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Laser scaling for generation of megatesla magnetic fields by microtube implosions

Published online by Cambridge University Press:  14 October 2021

D. Shokov
Affiliation:
Graduate School of Engineering, Osaka University, Suita, Osaka 565-0875, Japan Institute of Laser Engineering, Osaka University, Suita, Osaka 565-0871, Japan
M. Murakami*
Affiliation:
Institute of Laser Engineering, Osaka University, Suita, Osaka 565-0871, Japan
J. J. Honrubia
Affiliation:
ETSI Aeronáutica y del Espacio, Universidad Politécnica de Madrid, 28040 Madrid, Spain
*
Correspondence to: M. Murakami, Institute of Laser Engineering, Osaka University, Suita, Osaka 565-0871, Japan. Email: murakami-m@ile.osaka-u.ac.jp

Abstract

Microtube implosions are a novel scheme to generate ultrahigh magnetic fields of the megatesla order. These implosions are driven by ultraintense and ultrashort laser pulses. Using two- and three-dimensional particle simulations where megatesla-order magnetic fields can be achieved, we demonstrate scaling and criteria in terms of laser parameters, such as laser intensity and laser energy, to facilitate practical experiments toward the realization of extreme physical conditions, which have yet to be realized in laboratories. Microtube implosions should provide a new platform for studies in fundamental and applied physics relevant to ultrahigh magnetic fields.

Information

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2021. Published by Cambridge University Press in association with Chinese Laser Press
Figure 0

Figure 1 Illustration of a microtube implosion. Due to the laser-produced hot electrons with megaelectron volt energies, cold ions in the inner wall surface implode toward the central axis. By pre-seeding uniform magnetic fields of the kilotesla order, the Lorentz force induces a Larmor gyromotion of the imploding ions and electrons. Due to the resultant collective motion of relativistic charged particles around the central axis, strong spin currents of approximately peta-ampere/cm${}^2$ are produced with a few tens of nm size, generating megatesla-order magnetic fields.

Figure 1

Figure 2 Perspective views of the normalized ion density ${n}_{\mathrm{i}}/{n}_{\mathrm{i}0}$ and the $z$-component of the magnetic field ${B}_{{z}}$, respectively, observed at $t\sim 200$ fs, which is obtained by a 3D EPOCH simulation. A cubic aluminum target with a size of $14\ \unicode{x3bc}\text{m}\times 14\ \unicode{x3bc}\text{m}\times 14\ \unicode{x3bc}\text{m}$ is set at the center, which has a cylindrical cavity with a radius of ${R}_0=5\kern0.1em$ μm and an axis overlapping the $z$-axis. The seed magnetic field ${B}_0=6$ kT parallel to the $z$-axis is uniformly set over the entire domain. The four faces of the target parallel to the $z$-axis are normally irradiated by uniform laser pulses simultaneously, which are characterized by ${\lambda}_{\mathrm{L}}=0.8\kern0.1em$ μm, ${I}_{\mathrm{L}}=3\times {10}^{21}$ W cm${}^{-2}$ and ${\tau}_{\mathrm{L}}=50$ fs.

Figure 2

Figure 3 Temporal evolution of the central magnetic field, obtained from 2D EPOCH simulations, under four different laser intensities ${I}_{\mathrm{L}}$, which are labelled and applied to an aluminum target (${n}_{\mathrm{i}0}=5\times {10}^{22}$ cm${}^{-3}$, $A=27$ and $Z=13$). Other fixed parameters are ${R}_0=5\kern0.1em$ μm, ${D}_0=14\kern0.1em$ μm, ${\lambda}_{\mathrm{L}}=0.8\kern0.1em$ μm, ${\tau}_{\mathrm{L}}=50$ fs and ${B}_0=6$ kT. The target is assumed to be uniformly irradiated on the four sides. The laser peak time is $t=75$ fs. The four highlighted circles on the green curve correspond to the sampling times for the 2D patterns given in Figure 4.

Figure 3

Figure 4 Snapshots of the 2D patterns for the magnetic field (upper row), the total current vectors (middle row) and the electron density (lower row) normalized by the initial value (${n}_{\mathrm{e}0}={Zn}_{\mathrm{i}0}=6.5\times {10}^{23}$ cm${}^{-3}$), corresponding to the four highlighted times on the green curve in Figure 3 (${I}_{\mathrm{L}}=3.0\times {10}^{21}$ W/cm${}^2$). Generated magnetic fields are assumed to be positive if they are in the same direction as the seed magnetic field (${B}_0=6$ kT). Just after the collapse of the microtube cavity at around $t=130$ fs, the spin-structured plasma flow due to the seed magnetic field is formed, increasing the magnetic strength, as observed in the current patterns.

Figure 4

Figure 5 Scaling for ${B}_{\mathrm{max}}$, ${P}_{\mathrm{L}}$ and ${E}_{\mathrm{L}}$ in terms of ${I}_{\mathrm{L}}$. A square target is used with parameters ${R}_0=5\kern0.1em$ μm and ${D}_0=14\kern0.1em$ μm. The laser is assumed to uniformly irradiate the four target surfaces. The fixed parameters for the 2D simulations are ${\lambda}_{\mathrm{L}}=0.8\kern0.1em$ μm, ${\tau}_{\mathrm{L}}=50$ ps and ${B}_0=6$ kT. Yellow shading denotes the model prediction, which is given in Equation (4), and the two bounding dashed curves correspond to the minimum and maximum laser absorption efficiencies ($0.1\lesssim {\eta}_0\lesssim 0.8$) in Equation (3). To draw the model curve for ${P}_{\mathrm{L}}$ and ${E}_{\mathrm{L}}$, an optimized aspect ratio $1\lesssim {L}_0/{R}_0\lesssim 2$ is postulated.