A recent experiment has shown that the assumption about the X-ray spectra of black holes contradicts the Sandy Z indicators.
Z - the most energetic laboratory x-ray source on the planet. It is able to recreate the radiation around black holes. Of course, we cannot observe the emission itself near real black holes. But we see radiation before material is absorbed - an accretion disk.
The results showed that it is necessary to change the usual patterns. A black hole is an area in space, from which no single particle can escape from gravity. Its gravitational field is extremely intense.
It turns out that we will have to redo the scientific articles that have been promoting the well-known model for more than 20 years. The test shows how fast black holes absorb matter. Many scholars agree with the conclusions and are ready to reconsider entrenched views. The problem was that plasmas in black holes have an exotic nature, and theoretical models have not previously been tested under laboratory conditions.
Reality crowds out theory
It is worth noting that the prerequisites for discrepancy began two decades ago. Then physicists reported that the accretion disks of holes have iron ionization steps, although spectral lines did not indicate their existence. The theory explained this by the fact that with powerful gravity the electrons of iron did not return to a lower energy state.
Guillaume Loisel on the background of Sandia Z machine, where practical experiments did not coincide with the long-held assumption about the X-ray spectra of black holes
But research in Z showed that if photons do not appear, there is simply no generating element. To clarify, we conducted 5 experiments, and all displayed one result. Although black holes are extremely compact formations, their accretion disks are relatively blurred. In Z it was possible to expand silicon 50,000 times.
Fairy tale with spectra
The reason for the error is the lack of observations. Black holes were mentioned by Einstein, but were considered only a mathematical concept. Later, scientists were able to note their influence on neighboring objects during absorption, as well as their collisions. But they were small and located at a great distance, because of which it was impossible to conduct a detailed review.
Spectra are important because they guarantee a huge information array. If it were possible to analyze the accretion disk in the laboratory, then we could decipher the composition. But this is impossible, so you have to rely on models.
The error could arise due to the fact that black holes change spectral lines, because photons hardly leave the intense gravitational field. Now they are trying to create more sophisticated models that will display the real picture.
