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7 ta ish

Ish: Pulsars with Strong Magnetic Fields: Polar Gaps, Bound Pair Creation and Nonthermal Luminosities

  1. Particle acceleration and electromagnetic field of deformed neutron stars

    Javlon Rayimbaev, Bobur Turimov, Marcos Figueroa +2

    MaqolaPulsars and Gravitational Waves ResearchModern Physics Letters A201934 iqtibos
    ABI

  2. Can modified gravity silence radio-loud pulsars?

    Javlon Rayimbaev, Pulat Tadjimuratov

    MaqolaPulsars and Gravitational Waves ResearchPhysical review. D/Physical review. D.202034 iqtibos
    ABI

  3. Radio Pulsars in an Electromagnetic Universe

    Javlon Rayimbaev, Shokhzod Jumaniyozov, Maksud Umaraliyev +1

    MaqolaPulsars and Gravitational Waves ResearchUniverse202212 iqtibos
    ABI

  4. One-photon pair production in pulsars: non-relativistic and relativistic regimes

    J. Weise, D. B. Melrose

    MaqolaPulsars and Gravitational Waves ResearchMonthly Notices of the Royal Astronomical Society20020 iqtibos
    ABI

  5. Death line for radio pulsars in braneworlds

    Djavlanbek Rayimbaev, Satimbay Palvanov, Maksud Umaraliyev +1

    MaqolaPulsars and Gravitational Waves ResearchBulletin of National University of Uzbekistan Mathematics and Natural Sciences20200 iqtibos
    ABI

  6. Constraining spacetime deformation based on astrophysical observations from radio pulsars

    Nozima Juraeva, Javlon Rayimbaev, Kamoliddin Haydarov +2

    MaqolaPulsars and Gravitational Waves ResearchArabian Journal of Mathematics20220 iqtibos
    ABI

  7. Vacuum and plasma magnetosphere around rotating magnetized neutron stars in Bocharova–Bronnikov–Melnikov–Bekenstein geometry

    Sherzod Sayfiyev, Ashfaque H. Bokhari, Bobomurat Ahmedov +1

    MaqolaPulsars and Gravitational Waves ResearchThe European Physical Journal C20250 iqtibos
    ABI