A new breakthrough in cosmic mapping has unveiled the structure of a colossal filament, part of the vast cosmic web that connects galaxies.
Dark matter and gas shape these filaments, but their faint glow makes them hard to detect. By using advanced telescope technology and hundreds of hours of observation, astronomers have captured the most detailed image yet, bringing us closer to decoding the evolution of galaxies and the hidden forces shaping the universe.
The hidden order of the universe.
A new adaptive optics technology is set to transform gravitational-wave detection, allowing LIGO
LIGO, or the Laser Interferometer Gravitational-Wave Observatory, is a large-scale physics experiment and observatory to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. There are two LIGO observatories in the United States—one in Hanford, Washington, and the other in Livingston, Louisiana. These observatories use laser interferometry to measure the minute ripples in spacetime caused by passing gravitational waves from cosmic events, such as the collisions of black holes or neutron stars.
Ever since physicist Ernest Rutherford discovered the atomic nucleus in 1911, studying its structure and behavior has remained a challenging task. More than a century later, even with today’s high-tech tools for researching nuclear physics, mysteries of the universe abound.
Relying on leading-edge germanium detectors developed by researchers at the Department of Energy’s Oak Ridge National Laboratory, the scientific community pursues elusive nuclear processes to unlock persistent mysteries. Answers to questions they hope to resolve hold the potential to redefine the universe itself. Why does the universe contain more matter than antimatter? Can a particle be both a matter and antimatter version of itself? Is there a mismatch between what the Big Bang produced and what the Standard Model of particle physics suggests?
Long at the vanguard of international efforts to answer questions like these, ORNL’s contributions remain strong today. David Radford, head of the lab’s Fundamental Nuclear and Particle Physics section, is an internationally renowned expert in the field who has had an indelible impact on the development of germanium detectors. Vital experimentation tools at the forefront of fundamental physics research, germanium detectors are large, single crystals of germanium—a metallic element—used to detect radiation and enable incredibly precise energy measurements.
For the study, the researchers used NASA’s powerful James Webb Space Telescope to observe Sagittarius A* to better understand its activity. After conducting several observations between 2023 and 2024, the researchers found that Sagittarius A* exhibited near-endless flare activity, ranging from faint flashes lasting a few seconds to massive eruptions occurring every day. Since Sagittarius A* interacts with the massive disk of gas and dust that comprises our galaxy, these results could help researchers better understand the formation and evolution of supermassive black holes throughout the universe.
“Flares are expected to happen in essentially all supermassive black holes, but our black hole is unique,” said Dr. Farhad Yusef-Zadeh, who is a professor at northwestern University and lead author of the study. “It is always bubbling with activity and never seems to reach a steady state. We observed the black hole multiple times throughout 2023 and 2024, and we noticed changes in every observation. We saw something different each time, which is really remarkable. Nothing ever stayed the same.”
2.4 billion years from now there will be a black hole colliding with the Milky Way.
A supermassive black hole hidden in the Large Magellanic Cloud is on a collision course with the Milky Way! Scientists discovered it using hypervelocity stars, and in 2.4 billion years, it will merge with Sagittarius A at our galaxy’s center. This event could reshape our galaxy and trigger gravitational waves! 🌌 Want to know what happens next? Watch the full video to explore the science behind this cosmic collision. Don’t miss it—subscribe now for more space discoveries! 🚀
Paper link: https://arxiv.org/abs/2502.
Researchers have announced results from a new search at the European X-ray Free Electron Laser (European XFEL) Facility at Hamburg for a hypothetical particle that may make up the dark matter of the universe. The experiment is described in a study published in Physical Review Letters.
This experiment looks for axions, a particle which was proposed to solve a major problem in particle physics: why neutrons, although composed of smaller charged particles called quarks, do not possess an electric dipole moment. To explain this, it was suggested that axions, tiny and incredibly light particles, can “cancel out” this imbalance. If observed, this process would provide direct evidence for new physics beyond the Standard Model.
Additionally, axions turn out to be a natural candidate for dark matter, the mysterious substance that constitutes most of the structure of the universe.
New research suggests that dark energy isn’t needed to explain the acceleration in the expansion of the universe — instead suggesting giant voids in space are creating an illusion.
Researchers found for the first time evidence that even microquasars containing a low-mass star are efficient particle accelerators, which leads to a significant impact on the interpretation of the abundance of gamma rays in the universe.
Our home planet is bombarded with particles from outer space all the time. And while we are mostly familiar with the rocky meteorites originating from within our solar system that create fascinating shooting stars in the night sky, it’s the smallest particles that help scientists to understand the nature of the universe. Subatomic particles such as electrons or protons arriving from interstellar space and beyond are one of the fastest particles known in the universe and known as cosmic rays.
The origins and the acceleration mechanisms of the most energetic of these cosmic particles remains one of the biggest mysteries in astrophysics. Fast-moving matter outflows (or “jets”) launched from black holes would be an ideal site for particle acceleration, but the details on how and under which conditions acceleration processes can occur are unclear. The most powerful jets inside our Galaxy occur in microquasars: systems composed by a stellar-mass black hole and a “normal” star. The pair orbit each other, and, once they are close enough, the black hole starts to slowly swallow its companion. As a consequence of this, jets are launched from the region close to the black hole.
You may think that time started 13.8 billion years ago at the birth of the universe, but physicists with alternative definitions of time have other ideas.
