) The greatest idea of Stephen Hawking’s scientific career truly revolutionized the way we think about black holes. After all, they weren’t exactly black, and it was indeed Hawking who first understood and predicted the radiation they were supposed to emit: Hawking radiation. He arrived at this result in 1974, and it is one of the deepest links between the quantum world and our theory of gravity, Einstein’s general theory of relativity. However, in his landmark 1988 book A Brief History of Time, Hawking painted a picture of this radiation – A spontaneously created particle-antiparticle pair in which one member falls and the other escapes – this is very incorrect. For 32 years, it has been misleading physics students, laymen, and even professionals. Black holes do decay. Let’s see how they do it today.
Event Horizon Telescope Collaboration, etc.
What Hawking wants us to imagine is a relatively simple picture. Start with a black hole: a region of space where so much mass is concentrated into such a small volume that not even light can escape. Anything too close to it will inevitably be pulled into the central singularity, the boundary between the escapeable and non-escapable regions known as the event horizon.
- Each quanta of emitted radiation must have enormous energy: enough energy from Almost, , but not quite, was swallowed by a black hole.
Of course, none of these three points are true. Hawking radiation consists almost entirely of photons, rather than a mixture of particles and antiparticles. It emanated from a large area beyond the event horizon, not at the surface. And the single quanta emitted have tiny energies over a considerable range.
This is The key point behind Hawking radiation, Stephen Hawking himself knew. In 1974, when he first deduced the famous Hawking radiation, he performed the following calculation: Calculate the difference in zero-point energy in a quantum field from curved space around a black hole to infinitely far flat space.
The results of this calculation determine the properties of the radiation emitted from the black hole: not exactly from the event horizon, but from around it of the entire bending space. It tells us the temperature of the radiation, which depends on the mass of the black hole. It tells us the spectrum of radiation: a perfect black body, indicating the energy distribution of the photons, and – if enough energy passes through E=mc² – so are massive particles and antiparticles.
NASA; DANA BERRY, SKYWORKS DIGITAL, INC.
It also allows us to calculate an important detail that is often not understood: where the radiation from a black hole is coming from. While most pictures and visualizations show that 100% of a black hole’s Hawking radiation is emitted from the event horizon itself, it is more accurate to describe it as emitting d at a distance spanning approximately 10-20 Schwarzschild radii (radius to the event horizon) Volumetrically, the radiation decreases gradually with increasing distance. This leads us to a surprising conclusion: all collapsing objects that bend spacetime should emit Hawking radiation. It could be the tiny, imperceptible Hawking radiation that, to the extent we can count, is overwhelmed by thermal radiation even in long-dead white dwarfs and neutron stars. But it’s still there: it’s a computable, non-zero positive value that depends only on the object’s mass, spin, and physical dimensions.
NASA
Hawking The main problem with his interpretation of his theory is that he takes a computational tool — the concept of virtual particles — and treats that tool as equivalent to physical reality. In effect, the curved space around a black hole is constantly emitting radiation due to the curvature gradient around it, and the energy comes from the black hole itself, causing its event horizon to slowly contract over time.
The black hole did not decay because a virtual particle with negative energy fell; this is Hawking’s inadequacy to “save” him Another fantasy designed by analogy. Instead, the black hole is decaying and losing mass over time as the energy emitted by this Hawking radiation is slowly reducing the curvature of space in the region. Once enough time has passed, and the duration is enormous for realistic black holes, they evaporate completely.
Derek B. Leinweber In the context of quantum field theory, the lowest energy state of a quantum field corresponds to the absence of particles. But excited states, or states that correspond to higher energies, correspond to particles or antiparticles. A common method of visualization is to think of empty space as truly empty, but filled by particle-antiparticle pairs (due to conservation laws) that briefly pop up, but annihilate back into the void of nothingness shortly after.
Ulf Leonhardt / University of St Andrews
This is the first explanation I’ve heard myself as a theoretical astrophysicist about how black holes decay. If this explanation were true, then this would mean:
Hawking radiation consists of a 50/50 mix of particles and antiparticles, since which member falls and which escapes will be random,
- All Hawking The radiation, which causes the black hole to decay, will be emitted from the event horizon itself, and