Using gravitational lensing, scientists uncovered that dark matter may stretch over a million light-years from galactic centers, proposing significant adjustments to our gravitational theories or the concept of dark matter itself. Credit: SciTechDaily.com
Groundbreaking new research reveals that rotation curves of galaxies stay flat indefinitely far out, corroborating predictions of modified gravity theory as an alternative to dark matter.
This finding challenges the existing models of cosmology and suggests that either dark matter halos are vastly extended or our understanding of gravitational theory needs a fundamental reassessment.
Breakthrough in Cosmology
In a breakthrough discovery that challenges the conventional understanding of cosmology, scientists at Case Western Reserve University have unearthed new evidence that could reshape our perception of the cosmos.
Tobias Mistele, a post-doctoral scholar in the Department of Astronomy at Case Western Reserve’s College of Arts and Sciences, pioneered a revolutionary technique using “gravitational lensing” to delve into the enigmatic realm of dark matter. He discovered that the rotation curves of galaxies remain flat for millions of light years with no end in sight.
Scientists have previously believed that the rotation curves of galaxies must decline the farther out you peer into space.
Weak Lensing Rotation Curve modeling. Credit: Case Western Reserve University
Challenging Traditional Cosmic Models
Traditionally, the behavior of stars within galaxies has puzzled astronomers. According to Newtonian gravity, stars on the outer edges should be slower due to diminished gravitational pull. This was not observed, leading to the inference of dark matter. But even dark matter halos should come to an end, so rotation curves should not remain flat indefinitely.
Mistele’s analysis defies this expectation, providing a startling revelation: the influence of what we call dark matter extends far beyond previous estimates, , stretching at least a million light-years from the galactic center.
Tobias Mistele. Credit: Case Western Reserve University
Such a long-range effect may indicate that dark matter—as we understand it—might not exist at all.
“This finding challenges existing models,” he said, “suggesting there exist either vastly extended dark matter halos or that we need to fundamentally reevaluate our understanding of gravitational theory.”
Revolutionary Implications for Astrophysics
Stacy McGaugh, professor and director of the Department of Astronomy in the College of Arts and Sciences, said Mistele’s findings, slated for publication in the 
Stacy McGaugh. Credit: Case Western Reserve University
As part of the research, Mistele plotted out what’s called Tully–Fisher relation on a chart to highlight the empirical relationship between the visible mass of a galaxy and its rotation speed.
“We knew this relationship existed,” Mistele said. “But it wasn’t obvious that the relationship would hold the farther you go out. How far does this behavior persist? That’s the question, because it can’t persist forever.”
Mistele said his discovery underscores the necessity for further exploration and collaboration within the scientific community—and the possible analysis of other data.
Reevaluating Dark Matter Theories
McGaugh noted the Herculean—yet, so far, unsuccessful—efforts in the international particle physics community to detect and identify dark matter particles.
“Either dark matter halos are much bigger than we expected, or the whole paradigm is wrong,” McGaugh said. “The theory that predicted this behavior in advance is the modified gravity theory MOND hypothesized by Moti Milgrom as an alternative to dark matter in 1983. So, the obvious and inevitably controversial interpretation of this result is that dark matter is a chimera; perhaps the evidence for it is pointing to some new theory of gravity beyond what Einstein taught us.”
Reference: “Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing” by Tobias Mistele, Stacy McGaugh, Federico Lelli, James Schombert and Pengfei Li, Accepted, Astrophysical Journal Letters.
arXiv:2406.09685
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