Dark matter is aptly named. It emits no light and interacts with visible matter only via gravity. But dark matter might be only the tip of an invisible universe of unknown forces. This possibility has led to a hunt for “dark photons.” Such photons are analogous to ordinary photons, but they are exchanged among particles of dark matter, and according to some models, they may have mass.
Now, reports Phys.org, A team of researchers from the University of California and Lawrence Berkeley National Laboratory has conducted an ultra-precise measurement of the fine-structure constant, and in so doing, have found evidence that casts doubts on dark photon theory. In their paper published in the journal Science, the group describes their measurement process and what they found by using it.
The fine-structure constant is a number that represents the force of electromagnetic interactions between charged particles, such as those that are involved in keeping electrons from traveling outside of their atoms. Up until now, it has been derived using the magnetic properties of electrons and calculations that are still considered to be theoretical. As the researchers note, more precise measurements allow for testing the Standard Model of particle physics. To that end, they sought to measure the constant through more direct means.
To accomplish this feat, they aimed a laser at cesium-133 atoms (matter-wave interferometry) to force them into quantum superposition and then took a close look at what happened between them as they relaxed back to their natural state. The interference that occurred, the team reports, revealed the speed at which the atoms traveled when they were struck by the laser—they used that number to calculate the fine-structure constant. They claim their work has allowed for calculating the fine-structure constant to better than one part per billion.
The researchers report that the number they calculated was closely matched the theory, which offers some confirmation of theories that suggest electrons are not made up of smaller, unknown particles. But it also casts doubt on theories surrounding the existence of dark photons. On the bright side, because the number they calculated was close to that theorized, but not exact, there is still room for other particle theories to explain the discrepancy.
The image above shows a dwarf galaxy forming when the Universe was half its current age. The dark matter is in red, the stars in yellow and the gas in blue. Galaxy formation occurs along dark matter filaments, and is a violent process of merging of gas clouds, spawning stars deep within their sheltered cores. (Bourke, Crain and Duffy)
The Daily Galaxy via Physics and Phys.org