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Astrophysics

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2

Nanoom Lee, Tianji Zhou

Featured June 6, 2026

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Simply

Scientists found that changing how atoms formed long ago could fix the Hubble puzzle using early universe maps, but this fix breaks when adding new maps of how galaxies are spread out.

In depth
The paper investigates if modifying the cosmological recombination history can resolve the Hubble tension by using a data-driven framework to find minimal, perturbative changes to the time-varying electron mass . It demonstrates that while such modifications can reconcile early-universe and local measurements with CMB data alone, they fail when precise late-time BAO data are included due to fundamental parameter degeneracies.

Key Takeaways

  • 1
    The Fisher-bias formalism is applied to identify minimal, perturbative modifications to the electron mass that can shift the CMB-inferred Hubble constant () towards local measurements without degrading data fit.
  • 2
    With CMB data alone (Planck + ACT DR6), a time-varying can fully resolve the Hubble tension and ease the tension, demonstrating robustness across independent CMB datasets.
  • 3
    The inclusion of late-time BAO data (DESI DR2) reveals a fundamental limitation: recombination-based solutions cannot fully resolve the Hubble tension because raising generically lowers , which is tightly constrained by BAO.

Conceptual Flow

HIGH LEVEL
1
Methodology: Finding the Minimal Change

The scientists used a special math trick to find the smallest possible change to a tiny particle's weight that would make the universe's expansion speed match up, without messing up other measurements.

Universe Data
Target Speed
Calculate Smallest Change
Particle Weight Adjustment
2
Results: Early vs. Late Universe Views

They found that the change worked perfectly with early universe data, but when they added later universe data, the change no longer made everything fit together.

Early Universe Fit
Late Universe Fit
Compare Results
Solution Works (Early)
Solution Fails (Late)