Relativistic jets and event horizons for a kinetic spiral solution
作者: GraemeHeald
刊名: Physics Essays, 2018, Vol.31 (4), pp.387-396
来源数据库: Physics Essays
DOI: 10.4006/0836-1398-31.4.387
原始语种摘要: The Schwarzschild and Kerr solutions have never properly explained the existence of powerful axial relativistic jets of materials ejected from black holes. A full solution for the velocity and radius at any distance from a black hole will be given for the Kinetic Spiral (KS) equation and axial event horizons are found at radii, r : = 3 √ ( M θ ± √ ( M θ 2 − α θ 3 ) ) , where Mθ = GM.sec2θ/ω2 and αθ = c2.sec2θ/3.ω2. It will be shown how the two trajectories of particles into a black hole can differ, either away from a black hole for relativistic jets or inward to accrete at the centre of a black hole. The mechanism for relativistic jets has been explained: at the gravitational radius, if the kinetic energy is...
全文获取路径: 物理学论文  (合作)

  • event 事件
  • radius 半径
  • horizon 
  • black 炭黑
  • ejected 喷射
  • relativistic 相对论的
  • gravitational 重力
  • kinetic 动的
  • found 创立
  • profile 纵断图