Death line for radio pulsars in braneworlds

Djavlanbek Rayimbaev, S. Palvanov, M. Umaraliyev, Malika Khudoyberdiyeva
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Abstract

We investigate the effects of braneworlds on energetic processes in plasma magnetosphere of neutron stars. Obtained that the presence of brane charge causes an increase in the size of the polar cap region. It has shown that the polar capsize of neutron stars with larger rotation period and compactness parameter is also larger. We have studied deathline of radio pulsar in braneworld. Obtained that the deathline shifted down and the pulsars which lying on the deathline become visible in radio band. Moreover, we have extended particle acceleration in polar cap of neutron stars in the presence of the brane charge, obtain that in both curvature radiation (γ ∼ 106) and inverse Compton scattering (50 . γ . 104) cases the acceleration "rate" of the accelerating charged particle is significantly smaller in the presence of the brane charge.
星际中射电脉冲星的死亡线
研究了膜世界对中子星等离子体磁层能量过程的影响。得到了膜电荷的存在导致极帽区尺寸的增大。结果表明,旋转周期和紧度参数越大的中子星,其极性倾覆也越大。我们研究了膜界射电脉冲星的死亡线。得到了死亡线下移的结果,位于死亡线上的脉冲星在射电波段可见。此外,我们还扩展了膜电荷存在下中子星极帽中的粒子加速度,得到了曲率辐射(γ ~ 106)和逆康普顿散射(50。γ。104)在膜电荷存在的情况下,加速带电粒子的加速“速率”明显更小。
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