VV o n g B a
05-27-2003, 04:07 PM
sounds like a dr. evil plan to take over the world. :lol:
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But there are two major problems with observing the last gasp of a black hole. For one thing, the nearest black holes we know of are light-years away, making accurate measurements of Hawking Radiation nearly impossible. Secondly, black holes take a huge amount of time to evaporate, the time being proportional to their mass. Even relatively small stellar black holes would take longer than the current age of the universe to dissipate, and the monster black holes in the middle of galaxies may be the last things to exist in our universe, taking ten thousand trillion trillion trillion trillion trillion trillion trillion trillion years to die away (sorry, I just have to do that sometimes. That is the actual estimate of how long a massive black hole will last).
So what do you do if you can't wait around that long? For the best chance to observe Hawking Radiation and evaporation, you'd want a black hole that was much closer than naturally occurring black holes, and much less massive. It's a common misconception that you have to have a huge amount of mass to create a black hole. Any amount of mass will do, as long as you cram it into a sufficiently small space. A super-massive black hole with the mass of a billion Suns might be the size of our Solar System, but the Earth could be a black hole too if you packed it into the volume of a marble. Even a person will do, although you'd have to cram them into the space occupied by a single electron.
This line of reasoning has led scientists to the inevitable: If we really want to observe black holes and how they radiate, we'll have to whip them up in our own laboratories. And that's exactly what we are on the threshold of being able to do. Now, there is no kind of technology with the ability to physically crush matter to black hole densities, but there's an easy away around that. Einstein showed us that matter and energy are equivalent, so you can also make a black hole by pushing a huge amount of energy into a tiny volume. For those kinds of experiments, there's an obvious choice: particle accelerators. And the next generation is just about to be unveiled.
Amazingly, scientists are becoming increasingly confident that they will be able to create black holes on demand, in quantity, using the new atom-smashers due to come online in the next five years. Some estimates suggest that the new Large Hadron Collider (LHC) at the European Center for Nuclear Research (CERN -the acronym is in French) will be able to create an average of one black hole each second. LHC will bombard protons and antiprotons together with such a force that the collision will create temperatures and energy densities not seen since the first trillionth of a second after the Big Bang. This should be enough to pop off numerous tiny black holes, with masses of just a few hundred protons. Black holes of this size will evaporate almost instantly, their existence detectable only by dying bursts of Hawking radiation.
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full story (http://www.csmonitor.com/2003/0523/p25s02-stss.html)
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.
.
But there are two major problems with observing the last gasp of a black hole. For one thing, the nearest black holes we know of are light-years away, making accurate measurements of Hawking Radiation nearly impossible. Secondly, black holes take a huge amount of time to evaporate, the time being proportional to their mass. Even relatively small stellar black holes would take longer than the current age of the universe to dissipate, and the monster black holes in the middle of galaxies may be the last things to exist in our universe, taking ten thousand trillion trillion trillion trillion trillion trillion trillion trillion years to die away (sorry, I just have to do that sometimes. That is the actual estimate of how long a massive black hole will last).
So what do you do if you can't wait around that long? For the best chance to observe Hawking Radiation and evaporation, you'd want a black hole that was much closer than naturally occurring black holes, and much less massive. It's a common misconception that you have to have a huge amount of mass to create a black hole. Any amount of mass will do, as long as you cram it into a sufficiently small space. A super-massive black hole with the mass of a billion Suns might be the size of our Solar System, but the Earth could be a black hole too if you packed it into the volume of a marble. Even a person will do, although you'd have to cram them into the space occupied by a single electron.
This line of reasoning has led scientists to the inevitable: If we really want to observe black holes and how they radiate, we'll have to whip them up in our own laboratories. And that's exactly what we are on the threshold of being able to do. Now, there is no kind of technology with the ability to physically crush matter to black hole densities, but there's an easy away around that. Einstein showed us that matter and energy are equivalent, so you can also make a black hole by pushing a huge amount of energy into a tiny volume. For those kinds of experiments, there's an obvious choice: particle accelerators. And the next generation is just about to be unveiled.
Amazingly, scientists are becoming increasingly confident that they will be able to create black holes on demand, in quantity, using the new atom-smashers due to come online in the next five years. Some estimates suggest that the new Large Hadron Collider (LHC) at the European Center for Nuclear Research (CERN -the acronym is in French) will be able to create an average of one black hole each second. LHC will bombard protons and antiprotons together with such a force that the collision will create temperatures and energy densities not seen since the first trillionth of a second after the Big Bang. This should be enough to pop off numerous tiny black holes, with masses of just a few hundred protons. Black holes of this size will evaporate almost instantly, their existence detectable only by dying bursts of Hawking radiation.
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full story (http://www.csmonitor.com/2003/0523/p25s02-stss.html)