Gianluca Sarri
Queen's University Belfast
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Publication
Featured researches published by Gianluca Sarri.
Physical Review Letters | 2012
S. Kar; K. F. Kakolee; B. Qiao; Andrea Macchi; M. Cerchez; D. Doria; Michael Geissler; P. McKenna; D. Neely; J. Osterholz; R. Prasad; K. Quinn; B. Ramakrishna; Gianluca Sarri; O. Willi; X. Y. Yuan; M. Zepf; M. Borghesi
The acceleration of ions from ultrathin foils has been investigated by using 250 TW, subpicosecond laser pulses, focused to intensities of up to 3 × 10(20) W cm(-2). The ion spectra show the appearance of narrow-band features for protons and carbon ions peaked at higher energies (in the 5-10 MeV/nucleon range) and with significantly higher flux than previously reported. The spectral features and their scaling with laser and target parameters provide evidence of a multispecies scenario of radiation pressure acceleration in the light sail mode, as confirmed by analytical estimates and 2D particle-in-cell simulations. The scaling indicates that monoenergetic peaks with more than 100 MeV/nucleon are obtainable with moderate improvements of the target and laser characteristics, which are within reach of ongoing technical developments.
Nature Communications | 2015
Gianluca Sarri; K. Poder; J. M. Cole; W. Schumaker; A. Di Piazza; Brian Reville; T. Dzelzainis; D. Doria; L. A. Gizzi; G. Grittani; S. Kar; Christoph H. Keitel; K. Krushelnick; S. Kuschel; S. P. D. Mangles; Z. Najmudin; N. Shukla; L. O. Silva; D. R. Symes; A. G. R. Thomas; M. Vargas; Jorge Vieira; M. Zepf
Electron–positron pair plasmas represent a unique state of matter, whereby there exists an intrinsic and complete symmetry between negatively charged (matter) and positively charged (antimatter) particles. These plasmas play a fundamental role in the dynamics of ultra-massive astrophysical objects and are believed to be associated with the emission of ultra-bright gamma-ray bursts. Despite extensive theoretical modelling, our knowledge of this state of matter is still speculative, owing to the extreme difficulty in recreating neutral matter–antimatter plasmas in the laboratory. Here we show that, by using a compact laser-driven setup, ion-free electron–positron plasmas with unique characteristics can be produced. Their charge neutrality (same amount of matter and antimatter), high-density and small divergence finally open up the possibility of studying electron–positron plasmas in controlled laboratory experiments.
Physical Review Letters | 2013
Gianluca Sarri; W. Schumaker; A. Di Piazza; M. Vargas; B. Dromey; Mark E Dieckmann; V. Chvykov; Anatoly Maksimchuk; V. Yanovsky; Zhaohan He; B. Hou; John A. Nees; A. G. R. Thomas; Christoph H. Keitel; M. Zepf; K. Krushelnick
The generation of ultrarelativistic positron beams with short duration (τ(e+) ≃ 30 fs), small divergence (θ(e+) ≃ 3 mrad), and high density (n(e+) ≃ 10(14)-10(15) cm(-3)) from a fully optical setup is reported. The detected positron beam propagates with a high-density electron beam and γ rays of similar spectral shape and peak energy, thus closely resembling the structure of an astrophysical leptonic jet. It is envisaged that this experimental evidence, besides the intrinsic relevance to laser-driven particle acceleration, may open the pathway for the small-scale study of astrophysical leptonic jets in the laboratory.
Physics of Plasmas | 2012
Sharmin Sultana; Gianluca Sarri; Ioannis Kourakis
The propagation of ion acoustic shocks in nonthermal plasmas is investigated, both analytically and numerically. An unmagnetized collisionless electron-ion plasma is considered, featuring a superthermal (non-Maxwellian) electron distribution, which is modeled by a κ-(kappa) distribution function. Adopting a multiscale approach, it is shown that the dynamics of low-amplitude shocks is modeled by a hybrid Korteweg-de Vries–Burgers (KdVB) equation, in which the nonlinear and dispersion coefficients are functions of the κ parameter, while the dissipative coefficient is a linear function of the ion viscosity. All relevant shock parameters are shown to depend on κ: higher deviations from a pure Maxwellian behavior induce shocks which are narrower, faster, and of larger amplitude. The stability profile of the kink-shaped solutions of the KdVB equation against external perturbations is investigated. The spatial profile of the shocks is found to depend upon the dispersion and the dissipation term, and the role of ...
Physical Review Letters | 2012
Gianluca Sarri; Andrea Macchi; C. A. Cecchetti; S. Kar; T. V. Liseykina; X. H. Yang; Mark E Dieckmann; J. Fuchs; M. Galimberti; L. A. Gizzi; R. Jung; Ioannis Kourakis; J. Osterholz; Francesco Pegoraro; A. P. L. Robinson; L. Romagnani; O. Willi; M. Borghesi
The dynamics of magnetic fields with an amplitude of several tens of megagauss, generated at both sides of a solid target irradiated with a high-intensity (~10(19) W/cm(2)) picosecond laser pulse, has been spatially and temporally resolved using a proton imaging technique. The amplitude of the magnetic fields is sufficiently large to have a constraining effect on the radial expansion of the plasma sheath at the target surfaces. These results, supported by numerical simulations and simple analytical modeling, may have implications for ion acceleration driven by the plasma sheath at the rear side of the target as well as for the laboratory study of self-collimated high-energy plasma jets.
Physics of Plasmas | 2010
Gianluca Sarri; Mark E Dieckmann; Crd Brown; C. A. Cecchetti; D.J. Hoarty; Steven James; R. Jung; Ioannis Kourakis; H. Schamel; O. Willi; M. Borghesi
The direct observation and full characterization of a phase space electron hole (EH) generated during laser-matter interaction is presented. This structure, propagating in a tenuous, nonmagnetized plasma, has been detected via proton radiography during the irradiation with a ns laser pulse (Iλ2≈1014 W/cm2) of a gold hohlraum. This technique has allowed the simultaneous detection of propagation velocity, potential, and electron density spatial profile across the EH with fine spatial and temporal resolution allowing a detailed comparison with theoretical and numerical models.
Physical Review Letters | 2013
H. Ahmed; Mark E Dieckmann; L. Romagnani; D. Doria; Gianluca Sarri; M. Cerchez; E. Ianni; Ioannis Kourakis; A.L. Giesecke; M. Notley; R. Prasad; K. Quinn; O. Willi; M. Borghesi
We report on the temporally and spatially resolved detection of the precursory stages that lead to the formation of an unmagnetized, supercritical collisionless shock in a laser-driven laboratory experiment. The measured evolution of the electrostatic potential associated with the shock unveils the transition from a current free double layer into a symmetric shock structure, stabilized by ion reflection at the shock front. Supported by a matching particle-in-cell simulation and theoretical considerations, we suggest that this process is analogous to ion reflection at supercritical collisionless shocks in supernova remnants.
Laser and Particle Beams | 2010
T. Dzelzainis; G. Nersisyan; David Riley; L. Romagnani; H. Ahmed; A. Bigongiari; M. Borghesi; D. Doria; B. Dromey; M. Makita; S. White; S. Kar; D. Marlow; B. Ramakrishna; Gianluca Sarri; M. Zaka-Ul-Islam; M. Zepf; Ciaran Lewis
The multi-Terawatt laser system, terawatt apparatus for relativistic and nonlinear interdisciplinary science, has been recently installed in the Centre for Plasma Physics at the Queen’s University of Belfast. The system will support a wide ranging science program, which will include laser-driven particle acceleration, X-ray lasers, and high energy density physics experiments. Here we present an overview of the laser system as well as the results of preliminary investigations on ion acceleration and X-ray lasers, mainly carried out as performance tests for the new apparatus. We also discuss some possible experiments that exploit the flexibility of the system in delivering pump-probe capability.
New Journal of Physics | 2010
Gianluca Sarri; C. A. Cecchetti; L. Romagnani; C.M. Brown; D.J. Hoarty; Steven James; J. Morton; Mark E Dieckmann; R. Jung; O. Willi; S. V. Bulanov; Francesco Pegoraro; M. Borghesi
Plasma expansion following the interaction of an intense laser beam with the inner surface of gold hohlraums, emulating conditions relevant to indirect drive inertial confinement fusion (ICF), has been investigated by a radiographic technique which employs a beam of laser-accelerated protons. This probing technique has made it possible to measure the electric field distribution associated with the plasma front and its propagation throughout the interior of the hohlraum with a temporal and spatial resolution of the order of a few ps and μm, respectively. The data indicate that the expanding plasma slows down approaching the opposite walls, possibly due to the interaction with x-ray heated plasma from the non-irradiated walls. The electric field at the plasma front shows a bipolar structure, suggesting the presence of ion-acoustic soliton-like structures cotraveling with the front. Data obtained using enclosed hohlraums suggest the feasibility of this type of diagnosis in gas-filled hohlraums, as currently employed in ICF experiments.
Physics of Plasmas | 2010
Gianluca Sarri; Mark E Dieckmann; Ioannis Kourakis; M. Borghesi
The expansion of a dense plasma through a more rarefied ionized medium is a phenomenon of interest in various physics environments ranging from astrophysics to high energy density laser-matter laboratory experiments. Here this situation is modeled via a one-dimensional particle-in-cell simulation; a jump in the plasma density of a factor of 100 is introduced in the middle of an otherwise equally dense electron-proton plasma with an uniform proton and electron temperature of 10 eV and 1 keV, respectively. The diffusion of the dense plasma, through the rarefied one, triggers the onset of different nonlinear phenomena such as a strong ion-acoustic shock wave and a rarefaction wave. Secondary structures are detected, some of which are driven by a drift instability of the rarefaction wave. Efficient proton acceleration occurs ahead of the shock, bringing the maximum proton velocity up to 60 times the initial ion thermal speed.