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Atomic and Laser Physics
Credit: Jack Hobhouse

Dr Francesco Miniati

Researcher in Computational Physics

Sub department

  • Atomic and Laser Physics

Research groups

  • Quantum high energy density physics
francesco.miniati@physics.ox.ac.uk
Clarendon Laboratory, room Simon room
  • About
  • Publications

Self-organized electromagnetic field structures in laser-produced counter-streaming plasmas

Nature Physics 8:11 (2012) 809-812

Authors:

NL Kugland, DD Ryutov, PY Chang, RP Drake, G Fiksel, DH Froula, SH Glenzer, G Gregori, M Grosskopf, M Koenig, Y Kuramitsu, C Kuranz, MC Levy, E Liang, J Meinecke, F Miniati, T Morita, A Pelka, C Plechaty, R Presura, A Ravasio, BA Remington, B Reville, JS Ross, Y Sakawa, A Spitkovsky, H Takabe, HS Park

Abstract:

Self-organization occurs in plasmas when energy progressively transfers from smaller to larger scales in an inverse cascade. Global structures that emerge from turbulent plasmas can be found in the laboratory and in astrophysical settings; for example, the cosmic magnetic field, collisionless shocks in supernova remnants and the internal structures of newly formed stars known as Herbig-Haro objects. Here we show that large, stable electromagnetic field structures can also arise within counter-streaming supersonic plasmas in the laboratory. These surprising structures, formed by a yet unexplained mechanism, are predominantly oriented transverse to the primary flow direction, extend for much larger distances than the intrinsic plasma spatial scales and persist for much longer than the plasma kinetic timescales. Our results challenge existing models of counter-streaming plasmas and can be used to better understand large-scale and long-time plasma self-organization. © 2012 Macmillan Publishers Limited. All rights reserved.
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Generation of scaled protogalactic seed magnetic fields in laser-produced shock waves

Nature Springer Nature 481:7382 (2012) 480-483

Authors:

G Gregori, A Ravasio, CD Murphy, K Schaar, A Baird, AR Bell, A Benuzzi-Mounaix, R Bingham, C Constantin, RP Drake, M Edwards, ET Everson, CD Gregory, Y Kuramitsu, W Lau, J Mithen, C Niemann, H-S Park, BA Remington, B Reville, APL Robinson, DD Ryutov, Y Sakawa, S Yang, NC Woolsey, M Koenig, F Miniati

Abstract:

Experimental simulations of galaxy-forming conditions using lasers show that the Biermann battery generates seed magnetic fields, which turbulence can amplify to affect galaxy evolution.
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Large scale magnetic fields in galaxies at high redshifts

EAS Publications Series EDP Sciences 56 (2012) 109-112

Authors:

ML Bernet, F Miniati, SJ Lilly, PP Kronberg, M Dessauges-Zavadsky
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Magnetic field generation by Biermann battery and Weibel instability in laboratory shock waves

EAS Publications Series EDP Sciences 58 (2012) 23-26

Authors:

G Gregori, F Miniati, B Reville, RP Drake
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Primordial magnetic field constraints from the end of reionization

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 418:1 (2011) l143-l147

Authors:

Dominik RG Schleicher, Francesco Miniati
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