• How to have a blast like a black hole

    From ScienceDaily@1337:3/111 to All on Tue Sep 8 21:30:32 2020
    How to have a blast like a black hole

    Date:
    September 8, 2020
    Source:
    Osaka University
    Summary:
    Scientists have created magnetized-plasma conditions similar to
    those near a black hole using very intense laser pulses. This work
    may help show how X-rays can be produced by astronomical objects.



    FULL STORY ========================================================================== Laser Engineering at Osaka University have successfully used short, but extremely powerful laser blasts to generate magnetic field reconnection
    inside a plasma. This work may lead to a more complete theory of X-ray
    emission from astronomical objects like black holes.


    ==========================================================================
    In addition to being subjected to extreme gravitational forces, matter
    being devoured by a black hole can be also be pummeled by intense heat
    and magnetic fields. Plasmas, a fourth state of matter hotter than
    solids, liquids, or gasses, are made of electrically charged protons
    and electrons that have too much energy to form neutral atoms. Instead,
    they bounce frantically in response to magnetic fields. Within a plasma, magnetic reconnection is a process in which twisted magnetic field lines suddenly "snap" and cancel each other, resulting in the rapid conversion
    of magnetic energy into particle kinetic energy. In stars, including
    our sun, reconnection is responsible for much of the coronal activity,
    such as solar flares. Owing to the strong acceleration, the charged
    particles in the black hole's accretion disk emit their own light,
    usually in the X-ray region of the spectrum.

    To better understand the process that gives rise to the observed X-rays
    coming from black holes, scientists at Osaka University used intense
    laser pulses to create similarly extreme conditions on the lab. "We were
    able to study the high-energy acceleration of electrons and protons
    as the result of relativistic magnetic reconnection," Senior author
    Shinsuke Fujioka says. "For example, the origin of emission from the
    famous black hole Cygnus X-1, can be better understood." This level of
    light intensity is not easily obtained, however. For a brief instant,
    the laser required two petawatts of power, equivalent to one thousand
    times the electric consumption of the entire globe. With the LFEX laser,
    the team was able to achieve peak magnetic fields with a mind-boggling
    2,000 telsas. For comparison, the magnetic fields generated by an MRI
    machine to produce diagnostic images are typically around 3 teslas, and
    Earth's magnetic field is a paltry 0.00005 teslas. The particles of the
    plasma become accelerated to such an extreme degree that relativistic
    effects needed to be considered.

    "Previously, relativistic magnetic reconnection could only be studied
    via numerical simulation on a supercomputer. Now, it is an experimental
    reality in a laboratory with powerful lasers," first author King Fai
    Farley Law says. The researchers believe that this project will help
    elucidate the astrophysical processes that can happen at places in the
    Universe that contain extreme magnetic fields.


    ========================================================================== Story Source: Materials provided by Osaka_University. Note: Content may
    be edited for style and length.


    ========================================================================== Journal Reference:
    1. K. F. F. Law, Y. Abe, A. Morace, Y. Arikawa, S. Sakata, S. Lee, K.

    Matsuo, H. Morita, Y. Ochiai, C. Liu, A. Yogo, K. Okamoto,
    D. Golovin, M.

    Ehret, T. Ozaki, M. Nakai, Y. Sentoku, J. J. Santos, E. d'Humie`res,
    Ph.

    Korneev, S. Fujioka. Relativistic magnetic reconnection in laser
    laboratory for testing an emission mechanism of hard-state
    black hole system. Physical Review E, 2020; 102 (3) DOI:
    10.1103/PhysRevE.102.033202 ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2020/09/200908101638.htm

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