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Simulated black hole view in front of a large magellanic cloud. | Credit: Alain R, CC by-Sa 2.5
Star black holes are formed by the collapse of massive stars at the end of their lives, usually weighing 3 to 50 times the sunshine. When the star runs out of fuel, it explodes in supernova, leaving such a dense region that no one can escape, not even light.
On the contrary, the primordial black holes are theoretical objects that could have formed less than a second after the Great Bang from the extremely dense early regions of the universe. Unlike the star black holes, they can be much lighter and have been ancient relics since the universe was mostly hydrogen and helium.
The Messier 87 main region image, which lives a supermassive black hole, is processed from a small set of radio telescopes known as the horizon of the event. | Credit: Telescope of events horizon
Although black holes are usually known because they consume everything around them, physicists have long theoretical that they eventually explode at the end of their life through a process called Hawking Radiac. In the past, scientists believed that such explosions had only occurred once every 100,000 years. However, new research published in the Magazine’s Physical Review Letters shows that we can see this extraordinary phenomenon much earlier than expected.
“We believe that in the next 10 years there is 90 percent of the likelihood of witnessing an explosive black hole, the most important thing is that the current park of our space and ground telescopes is already able to detect such an explosion,” said Aidan Symons, a graduate of Massachusetts University.
Black holes, probably exploding, are not the huge remains of the stars we usually think about, and rather the initial black hole (pbhs.) Like the 1970s. Showed by physicist Stephen Hawking, the lighter the black hole is, the hotter and the more particles it emits through the hawk radiation. As the PBH evaporates, they become easier and so hot, with even greater radiation to the explosion.
The breakthrough occurred when the research team began to question the long -considered assumptions of the electrical properties of the black holes. Although the standard black holes do not have an electric charge, the team has investigated what can happen if the primordial black holes formed by a low electrical charge that includes hypothetical heavy particles they call “dark electrons”.
The dark electron would be like a much heavier version of the conventional electron, but interacts through dark electromagnetic forces rather than conventional electromagnetism. In theoretical models called Dark-Qed, these particles would carry a dark electrical charge and interact through dark photons, which can affect how the material behaves around black holes.
Credit: NASA’s Goddard Space Flight Center
The research team made a different prerequisite about the electrical properties of primordial black holes. They postulate that their model shows whether the primeval black holes are formed with a low dark electric charge, it should be temporarily stabilized until finally exploded. This effect of stabilization can significantly increase the likelihood of tracking such explosions once every 100,000 years to possible once every decade.
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The explosive black hole would not only be an impressive light show, but also give scientists a catalog of each existing subatomic particle. This includes not only the particles we discovered like, such as electrons, quarks and Higgs bosons, but also particles, perhaps even dark substances, which are now unnoticed.
The team claims that although they do not guarantee the explosion this decade, there is a good chance that we should be prepared. Fortunately, the current technology of our telescope can already detect signal signs of rider radiation from the explosive primary black hole. If their calculations appear correct, we can explain one of our oldest questions; Where did everything come from?!
Original version This article has been published Universe today;