Giant collimated gamma-ray flashes

被引:56
作者
Benedetti, Alberto [1 ]
Tamburini, Matteo [1 ]
Keitel, Christoph H. [1 ]
机构
[1] Max Planck Inst Kernphys, Heidelberg, Germany
关键词
RELATIVISTIC ELECTRON-BEAMS; FILAMENTATION INSTABILITY; PAIR PRODUCTION; BREMSSTRAHLUNG; PLASMA; EVOLUTION;
D O I
10.1038/s41566-018-0139-y
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Bright sources of high-energy electromagnetic radiation are widely employed in fundamental research, industry and medicine(1,2). This motivated the construction of Compton-based facilities planned to yield bright gamma-ray pulses with energies up to(3) 20 MeV. Here, we demonstrate a novel mechanism based on the strongly amplified synchrotron emission that occurs when a sufficiently dense ultra-relativistic electron beam interacts with a millimetre-thickness conductor. For electron beam densities exceeding approximately 3 x 101(9) cm(-3), electromagnetic instabilities occur, and the ultra-relativistic electrons travel through self-generated electromagnetic fields as large as 10(7)-10(8) gauss. This results in the production of a collimated gamma-ray pulse with peak brilliance above 10(25) photons s(-1) mrad(-2) mm(-2) per 0.1% bandwidth, photon energies ranging from 200 keV to gigaelectron-volts and up to 60% electron-to-photon energy conversion efficiency. These findings pave the way to compact, high-repetition-rate (kilohertz) sources of short (less than or similar to 30 fs), collimated (milliradian) and high-flux (> 10(12) photons s(-1)) gamma-ray pulses.
引用
收藏
页码:319 / +
页数:7
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