2005
DOI: 10.1007/11377306_3
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Introduction to Quantum-Gravity Phenomenology

Abstract: After a brief review of the first phase of development of Quantum-Gravity Phenomenology, I argue that this research line is now ready to enter a more advanced phase: while at first it was legitimate to resort to heuristic order-of-magnitude estimates, which were sufficient to establish that sensitivity to Planck-scale effects can be achieved, we should now rely on detailed analyses of some reference test theories. I illustrate this point in the specific example of studies of Planck-scale modifications of the e… Show more

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Cited by 45 publications
(59 citation statements)
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“…The global or bulk extent of the position probability density of the D-dimensional hydrogenic atoms is best measured by the Shannon entropy S given by (1). From Eqs.…”
Section: The Shannon Entropy In Position Spacementioning
confidence: 99%
See 1 more Smart Citation
“…The global or bulk extent of the position probability density of the D-dimensional hydrogenic atoms is best measured by the Shannon entropy S given by (1). From Eqs.…”
Section: The Shannon Entropy In Position Spacementioning
confidence: 99%
“…Their deeper knowledge is basic not only to gain full insight into the intimate structure of matter but also for numerous phenomena of quantum cosmology [1], nanotechnology [2,3] (e.g., for low-dimensional semiconductor nanostructures such as quantum wells, wires, and dots), quantum computation [4,5] (e.g., one-and two-dimensional hydrogenic atoms have been proposed as qubits), D-dimensional physics [6 -12], and quantum field theory [11,[13][14][15]. The existence of hydrogenic systems with dimensionality other than 3 has been observed for D Ͻ 3 [2] and suggested for D Ͼ 3 [7].…”
Section: Introductionmentioning
confidence: 99%
“…The only natural UV cutoff frequency seems to be the Planck frequency but if this value is used the resulting finite vacuum energy density would provide a 'cosmological constant' 10 120 times above the observational limit, measured to be a fraction of the critical density of the Universe. This is the well known cosmological constant problem [31,38,39]. A UV cutoff imposed on the Planckian spectrum will lead to Lorentz invariance.…”
Section: Quantum Vacuum Atom Wave Decoherencementioning
confidence: 99%
“…In such a scenario, over the last twenty five years or so, a variety of approaches have been constructed by hand to investigate possible imprints of Planck scale effects on phenomena involving matter fields (see, for instance, the reviews [1][2][3][4]). These methods evidently involve a new scale (often assumed to be of the order of the Planck scale) and they strive to capture one or more features that are expected to arise in the complete quantum theory of gravity.…”
Section: Introductionmentioning
confidence: 99%