Abstract
Based on the idea that tensor unparticles can enhance the gravitational interactions between standard model particles, potential black hole formation in high energy collisions is examined. Modifications to the horizon radius rH are derived, and the corresponding geometric cross-sections of such objects are calculated. It is shown that rH increases dramatically to the electroweak scale for masses M BH ∼1–10 TeV, yielding a geometric cross-section σ BH =πr 2 H on the order of ⩽50 pb. This suggests that unparticle physics provides a mechanism for black hole formation in future accelerators, without the requirement of extra spatial dimensions.
Original language | English |
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Pages (from-to) | 561-566 |
Number of pages | 6 |
Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
Volume | 660 |
Issue number | 5 |
DOIs | |
State | Published - Mar 6 2008 |
ASJC Scopus Subject Areas
- Nuclear and High Energy Physics