One of the great mysteries of cosmology is the fact that the cosmos is speeding up as it expands. Scientists explain this acceleration by an invisible pressure called dark energy which makes up about 70% of the energy in the cosmos.
This explanation is based on an assumption called the Friedmann-Lemaitre-Robertson-Walker metric which took Einstein’s equations and applied them to a universe they assumed to be homogeneous and isotropic. In other words, it assumes a smooth universe. Science has determined that the universe is not smooth. It is made up of great voids separating networks of dense galaxy clusters and filaments.
Emily Conover writing in Science News for November 25, 2017, (page 22) said, “If the universe were soup, it would be more of a chunky minestrone than a silky smooth tomato bisque.” When the equations are applied to a universe that is not isotropic and homogeneous, the acceleration of the cosmos seems to be explained without the need for dark energy. By the very nature of the lumpy design of the cosmos, its collapse is avoided.
It is interesting to note that the cosmos was created in such a way that its very existence contains the fingerprint of a design that allows great stability over an infinite amount of time. The more we know of the creation, the closer we get to the Creator.
Many aspects of the creation we may never understand, but as our instruments get better and data accumulates, we understand that we have, in the words of Issac Newton, “found a pebble of knowledge while an ocean of truth lays before us.”
One of the most interesting areas of scientific research today is the study of dark matter. We have known for more than half a century that galaxies are groups of billions of stars revolving around a core. Science had assumed that the glue holding galaxies together was the gravitational force produced by the mass of the stars in the galaxy. The problem with this explanation was that the stars were spiraling too fast for the gravity produced by their mass to hold the galaxy together.
If you stand in the center of a circle and spin a bucket of water on a rope, you have to spin it at a certain speed to keep the water in the bucket. If you go too slow, the bucket will hit the ground, and if you go too fast, it will break the rope. In the case of galaxies, the stars were going so fast for the gravity of the stars to hold the system together. Some other gravitational force must be the glue doing the job. The discovery of black holes in the center of galaxies was thought to be a possible answer, but the speed was much too fast for even that source. The amount of mass it would take to hold some of the galaxies together is as much as 85% higher than what we can observe.
This problem led to the proposal that there is a missing mass. Scientists suggested particles called WIMPS, which is an acronym for “weakly interacting massive particles.” For some time now, experiments have been conducted to find evidence for WIMPS. The Large Hadron Collider near Geneva, Switzerland, has been smashing protons together in hopes of detecting the particle. The Large Underground Xenon experiment in South Dakota has been looking for traces of them as well. So far neither attempt has been successful. In an article in Scientific American (October 2016, page 16) Edward Kolb, who was involved in proposing the existence of WIMPS, said: “We are more in the dark about dark matter than we were five years ago.” David Spergel who is an astrophysicist at Princeton says, “…we now need more hints from nature about where to go next.”
It seems that God has already taught us quite a bit about the complexity of creation. Thanks to Isaac Newton we know that mass has a connection to gravity. Thanks to Albert Einstein we know that the shape of space has something to do with it as well. Making a galaxy is not a simple task. Just like the making of electric charge, the process involves understandings that science is just beginning to comprehend. Quantum mechanics has taught us that a whole new set of laws governs what happens in forming these building blocks of what we see.