Tension for a Hubble-Tension Solution

Physics 16, s164
An early-Universe spike in dark energy could resolve a disagreement between two cosmic-expansion-rate measurements, but such a spike may conflict with observations of quasar spectra.
Scott Goldstein

The Hubble tension is a discrepancy between the results of two methods for determining the cosmic-expansion rate. One solution to this tension is to assume that there was a spike in the amount of dark energy early in the Universe’s history (see Synopsis: Dark Energy Solution for Hubble Tension). However, there could be unwanted effects from “early dark energy,” such as a change in the growth rate of galaxies and other large-scale structures. Now Samuel Goldstein from Columbia University and his colleagues find that the early-dark-energy scenario could also lead to a mismatch between predictions and observations of a series of quasar-spectra absorption lines, collectively known as the Lyman- 𝛼 forest [1].

The Lyman- 𝛼-forest lines come from the absorption of light from quasars by clumps of hydrogen gas lying along the line of sight to these bright quasistellar objects. Cosmological models can predict the spatial distribution of hydrogen clumps—that is, how many clumps of a certain size there should be within a certain volume. And those predictions can be compared to Lyman- 𝛼-forest data. Goldstein and his colleagues performed such a comparison using a model with early dark energy.

The researchers varied the density of early dark energy while also tuning various cosmological parameters, including the density of dark matter and the strength of primordial-matter fluctuations. To match current Lyman- 𝛼 observations, the team’s model required that early dark energy be less than 3% of the early Universe’s energy budget, which is far below the 10% assumed in Hubble-tension-resolving scenarios. The results are “the most stringent constraints on early dark energy to date,” Goldstein says.

–Michael Schirber

Michael Schirber is a Corresponding Editor for Physics Magazine based in Lyon, France.


  1. S. Goldstein et al., “Canonical Hubble-tension-resolving early dark energy cosmologies are inconsistent with the Lyman-𝛼 forest,” Phys. Rev. Lett. 131, 201001 (2023).

Subject Areas


Related Articles

“Spin” Leaves Its Mark on Some Meteorite Craters
Materials Science

“Spin” Leaves Its Mark on Some Meteorite Craters

Numerical simulations reveal that an impact crater’s shape can depend on the impactor’s spin and its degree of cohesion. Read More »

Milky Way Pulsars Rule Out Some Extremely Light Dark Matter Particles

Milky Way Pulsars Rule Out Some Extremely Light Dark Matter Particles

If ultralight dark matter particles exist, they can contribute no more than 70% of the dark matter between Earth and a set of monitored pulsars. Read More »

Galaxy’s Gamma Glow Illuminates Cosmic-Ray Origins
Particles and Fields

Galaxy’s Gamma Glow Illuminates Cosmic-Ray Origins

Interstellar magnetic fields perturb the trajectories of cosmic rays, making it difficult to identify their sources. A new survey of gamma radiation produced when cosmic rays interact with the interstellar medium should help in this identification. Read More »

More Articles