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Why the Length of a Quantum String Cannot Be Lorentz Contracted
Author(s) -
A. Aurilia,
Euro Spallucci
Publication year - 2013
Publication title -
advances in high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.59
H-Index - 49
eISSN - 1687-7365
pISSN - 1687-7357
DOI - 10.1155/2013/531696
Subject(s) - physics , planck length , quantum gravity , length contraction , loop quantum gravity , schwarzschild radius , theoretical physics , quantum mechanics , virtual black hole , string theory , length scale , lorentz transformation , mathematical physics , classical mechanics , quantum , gravitation , planck scale , charged black hole
We propose a quantum gravity-extended form of the classical length contraction law obtained in special relativity. More specifically, the framework of our discussion is the UV self-complete theory of quantum gravity. We show how our results are consistent with (i) the generalized form of the uncertainty principle (GUP), (ii) the so-called hoop-conjecture, and (iii) the intriguing notion of “classicalization” of trans-Planckian physics. We argue that there is a physical limit to the Lorentz contraction rule in the form of some minimal universal length determined by quantum gravity, say the Planck Length, or any of its current embodiments such as the string length, or the TeV quantum gravity length scale. In the latter case, we determine the critical boost that separates the ordinary “particle phase,” characterized by the Compton wavelength, from the “black hole phase,” characterized by the effective Schwarzschild radius of the colliding system

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