• Pulsar Radio Emission from Closed Field Lines Near Light Cylinder

    Subjects: Astronomy >> Astrophysics submitted time 2024-01-16

    Abstract:
    The pulsar radio emission mechanism remains an enigma  over half a century.
    A successful radiation process requires not only to explain the coherency, but also
    microstructures,  characteristic frequency of emission, and the “death line" problem, etc.
    These challenge both the long standing gap models  and recent models of magnetic reconnection
    with emission based on open field lines.
    This article points out that each intermittent plasma ejection from Y-point,
    the boundary of closed zone intersecting the equatorial plane,
    near the light cylinder of pulsar magnetosphere can
    stretch a bundle of closed field lines significantly.  Corresponding magnetic pressure imposed on the trapped plasma provides ideal site of
    magnetic reconnection and hence generating pairs and Alfven wave near light cylinder.
    The resultant  marginal stable  instability is expected for coherent curvature emission. This   not only interprets  above problems in a simple and unified way, but also offers hints to the behavior of  Rotating Radio Transients (RRATs) and Fast Radio Bursts (FRBs).

  • Pulsar Radio Emission under Global-Local Interaction of Pulsar Magnetosphere

    Subjects: Astronomy >> Astrophysics submitted time 2023-12-04

    Abstract: The pulsar radio emission mechanism remains an enigma  over half a century.
    A successful radiation process requires not only to explain the coherency and high degree of polarization of the emission, but also
    microstructures,  characteristic frequency of emission, and the “death line" problem, etc. These issues challenge both the long standing cap models  and recent models of magnetic reconnection assuming stationary magnetosphere of a pulsar.
    This article proposes a radio emission through global-local interaction of pulsar magnetosphere. The centrifugal force at the light cylinder   leads to the concentration of both field lines and plasma in an equatorial layer much less than that of  a pulsar magnetosphere.
    The resultant magnetic reconnection with chain of plasmoids interprets not only  the above problems in a simple and unified way, but also Rotating Radio Transients (RRATs) and Fast Radio Bursts (FRBs).