8–12 Jul 2019
University of Milano-Bicocca UNIMIB
Europe/Rome timezone

Session

BSAP-BPIF

9 Jul 2019, 10:40
Aula U6-09, Building U6 (University of Milano-Bicocca UNIMIB)

Aula U6-09, Building U6

University of Milano-Bicocca UNIMIB

Piazza dell’Ateneo Nuovo, 1 20126 Milan (Italy)

Conveners

BSAP-BPIF

  • L. Gremillet (CEA)

Presentation materials

There are no materials yet.

  1. A.S. Davies (EPS 2019)
    09/07/2019, 10:40
    Joint Sessions

    See the full abstract here http://ocs.ciemat.es/EPS2019ABS/pdf/I2.J501.pdf

    The rapid, picosecond time-scale evolution of electron density and temperature in a laser-produced plasma was measured using collective Thomson scattering [1]. As is the case for many laser-plasma applications, an underdense (~10^19 cm^-3) H2 plasma was created by a 60-ps, 1053-nm laser pulse with an intensity of ~3 x...

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  2. M. Tamburini (EPS 2019)
    09/07/2019, 11:10
    Joint Sessions

    See the full abstract here http://ocs.ciemat.es/EPS2019ABS/pdf/I2.J502.pdf

    Powerful gamma-ray emissions are ubiquitous in astrophysics, from active galactic nuclei [1] to pulsars [2] and neutron star mergers [3]. One of the key mechanisms leading to powerful gamma-ray emissions is thought to be the interaction of ultrarelativistic particle beams with a surrounding plasma environment, which...

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  3. G. Vieux (EPS 2019)
    09/07/2019, 11:40
    Joint Sessions

    See the full abstract here http://ocs.ciemat.es/EPS2019ABS/pdf/I2.J503.pdf

    High power, short pulse lasers have become valuable tools for scientists exploring a wide range of phenomena and developing new technologies such as ultra-compact wakefield accelerators [1] and compact light sources [2] with applications ranging from particle physics to biology. To produce ultra-intense, short pulses,...

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  4. L. Willingale (EPS 2019)
    09/07/2019, 12:10
    Joint Sessions

    See the full abstract here http://ocs.ciemat.es/EPS2019ABS/pdf/I2.J504.pdf

    The extremely energetic class of astrophysical phenomena - including high-energy pulsar winds, gamma ray bursts, and jets from galactic nuclei - have plasma conditions where the energy density of the magnetic fields exceeds the rest mass energy density (sigmacold = B^2/(µ0nemec^2)), the cold magnetization parameter)....

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