A star runs out of fuel and rapidly collapses under its own gravity. According to classical ideas, it collapses into a point of infinite density — a singularity. But what if nature abhors infinities? In models of regular black holes, instead of a singularity, a dense core of unknown matter forms at the center. This matter did not exist in the star initially: it is born right during the collapse.
The authors traced how ordinary stellar matter transforms into a 'patch' for the singularity. They used the Dymnikova–Hayward–Bardeen model and calculated how much energy goes into radiation when new matter is born. It turns out that this process should produce a powerful flash of electromagnetic radiation — exactly like a gamma-ray burst.
But the most intriguing part is the comparison with observations. For the calculated flash to match real gamma-ray bursts, the 'patch' at the center must be very small. So small that from a distance, such a black hole is almost indistinguishable from an ordinary Schwarzschild one. Nature seems to hide its secrets behind nearly perfect camouflage. Thus, the birth of a regular black hole becomes a natural mechanism for gamma-ray bursts, while the holes themselves remain almost exactly as described by Karl Schwarzschild.
The term 'black hole' was coined by journalist Ann Ewing in 1964, although the possibility of such objects was discussed as early as the 18th century.
In the movie 'Interstellar', the characters travel through a wormhole that, like a regular black hole, lacks a destructive singularity.