv today. The authors claim that there is observational evidence that we live in a region with slightly lower density than the universe average, just by chance. Taking this into account can explain as much as 5.5% of the discrepancy in the Hubble constant between the local measurements and the CMB measurement. If you shift the local measurements to lower values by 5.5% (about 3.8 km/sec/Mpc), then the discrepancy is within the experimental errors.

I don't think 5.5% is enough to be consistent with experimental errors. The authors say "This is a differ-ence of about 9.6%, much larger than the combined error. The local estimates for the Hubble constant have been obtained well within a distance less than 100 Mpc, inside the region for which we found a significant underdensity in the matter distribution.Therefore our finding can at least explain part of the difference. But the discrepancy is larger than what could plausibly be accommodated by our observations. Thus one has to look in addition for other reasons for this discrepancy. There could wellbe further systematic effects which may have been overlooked or have been underestimated so far. "
 
atyy said:
I don't think 5.5% is enough to be consistent with experimental errors. The authors say "This is a differ-ence of about 9.6%, much larger than the combined error. The local estimates for the Hubble constant have been obtained well within a distance less than 100 Mpc, inside the region for which we found a significant underdensity in the matter distribution.Therefore our finding can at least explain part of the difference. But the discrepancy is larger than what could plausibly be accommodated by our observations. Thus one has to look in addition for other reasons for this discrepancy. There could wellbe further systematic effects which may have been overlooked or have been underestimated so far. "
What I meant was that if you remove the 5.5%, then the remaining discrepancy could just be statistical errors. The 9.6% discrepancy is claimed to be 4.4σ, if you believe all systematic errors have been accounted for ( for the record, I don't believe this). If 5.5% is due to the local underdensity, then the remaining 4.1% would just be just 1.9σ, which could just be statistical errors.
 

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