Led by Rajendra Gupta, Adjunct Professor in the Department of physics at the University of Ottawa, the study asserts that if the basic strengths of nature鈥檚 forces (like gravity) slowly change over time and in space, they can explain the strange phenomena we observe, such as the way galaxies evolve and spin and how the universe expands.

鈥淲ith our model, you don鈥檛 need to assume any exotic particles or break the rules of physics鈥
Rajendra Gupta
鈥 Adjunct Professor in the Department of physics at the University of Ottawa
Challenging established concepts
鈥淭he universe鈥檚 forces actually get weaker on the average as it expands,鈥 Professor Gupta explains. 鈥淭his weakening makes it look like there鈥檚 a mysterious push making the universe expand faster (which is identified as dark energy). However, at galactic and galaxy-cluster scale, the variation of these forces over their gravitationally bound space results in extra gravity (which is considered due to dark matter). But those things might just be illusions, emergent from the evolving constants defining the strength of the forces.鈥
He adds, 鈥淭here are two very different phenomena needed to be explained by dark matter and dark energy: The first is at cosmological scale, that is, at a scale larger than 600 million light years assuming the universe is homogeneous and the same in all directions. The second is at astrophysical scale, that is, at smaller scale the universe is very lumpy and direction dependent. In the standard model, the two scenarios require different equations to explain observations using dark matter and dark energy. Ours is the only one that explains them with the same equation, and without needing dark matter or dark energy.鈥
He adds, 鈥淲hat鈥檚 really exciting is that this new approach lets us explain what we see in the sky: galaxy rotation, galaxy clustering, and even the way light bends around massive objects, without having to imagine there鈥檚 something hiding out there. It鈥檚 all just the result of the constants of nature varying as the universe ages and becomes lumpy.鈥
New model applied at Astrophysical Scale
Last year, Professor Gupta challenged the existence of dark matter in the universe in his cosmological-scale study. In this astrophysical-scale work, hequestioned the current theoretical models for the galaxy rotation curves.
- In the new model, the parameter often denoted 伪 emerges from allowing the coupling constants to evolve. In effect, 伪 behaves like an extra 鈥渃omponent鈥 in the gravitational equations that produces effects similar to what astronomers attribute to dark matter and dark energy.
- On cosmological scales, 伪 is treated as a constant (e.g., determined by fitting supernovae data). But locally (on astrophysical scale), in a galaxy, because the standard matter (black holes, stars, planets, gas, etc.) distribution varies drastically, 伪 varies causing the extra gravitational effect to depend on where such matter is. So the new theory predicts that in regions where there鈥檚 a lot of standard matter, the extra gravity effect is less, and where detectable matter density is low, it is larger.
- In effect, instead of adding dark matter halos around galaxies, the extra gravitational pull comes from 伪 in the new model. It reproduces the observed 鈥渇lat rotation curves鈥 (stars moving faster than expected in the outer parts of galaxies).
Implications for astronomy
Professor Gupta believes this idea could solve some of the biggest puzzles in astronomy. 鈥淔or years, we鈥檝e struggled to explain how galaxies in the early universe formed so quickly and became so massive,鈥 he says. 鈥淲ith our model, you don鈥檛 need to assume any exotic particles or break the rules of physics. The timeline of the universe simply stretches out, almost doubling the universe鈥檚 age, and making room for everything we observe.鈥
Effectively, the stretched out timeline for how stars and galaxies form, makes it much easier to explain how big, complex structures like galaxies and black holes could have appeared so early in the universe.
This theory could completely change how we think about the universe. It even hints that searching for dark matter particles, something scientists have spent years and billions of dollars on, might not be necessary after all. Even if the exotic particles are experimentally found they would need to constitute about six times the mass of the standard matter.
鈥淪ometimes, the simplest explanation is the best one. Maybe the universe鈥檚 biggest secrets are just tricks played by the evolving constants of nature,鈥 Professor Gupta concludes.
The study, titled 鈥溾, was published in the peer-reviewed journal Galaxies.