• Atomic physics: Radiation pressure with

    From ScienceDaily@1337:3/111 to All on Mon Jun 15 21:30:32 2020
    Atomic physics: Radiation pressure with recoil
    Researchers deliver experimental proof for a 90 year-old theory

    Date:
    June 15, 2020
    Source:
    Goethe University Frankfurt
    Summary:
    Light exerts a certain amount of pressure onto a body: sun sails
    could thus power space probes in the future. However, when light
    particles (photons) hit an individual molecule and knock out
    an electron, the molecule flies toward the light source. Atomic
    physicists have now observed this for the first time, confirming
    a 90 year-old theory.



    FULL STORY ========================================================================== Light exerts a certain amount of pressure onto a body: sun sails could
    thus power space probes in the future. However, when light particles
    (photons) hit an individual molecule and knock out an electron, the
    molecule flies toward the light source. Atomic physicists at Goethe
    University have now observed this for the first time, confirming a 90
    year-old theory.


    ==========================================================================
    As early as the 16th century, the great scholar Johannes Kepler postulated
    that sunlight exerted a certain pressure, as the tail of the comets he
    observed consistently pointed away from the sun. In 2010 the Japanese
    space probe Ikaros used a sun sail for the first time in order to use
    the power of sunlight to gain a little speed.

    Physically and intuitively, the pressure of light or radiation can
    be explained by the particle characteristic of light: light particles
    (photons) strike the atoms of a body and transfer a portion of their
    own momentum (mass times speed) onto that body, which thus becomes faster.

    However, when in the 20th century physicists studied this momentum
    transfer in the laboratory during experiments on photons of certain
    wavelengths which knocked individual electrons out of atoms, they were
    met by a surprising phenomenon: the momentum of the ejected electron
    was greater than that of the photon that struck it. This is actually
    impossible -- since Isaac Newton it has been known that within a system,
    for every force there must exist an equal but opposite force: the recoil,
    so to speak. For this reason, the Munich scientist Arnold Sommerfeld
    concluded in 1930 that the additional momentum of the ejected electron
    must come from the atom it left. This atom must fly in the opposite
    direction; in other words, toward the light source. However, this was impossible to measure with the instruments available at that time.

    Ninety years later the physicists in the team of doctoral student Sven Grundmann and Professor Reinhard Do"rner from the Institute for Nuclear
    Physics have succeeded for the first time in measuring this effect
    using the COLTRIMS reaction microscope developed at Goethe University Frankfurt. To do so, they used X-rays at the accelerators DESY in Hamburg
    and ESRF in French Grenoble, in order to knock electrons out of helium
    and nitrogen molecules. They selected conditions that would require
    only one photon per electron. In the COLTRIMS reaction microscope,
    they were able to determine the momentum of the ejected electrons and
    the charged helium and nitrogen atoms -- which are called ions - -
    with unprecedented precision.

    Professor Reinhard Do"rner explains: "We were not only able to measure
    the ion's momentum, but also see where it came from -- namely, from
    the recoil of the ejected electron. If photons in these collision
    experiments have low energy, the photon momentum can be neglected for theoretical modelling. With high photon energies, however, this leads to imprecision. In our experiments, we have now succeeded in determining
    the energy threshold for when the photon momentum may no longer be
    neglected. Our experimental breakthrough allows us to now pose many more questions, such as what changes when the energy is distributed between
    two or more photons."

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


    ========================================================================== Journal Reference:
    1. Sven Grundmann, Max Kircher, Isabel Vela-Perez, Giammarco Nalin,
    Daniel
    Trabert, Nils Anders, Niklas Melzer, Jonas Rist, Andreas Pier,
    Nico Strenger, Juliane Siebert, Philipp V. Demekhin, Lothar
    Ph. H. Schmidt, Florian Trinter, Markus S. Scho"ffler, Till Jahnke,
    Reinhard Do"rner.

    Observation of Photoion Backward Emission in Photoionization of
    He and N2. Physical Review Letters, 2020; 124 (23) DOI: 10.1103/
    PhysRevLett.124.233201 ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2020/06/200615140846.htm

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