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arXiv 1104.4802gr-qcastro-ph.HEhep-th
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黑洞对粒子的加速:运动学解释

Acceleration of particles by black holes: kinematic explanation

O. B. Zaslavskii

摘要:

本文在质心系中对黑洞加速粒子到无穷大能量的效应提出了一种新的简单而普遍的解释。它是基于运动学的粒子在地平线附近移动。当两种粒子在视界附近碰撞时,就会产生这种效应。对于有质量的粒子,第一种粒子代表具有一般能量和角动量的粒子(我称它们为“通常”)。在视界附近,这样一个粒子的速度几乎等于与黑洞共转的坐标系中的光速(如果黑洞是静态的,那么这个坐标系就是静态的)。第二类(称为“临界”)由速度v<c的粒子组成,由于能量和角动量(或电荷)之间的特殊关系。结果,相对速度接近光速c,洛伦兹因子变得不受约束。这种解释既适用于一般的旋转黑洞,也适用于带电黑洞(甚至适用于粒子的径向运动)。如果碰撞粒子之一是无质量的(光子),临界粒子的区别在于它的频率在视界附近是有限的。这种效应的存在(或不存在)取决于两个因素的竞争--向黑洞传播的光子的引力蓝移和由局部非旋转坐标系向共动坐标系转换产生的多普勒效应。所有可能的碰撞类型的分类建议取决于是否有质量或无质量的粒子是关键的或常见的。

英文摘要:

A new simple and general explanation of the effect of acceleration of particles by black holes to infinite energies in the centre of mass frame is suggested. It is based on kinematics of particles moving near the horizon. This effect arises when particles of two kinds collide near the horizon. For massive particles, the first kind represents a particle with the generic energy and angular momentum (I call them "usual"). Near the horizon, such a particle has a velocity almost equal to that of light in the frame that corotates with a black hole (the frame is static if a black hole is static). The second kind (called "critical") consists of particles with the velocity v<c near the horizon due to special relationship between the energy and angular momentum (or charge). As a result, the relative velocity approaches the speed of light c, the Lorentz factor grows unbound. This explanation applies both to generic rotating black holes and charged ones (even for radial motion of particles). If one of colliding particles is massless (photon), the critical particle is distinguished by the fact that its frequency is finite near the horizon. The existence (or absence) of the effect is determined depending on competition of two factors - gravitational blue shift for a photon propagating towards a black hole and the Doppler effect due to transformation from the locally nonrotating frame to a comoving one. Classification of all possible types of collisions is suggested depending on whether massive or massless particle is critical or usual.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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