activity
20042024
most citedRadiation Pressure Dominate Regime of Relativistic Ion Acceleration

1k citations · 2k across the 27 of their papers we have counts for

collaborators

27 papers

physics.plasm-ph2024

Weibel- and non-resonant Whistler wave growth in an expanding plasma in a 1D simulation geometry

M E Dieckmann, L Palodhi, C Fegan +1

Ablating a target with an ultraintense laser pulse can create a cloud of collisionless plasma. A density ramp forms, in which the plasma density decreases and the ion's mean speed…

physics.plasm-ph2022

Optimizing laser coupling, matter heating, and particle acceleration from solids using multiplexed ultraintense lasers

Weipeng Yao, Motoaki Nakatsutsumi, Sébastien Buffechoux +20

Realizing the full potential of ultrahigh-intensity lasers for particle and radiation generation will require multi-beam arrangements due to technology limitations. Here, we invest…

physics.acc-ph2018★ 26 cited

A new energy spectrum reconstruction method for Time-Of-Flight diagnostics of high-energy laser-driven protons

G. Milluzzo, V. Scuderi, A. Alejo +20

The Time-of-Flight (ToF) technique coupled with semiconductor-like detectors, as silicon carbide and diamond, is one of the most promising diagnostic methods for high-energy, high…

physics.plasm-ph2018★ 14 cited

Expansion of a radially symmetric blast shell into a uniformly magnetized plasma

M E Dieckmann, Q Moreno, D Doria +7

The expansion of a thermal pressure-driven radial blast shell into a dilute ambient plasma is examined with two-dimensional PIC simulations. The purpose is to determine if laminar…

physics.plasm-ph2017

Expansion of a radial plasma blast shell into an ambient plasma

M E Dieckmann, D Doria, H Ahmed +6

The expansion of a radial blast shell into an ambient plasma is modeled with a particle-in-cell (PIC) simulation. The unmagnetized plasma consists of electrons and protons. The for…

astro-ph.SR2017★ 2 cited

Laboratory unravelling of matter accretion in young stars

G. Revet, S. N. Chen, R. Bonito +22

Accretion dynamics in the forming of young stars is still object of debate because of limitations in observations and modelling. Through scaled laboratory experiments of collimated…