Advances in High Energy Physics
Volume 2016 (2016), Article ID 9897051, 7 pages
http://dx.doi.org/10.1155/2016/9897051

Research Article

On the UV Dimensions of Loop Quantum Gravity

Michele Ronco1,2

¹Dipartimento di Fisica, Sapienza-Università di Roma, Piazzale A. Moro 2, 00185 Roma, Italy
²INFN, Sez. Roma1, Piazzale A. Moro 2, 00185 Roma, Italy

Received 1 May 2016; Accepted 22 June 2016

Academic Editor: Ahmed Farag Ali

Copyright © 2016 Michele Ronco. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP³.

Abstract.

Planck-scale dynamical dimensional reduction is attracting more and more interest in the quantum-gravity literature since it seems to be a model independent effect. However, different studies base their results on different concepts of space-time dimensionality. Most of them rely on the spectral dimension; others refer to the Hausdorff dimension; and, very recently, the thermal dimension has also been introduced. We here show that all these distinct definitions of dimension give the same outcome in the case of the effective regime of Loop Quantum Gravity (LQG). This is achieved by deriving a modified dispersion relation from the hypersurface-deformation algebra with quantum corrections. Moreover, we also observe that the number of UV dimensions can be used to constrain the ambiguities in the choice of these LQG-based modifications of the Dirac space-time algebra. In this regard, introducing the polymerization of connections, that is, , we find that the leading quantum correction gives . This result may indicate that the running to the expected value of two dimensions is ongoing, but it has not been completed yet. Finding at ultrashort distances would require going beyond the effective approach we here present.

1. Introduction

There is an increasing interest in the quantum-gravity literature about the effect of dynamical dimensional reduction of space-time. It consists in scale dependence of the dimension that runs from the standard IR value of four space-time dimensions to the lower value at Planckian energies. Remarkably, despite the fact that quantum-gravity approaches start from different conceptual premises and adopt different formalism types, this dimensional running has been found in the majority of them, such as Causal Dynamical Triangulation (CDT) [1], Horava-Lifshitz gravity [2], Causal Sets [3], Asymptotic Safety [4], Space-Time Noncommutativity [5], and LQG [6–8], which is here of interest.

However, in quantum gravity, even the concept of space-time dimension is a troublesome issue and it requires some carefulness. In fact, nonperturbative, background independent approaches (e.g., LQG [9, 10] and CDT [11]) generally rely on nongeometric quantities and they have discreteness as their core feature. For this reason, in order to extract phenomenological predictions, a coarse-graining process would be necessary aimed at deriving a more manageable effective description from the fundamental discrete blocks, which characterize the Planckian realm. It is a common expectation that this procedure should leave some traces in a semiclassical regime where the emerging picture would be given in terms of quantum space-time. This reduction has the advantage of allowing us to recover at least some of our more familiar physical observables or, when it would not be possible, analogous ones with potential departures from their classical counterparts. The dimension belongs to this latter set of semiclassical observables because the usual Hausdorff dimension is ill-defined for quantum space-time [12]. In the CDT approach [1, 11], it was recognized for the first time that a proper “quantum analogue” could be the spectral dimension , which is the scaling of the heat-kernel trace, and it reproduces the standard Hausdorff dimension when the classical smooth space-time is recovered. What is more, it was found that in the UV (see however [13] for recent CDT simulations favouring a smaller value of the dimension), which is now a recurring number in the literature [14–17]. In the Asymptotic Safety program, such a value is also intimately connected to the hope of having a fixed point in the UV. In fact, it has been proven that renormalizability is accomplished only if the dimension runs to two [18]. Furthermore, this prediction finds support in a recently developed approach [19] that has the advantage of relying on a minimal set of assumptions. Provided that quantum gravity will host an effective limit characterized by the presence of a minimum allowed length (identified with the Planck length), then it is shown [19] that the Euclidean volume becomes two-dimensional near the Planck scale (the author is grateful to Thanu Padmanabhan for pointing this out).

However, in a recent paper [20], the physical significance of has been questioned. Such a concern is based on two observations: the computation of requires preliminary Euclideanization of the space-time and also it turns out to be invariant under diffeomorphisms on momentum space. Both of these features are regarded as evidence of the fact that is an unphysical quantity [20]. Given that, it has been proposed to describe the phenomenon of dimensional reduction in terms of the thermal (or thermodynamical) dimension , which can be defined as the exponent of the Stefan-Boltzmann law. Then, the UV flowing of is realized through a modified dispersion relation (MDR) that affects the partition function used to compute the energy density (see [20] or Section 3 for further details). Thus, the value of near the Planck scale depends crucially on the specific form of the MDR. Furthermore, it has been recently noticed (see [21, 22]) that, from the MDR, it is also possible to infer the Hausdorff dimension of energy-momentum space. If the duality between space-time and momentum space is preserved in quantum gravity, this framework should provide another alternative characterization of the UV running. In this way, we are in presence of proliferation of distinct descriptions of the UV dimensionality of quantum space-time. These pictures make use of very different definitions of the dimension and, in principle, there is no reason why they should give the same outcome. On the other hand, they all coincide in the IR-low-energy regime where they reduce to 4 and, thus, we could expect that this should happen also in the UV.

In this paper, we show that this advisable convergence can be achieved in the semiclassical limit of LQG under rather general assumptions. The insight we gain is based on the recently proposed quantum modifications of the hypersurface-deformation algebra (or the algebra of smeared constraints) [23–27], which reduces to a correspondingly deformed Poincaré algebra in the asymptotic region, as shown in [28]. These Planckian deformations of the relativistic symmetries are a key feature of the Deformed Special Relativity scenario [29, 30], as already pointed out in [28], and, what is more, it has been recently shown in [31] that they are consistent with -Minkowski noncommutativity of the space-time coordinates [32, 33]. We here exploit them to compute the MDR, thereby linking the LQG-based quantum corrections to the deformation of the dispersion relation. The general form of the MDR we derive allows us to find that the spectral, the thermal, and the Hausdorff (notice that we are always referring to the Hausdorff dimension of momentum space since, as we mentioned, that of quantum space-time cannot be defined) dimensions follow the same UV flowing; that is, .

Another significant observation we make is that, following our analysis “in reverse,” we can get information about the LQG quantum-geometric deformations, which affect the Dirac algebra, from the value of the UV dimension. The importance of this recognition resides in the fact that these modifications are subjected to many sources of possible ambiguities [34–36] coming, for example, from the regularization techniques used to formally quantize the Hamiltonian constraint. These ambiguities are far from being resolved and it is still not clear whether they may affect potentially physical outcomes [37]. Thus, they are usually addressed only on the basis of mere theoretical arguments or being guided by a principle of technical simplification. The main sources of ambiguities are the spin representations of the quantum states of geometry as well as the choice of the space lattice and, in effective models we will here consider, they correspond, respectively, to holonomy and inverse-triad corrections. We here partially fix them with what is believed to be a phenomenological prediction, that is, the number of UV dimensions. Notably, we notice that the leading-order correction provided by the holonomy corrections of homogeneous connections [38, 39], which are often implemented by simply taking the expression instead of , for example, in Loop Quantum Cosmology (LQC) [40, 41] (see also [42] for a recent review on symmetry reduced models of LQG), is compatible with . Thus, as we would have expected, the number of dimensions is correctly flowing to lower values even if it has not already reached the value of 2, a value which is favoured in the quantum-gravity literature for the aforementioned reasons. On the basis of the steps we sketch out in the analysis, we are here reporting that it should be possible to exclude all the deformation functions that are not consistent with . Remarkably, those quantum corrections, which are related to LQC as well as to the semiclassical limit of the theory, seem to point toward the right UV flowing. As already stated, the prediction of Planckian dimensional reduction has been also confirmed by previous LQG analyses [6, 7] but more refined computations of [8] have revealed that the “magic” number of 2 can be reproduced only focusing on specific superposition of kinematical spin-networks states (see [8] for the details). Relying on the recently developed effective methods for LQG, we here provide further support to the idea that the effective space-time of LQG may be two-dimensional at ultra-Planckian scales.

2. Modified Dispersion Relation

We start considering the classical hypersurface-deformation algebra (HDA), which was first introduced by Dirac [43]. It is the set of Poisson brackets closed by the smeared constraints of the Arnowitt-Deser-Misner formulation of General Relativity (GR) [44]. The Dirac algebra of constraints is the way in which general covariance is implemented once the space-time manifold has been split into the time direction and the three spatial surfaces, that is, .

It is given by

where is the Hamiltonian (or scalar) constraint, while is the momentum (or vector) constraint. The function is called the lapse and it is needed to implement time diffeomorphisms, while is the shift vector necessary to move along a given hypersurface and, finally, is the inverse metric induced on . Thus, and have to be understood as the generators of gauge transformations which, in the case of GR, are space-time diffeomorphisms. For the purposes of our analysis, it is relevant to point out the well established fact (see [45]) that when the spatial metric is flat , if we take (where is the infinitesimal boost parameter) and (where is the matrix that generates infinitesimal rotations), we can infer the Poincaré algebra from the Dirac algebra [45]. This classical relation is expected to hold also at the quantum level.

One of the open issues in the LQG research is the search for fully quantized versions of the constraints and on a Hilbert space. While it is known how to treat spatial diffeomorphisms and also how to solve the momentum constraint [46, 47] thereby obtaining the kinematical Hilbert space of the theory, the finding of a Hamiltonian operator is far from being completed. However, over the last fifteen years, several techniques have been developed, using both effective methods and discrete operator computations. In this way, some candidates for an effective scalar constraint have been identified [48–50]. For the analysis we are here reporting, the interesting fact is that the semiclassical corrections introduced in the Hamiltonian leave trace in the algebra of constraints. Remarkably, even if these calculations use different formalism types and they are based on different assumptions, the general form of the modified HDA turns out to be the same in all these studies; that is, only the Poisson bracket between two scalar constraints is affected by quantum effects [39, 51]:

where the specific form of the deformation function as well as its dependence on the phase space variables, which are if we use the metric formulation or if we use Ashtekar’s one, varies with the quantum corrections considered to define .

One of the causes of these quantum modifications of the scalar constraint is the fact that LQG cannot be quantized directly in terms of the Ashtekar variables , which have to be replaced with their parallel propagators (or holonomies) [9, 10, 38, 39] (where is the path-ordering operator, the tangent vector to the curve , and the generators of ). If is the spatial index of a direction along which space-time is homogeneous, then one has to consider just the local point-wise holonomies (where  m is connected to the square root of the minimum eigenvalue of the area operator [41]). These are the kinds of quantum effects considered in effective (semiclassical) LQG theories as well as both in spherically reduced models and in cosmological contexts [42]. In particular, for spherically symmetric LQG (see, e.g., [28, 50, 51]), the deformation function depends on the homogeneous angular connection and it is directly related to the second derivative of the square of the holonomy correction ; that is, . Then, the important contribution of [28] has been to establish a link between these LQG-inspired quantum corrections and DSR-like deformations of the relativistic symmetries, thanks to the recognition that the angular connection is proportional to the Brown-York radial momentum [52] that generates spatial translations at infinity (see [28, 31] for the details). In fact, it has been shown that, taking the Minkowski limit of (2) as we sketched above for the classical case, the LQG-deformed HDA produces a corresponding Planckian deformation of the Poincaré algebra:

where the other commutation relations remain unmodified. Here, is the generator of radial boosts and is the energy. The explicit form of is unknown and as we already stressed it is affected by ambiguities. In light of this, for our analysis, we assume a rather general form:

which is motivated by the above considerations and, obviously, satisfies the necessary requirement: ; that is, we want to recover the standard Poincaré algebra in the continuum limit. We leave the constants of order one and that parametrize the aforementioned ambiguities unspecified. These parameters should encode at least the leading-order quantum correction to the Poincaré algebra.

Using (3) and (4) and taking into account the fact that and , a straightforward computation gives us the following MDR:

This completes the analysis started in [28] and carried on in [31], which aimed at building a bridge between the formal structures of loop quantization to the more manageable DSR scenario with the objective of enhancing the possibilities of linking mathematical constructions to observable quantities. The remarkable fact of having derived (5) from the LQG-deformed algebra of constraints (2) is that it will give us the opportunity to constrain experimentally the formal ambiguities of the LQG approach exploiting the ever-increasing phenomenological implications of MDRs (see [53] and the references therein). We are often in the situation in which quantum-gravity phenomenology misses clear derivation from full-fledged developed approaches to quantum gravity or, on the contrary, the high complexity of these formalism types does not allow inferring testable effects. Following the work initiated in [31], we are here giving a further contribution to fill this gap. We also find it interesting to notice that our MDR confirms a property of two previously proposed MDRs (see [54, 55]); that is, LQG corrections affect only the momentum sector of the dispersion relation leaving the energy dependence untouched. Therefore, this property, which has rigorous justification in the spherically symmetric framework [28, 50, 51] we are here adopting, seems to be a recurring feature of LQG. Moreover, all the precedent analyses were confined to the kinematical Hilbert space of LQG, while we have here obtained (5) from the flat-space-time limit of the full HDA including also the semiclassical Hamiltonian constraint (2). Thus, even if we are working off shell (i.e., we do not solve the constraint equations), the MDR (5) should contain at least part of the dynamical content of LQG. In the next section, we will see that the form of (5) is crucial to prove that the running of dimensions does not depend on the chosen definition of the dimension.

3. Dimensions and Quantum Corrections

Our next task is to use the MDR (5) we derived in Section 2 in order to show that, regardless of the value of the unknown parameters and , the different characterizations of the UV flowing introduced in the literature predict the same number of dimensions if we consider the effective regime of LQG in the sense introduced in [28, 50, 51] and sketched in the previous section. To see this, we start by the computation of the spectral dimension, which is defined as follows:

where is the average return probability of a diffusion process in Euclidean space-time with fictitious time . Following [20, 56–60], we compute from the Euclidean version of our MDR (5) which is a d’Alembertian operator on momentum space:

Then, a lengthy but straightforward computation (see [58–60]) leads to the following result:

Notice that the value of does not depend on but only on , that is, only on the order of Planckian correction to the dispersion relation (see (5)). We will use this fact later on.

Now we want to show that also the thermal dimension is given by (8). To this end, we recall the definition of introduced in [20]. If you have deformed Lorentzian d’Alembertian , then is the exponent of the temperature in the modified Stefan-Boltzmann law:

which can be obtained as usual deriving the logarithm of the thermodynamical partition function [20] with respect to the temperature . Evidently, in our case, we have that and and, thus, we find ; that is, the thermal dimension agrees with the spectral dimension .

Finally, we can calculate also the Hausdorff dimension of momentum space that if the duality with space-time is not broken by quantum effects should agree with both and . As pointed out in [21], a way to compute is to find a set of momenta that “linearize” the MDR. Given (5), a possible choice is given by

In terms of these new variables , the UV measure on momentum space becomes

From (11), we can read off :

which, evidently, coincides with both and . Thus, no matter which definition of dimensionality is used, in the semiclassical limit (or in symmetry reduced models) of LQG, the UV running is free of ambiguities since we have found that .

The last consideration we want to make concerns what the number of UV dimensions can teach us about LQG. In the analysis we here reported, the value of should be provided by the LQG corrections used to build , which, though, are far from being unique. On the other hand, we mentioned that the number of dimensions runs to two in the UV, a prediction that seems to be model independent. Moreover, support in LQG has been also found by the studies of [6, 8] under certain assumptions. It is evident from (8) and (12) that in order to reproduce such a shared expectation we should take . A recurring form of holonomy corrections both in spherically symmetric LQG [24, 28, 39, 61] and in LQC [40, 41] is represented by the choice that implies . In light of the above arguments, if we keep restricted to mesoscopic scales where the MDR is well approximated by the first-order correction, it is easy to realize that this implies (see [31] for the explicit computation). In this way, we would have at scales near but below the Planck scale. We find the fact that we obtain a value which is greater than 2 rather encouraging, since such an outcome may signal that the descent from the classical value of 4 to the UV value is in progress but it has not been completed yet. In fact, at ultra-Planckian energies, the Taylor expansion of the correction function in series of powers of is no more reliable and, as a consequence, it cannot fully capture the flowing of . Therefore, we are led to conclude that the much-used polymerization of homogeneous connections, which is a direct consequence of evaluating the holonomies in the fundamental representation of , realizes at least partially the expected running of dimensions. Polymerizing configuration variables is used not only in LQC and in symmetry reduced contexts but also in the definition of the semiclassical regime of LQG, which is based on the introduction of spin-network states peaked around a single representation, in the majority of cases . We have here shown that these quantum modifications can be related to the phenomenon of dimensional reduction. This link we have established gives us the possibility of constraining part of the quantization ambiguities in LQG. In fact, the value of fixes a specific choice of the parameter in (4), thereby restricting the form of the allowed deformation functions . In light of our analysis, one should select only those modifications which are compatible with the prediction of two-dimensional space-time at ultrashort distances, that is, those giving (or equivalently ) to a first approximation.

4. Outlook

In the recent quantum-gravity literature, basically three different definitions of dimension have been proposed with the aim of generalizing this notion for quantum space-time. It is well known that they all provide a possible characterization of the UV running but, in the majority of cases, they also give different outcomes for the value of the dimension. This clashes with the growing consensus on the fact that the phenomenon of dynamical dimensional reduction is a model independent feature of quantum gravity that gives the unique predictions . Thus, if , and are really proper definitions of the UV dimension, we would like to have that .

In this paper, we showed that this striking convergence can be accomplished in the case of the LQG approach. To achieve such a result, we relied on the deformations of the constraint algebra recently proposed in the framework of both effective spherically symmetric LQG and LQC. Remarkably, in the former case, it has been proven that these quantum corrections leave traces in the Minkowski limit in terms of a DSR-like Poincaré algebra where the relevant deformations are functions of the spatial momentum. We here exploited these LQG-motivated deformations of the relativistic symmetries to infer the generic form of the MDR. Interestingly, our MDR is qualitatively of the same type of the two previously proposed MDRs for LQG [54, 55]; namely, the modifications affect only the momentum sector. From the MDR, we derived the spectral, the thermal, and the Hausdorff dimensions proving that they all agree. Thus, in the top-down approach of LQG, the desirable convergence of different characterization of the concept of dimensionality is accomplished. On the other hand, the analysis we here reported may provide a guiding principle for the construction of bottom-up approaches.

Moreover, our analysis led us to give a contribution toward enforcing the fecund bond between theoretical formalism types and phenomenological predictions. In fact, we found that the simple polymerization of connections, which is much used both in midi-superspace models and in LQC where semiclassical states are exploited to compute effective constraints, is able to generate the running of the dimension. In this way, we have provided further evidence that the phenomenon of UV dimensional reduction can be realized also in the LQG approach, thereby confirming the results of previous studies. Remarkably, the value of is sensible to the specific choice of quantum corrections which are considered in the model. Therefore, we pointed out that there is an observable whose value can be used to select a particular form for the quantum correction functions, thereby reducing the LQG quantization ambiguities. In particular, we showed that the evaluation of the Hamiltonian constraint over semiclassical states peaked at (that can be also implemented with the substitution at an effective level) corresponds to . Since we inferred such a value from the parametrization of the first LQG correction (4) (which corresponds to a second-order correction in the Planck length ~ ), then it is reasonable to regard our result as a first approximation that cannot capture the ending outcome of the dimensional running. From this perspective, we observed that obtaining a dimension greater than at energies near but below the Planck scale might be significant, because it can be read as a hint that the dimension is flowing to the “magic” number of that we can expect to be reached in the deep UV. Developing the off-shell constraint algebra in full generality without any symmetrical reduction or semiclassical approximation would be of fundamental importance to extend our observations to the full LQG framework.

Competing Interests

The author declares that he has no competing interests.

Acknowledgments

The author is grateful to Giovanni Amelino-Camelia and Giorgio Immirzi for useful and critical discussions during the first stages of the elaboration of this work. He also wants to thank Gianluca Calcagni for carefully reading the paper and giving many helpful comments that improved this work.

References

J. Ambjørn, J. Jurkiewicz, and R. Loll, “Reconstructing the universe,” Physical Review D, vol. 72, no. 6, Article ID 064014, 2005.

P. Hořava, “Spectral dimension of the universe in quantum gravity at a Lifshitz point,” Physical Review Letters, vol. 102, no. 16, Article ID 161301, 4 pages, 2009.

S. Carlip, “Dimensional reduction in causal set gravity,” Classical and Quantum Gravity, vol. 32, article 23, Article ID 232001, 2015.

M. Niedermaier and M. Reuter, “The asymptotic safety scenario in quantum gravity,” Living Reviews in Relativity, vol. 9, p. 5, 2006.

D. Benedetti, “Fractal properties of quantum spacetime,” Physical Review Letters, vol. 102, no. 11, Article ID 111303, 4 pages, 2009.

L. Modesto, “Fractal spacetime from the area spectrum,” Classical and Quantum Gravity, vol. 26, no. 24, Article ID 242002, 9 pages, 2009.

G. Calcagni, D. Oriti, and J. Thürigen, “Spectral dimension of quantum geometries,” Classical and Quantum Gravity, vol. 31, no. 13, Article ID 135014, 2014.

G. Calcagni, D. Oriti, and J. Thrigen, “Dimensional flow in discrete quantum geometries,” Physical Review D, vol. 91, no. 8, Article ID 084047, 11 pages, 2015.

A. Ashtekar and J. Lewandowski, “Background independent quantum gravity: a status report,” Classical and Quantum Gravity, vol. 21, no. 15, pp. R53–R152, 2004.

C. Rovelli, “Loop quantum gravity,” Living Reviews in Relativity, vol. 11, article 5, 2008.

J. Ambjørn, A. Görlich, J. Jurkiewicz, and R. Loll, “Nonperturbative quantum gravity,” Physics Reports, vol. 519, no. 4-5, pp. 127–210, 2012.

S. Carlip, “Spontaneous dimensional reduction in short‐distance quantum gravity?” in AIP Conference Proceedings, vol. 1196, p. 72, Wroclaw, Poland, 2009.

J. Ambjorn, D. Coumbe, J. Gizbert-Studnicki, and J. Jurkiewicz, “Recent results in CDT quantum gravity,” http://arxiv.org/abs/1509.08788

O. Lauscher and M. Reuter, “Fractal spacetime structure in asymptotically safe gravity,” Journal of High Energy Physics, vol. 2005, no. 10, article 050, 2005.

G. Calcagni, A. Eichhorn, and F. Saueressig, “Probing the quantum nature of spacetime by diffusion,” Physical Review D, vol. 87, no. 12, Article ID 124028, 14 pages, 2013.

D. Benedetti and J. Henson, “Spectral geometry as a probe of quantum spacetime,” Physical Review D, vol. 80, no. 12, Article ID 13, 124036 pages, 2009.

S. Carlip, “Spontaneous dimensional reduction in quantum gravity,” Third award, 2016 Gravity Research Foundation Essay contest, https://arxiv.org/abs/1605.05694

R. Percacci and D. Perini, “On the ultraviolet behaviour of Newton's constant,” Classical and Quantum Gravity, vol. 21, no. 22, pp. 5035–5041, 2004.

T. Padmanabhan, S. Chakraborty, and D. Kothawala, “Spacetime with zero point length is two-dimensional at the Planck scale,” General Relativity and Gravitation, vol. 48, article 55, 2016.

G. Amelino-Camelia, F. Brighenti, G. Gubitosi, and G. Santos, “Thermal dimension of quantum spacetime,” https://arxiv.org/abs/1602.08020

G. Amelino-Camelia, M. Arzano, G. Gubitosi, and J. Magueijo, “Dimensional reduction in the sky,” Physical Review D—Particles, Fields, Gravitation and Cosmology, vol. 87, no. 12, Article ID 123532, 2013.

G. Amelino-Camelia, M. Arzano, G. Gubitosi, and J. Magueijo, “Planck-scale dimensional reduction without a preferred frame,” Physics Letters. B, vol. 736, pp. 317–320, 2014.

M. Bojowald, G. M. Hossain, M. Kagan, and S. Shankaranarayanan, “Anomaly freedom in perturbative loop quantum gravity,” Physical Review D. Particles, Fields, Gravitation, and Cosmology, vol. 78, no. 6, 063547, 31 pages, 2008.

T. Cailleteau, J. Mielczarek, A. Barrau, and J. Grain, “Anomaly-free scalar perturbations with holonomy corrections in loop quantum cosmology,” Classical and Quantum Gravity, vol. 29, no. 9, Article ID 095010, 17 pages, 2012.

A. Perez and D. Pranzetti, “On the regularization of the constraint algebra of quantum gravity in dimensions with a nonvanishing cosmological constant,” Classical and Quantum Gravity, vol. 27, no. 14, Article ID 145009, 2010.

C. Tomlin and M. Varadarajan, “Towards an anomaly-free quantum dynamics for a weak coupling limit of Euclidean gravity: diffeomorphism covariance,” Physical Review D, vol. 87, Article ID 044040, 2013.

A. Barrau, M. Bojowald, G. Calcagni, J. Grain, and M. Kagan, “Anomaly-free cosmological perturbations in effective canonical quantum gravity,” Journal of Cosmology and Astroparticle Physics, vol. 2015, no. 5, article 051, 2015.

M. Bojowald and G. M. Paily, “Deformed general relativity,” Physical Review D, vol. 87, Article ID 044044, 2013.

G. Amelino-Camelia, “Testable scenario for relativity with minimum length,” Physics Letters B, vol. 510, no. 1–4, pp. 255–263, 2001.

G. Amelino-Camelia, “Relativity in spacetimes with short-distance structure governed by an observer-independent (Planckian) length scale,” International Journal of Modern Physics. D. Gravitation, Astrophysics, Cosmology, vol. 11, no. 1, pp. 35–59, 2002.

G. Amelino-Camelia, M. M. Da Silva, M. Ronco, L. Cesarini, and O. M. Lecian, “Spacetime-noncommutativity regime of Loop Quantum Gravity,” https://arxiv.org/abs/1605.00497

S. Majid and H. Ruegg, “Bicrossproduct structure of κ-Poincare group and non-commutative geometry,” Physics Letters B, vol. 334, no. 3-4, pp. 348–354, 1994.

J. Lukierski, H. Ruegg, and W. J. Zakrzewski, “Classical and quantum mechanics of free κ-relativistic systems,” Annals of Physics, vol. 243, no. 1, pp. 90–116, 1995.

D.-W. Chiou and L.-F. Li, “Loop quantum cosmology with higher order holonomy corrections,” Physical Review D. Particles, Fields, Gravitation, and Cosmology, vol. 80, no. 4, 043512, 19 pages, 2009.

A. Laddha and M. Varadarajan, “Hamiltonian constraint in polymer parametrized field theory,” Physical Review D, vol. 83, Article ID 025019, 2011.

A. Corichi and P. Singh, “Is loop quantization in cosmology unique?” Physical Review D: Particles, Fields, Gravitation, and Cosmology, vol. 78, no. 2, Article ID 024034, 13 pages, 2008.

H. Nicolai, K. Peeters, and M. Zamaklar, “Loop quantum gravity: an outside view,” Classical and Quantum Gravity, vol. 22, no. 19, pp. R193–R247, 2005.

E. Wilson-Ewing, “Holonomy corrections in the effective equations for scalar mode perturbations in loop quantum cosmology,” Classical and Quantum Gravity, vol. 29, no. 8, 085005, 19 pages, 2012.

M. Bojowald and G. M. Paily, “Deformed general relativity and effective actions from loop quantum gravity,” Physical Review D, vol. 86, Article ID 104018, 2012.

A. Ashtekar and P. Singh, “Loop quantum cosmology: a status report,” Classical and Quantum Gravity, vol. 28, no. 21, 213001, 122 pages, 2011.

M. Bojowald, “Loop quantum cosmology,” Living Reviews in Relativity, vol. 8, p. 11, 2005.

A. Ashtekar, “Symmetry reduced loop quantum gravity: a bird's eye view,” https://arxiv.org/abs/1605.02648

P. A. M. Dirac, “The theory of gravitation in hamiltonian form,” Proceedings of the Royal Society of London A, vol. 246, no. 1246, 1958.

R. L. Arnowitt, S. Deser, and C. W. Misner, “Republication of: the dynamics of general relativity,” General Relativity and Gravitation, vol. 40, no. 9, pp. 1997–2027, 2008.

T. Regge and C. Teitelboim, “Role of surface integrals in the Hamiltonian formulation of general relativity,” Annals of Physics, vol. 88, pp. 286–318, 1974.

A. Ashtekar, J. Lewandowski, D. Marolf, J. Mourao, and T. Thiemann, “Quantization of diffeomorphism invariant theories of connections with local degrees of freedom,” Journal of Mathematical Physics, vol. 36, no. 11, pp. 6456–6493, 1995.

J. Lewandowski, A. Okolow, H. Sahlmann, and T. Thiemann, “Uniqueness of diffeomorphism invariant states on holonomy-flux algebras,” Communications in Mathematical Physics, vol. 267, no. 3, pp. 703–733, 2006.

M. Bojowald and R. Swiderski, “Spherically symmetric quantum geometry: hamiltonian constraint,” Classical and Quantum Gravity, vol. 23, no. 6, pp. 2129–2154, 2006.

K. Banerjee and G. Date, “Discreteness corrections to the effective Hamiltonian of isotropic loop quantum cosmology,” Classical and Quantum Gravity, vol. 22, no. 11, pp. 2017–2033, 2005.

M. Bojowald, M. Kagan, H. H. Hernández, and A. Skirzewski, “Effective constraints of loop quantum gravity,” Physical Review D: Particles, Fields, Gravitation, and Cosmology, vol. 75, no. 6, Article ID 064022, 25 pages, 2007.

S. Brahma, “Spherically symmetric canonical quantum gravity,” Physical Review D. Particles, Fields, Gravitation, and Cosmology, vol. 91, no. 12, 124003, 12 pages, 2015.

J. D. Brown and J. W. York Jr., “Quasilocal energy and conserved charges derived from the gravitational action,” Physical Review D, vol. 47, no. 4, pp. 1407–1419, 1993.

G. Amelino-Camelia, “Quantum-spacetime phenomenology,” Living Reviews in Relativity, vol. 16, p. 5, 2013.

R. Gambini and J. Pullin, “Nonstandard optics from quantum space-time,” Physical Review D, vol. 59, no. 12, Article ID 124021, 4 pages, 1999.

J. Alfaro, H. A. Morales-Técotl, and L. F. Urrutia, “Loop quantum gravity and light propagation,” Physical Review D, vol. 65, no. 10, Article ID 103509, 2002.

L. Modesto, “Spectral dimension of a quantum universe,” Physical Review D, vol. 81, Article ID 104040, 2010.

G. Calcagni, L. Modesto, and G. Nardelli, “Quantum spectral dimension in quantum field theory,” International Journal of Modern Physics D, vol. 25, no. 5, Article ID 1650058, 26 pages, 2016.

T. P. Sotiriou, M. Visser, and S. Weinfurtner, “From dispersion relations to spectral dimension—and back again,” Physical Review D, vol. 84, Article ID 104018, 2011.

M. Arzano, G. Gubitosi, J. Magueijo, and G. Amelino-Camelia, “Anti-de Sitter momentum space,” Physical Review D, vol. 92, no. 2, Article ID 024028, 12 pages, 2015.

G. Calcagni, “Diffusion in multiscale spacetimes,” Physical Review E, vol. 87, no. 1, Article ID 012123, 20 pages, 2013.

M. Campiglia, R. Gambini, J. Olmedo, and J. Pullin, “Quantum self-gravitating collapsing matter in a quantum geometry,” http://arxiv.org/abs/1601.05688