Strong Radiation Emission from Plasma Dipole Oscillation
ORAL
Abstract
The plasma oscillation and Langmuir wave are usually regarded as non-radiating, because their electrostatic, curl-free nature of the electric field prohibits its coupling with the electromagnetic wave in plasma. However, in a non-uniform plasma, the plasma oscillation can take on a non-zero component of the curl of the electric field, leading to the emission of electromagnetic radiation by mechanisms of mode conversion or travelling wave antennae. These mechanisms, in non-uniform plasmas, inevitably yield broadband emission spectra. In contrast, we conceived a novel method of obtaining quasi-narrowband radiation from a localized plasma dipole oscillation, which is generated by colliding, detuned laser pulses in plasma. The radiation exhibits a quasi-narrowband peak around the plasma frequency, typically a few THz, which should yield diverse novel applications where strong terahertz fields are required for pump-probe studies of materials. Furthermore, we show that the field emitted from a plasma oscillation immersed in uniform plasma can transport its energy through the uniform plasma over a large distance without significant decay, in contradiction with the common wisdom of radiation cut-off in ambient plasma. The new discovery may be pertinent to solar radio bursts.
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Presenters
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Min Sup Hur
UNIST
Authors
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Min Sup Hur
UNIST
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Teyoun Kang
UNIST, Ulsan Natl Inst of Sci & Tech
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Bernhard Ersfeld
Univ. Strathclyde
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Dino Jaroszynski
Univ. Strathclyde
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Kenan Qu
Princeton Univ/PPPL, Department of Astrophysical Science, Princeton University
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Nathaniel J Fisch
Princeton Plasma Phys Lab, Princeton Univ, Princeton Univ/PPPL, Princeton Plasma Phys Lab, Department of Astrophysical Science, Princeton University, Princeton Plasma Phys Lab, Princeton University, Princeton Univ, PPPL, Princeton Plasma Physics Laboratory, Princeton Plasma Phys Lab, Department of Astrophysical Sciences, Princeton University, USA, Princeton Plasma Physics Lab, Princeton University