Are We Near the Center of a Large Under-Density of Matter in the Universe?

When modern cosmologists began to tackle cosmic acceleration and dark energy, they dusted off Einstein’s cosmological constant as interchangeable with dark energy, given the new knowledge about cosmic acceleration.

That explanation didn’t satisfy mathematicians Blake Temple and Zeke Vogler at the University of California, Davis, and Joel Smoller at the University of Michigan, Ann Arbor.

“We set out to find the best explanation we could come up with for the anomalous acceleration of the galaxies within Einstein’s original theory without dark energy,” Temple said.

The original theory of General Relativity has given correct predictions in every other context, Temple said, and there is no direct evidence of dark energy. So why add a “fudge factor” (dark energy or the cosmological constant) to equations that already appear correct? Instead of faulty equations that need to be tweaked to get the right solution, the mathematicians argue that the equations are correct, but the assumption of a uniformly expanding universe of galaxies is wrong, with or without dark energy, because that configuration is unstable.
An unstable solution

Cosmological models start from a “Friedmann universe,” which assumes that all matter is expanding but evenly distributed in space at every time, Temple said.

Temple, Smoller and Vogler worked out solutions to General Relativity without invoking dark energy. They argue that the equations show that the Friedmann space-time is actually unstable: Any perturbation — for example if the density of matter is a bit lower than average — pushes it over into an accelerating universe.

Temple compares this to an upside-down pendulum. When a pendulum is hanging down, it is stable at its lowest point. Turn a rigid pendulum the other way, and it can balance if it is exactly centered — but any small gust will blow it off.

This tells us that we should not expect to measure a Friedmann universe, because it is unstable, Temple said. What we should expect to measure instead are local space-times that accelerate faster. Remarkably, the local space-times created by the instability exhibit precisely the same range of cosmic accelerations as you get in theories of dark energy, he said.

“The math isn’t controversial, the instability isn’t controversial,” Temple said. “What we don’t know is, does our Milky Way galaxy lie near the center of a large under-density of matter in the universe.”

The paper does include testable predictions that distinguish their model from dark energy models, Temple said.

Joel Smoller died in September 2017, while the paper was under review. The work was partially supported by the National Science Foundation.

Contacts and sources:
Andy Fell,
Blake Temple, Mathematics(
University of California – Davis (UC Davis)