*Taking dark energy out of the equation: Mathematicians challenge the
standard cosmological model of the universe*



Mathematicians are challenging the idea that dark energy is responsible for
the accelerating expansion of the universe. In a new paper published
<https://royalsocietypublishing.org/rspa/article/482/2338/20250912/481920/The-instability-of-critical-and-underdense>
 in *Proceedings of the Royal Society A*, mathematicians from the
University of California, Davis, provide mathematical proof that
instabilities inherent in the Einstein-Euler equations imply that the
current model of the expanding universe is not viable.

The Einstein-Euler equations are a union of general relativity and fluid
dynamics equations used to model astronomical phenomena such as galaxies,
black holes, and cosmic expansion.

The research directly challenges the Lambda-cold dark matter model
<https://phys.org/news/2025-01-scientists-mysterious-suppression-cosmic-growth.html?utm_source=embeddings&utm_medium=related&utm_campaign=internal>,
the standard cosmological model of the Big Bang.

Study corresponding author Blake Temple, a distinguished professor emeritus
of mathematics at UC Davis, compared the standard cosmological model to a
pencil standing on its tip.

"All the forces are in balance when a pencil is standing on end, so it is a
'solution of the equations,'" he said. "But it's unstable. Any breath of
air and it falls away."

The mathematics, Temple said, prove that Friedmann spacetimes—mathematical
models that govern cosmic expansion—are unstable at both small and large
length scales at the Big Bang, making it the most unstable solution of all.

"Unstable solutions in physics and science are considered not physical,"
Temple said. "You'll never observe them in nature."

Temple noted that this instability suggests a simpler explanation—one based
entirely within the framework of Einstein's original theory.

"The instability of all Friedmann spacetimes to accelerated expansion
suggests a simpler, more natural explanation for the acceleration of the
universe than dark energy," he said.

*Explaining the universe's accelerating expansion*

Almost 30 years ago, dark energy was proposed as the force responsible for
the accelerating expansion of the universe.

The idea harkens back to Albert Einstein's original 1915,
gravity-describing equations for general relativity. To produce a static
universe, Einstein initially introduced an antigravity factor in his
theory. He called this factor the "cosmological constant."

After Edwin Hubble discovered the universe was expanding in 1929, Einstein
famously called the cosmological constant his "biggest blunder" because
without it he could have predicted the expansion.

However, the cosmological constant, and the idea that it's interchangeable
with dark energy, was reintroduced to explain the universe's accelerating
expansion in the 1990s. Standard cosmological models are based on what's
called the "Friedmann universe," which describes all matter as expanding
but being evenly distributed throughout space at each fixed time.

But the math didn't add up to Temple and his colleagues, leading them to
pursue alternative explanations for the accelerating expansion of the
universe.

"Our first idea was that maybe the universe was expanding because there was
a shockwave, and the anomalous acceleration was the expanding wave behind
that shockwave," Temple said. "Then we realized there's a family of
self-similar solutions during the radiation epoch of the Big Bang, which
might model that expanding wave."

Self-similar equations describe physical phenomena that maintains a pattern
or structure, regardless of its scale.

In the current paper, the mathematicians use a self-similar version of the
Einstein equations, which they derived in prior work, to represent the
standard model of cosmology as a rest point of the equations. This provides
the framework for a complete mathematical characterization of the standard
model's stability, and more generally, the stability of all Friedmann
spacetimes during the matter-dominated epoch of the Big Bang.

"We prove that, like Einstein's static model, the Friedmann spacetimes are
all unstable to radial perturbation at large length scales," Temple said.
"This appears to rule out the Lambda-cold dark matter model as a viable
stable solution of the Einstein equations of general relativity, with or
without dark energy."

"This means," he added, "that the Big Bang should generically look exactly
like a Friedmann spacetime near the center of symmetry, but generically one
should observe accelerations away from Friedmann far from the center."

The phase portrait for the STV-ODE of order n = 2⁠. Credit: *Proceedings of
the Royal Society A Mathematical Physical and Engineering Science* (2026).
DOI: 10.1098/rspa.2025.0912

*Rethinking the Copernican principle?*

Temple and his colleagues found that the accelerating expansion of the
universe is a direct consequence of the Einstein-Euler equations without
the insertion of a cosmological constant or dark energy.

The math also calls into question the Copernican principle—the idea that
Earth's location does not occupy a special place in the universe.

"Both the Lambda-cold dark matter model and a spherically symmetric
spacetime produce a special place where we must lie for the model to be
physically plausible," Temple said. "If this principle rules out one, it
has to rule out the other."

K RAJARAM IRS 29526

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