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  1. ui.adsabs.harvard.edu

    How these "weak pulsars" fill their magnetospheres without efficient photon-photon pair conversion in the outer magnetosphere is still an open question. In this paper, we present a range of self-consistent solutions to the pulsar magnetosphere that do not require pair production near the light cylinder. When pair production is very efficient ...
    Author:Alexander Y. Chen, Fábio Cruz, Anatoly SpitkovskyPublished:2020
  2. iopscience.iop.org

    We consider only magnetic conversion of γ-ray photons into pairs since it is the dominant pair production mechanism in the magnetospheres of weak pulsars.The cross section of this process depends exponentially on the ratio between local magnetic field B and the quantum critical field, B/B Q, where (see, e.g., Erber 1966).When B ≪ B Q this process is exponentially suppressed, which means it ...
    Author:Alexander Y. Chen, Fábio Cruz, Anatoly SpitkovskyPublished:2020
  3. How these "weak pulsars" fill their magnetospheres without efficient photon-photon pair conversion in the outer magnetosphere is still an open question. In this paper, we present a range of self-consistent solutions to the pulsar magnetosphere that do not require pair production near the light cylinder. When pair production is very efficient ...
    Author:Alexander Y. Chen, Fabio Cruz, Anatoly SpitkovskyPublished:2019
  4. collaborate.princeton.edu

    How these "weak pulsars" fill their magnetospheres without efficient photon-photon pair conversion in the outer magnetosphere is still an open question. In this paper, we present a range of self-consistent solutions to the pulsar magnetosphere that do not require pair production near the light cylinder. When pair production is very efficient ...
    Author:Alexander Y. Chen, Fábio Cruz, Anatoly SpitkovskyPublished:2020
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  6. epp.tecnico.ulisboa.pt

    extreme plasma physics > Publications > Filling the Magnetospheres of Weak Pulsars. Filling the Magnetospheres of Weak Pulsars. Latest News / Press Releases. GoLP researchers secure 30 million core hours on MareNostrum 5 November 21, 2024.
  7. pubs.aip.org

    Time-dependent cascades of electron-positron pairs are thought to be the main source of plasma in pulsar magnetospheres and a primary ingredient to explain the . ... Current flow and pair creation at low altitude in rotation-powered pulsars' force-free magnetospheres: Space charge limited flow ... Filling the magnetospheres of weak pulsars,"
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