SiteMap
close
Research
Research News
A prestigious global university that fosters Sejong-type talent who challenges creative thinking and communicates with the world.
|
New measurements of the gravitational anomaly in wide binaries are against Newton in favor of modified gravity 2024.09.09 1545 |
|
|---|---|
|
New measurements of the gravitational anomaly in wide binaries are against Newton in favor of modified gravity Prof. Kyu-Hyun Chae at Department of Physics and Astronomy Wide binary stars (Figure 1) have recently been hotly debated as direct probes of the nature of gravity at low acceleration weaker than about 1 nanometer per second squared. The nature of gravity at such low acceleration is of utmost importance because the concept of dark matter, the gravitational dynamics of astrophysical systems, fundamental theories of physics, and cosmology are all inextricably intertwined with it. For example, a deviation from Newtonian expectation at such low acceleration would require a modification or extension of Eistein’s general relativity despite all its successes outside the low acceleration regime. Two recent independent studies led by Kyu-Hyun Chae (Figure 2) and Xavier Hernandez claim that the statistical properties of wide binary stars based on European Space Agency’s latest Gaia database deviate from the Newtonian expectation in agreement with the prediction of modified gravity theories under the new theoretical framework called modified Newtonian dynamics (MOND, sometimes referred to as Milgromian dynamics), introduced 40 years ago by Mordehai (Moti) Milgrom. The breakdown of Newtonian gravity at low acceleration would mean a scientific revolution whose full implications are immeasurably far-reaching. Because of this importance and considering other divergent claims, Chae has carried out a new analysis to address all the issues raised so far, in particular the challenges to the specific low-acceleration gravitational anomaly obtained by himself. For this, Chae has considered a full range of samples allowing various fractions of hierarchical systems where a binary has an unseen nested inner binary, and applied various methods that cover essentially all the methods published so far including the method used by some researchers to claim against the gravitational anomaly. Chae recalls this new study that was published in the Astrophysical Journal on 9 September 2024, “To some extent, it was my obligation to the science community to carry out this new work. I had to clarify the issues and challenges raised to my claimed conclusion and explain the causes of the divergent claims by others.” Chae finds that all methods with various samples give consistent results. The magnitude of the gravitational anomaly first identified last year appears robust. Chae reflects on the results, “The gravitational anomaly is clearly imprinted in the data. One cannot remove it. It is mysterious to many scientists why gravity is boosted by about 40 percent when the internal acceleration between the orbiting pair of stars is weaker than about 0.1 nanometer per second squared. However, the presence and the degree of the gravitational anomaly were, in fact, predicted by MOND or Milgromian dynamics." Like Newton’s universal law of gravitation and Einstein’s general relativity, MOND satisfies the universality of free fall (also referred to as the weak equivalence principle) that is known to be first suggested by Galileo Galilei though experiments at the leaning tower of Pisa (Figure 2). Newton and Einstein go one step further and postulate the strong equivalence principle by which the internal dynamics of a gravitational system falling freely under a nearly constant external field is not affected by the external field. In contrast, MOND postulates the breakdown of the strong equivalence principle. Thus, wide binaries falling freely under the external field of the Milky Way are expected to obey Kepler’s laws according to Newton’s and Einstein’s theories. In contrast, MOND predicts that the wide binary internal motion deviates from the Newton-Einstein prediction by the degree dictated by Milky Way’s external field strength of about 0.2 nano meter per second squared. That is right about 40 percent! as measured by the new study in agreement with previous results. While these consistent results are arresting, unlimited reproductions and confirmations are needed for the reported gravitational anomaly to become a true scientific fact. Also, the reported gravitational anomaly will have to be better characterized continually to provide useful constraints on theories. The eyes of researchers are on new data and better methodologies for that purpose. In particular, existing research results were obtained with only the sky-projected transverse velocities of stars because the line-of-sight velocity components have not yet been precisely measured. Researchers including Chae are considering new measurements of the line-of-sight velocities of stars. Reference: “Measurements of the Low-Acceleration Gravitational Anomaly from the Normalized Velocity Profile of Gaia Wide Binary Stars and Statistical Testing of Newtonian and Milgromian Theories” published in the Astrophysical Journal on 9 September 2024 https://doi.org/10.3847/1538-4357/ad61e9
Figure 1. A wide binary system (Gaia DR3 source IDs '3046204180298475264' and '3046204150242468480') separated by 6000AU on the sky. This system is at a distance of 87 parsec or 280 light years from the Sun. Note that there are background stars at farther distances that are not physically associated with the binary system. Image credit: Gaia DR3 data archive.
Figure 2. Kyu-Hyun Chae in front of the tower of Pisa |
|
| Next | Discovering the physical trigger of the Universe's Most Powerful Supernovae with Gravitational Waves |
| Previous | Breakdown of the Newton-Einstein Standard Gravity in Wide Binary Stars: A Revolution in Astrophysics and Cosmology |
