![Gamma-ray burst [GRB]. Credit: Cruz Dewilde/ NASA SWIFT.](https://nasaspacenews.com/wp-content/uploads/2025/05/gamma-ray-burst-credit-nasa-swift-cruz-dewilde-1-75x75.jpg)
For nearly a century, scientists have been on a relentless hunt for dark matter—an invisible yet dominant force shaping our universe. Despite making up about 27% of the cosmos, it has never been directly observed. It doesn’t emit light, it doesn’t absorb radiation, and it doesn’t interact with ordinary matter in any way we can easily detect.
What Exactly Is Dark Matter, and Why Is It Important?
Dark matter is the unseen glue that holds galaxies together. Without it, our universe would look drastically different. The rotation speeds of galaxies, for instance, suggest that there’s five times more invisible mass than what we can account for with stars, gas, and dust.
Despite all the evidence pointing toward dark matter’s existence, we have yet to detect it directly. Scientists have proposed various candidates for dark matter particles, including Weakly Interacting Massive Particles (WIMPs) and axions. Among them, axionlike particles (ALPs) have emerged as particularly promising candidates due to their ability to interact weakly with electromagnetic fields and their potential role in explaining astrophysical phenomena.
If we can pinpoint what dark matter is made of, we unlock the key to understanding the very fabric of the universe. It would revolutionize physics, much like how the discovery of the Higgs boson reshaped our understanding of particle interactions.
This is why the study from Tokyo Metropolitan University is so crucial—it pushes the limits of our knowledge about ALPs and their potential role in dark matter.
The Hunt for Axionlike Particles (ALPs): A New Frontier in Dark Matter Research
Dark matter detection is notoriously difficult. Since it does not emit any light, scientists have to think outside the box to find it.
One of the most promising approaches is searching for axionlike particles (ALPs), which might decay into photons (light particles) over time.
The study conducted by Tokyo Metropolitan University used advanced infrared spectroscopy and the Magellan Clay Telescope to observe distant galaxies Leo V and Tucana II. Scientists were looking for specific infrared light signals that could result from the decay of ALPs.
ALPs, if they exist, should produce a faint but detectable glow in the infrared spectrum due to their decay. If such a signal is found, it would be a smoking gun for dark matter.
This method represents a novel approach in the search for dark matter, complementing other experimental efforts such as particle colliders and underground detectors.
How Scientists Used Infrared Spectroscopy to Search for Dark Matter
Scientists needed to filter out all possible noise and background signals to ensure they were looking at genuine dark matter interactions.
The team used the WINERED spectrograph on the 6.5-meter Magellan Clay Telescope in Chile to analyze faint infrared signals.
The infrared spectrum is particularly difficult to study because it contains interference from multiple sources:
- Zodiacal light (scattered sunlight from interplanetary dust)
- Atmospheric emissions (light emitted by Earth’s own atmosphere)
- Other cosmic background radiation
By using a sophisticated filtering method, the researchers were able to differentiate potential ALP decay signals from background noise. They analyzed how light from decay processes should behave differently from natural background radiation—essentially isolating a “fingerprint” of potential dark matter interactions.
This technique is one of the most advanced approaches in dark matter detection, leveraging cutting-edge telescope technology to peer deeper into the unknown.
Key Findings: Setting New Records in Dark Matter Research
So, did they find dark matter? Not quite—but their findings set new records in the search.
The study did not detect a definitive ALP signal but set the most stringent limits yet on the possible lifetime of these particles.
The lower bound for the ALP lifetime was estimated to be 10^25 to 10^26 seconds—this is millions to billions of times longer than the age of the universe!
This means that if ALPs exist, they decay at an incredibly slow rate, making them even harder to detect directly. However, this data is crucial because it helps rule out certain theoretical models and narrow down the possible properties of dark matter.
Why Is This Discovery Important?
Beyond just placing constraints on ALPs, this study is a proof of concept for using infrared spectroscopy in dark matter research.
This study proves that infrared spectroscopy can be a powerful tool in the hunt for dark matter.
Traditional searches rely on particle accelerators or underground detectors. This study shows that astronomical observations can provide just as valuable insights into fundamental physics.
By analyzing light from ancient galaxies, we are essentially using the universe itself as a giant dark matter detector.
This opens exciting new avenues for future research, potentially using more advanced instruments like the James Webb Space Telescope (JWST) and future next-generation telescopes.
Conclusion: A Step Closer to the Universe’s Hidden Mass
While dark matter remains elusive, this study represents a significant milestone. We may not have found ALPs yet, but we have placed new limits that refine our understanding of what dark matter can and cannot be.
Reference:
“First Result for Dark Matter Search by WINERED” by Wen Yin, Taiki Bessho, Yuji Ikeda, Hitomi Kobayashi, Daisuke Taniguchi, Hiroaki Sameshima, Noriyuki Matsunaga, Shogo Otsubo, Yuki Sarugaku, Tomomi Takeuchi, Haruki Kato, Satoshi Hamano and Hideyo Kawakita, 7 February 2025, Physical Review Letters.
DOI: 10.1103/PhysRevLett.134.051004
