Astronomers have had good reasons for quite a while to think that shock waves in supernova remnants create cosmic rays. These are charged particles that have been accelerated to very near light-speed; some of them have been boosted to energies far higher than the best particle accelerators can do on Earth.
Yes, according to a new study published today in Science Express (Thursday, June 25th). Expanding supernova remnants could put half or more of their energy into cosmic-ray acceleration, accounting for all the "intermediate-energy" particle Earth receives. No one knew the process was so efficient.
High and very-high energies
Cosmic rays are the highest-energy particles in the universe. At the very highest-end, a single proton can pack as much kinetic energy as a well-served tennis ball (1020 electron-volts). These probably have extragalactic sources related to active galactic nuclei. Much more abundant are particles with millions of times less energy, but still much more than the best accelerators on Earth can impart. These are the ones in the new study, and they likely come from within our galaxy.
Enrico Fermi even described a plausible mechanism in 1949. When a star explodes, says Vink, "the supernova ejecta material goes at a speed much larger than the speed of sound" (pressure waves) in the surrounding interstellar medium. So it forms a shock wave, in which particle density and magnetic field strengths vary wildly. Such a magnetic field can repeatedly send charged particles back and forth behind the shock front, where they can gain momentum -at the expense of the shock wave's speed- until they reach extremely high energies.
The Missing Energy
Three supernovae explode in the Milky Way on average per century. On paper, that's more than enough energy to accelerate all the cosmic rays we see. But is the process efficient enough actually to do it? "The only missing link now was: can they convert this energy into cosmic rays?" says Vink. "The answer seems to be: Yes!"
"At least half the energy of the shock goes into cosmic rays," says lead author Eveline Helder (Astronomical Institute Utrecht, Netherlands). That, anyway, is the case for the part of the ejecta ring that Helder and collaborators studied in the young supernova remnant RCW 86, located 8,200 light-years away. Chinese (and even maybe Roman) records from 185 AD mention a corresponding nine-month-lived star.
The scientists deduced the energy of the shock wave by comparing X-ray images three years apart, taken by NASA's Chandra X-Ray Observatory. The motion of the shock wave between the images amounted to approximately 6,000 km per second, or about 2 percent of the speed of light.
Behind the shock, the scientists found the thin gas to be much less hot than expected: 30 million degrees centigrade instead of half a billion. To measure the temperature of the gas, the scientists used ESO's Very Large Telescope to observe visible light emitted by hydrogen atoms. The width of the hydrogen emission lines, created by the Doppler shift due to the random thermal motion of atoms, told the temperature.
This is more than a simple confirmation of previous results. "It's a much more sophisticated set of measurements," says Luke Drury (IAS Dublin, Ireland). "This one I think will generate much more interest from the community."
The new result confirms that the cosmic-ray production process is remarkably efficient. "Everyone was a bit nervous about saying that, because it seemed so outlandish," says Drury.
This research may also help in understanding similar acceleration processes occurring in gamma-ray bursts and radio jets, says Don Ellison (North Carolina State): "Supernova remnants offer the best laboratory to study the mechanism."
Fonte da notícia: http://www.skyandtelescope.com/news/49089086.html