Generation of neutral and high-density electron-positron pair plasmas in the laboratory
Year: 2015
Authors: Sarri G., Poder K., Cole J.M., Schumaker W., Di Piazza A., Reville B., Dzelzainis T., Doria D., Gizzi LA., Grittani G., Kar S., Keitel C.H., Krushelnick K., Kuschel S., Mangles S.P.D., Najmudin Z., Shukla N., Silva L.O., Symes D., Thomas A.G.R., Vargas M., Vieira J., Zepf M.
Autors Affiliation: Queens Univ Belfast, Sch Math & Phys, Belfast BT7 1NN, Antrim, North Ireland; Univ London Imperial Coll Sci Technol & Med, John Adams Inst Accelerator Sci, Blackett Lab, London SW7 2BZ, England; Univ Michigan, Ctr Ultrafast Opt Sci, Ann Arbor, MI 48109 USA; Max Planck Inst Kernphys, D-69117 Heidelberg, Germany; CNR, Ist Nazl Ott, I-56124 Pisa, Italy; INFN, Sez Pisa, I-56127 Pisa, Italy; Helmholtz Inst Jena, D-07743 Jena, Germany; Univ Lisbon, Inst Super Tecn, Inst Plasmas & Fusao Nucl, GoLP, P-1699 Lisbon, Portugal; Rutherford Appleton Lab, Cent Laser Fac, Didcot OX11 0QX, Oxon, England.
Abstract: 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.
Journal/Review: NATURE COMMUNICATIONS
Volume: 6 Pages from: 6747-1 to: 6747-8
More Information: We are grateful for the support of the Central Laser Facility staff. The work of W.S., A.G.R.T., K.K. and M.V. was partially supported by the funding schemes National Science Foundation CAREER (grant 1054164) and National Science Foundation/Domestic Nuclear Detection Office (award no. F021166). G.S. and M.Z. wish to acknowledge financial support from the Engineering and Physical Sciences Research Council (grants: EP/L013975/1 and EP/I029206/1, respectively). LAG and G.G. acknowledge financial support from Consiglio Nazionale delle Ricerche (ELI-Italy) and Istituto Nazionale di Fisica Nucleare (CN5-g-RESIST). J.V., N.S. and L.O.S. wish to acknowledge the European Research Council (ERC-2010-AdG grant no. 267841), Fundacao para a Ciencia e Tecnologia, through grant EXPL/FIS-PLA/0834/2012. Z.N., S.P.D., J.M.C, K.P. wish to acknowledge financial support from STFC (grant no. ST/J002062/1). Access to the SuperMUC based in Germany at Leibniz research center was obtained through PRACE.KeyWords: Energy; Instability; Evolution; Waves; Jets; CodeDOI: 10.1038/ncomms7747ImpactFactor: 11.329Citations: 254data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-10-13References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here