Latest Findings from DESI Collaboration

  • Context: Undergrad 
  • Thread starter Thread starter MrRobotoToo
  • Start date Start date
  • Tags Tags
    Cosmology Hubble
Click For Summary
SUMMARY

The latest findings from the DESI collaboration indicate that the Hubble constant derived from baryon acoustic oscillations aligns closely with the value obtained from Lambda-CDM using Planck data. Notably, DESI suggests a sum of the three neutrino masses that is lower than the minimum value established by neutrino oscillation data. Despite this consistency, the Hubble tension remains unresolved due to conflicting late-time measurements of the Hubble constant. The need to reconcile these credible measurements is critical for advancing our understanding of cosmological parameters.

PREREQUISITES
  • Understanding of baryon acoustic oscillations
  • Familiarity with Lambda-CDM cosmological model
  • Knowledge of neutrino oscillation data and mass hierarchy
  • Awareness of Hubble constant measurement techniques
NEXT STEPS
  • Research the implications of baryon acoustic oscillations on cosmology
  • Study the Lambda-CDM model and its significance in modern astrophysics
  • Examine the latest neutrino oscillation experiments and their findings
  • Investigate methods for reconciling discrepancies in Hubble constant measurements
USEFUL FOR

Astronomers, cosmologists, and physicists interested in the latest developments in cosmological measurements and the ongoing Hubble tension debate.

Space news on Phys.org
The more notable finding from DESI, in my humble opinion, is that it favors a sum of the three neutrino masses which is less than the minimum value of that quantity derived from neutrino oscillation data. See Nathaniel Craig, Daniel Green, Joel Meyers, Surjeet Rajendran, "No νs is Good News" arXiv:2405.00836 (May 1, 2024).

A DESI Hubble Constant value consistent with the Planck CMB based estimate doesn't solve the Hubble tension because there are still plenty of late time measurements of the Hubble constant with values inconsistent with that lower CMB based value. Adding one more measurement to the mix doesn't resolve the fact that we have different values from what are each credible ways to do the measurement. We need to figure out how to reconcile all of the credible measurements of the Hubble constant to resolve the tension. See my previous discussion of this issue here.
 
And T2K + NoVA see the opposite with respect to the hierarchy.

You can drive yourself crazy chasing one and two sigma tensions. Excited theorists just add entropy - you can't get a paper that says "wait and see" published.
 
  • Like
Likes   Reactions: ohwilleke

Similar threads

  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 30 ·
2
Replies
30
Views
5K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 29 ·
Replies
29
Views
7K
  • · Replies 0 ·
Replies
0
Views
2K
  • · Replies 18 ·
Replies
18
Views
2K
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 1 ·
Replies
1
Views
3K