Dark matter isn’t so cold after all ⚡ экспресс
Scientists have found that dark matter might not be as 'cold' as we thought: imagine it with a gentle negative pressure, like a stretched spring—that new model explains telescope data better. While it doesn't crack the long-standing puzzle of the universe's expansion speed, it drops a hint that dark matter is more intricate than we believed. What other secrets does this enigmatic substance hold?
The enigma of dark matter was already studied by Fritz Zwicky and Vera Rubin. For decades, it was depicted as a cold, listless skeleton that only draws galaxies together. A fresh look at data from supernovae, dark energy, and measurements of the universe’s expansion hints that this skeleton not only holds but also flexes gently, pushing itself apart. This effect—negative pressure—is billions of times weaker than the familiar gravitational attraction of particles, yet it reshapes the notion of dark matter’s passive nature. Researchers emphasize that the finding doesn’t depend on the chosen dark energy model. Maybe the standard cosmological model will soon embrace new physics, even though the mystery of the universe’s differing expansion rates remains unsolved.
🎯 Negative pressure is a minuscule self-repulsion, billions of times weaker than the gravitational pull we're used to.
🎬 Sci-fi writers have long exploited negative pressure for space jumps; now it turns out dark matter itself contains this ingredient, albeit in tiny doses.