Gravitational waves show black holes prefer certain masses before they collide

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Gravitational waves show black holes prefer certain masses before they collide
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Keith Cooper is a freelance science journalist and editor in the United Kingdom, and has a degree in physics and astrophysics from the University of Manchester. He's the author of 'The Contact Paradox: Challenging Our Assumptions in the Search for Extraterrestrial Intelligence' (Bloomsbury Sigma, 2020) and has written articles on astronomy, space, physics and astrobiology for a multitude of magazines and websites.

, in other cases there is no explosion. Instead, the star's core collapses under gravity so severely it forms a black hole that eventually causes the rest of the star to cave in around it.

"What our study shows is that there is always a gap in black-hole masses between 9 and 16 solar masses,” Schneider told Space.com.The existence of the mass gap is dictated by what is happening inside a massive star as it nears the end of its life. processes; in massive stars, the dominant version of this process is known as the carbon–nitrogen–oxygen cycle.

An illustration of gravitational waves being emitted by binary black holes spiraling towards a merger In a binary system, this can lead to two black holes that eventually merge with a chirp of gravitational waves.

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