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10$^4$-fold amplification of a tiny magnetic field to megagauss scale in femtosecond, ultraintense laser-solid interaction
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abstract
Generating a powerful and quasistatic magnetic field within the confines of a tabletop laboratory experiment has proven to be a persistent challenge. The creation of magnetized high-energy-density plasma through such experiments presents significant opportunities for exploring several terrestrial as well as astrophysical phenomena, apart from controlling relativistic electron transport, directly relevant for fusion schemes. Here we demonstrate that the modest magnetic field (10$^{-3}$ megagauss ) in a common, readily available Neodymium magnet is amplified to 10's of megagauss levels lasting a few picoseconds, when excited by an ultraintense, femtosecond laser pulse. The experimental findings are strongly supported by particle-in-cell simulations, which not only validate the observations but also unveil a potential dynamo mechanism responsible for the enhancement and amplification of the axial magnetic field. These outcomes are of utmost importance in comprehending the intricacies of relativistic electron transport and the realm of magnetized laboratory astrophysics.
Forward citations
Cited by 3 Pith papers
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Quasi mono-energetic, relativistic electron acceleration in a femtosecond, high intensity laser excited solid magnet
Magnetized overdense laser-plasma interaction excites electron Bernstein waves whose Landau damping yields tunable ~2 MeV quasi-monoenergetic electrons at a claimed 3.6 MeV/μm gradient.
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Universal energy cascade and relaxation in three-dimensional inertial electron magnetohydrodynamic turbulence
An exact energy cascade relation for 3D inertial EMHD turbulence is derived and numerically verified, with a universal flux across the electron inertial length and a pressure-balanced relaxation state.
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Observation of poloidal magnetic flux emission from a low-pressure spark: validation of the hypothesis of constrained plasma dynamics?
A spark emits poloidal magnetic flux in transients near current zeroes, tentatively supporting the authors' electron-inertia constrained-dynamics hypothesis.
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