https://www.opednews.com/articles/Cosmol...9-115.html
EXCERPT (Josh Mitteldorf ): . . . Conservative leaders in the field speak of a crisis in cosmology. Two such articles have appeared in recent months. The one that I just linked (by my Harvard classmate of 50 years ago, Joseph Silk) notes that theorists have indulged in a kind of cheating to make their models appear consistent with the data. They have chosen parameters for the expansion and the density of the universe that are halfway between values measured by two kinds of methodologies.
If you compare Observation A to the model, it is just on the edge of being plausible. If you compare Observation B to the model, it is just on the edge of being plausible in the other direction. But, as Dr Silk points out, if you compare Observation A directly to Observation B, you realize that the two are too far apart to be compatible, and that our research and analysis methods must be called into question.
Dr Becky Smethurst [second video below] emphasizes that one implication of the new perspective is that the universe is closed and finite and will not expand forever.
The other recent article notes that all of the measurements that pointed to speed-up in the expansion (and the need for dark energy) came from one direction in the sky. If you look in the opposite direction, the expansion is slowing down. Maybe it's not that the whole universe is changing its expansion at all, but only that our little neighborhood has shifted direction. But we're out of the frying pan, into the fire, because the same evidence suggests that the universe may not be completely uniform and symmetrical, as theories have always assumed. The trouble with asymmetrical models is that they call into question the very simple equations that are our hope for staying within 6 or 7 free parameters. There's a worse problem, actually: The equations of gravity (Einstein's General Relativity) are so insanely complicated that they cannot be solved even with the largest supercomputers we have except in the case where the equations are enormously simplified either by (1) a very high degree of symmetry that vastly reduces the complexity, or (2) weak fields, called the "Newtonian limit".
Sabine Hossenfelder does a good job of explaining the context in this video. (MORE - details)
https://www.youtube-nocookie.com/embed/oqgKXQM8FpU
https://www.youtube-nocookie.com/embed/cnn_5YMpo3Q
https://www.youtube-nocookie.com/embed/c6Eq2sI1NDY
EXCERPT (Josh Mitteldorf ): . . . Conservative leaders in the field speak of a crisis in cosmology. Two such articles have appeared in recent months. The one that I just linked (by my Harvard classmate of 50 years ago, Joseph Silk) notes that theorists have indulged in a kind of cheating to make their models appear consistent with the data. They have chosen parameters for the expansion and the density of the universe that are halfway between values measured by two kinds of methodologies.
If you compare Observation A to the model, it is just on the edge of being plausible. If you compare Observation B to the model, it is just on the edge of being plausible in the other direction. But, as Dr Silk points out, if you compare Observation A directly to Observation B, you realize that the two are too far apart to be compatible, and that our research and analysis methods must be called into question.
Dr Becky Smethurst [second video below] emphasizes that one implication of the new perspective is that the universe is closed and finite and will not expand forever.
The other recent article notes that all of the measurements that pointed to speed-up in the expansion (and the need for dark energy) came from one direction in the sky. If you look in the opposite direction, the expansion is slowing down. Maybe it's not that the whole universe is changing its expansion at all, but only that our little neighborhood has shifted direction. But we're out of the frying pan, into the fire, because the same evidence suggests that the universe may not be completely uniform and symmetrical, as theories have always assumed. The trouble with asymmetrical models is that they call into question the very simple equations that are our hope for staying within 6 or 7 free parameters. There's a worse problem, actually: The equations of gravity (Einstein's General Relativity) are so insanely complicated that they cannot be solved even with the largest supercomputers we have except in the case where the equations are enormously simplified either by (1) a very high degree of symmetry that vastly reduces the complexity, or (2) weak fields, called the "Newtonian limit".
Sabine Hossenfelder does a good job of explaining the context in this video. (MORE - details)