scholarly journals Spectral asymptotics of Euclidean quantum gravity with diff-invariant boundary conditions

2005 ◽  
Vol 22 (6) ◽  
pp. 957-974 ◽  
Author(s):  
Giampiero Esposito ◽  
Guglielmo Fucci ◽  
Alexander Yu Kamenshchik ◽  
Klaus Kirsten
2006 ◽  
Vol 39 (21) ◽  
pp. 6317-6322
Author(s):  
Giampiero Esposito ◽  
Guglielmo Fucci ◽  
Alexander Yu Kamenshchik ◽  
Klaus Kirsten

2021 ◽  
pp. 2140004
Author(s):  
Edward Witten

We review what is known about boundary conditions in General Relativity on a spacetime of Euclidean signature. The obvious Dirichlet boundary condition, in which one specifies the boundary geometry, is actually not elliptic and in general does not lead to a well-defined perturbation theory. It is better-behaved if the extrinsic curvature of the boundary is suitably constrained, for instance if it is positive- or negative-definite. A different boundary condition, in which one specifies the conformal geometry of the boundary and the trace of the extrinsic curvature, is elliptic and always leads formally to a satisfactory perturbation theory. These facts might have interesting implications for semiclassical approaches to quantum gravity. April, 2018


2020 ◽  
Vol 135 (10) ◽  
Author(s):  
Iberê Kuntz

AbstractWe remark that Ostrogradsky ghosts in higher-derivative gravity, with a finite number of derivatives, are fictitious as they result from an unjustified truncation performed in a complete theory containing infinitely many curvature invariants. The apparent ghosts can then be projected out of the quadratic gravity spectrum by redefining the boundary conditions of the theory in terms of an integration contour that does not enclose the ghost poles. This procedure does not alter the renormalizability of the theory. One can thus use quadratic gravity as a quantum field theory of gravity that is both renormalizable and unitary.


1996 ◽  
Vol 10 (18n19) ◽  
pp. 2431-2440
Author(s):  
M. MARTELLINI ◽  
M. SPREAFICO ◽  
K. YOSHIDA

Starting from a generalized version of David-Distler-Kawai treatment of 2d-induced quantum gravity, we impose a series of “physical” boundary conditions to obtain an unique field theoretical Lagrangian describing random surface models and strings at given dimensions d>1. Our theory reproduces the critical exponents obtained by numerical simulations on d-dimensional Ising-like models for lower d-values. One observes, at appropriate dimensions d, the transition to the so-called branched polymer phase.


Author(s):  
Ding Jia

Abstract An important task faced by all approaches of quantum gravity is to incorporate superpositions and quantify quantum uncertainties of spacetime causal relations. We address this task in 2D. By identifying a global Z2 symmetry of 1+1D quantum gravity, we show that gravitational path integral configurations come in equal amplitude pairs with timelike and spacelike relations exchanged. As a consequence, any two points are equally probable to be timelike and spacelike separated in a universe without boundary conditions. In the context of simplicial quantum gravity we identify a local symmetry of the action which shows that even with boundary conditions causal uncertainties are generically present. Depending on the boundary conditions, causal uncertainties can still be large and even maximal.


1995 ◽  
Vol 12 (11) ◽  
pp. 2715-2722 ◽  
Author(s):  
Giampiero Esposito ◽  
Alexander Yu Kamenshchik

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