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Relativistic plasma physics in supercritical fields

Publication type
Citation

P. Zhang, S. S. Bulanov, D. Seipt, A. Arefiev, and A. G. R. Thomas, "Relativistic plasma physics in supercritical fields", Phys. Plasmas 27, 050601 (2020).

Abstract

Since the invention of chirped pulse amplification, which was recognized by a Nobel Prize in physics in 2018, there has been a continuing increase in available laser intensity. Combined with advances in our understanding of the kinetics of relativistic plasma, studies of laser–plasma interactions are entering a new regime where the physics of relativistic plasmas is strongly affected by strong-field quantum electrodynamics (QED) processes, including hard photon emission and electron–positron (ee+) pair production. This coupling of quantum emission processes and relativistic collective particle dynamics can result in dramatically new plasma physics phenomena, such as the generation of dense ee+ pair plasma from near vacuum, complete laser energy absorption by QED processes, or the stopping of an ultra-relativistic electron beam, which could penetrate a cm of lead, by a hair's breadth of laser light. In addition to being of fundamental interest, it is crucial to study this new regime to understand the next generation of ultra-high intensity laser-matter experiments and their resulting applications, such as high energy ion, electron, positron, and photon sources for fundamental physics studies, medical radiotherapy, and next generation radiography for homeland security and industry.

Power Scaling for Collimated γ-Ray Beams Generated by Structured Laser-Irradiated Targets and Its Application to Two-Photon Pair Production

Publication type
Citation

T. Wang, X. Ribeyre, Z. Gong, O. Jansen, E. d'Humieres, D. Stutman, T. Toncian, and A. Arefiev, "Power scaling for collimated gamma-ray beams generated by structured laser-irradiated targets and its application to two-photon pair production", Phys. Rev. Applied 13, 054024 (2020).

Abstract

Using three-dimensional kinetic simulations, we examine the emission of collimated γ -ray beams from structured laser-irradiated targets with a prefilled cylindrical channel and its scaling with laser power (in the multi-PW range). The laser power is increased by increasing the laser energy and the size of the focal spot while keeping the peak intensity fixed at 5×1022 W/cm2. The channel radius is increased proportionally to accommodate the change in laser spot size. The efficiency of conversion of the laser energy into a beam of MeV-level γ rays (with a 10o opening angle) increases rapidly with the incident laser power P before it roughly saturates above P ≈ 4 PW. Detailed particle tracking reveals that the power scaling is a result of enhanced electron acceleration at higher laser powers. One application that directly benefits from such a strong scaling is pair production via two-photon collisions. We investigate two schemes for generating pairs through the linear Breit-Wheeler process: colliding two γ-ray beams and colliding one γ-ray beam with black-body radiation. The two scenarios project up to 104 and 105 pairs, respectively, for the γ -ray beams generated at P = 4 PW. A comparison with a regime of laser-irradiated hollow channels corroborates the robustness of the setup with prefilled channels.

Magnetic field generation in a laser-irradiated thin collisionless plasma target by return current electrons carrying orbital angular momentum

Publication type
Citation

Y. Shi, K. Weichman, R. J. Kingham, and A. V. Arefiev, "Magnetic field generation in a laser-irradiated thin collisionless plasma target by return current electrons carrying orbital angular momentum", New J. Phys. 22, 073067 (2020).

Abstract

Magnetized high energy density physics offers new opportunities for observing magnetic field-related physics for the first time in the laser-plasma context. We focus on one such phenomenon, which is the ability of a laser-irradiated magnetized plasma to amplify a seed magnetic field. We performed a series of fully kinetic 3D simulations of magnetic field amplification by a picosecond-scale relativistic laser pulse of intensity 4.2×1018 W/cm2 incident on a thin overdense target. We observe axial magnetic field amplification from an initial 0.1 kT seed to 1.5 kT over a volume of several cubic microns, persisting hundreds of femtoseconds longer than the laser pulse duration. The magnetic field amplification is driven by electrons in the return current gaining favorable orbital angular momentum from the seed magnetic field. This mechanism is robust to laser polarization and delivers order-of-magnitude amplification over a range of simulation parameters.

Birefringence in thermally anisotropic relativistic plasmas and its impact on laser-plasma interactions

Publication type
Citation

A. Arefiev, D. Stark, T. Toncian, and M. Murakami, "Birefringence in thermally anisotropic relativistic plasmas and its impact on laser-plasma interactions", Phys. Plasmas 27, 063106 (2020).

Abstract

One of the paradigm-shifting phenomena triggered in laser–plasma interactions at relativistic intensities is the so-called relativistic transparency. As the electrons become heated by the laser to relativistic energies, the plasma becomes transparent to the laser light even though the plasma density is sufficiently high to reflect the laser pulse in the non-relativistic case. This paper highlights the impact that relativistic transparency can have on laser-matter interactions by focusing on a collective phenomenon that is associated with the onset of relativistic transparency: plasma birefringence in thermally anisotropic relativistic plasmas. The optical properties of such a system become dependent on the polarization of light, and this can serve as the basis for plasma-based optical devices or novel diagnostic capabilities.

Direct laser acceleration of electrons assisted by strong laser-driven azimuthal plasma magnetic fields

Publication type
Citation

Z. Gong, F. Mackenroth, T. Wang, X. Q. Yan, T. Toncian, and A. Arefiev, "Direct laser acceleration of electrons assisted by strong laser-driven azimuthal plasma magnetic fields", Phys. Rev. E 102, 013206 (2020).

Abstract

A high-intensity laser beam propagating through a dense plasma drives a strong current that robustly sustains a strong quasistatic azimuthal magnetic field. The laser field efficiently accelerates electrons in such a field that confines the transverse motion and deflects the electrons in the forward direction. Its advantage is a threshold rather than resonant behavior, accelerating electrons to high energies for sufficiently strong laser-driven currents. We study the electron dynamics via a test-electron model, specifically deriving the corresponding critical current density. We confirm the model’s predictions by numerical simulations, indicating energy gains two orders of magnitude higher than achievable without the magnetic field.

Strong surface magnetic field generation in relativistic short pulse laser-plasma interaction with an applied seed magnetic field

Publication type
Citation

K. Weichman, A. P. L. Robinson, M. Murakami, and A. V. Arefiev, "Strong surface magnetic field generation in relativistic short pulse laser-plasma interaction with an applied seed magnetic field", New J. Phys. 22, 113009 (2020).

Abstract

While plasma often behaves diamagnetically, we demonstrate that the laser irradiation of a thin opaque target with an embedded target-transverse seed magnetic field Bseed can trigger the generation of an order-of-magnitude stronger magnetic field with opposite sign at the target surface. Strong surface field generation occurs when the laser pulse is relativistically intense and results from the currents associated with the cyclotron rotation of laser-heated electrons transiting through the target and the compensating current of cold electrons. We derive a predictive scaling for this surface field generation, Bgen∼−2πBseedΔx/λ0, where Δx is the target thickness and λ0 is the laser wavelength, and conduct 1D and 2D particle-in-cell simulations to confirm its applicability over a wide range of conditions. We additionally demonstrate that both the seed and surface-generated magnetic fields can have a strong impact on application-relevant plasma dynamics, for example substantially altering the overall expansion and ion acceleration from a μm-thick laser-irradiated target with a kilotesla-level seed magnetic field.