Most galaxies visible from Earth resemble a flat disk with a thickened center. They are therefore similar to the sports equipment of a discus thrower. According to the Standard Model of Cosmology, however, such disks should form rather rarely. This is because in the model, every galaxy is surrounded by a halo of dark matter. This halo is invisible, but exerts a strong gravitational pull on nearby galaxies due to its mass. "That's why we keep seeing galaxies merging with each other in the model universe," explains Prof. Dr. Pavel Kroupa of the Helmholtz Institute for Radiation and Nuclear Physics at the University of Bonn.
This crash has two effects, the physicist explains: "First, the galaxies penetrate in the process, destroying the disk shape. Second, it reduces the angular momentum of the new galaxy created by the merger." Put simply, this greatly decreases its rotational speed. The rotating motion normally ensures that the centrifugal forces acting during this process cause a new disk to form. However, if the angular momentum is too small, a new disk will not form at all.
Large discrepancy between prediction and reality
In the current study, Kroupa's doctoral student, Moritz Haslbauer, led an international research group to investigate the evolution of the universe using the latest supercomputer simulations. The calculations are based on the Standard Model of Cosmology; they show which galaxies should have formed by today if this theory were correct. The researchers then compared their results with what is currently probably the most accurate observational data of the real Universe visible from Earth.
"Here we encountered a significant discrepancy between prediction and reality," Haslbauer says: "There are apparently significantly more flat disk galaxies than can be explained by theory." However, the resolution of the simulations is limited even on today's supercomputers. It may therefore be that the number of disk galaxies that would form in the Standard Model of Cosmology has been underestimated. "However, even if we take this effect into account, there remains a serious difference between theory and observation that cannot be remedied", Haslbauer points out.
The situation is different for an alternative to the Standard Model, which dispenses with dark matter. According to the so-called MOND theory (the acronym stands for "MilgrOmiaN Dynamics), galaxies do not grow by merging with each other. Instead, they are formed from rotating gas clouds that become more and more condensed. In a MOND universe, galaxies also grow by absorbing gas from their surroundings. However, mergers of full-grown galaxies are rare in MOND. "Our research group in Bonn and Prague has uniquely developed the methods to do calculations in this alternative theory," says Kroupa, who is also a member of the Transdisciplinary Research Units "Modelling" and "Matter" at the University of Bonn. "MOND's predictions are consistent with what we actually see."
Challenge for the Standard Model
However, the exact mechanisms of galaxy growth are not yet fully understood, even with MOND. Additionally, in MOND, Newton's laws of gravity do not apply under certain circumstances, but need to be replaced by the correct ones. This would have far-reaching consequences for other areas of physics. "Nevertheless, the MOND theory solves all known extragalactic cosmological problems despite being originally formulated to address galaxies only," says Dr. Indranil Banik, who was involved in this research. "Our study proves that young physicists today still have the opportunity to make significant contributions to fundamental physics," Kroupa adds.
Publication: Moritz Haslbauer, Indranil Banik, Pavel Kroupa, Nils Wittenburg and Behnam Javanmardi: The high fraction of thin disk galaxies continues to challenge ΛCDM cosmology; Astrophysical Journal; DOI: 10.3847/1538-4357/ac46ac; URL: https://iopscience.iop.org/article/10.3847/1538-4357/ac46ac; https://arxiv.org/abs/2202.01221
Contact:
Moritz Haslbauer
Helmholtz Institute for Radiation and Nuclear Physics at the
University of Bonn and Max-Planck Institute for Radio Astronomy Bonn
Phone +49-228-739399 or +49-173 6616584
E-mail: mhaslbauer@mpifr-bonn.mpg.de
Prof. Dr. Pavel Kroupa
Helmholtz Institute for Radiation and Nuclear Physics at the University of Bonn
Phone +49-228/73-6140
E-mail: pkroupa@uni-bonn.de