scholarly journals Fundamental length scale of quantum spacetime foam

JETP Letters ◽  
2007 ◽  
Vol 86 (2) ◽  
pp. 73-77 ◽  
Author(s):  
F. R. Klinkhamer
1980 ◽  
Vol 170 (2) ◽  
pp. 228-264 ◽  
Author(s):  
R. Brout ◽  
F. Englert ◽  
J.-M. Frère ◽  
E. Gunzig ◽  
P. Nardone ◽  
...  

2005 ◽  
Vol 870 ◽  
Author(s):  
V. G. Karpov ◽  
Diana Shvydka ◽  
Yann Roussillon

AbstractThe recently developed physics of thin-film photovoltaics is suggested to be representative of other giant area electronics. We show that (i) giant-area devices are intrinsically nonuniform in the lateral directions, (ii) the nonuniformity spans length scales from millimeters to meters depending on external drivers such as light intensity and bias, and (iii) it significantly impacts the device performance. We derive a fundamental length scale that discriminates between the cases of small and large-area devices, and beyond which a new physics emerges. In addition, we present a practical method of mitigating the nonuniformity effects.


2000 ◽  
Vol 477 (4) ◽  
pp. 424-428 ◽  
Author(s):  
Ronald J. Adler ◽  
Ilya M. Nemenman ◽  
James M. Overduin ◽  
David I. Santiago

2006 ◽  
Vol 03 (07) ◽  
pp. 1293-1302
Author(s):  
JOSÉ M. ISIDRO

It has been argued that, underlying the M-theoretic dualities, there should exist a symmetry relating the semiclassical and the strong-quantum regimes of a given action integral. On the other hand, a field-theoretic exchange between long and short distances (similar in nature to the T-duality of strings) has been shown to provide a starting point for quantum gravity, in that this exchange enforces the existence of a fundamental length scale on spacetime. In this paper, we prove that the above semiclassical vs. strong-quantum symmetry is equivalent to the exchange of long and short distances. Hence the former symmetry, as much as the latter, also enforces the existence of a length scale. We apply these facts in order to classify all possible duality groups of a given action integral on spacetime, regardless of its specific nature and of its degrees of freedom.


2000 ◽  
Vol 09 (01) ◽  
pp. 91-95
Author(s):  
LIAO LIU ◽  
YONGGE MA

We show from one-loop quantum gravity and statistical thermodynamics that the thermodynamics of quantum foam in flat spacetime and Schwarzschild spacetime is exactly the same as that of Hawking–Unruh radiation in thermal equilibrium. This means we show unambiguously that Hawking–Unruh thermal radiation should contain thermal gravitons or the contribution of quantum spacetime foam. As a by-product, we give also the quantum gravity correction in one-loop approximation to the classical black hole thermodynamics.


2000 ◽  
Vol 63 (6) ◽  
pp. 1088-1096
Author(s):  
D. V. Nanopoulos

2018 ◽  
Vol 27 (14) ◽  
pp. 1847007
Author(s):  
Michael J. Kavic ◽  
Djordje Minic ◽  
John Simonetti

We argue that the Black Hole-Neutron Star (BH-NS) binaries are the natural astrophysical probes of quantum gravity in the context of the new era of multi-messenger astronomy. In particular, we discuss the observable effect of enhanced BH mass loss in a BH-NS binary, due to the presence of an additional length scale tied to the intrinsic noncommutativity of quantum spacetime in quantum gravity.


1993 ◽  
Vol 47 (6) ◽  
pp. R2163-R2167 ◽  
Author(s):  
Ian H. Redmount ◽  
Wai-Mo Suen

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