From our current perspective, the Universe seems to be dominated by two things we find frustratingly difficult to understand. One of these is dark matter, which describes the fact that everything from galaxies on up behaves as if it has more mass than we can detect. While that has spawned extensive searches for particles that could account for the visual discrepancy, it's also triggered the development of alternative theories of gravity, ones that can replace relativity while accounting for the discrepancies in apparent mass.
So far, these proposals have fallen well short of replacing general relativity. And they say nothing about the other big mystery, dark energy, which appears to be accelerating the expansion of the Universe. Instead, researchers have developed an entirely separate class of theories that could modify gravity in a way that eliminates the need for dark energy. Now, researchers have run simulations of galaxy and star formation using this alternative version of physics, and they found we might be on the cusp of testing some of them.
General relativity explains a broad range of phenomena, and it works well to describe the Universe as a whole, provided dark matter and dark energy exist as separate entities. Any alternatives to gravity have to account for everything that's explained by general relativity while also accounting for the additional effects of at least one of these two dark forces. A class of theories, collectively termed MOND (for Modified Newtonian Dynamics), is intended to do away with dark matter, but it struggles to account for things relativity handles with easy.
And, when it comes to dark energy, MOND is silent, in part because it was originally developed before dark energy was known to be an issue. Instead, an entirely separate class of theories has been developed that handle gravity while eliminating the need for a separate dark energy. These are known as f(R) models and are commonly described as having a "chameleon" mechanism. That's because they posit an additional force that changes its behavior based on its surroundings.
Where there's a lot of matter, the chameleon force is minimized, allowing it to blend in with its surroundings. As matter becomes sparse on larger scales, it starts to make its presence felt. That's why we can't detect any major deviations from relativity on Earth or near objects like neutron stars, but we do detect them when we start looking at the large scale structure of the Universe. The net result is an acceleration of the expansion of the Universe that's only apparent at large scales—just like dark energy.
For any additions to physics to be successful, they have to make sense with what we know of relativity, plus handle details it can't. That makes it difficult to test, because the new models are already crafted to match existing data (and would be pretty pointless if they weren't). So, the trick is finding data we don't yet have, but could show a difference between relativity and these new models.
To search for these sorts of discrepancies, a group of cosmologists at Durham University decided to plug some chameleon proposals into massive computational models that simulate the formation of structures ranging from stars to galaxy clusters.
A model universe
The researchers worked with the IllustrisTNG model, a mini-Universe that can simulate galaxy formation and evolution. Under standard conditions, the model controls this evolution in part by having everything obey general relativity. But for this test, the research team also ran a version where relativity was replaced with a chameleon f(R) version of gravity. (They also ran an exaggerated version of f(R) in order to accentuate the differences.)
All models assumed the presence of large amounts of dark matter; remember it's MOND that hopes to get rid of that. Simulations were run under two conditions: with feedback from regular matter, and without. Unlike dark matter, regular matter ignites into stars and forms black holes, and those provide feedbacks that alter the behavior of nearby matter.
The simulations indicated that the gas in the inner regions of galaxies doesn't feel the effect of modified gravity, behaving much as it would with general relativity. This includes gas flowing into the area near supermassive black holes that power active galaxies. In contrast, the outer regions of galaxies should show some differenceRead More – Source