Write a comment
Black holes and neutron stars are among the densest known objects in the universe. Within and around these environments exist plasmas, the fourth state of matter alongside solids, liquids, and gases. Specifically, these plasmas are known as relativistic electron-positron pair plasmas because they consist of electrons and positrons moving at nearly the speed of light.
While these plasmas ar by Amcen West
Rochester NY (SPX) Jun 17, 2024
Black holes and neutron stars are among the densest known objects in the universe. Within and around these environments exist plasmas, the fourth state of matter alongside solids, liquids, and gases. Specifically, these plasmas are known as relativistic electron-positron pair plasmas because they consist of electrons and positrons moving at nearly the speed of light.
While these plasmas are common in deep space, creating them in a laboratory has been challenging.
An international team of scientists, including researchers from the University of Rochester's Laboratory for Laser Energetics (LLE), has experimentally generated high-density relativistic electron-positron pair-plasma beams by producing two to three orders of magnitude more pairs than previously reported. The team's findings appear in Nature Communications.
The laboratory generation of plasma 'fireballs' composed of matter, antimatter, and photons is a research goal at the forefront of high-energy-density science, says lead author Charles Arrowsmith, a physicist from the University of Oxford who is joining LLE in the fall. But the experimental difficulty of producing electron-positron pairs in sufficiently high numbers has, to this point, limited our understanding to purely theoretical studies.
Rochester researchers Dustin Froula, the division director for plasma and ultrafast laser science and engineering at LLE, and Daniel Haberberger, a staff scientist at LLE, collaborated with Arrowsmith and other scientists to design a novel experiment using the HiRadMat facility at the Super Proton Synchrotron (SPS) accelerator at the European Organization for Nuclear Research (CERN) in Geneva, Switzerland.
That experiment generated extremely high yields of quasi-neutral electron-positron pair beams using more than 100 billion protons from the SPS accelerator. Each proton carries a kinetic energy that is 440 times larger than its resting energy. When the proton collides with an atom, it releases its internal constituents-quarks and gluons-which then recombine to produce a shower that decays into electrons and positrons.
This opens up an entirely new frontier in laboratory astrophysics by making it possible to experimentally probe the microphysics of gamma-ray bursts or blazar jets, Arrowsmith says.
The team has also developed techniques to modify the emittance of pair beams, making it possible to perform controlled studies of plasma interactions in scaled analogues of astrophysical systems.
Satellite and ground telescopes are not able to see the smallest details of those distant objects and so far we could only rely on numerical simulations. Our laboratory work will enable us to test those predictions obtained from very sophisticated calculations and validate how cosmic fireballs are affected by the tenuous interstellar plasma, says coauthor Gianluca Gregori, a professor of physics at the University of Oxford.
Moreover, he adds, The achievement highlights the importance of exchange and collaboration between experimental facilities around the world, especially as they break new ground in accessing increasingly extreme physical regimes.
Research Report:Laboratory realization of relativistic pair-plasma beams
Related Links
University of Rochester
Understanding Time and Space