2016
DOI: 10.1088/0264-9381/33/10/105014
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Collisions of spinning massive particles in a Schwarzschild background

Abstract: It is known that the center-of-mass energy of the collision of two massive particles following geodesics around a black hole presents a maximum. The maximum energy increases when the black hole is endowed with spin, and for a maximally rotating hole this energy blows up, offering, in principle, a unique probe of fundamental physics. This work extends the latter studies by considering that the colliding particles possess intrinsic angular momentum (spin), described by the Hanson-Regge-Hojman theory of spinning … Show more

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Cited by 59 publications
(97 citation statements)
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“…The CM energy for the extremal KN black hole near the horizon is (25) where the K 4 is defined in appendix A. We can see that when a 2 −j 1 a + 1 = 0 or a 2 −j 2 a + 1 = 0 the CM energy will be divergent and the critical total angular momentumj i = 1+a 2 a (i = 1, 2), which is the same as that of Ref.…”
Section: Extremal Kerr-newman Black Hole Casementioning
confidence: 74%
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“…The CM energy for the extremal KN black hole near the horizon is (25) where the K 4 is defined in appendix A. We can see that when a 2 −j 1 a + 1 = 0 or a 2 −j 2 a + 1 = 0 the CM energy will be divergent and the critical total angular momentumj i = 1+a 2 a (i = 1, 2), which is the same as that of Ref.…”
Section: Extremal Kerr-newman Black Hole Casementioning
confidence: 74%
“…The case with a = Q = 0 describes the Schwarzschild black hole as an accelerator of spinning test particles given in Ref. [25].…”
Section: Spinning Particles In Charged Spinning Black Hole Backgmentioning
confidence: 99%
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