论文标题
粒子碰撞引力辐射
Gravitation radiation from the collision of particles
论文作者
论文摘要
目前，宇宙射线物理学中存在一个尚未解决的问题。问题涉及超高能量宇宙射线的起源。这种能量的粒子出生的可能机制之一与星系活跃核发生的过程结合。在本文中，我们检查了超重量颗粒的碰撞。使用温伯格形式主义，我们估计了第一个近似值中碰撞期间发出的重力辐射。结果表明，在一定的碰撞时间内，超层析粒子损失的能量小于碰撞质量中心和碰撞颗粒质量的能量的值。
At the present moment, there is an unresolved problem in the physics of cosmic rays. The problem concerns the origin of the ultrahigh energy cosmic rays. One of the possible mechanisms of the particle's birth with such energy is bound to the processes occurring in the active nuclei of the galaxies. In this paper, we have examined a collision of superheavy particles. Using the Weinberg formalism, we have estimated gravitational radiation emitted during the collision in the first approximation. It was shown that, for a certain collision time, the energy lost by the ultrarelativistic particle is less than the value of the energy of the mass center of the collision and the mass of the colliding particles.
