Out there among the stars lies a hidden swarm of black holes. They have been around ever since the dawn of time, quietly and not so subtly influencing the evolution of the universe. Without them, there would be no stars, no planets, and no life to marvel at the universe's wonders. Now, for the first time, we may finally have the tools to find them. Black holes are one of astronomy's most famous objects. Their gravity is so extreme that escape is impossible if you venture too close. There are different sizes of black holes, but they are normally gargantuan monsters considerably more massive than our own sun. They usually remain hidden from view because no light can escape to reveal them to us.
Yet we have seen them, thanks to gravitational wave detectors like LIGO and VIRGO that have detected signals from colliding black holes. We've never been more confident that these cosmic trapdoors exist.
However, there is one type of black hole that still remains theoretical - one that could solve a longstanding cosmological conundrum to boot.
Immediately after the Big Bang, there were small fluctuations in the new universe's density - regions that had slightly more or less mass than the average. Where the mass was above the norm, the material could have collapsed to form mini black holes. As they've been around for pretty much as long as the universe itself, these black holes are called 'primordial' black holes.
According to theoretical models, primordial black holes can have a wide range of masses. They could be lighter than an eyelash or heavier than a star. So far, we've been able to rule out some masses through observations, opening up two possible mass ranges or 'windows' for primordial black holes.
この記事は Very Interesting の March/April 2022 版に掲載されています。
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7 日間の Magzter GOLD 無料トライアルを開始して、何千もの厳選されたプレミアム ストーリー、9,000 以上の雑誌や新聞にアクセスしてください。
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