Loop quantum gravity

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Loop quantum gravity (LQG), also known as loop gravity and quantum geometry, is a proposed quantum theory of spacetime which attempts to reconcile the theories of quantum mechanics and general relativity. It preserves many of the important features of general relativity, while at the same time employing quantization of both space and time at the Planck scale in the tradition of quantum mechanics. The technique of loop quantization was developed for the nonperturbative quantization of diffeomorphism-invariant gauge theory. Roughly, LQG tries to establish a quantum theory of gravity in which the very space, where all other physical phenomena occurs, becomes quantized.

LQG is one of a family of theories called canonical quantum gravity. A list of quantum gravity theories can be found on the quantum gravity page. The LQG theory includes also matter and forces, but the theory does not address the problem of the unification of all physical forces, as other tentative quantum gravity theories do (for instance string theory).

Contents

Loop quantum gravity in general, and its ambitions

Though not proven, it may be impossible to quantize gravity in 3+1 dimensions without creating matter and energy artifacts. Should LQG succeed as a quantum theory of gravity, the known matter fields will have to be incorporated into the theory a posteriori. Many of the approaches now being actively pursued (by Loll, Smolin, Bilson-Thompson, Freidel, Wise and others) combine matter with geometry. Several of these current efforts would be proven wrong if evidence were found of extra spatial dimensions.

The main successes of loop quantum gravity are:

1. It is a nonperturbative quantization of 3-space geometry, with quantized area and volume operators.

2. It includes a calculation of the entropy of black holes.

3. It replaces the Big Bang spacetime singularity with a Big Bounce.

These claims are not universally accepted among the physics community, which is presently divided between different approaches to the problem of quantum gravity. Many of the core results are rigorous mathematical physics, their physical interpretations remain speculative. LQG may possibly be viable as a refinement of either gravity or geometry. It has not been shown that loop quantum gravity reproduces general relativity as a low energy limit.

There are several other approaches to quantum gravity, such as spin foam models, are closely related to loop quantum gravity.

The apparent incompatibility between quantum mechanics and general relativity

Main article: quantum gravity

In general relativity, the Einstein field equations assign a geometry (via a metric) to space-time. Before this, there is no physical notion of distance or time measurements. In this sense, general relativity is said to be background independent. An immediate conceptual issue that arises is that the usual framework of quantum mechanics, including quantum field theory, relies on a reference (background) space-time. Therefore, one approach to finding a quantum theory of gravity is to understand how to do quantum mechanics without relying on such a background; this is the approach of the canonical quantization/loop quantum gravity/spin foam approaches.

Furthermore, in the framework of quantum field theory, and using the standard techniques of perturbative calculations, one finds that gravitation is non-renormalizable in contrast to the electroweak and strong interactions of the Standard Model of particle physics. This technical term implies that there are infinitely many free parameters in the theory and thus that it cannot be predictive.

Another interface between general relativity and quantum mechanics occurs in quantum field theory studied on curved (non-Minkowskian) backgrounds. The vacuum, when it exists, is shown in general relativity to depend on the path of the observer through space-time (see Unruh effect). The Unruh effect can be described semi-classically in the case of a fixed background geometry on which propagate non-gravitational quantum mechanical particles (quanta). It's then natural to wonder about the inclusion of quantum gravitational effects, including interactions with the graviton (in analogy with the electron's interactions with the electromagnetic field of the nucleus within an atom).

History of LQG

Main article: history of loop quantum gravity

In 1986, Abhay Ashtekar reformulated Einstein's field equations of general relativity, using what have come to be known as Ashtekar variables, a particular flavor of Einstein-Cartan theory with a complex connection. In 1988, Carlo Rovelli and Lee Smolin used this formalism to introduce the loop representation of quantum general relativity, which was soon developed by Ashtekar, Rovelli, Smolin and many others. In the Ashtekar formulation, the fundamental objects are a rule for parallel transport (technically, a connection) and a coordinate frame (called a vierbein) at each point. Because the Ashtekar formulation was background-independent, it was possible to use Wilson loops as the basis for a nonperturbative quantization of gravity. Explicit (spatial) diffeomorphism invariance of the vacuum state plays an essential role in the regularization of the Wilson loop states.

Around 1990, Carlo Rovelli and Lee Smolin obtained an explicit basis of states of quantum geometry, which turned out to be labelled by Penrose's spin networks, and showed that the geometry is quantized, that is, the (non-gauge-invariant) quantum operators representing area and volume have a discrete spectrum. In this context, spin networks arose as a generalization of Wilson loops necessary to deal with mutually intersecting loops. Mathematically, spin networks are related to group representation theory and can be used to construct knot invariants such as the Jones polynomial.

The ingredients of loop quantum gravity

Loop quantization

At the core of loop quantum gravity is a framework for nonperturbative quantization of diffeomorphism-invariant gauge theories, which one might call loop quantization. While originally developed in order to quantize vacuum general relativity in 3+1 dimensions, the formalism can accommodate arbitrary spacetime dimensionalities, fermions, an arbitrary gauge group (or even quantum group), and supersymmetry, and results in a quantization of the kinematics of the corresponding diffeomorphism-invariant gauge theory. Much work remains to be done on the dynamics, the classical limit and the correspondence principle, all of which are necessary in one way or another to make contact with experiment.

In a nutshell, loop quantization is the result of applying C*-algebraic quantization to a non-canonical algebra of gauge-invariant classical observables. Non-canonical means that the basic observables quantized are not generalized coordinates and their conjugate momenta. Instead, the algebra generated by spin network observables (built from holonomies) and field strength fluxes is used.

Loop quantization techniques are particularly successful in dealing with topological quantum field theories, where they give rise to state-sum/spin-foam models such as the Turaev-Viro model of 2+1 dimensional general relativity. A much studied topological quantum field theory is the so-called BF theory in 3+1 dimensions. Since classical general relativity can be formulated as a BF theory with constraints, scientists hope that a consistent quantization of gravity may arise from the perturbation theory of BF spin-foam models.

This discrete structure may require modifications of quantum mechanics, and a line of research called polymer quantum mechanics has been pursued.

Lorentz invariance

Main article: Lorentz covariance

LQG is a quantization of a classical Lagrangian field theory which is equivalent to the usual Einstein-Cartan theory in that it leads to the same equations of motion describing general relativity with torsion. As such, it can be argued that LQG respects local Lorentz invariance. Global Lorentz invariance is broken in LQG just as in general relativity. A positive cosmological constant can be realized in LQG by replacing the Lorentz group with the corresponding quantum group.

Diffeomorphism invariance and background independence

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General covariance is the invariance of physical laws under arbitrary coordinate transformations. This condition is most noteworthy in the context of general relativity where it has some profound implications, as Einstein discovered. The argument involves only the very basics of GR, as we will see below. More details and discussions can be found in Rovelli's book or the papers by Rovelli and Gaul and by Smolin.

It begins with a mathematical observation. Here is written the differential equation for the simple harmonic oscillator twice

 \frac{d^2 f(x)}{dx^2} + f(x) = 0  \frac{d^2 g(y)}{dy^2} + g(y) = 0

except in Eq(1) the independent variable is x and in Eq(2) the independent variable is y. Once we find out that a solution to Eq(1) is f(x) = cosx, we immediately know that g(y) = cosy solves Eq(2). This observation combined with general covariance has profound implications for GR.

\tilde{g}_{ab}
\tilde{g}_{ab}(P) = g_{ab}(P_0)

(see figure 1(a)). Now consider a coordinate system which assigns to P the same coordinate values that P0 has in the x-coordinates (see figure 1(b)). We then have

Eq(4)  \tilde{g}_{ab} (y_0=u_0,y_1=u_1, y_2=u_2, y_3=u_3) = g_{ab}
(x_0=u_0,x_1=u_1, x_2=u_2 , x_3=u_3),

where u0,u1,u2,u3 are the coordinate values of P0 in the x-coordinate system.

Figure 1Figure 1

When we allow the coordinate values to range over all permissible values, Eq(4) is precisely the condition that the two metric functions have the same functional form! We see that the new solution is generated by dragging the original metric function over the spacetime manifold while keeping the coordinate lines "attached", see Fig 1. It is important to realise that we are not performing a coordinate transformation here, this is what's known as an active diffeomorphism (coordinate transformations are called passive diffeomorphisms). It should be easy to see that when we have matter present, simultaneously performing an active diffeomorphism on the gravitational and matter fields generates the new distinct solution.

The resolution to the hole argument (mainly taken from Rovelli's book) is as follows. As GR does not determine the distance between spacetime points, how the gravitational and matter fields are located over spacetime, and so the values they take at spacetime points, can have no physical meaning. What GR does determine, however, are the mutual relations that exist between the gravitational field and the matter fields (i.e. the value the gravitational field takes where the matter field takes such and such value). From these mutual relations we can form a notion of matter being located with respect to the gravitational field and vice-versa, (see Rovelli's for exposition). What Einstein discovered was that physical entities are located with respect to one another only and not with respect to the spacetime manifold. This is what background independence is! And that is the context for Einstein's remark "beyond my wildest expectations".

Since the Hole Argument is a direct consequence of the general covariance of GR, this led Einstein to state:

"That this requirement of general covariance, which takes away from space and time the last remnant of physical objectivity, is a natural one, ..."

LQG preserves this symmetry under active diffeomorphisms by requiring that the physical states remain invariant under the generators of active diffeomorphisms. The interpretation of this condition is well understood for purely spatial active diffeomorphisms. However, the understanding of active diffeomorphisms involving time (the Hamiltonian constraint) is more subtle because it is related to dynamics and the so-called problem of time in general relativity. A generally accepted calculational framework to account for this constraint is yet to be found.

The term "active diffeomorphism" has been used, instead of just "diffeomorphism", to emphasize that this is not a case of simple coordinate transformations. It is active diffeomorphisms which are the gauge transformations of GR and they should not be confused with the freedom of choosing coordinates on the space-time M. Invariance under coordinate transformations is not a special feature of GR as all physical theories are invariant under coordinate transformations. (Indeed, the mathematical definition of a diffeomorphism is a transformation which relates manifolds with equivalent topological and differentiable structure, but not necessarily equivalent metrics. For example, a diffeomorphism can turn a doughnut into a tea cup.)

Whether or not Lorentz invariance is broken in the low-energy limit of LQG, the theory is formally background independent. The equations of LQG are not embedded in, or presuppose, space and time, except for its invariant topology. Instead, they are expected to give rise to space and time at distances which are large compared to the Planck length. At present, it remains unproven that LQG's description of spacetime at the Planckian scale has the right continuum limit, described by general relativity with possible quantum corrections.

LQG and the big bang singularity

Main article: loop quantum cosmology

Abhay Ashtekar and Martin Bojowald have released papers stating that according to loop quantum gravity, the singularity of the Big Bang is avoided. What the researchers found was a prior collapsing universe. Since gravity becomes repulsive near Planck density according to their simulations, this resulted in a "Big Bounce" and the birth of our current universe. These topics are an active research in loop quantum cosmology. However these results involve a truncation of the theory and so do not properly apply to loop quantum gravity itself.

LQG and particle physics

Main article: preon

There have been recent claims that loop quantum gravity may be able to reproduce features resembling the Standard Model. So far only the first generation of fermions (leptons and quarks) with correct parity properties have been modelled by Sundance Bilson-Thompson using preons constituted of braids of spacetime as the building blocks. However, there is no derivation of the Lagrangian that would describe the interactions of such particles, nor is it possible to show that such particles are fermions, nor that the gauge groups or interactions of the Standard Model are realised. Utilization of quantum computing concepts made it possible to demonstrate that the particles are able to survive quantum fluctuations. Other recent results suggest that LQG's framework may allow for the derivation of certain spin-1 bosons such as the photon, and gluon, and possibly the spin-2 graviton. This line of research follows the reductionist paradigm of finding a building block of elementary particles.

Independent of the above discussion, there exist various proposals on how to incorporate fermions (matter) within LQG's framework. A single framework that can account for the standard model and gravity is known in physics as a theory of everything.

It currently appears that nothing forbids coupling anomalous - i.e. quantum mechanically inconsistent - chiral fermions to LQG [citation needed].

LQG and the Graviton

There have been recent results in LQG using the spinfoam formalism by Carlo Rovelli, Eugenio Bianchi, Leonardo Modesto, and Simone Spezialethat LQG does give rise to gravitons, and allows gravitons to interact as expected, reproducing Newton's law of gravity.

The Kodama state

Main article: Immirzi parameter

In 1988, Hideo Kodama wrote down the equations of the Kodama state, but as it described a positive (de Sitter universe) spacetime, which was believed to be inconsistent with observation, it was largely ignored.

Lee Smolin's paper, "Quantum gravity with a positive cosmological constant" suggests that the Kodama state is a ground state which has a good semiclassical limit which reproduces the dynamics of general relativity with a positive (de Sitter) cosmological constant, 4 dimensions, and gravitons, and is an exact solution to ordinary constraints on background independent quantum gravity, providing evidence that loop quantum gravity is indeed a quantum gravity with the correct semiclassical description. Edward Witten published a paper titled "A Note On The Chern-Simons And Kodama Wavefunctions" in response to Lee Smolin's, arguing that the Kodama state is unphysical, due to an analogy to a state in Chern-Simons theory wavefunction resulting in negative energies, and citing Smolin's paper. Recently, Andrew Randono has published two papers that cite Witten's paper, and address these objections, by generalizing the Kodama state, with the conclusion that the Immirzi parameter, when generalized with a real value, fixed by matching with black hole entropy, describes parity violation in quantum gravity, and is CPT invariant, and is normalizable, and chiral, consistent with known observations of both gravity and quantum field theory. Randono claims that Witten's conclusions rest on the immirizi parameter taking on an imaginary number, which simplifies the equation. The physical inner product may resemble the MacDowell-Mansouri action formulation of gravity.

Spinfoam

Main article: spin foam

Spinfoam may be regarded as the path integral formulation of LQG. There have been results to show that in 2+1 dimensions, LQG and spin foam are exactly equivalent, , but spin foam models based on the Barrett-Crane model are known to be inequivalent to 3+1 Hamiltonian formulation. Rovelli has provided results with a modified spin foam, one that incorporates an immirizi parameter, is equivalent in spinfoam in 3+1 dimensions. .

non commutative geometry and loop gravity

Main article: Noncommutative standard model

Non commutative geometry and loop quantum gravity may be linked, according to recent papers published by Johannes Aastrup, Jesper M. Grimstrup, Ryszard Nest. , as well as Abhay Ashtekar . Should this research program succeed, Alaine Conne's Noncommutative geometry would give gravity and the standard model, with LQG providing techniques to quantize the gravity. LQG on a noncommutative space may have the standard model, hence making it a candidate theory of everything.

LQG and analogues to condensed matter physics

Condensed matter physics is the field of physics that deals with the macroscopic physical properties of matter. In particular, it is concerned with the "condensed" phases that appear whenever the number of constituents in a system is extremely large and the interactions between the constituents are strong.

Loop quantum gravity offers a candidate spacetime atom, the spin network, that may strongly interact with one another quantum mechanically. There maybe 10^99 spin network units in a volume contained by a hydrogen atom, a number far in excess to the 10^28 atoms present in a molar amount of a substance. There have been two research programs, "quantum graphity" and group field theory" that attempt to apply principles and mechanisms that condensed matter physics uses when they apply it to matter. There are two outstanding issues in loop quantum gravity -- incorporating the standard model within its framework, or even better, deriving the standard model, and explaining how a continuous spacetime emerges from a discrete model. The two may be interrelated, and perhaps condensed matter physics mechanisms may play an analogous role. There has been an increasing interest and research programs in the loop quantum gravity community to appropriate results from condensed matter physics analogues. Various forms of topological order may give rise to some features of the standard model through string nets, and group field theory may model continuous spacetime from discrete atoms as a Bose Einstein condensate. Interestingly, both group field theory and quantum graphity make use of bosonic systems, rather than fermionic.

LQG and string nets

Main article: string-net

MIT's Xiao-Gang Wen and Harvard University's Michael Levin are two condensed matter physics researchers who have attempted to model elementary particles such as electrons and photons as resulting from a discrete lattice structure of spacetime in analogy to phonons in solid state physics. They attempt to model elementary particles as emergent properties of a string-net condensation based on a mechanism called topological order in condensed matter physics, and LQG's spin networks have the properties necessary to reproduce the standard model as the result of the collective behavior of a group of spin networks. This approach differs from the preon approach, in that Wen and Levin see particles as an emergent property of quantum spacetime, rather than built up of smaller substructures as is the case with Bilson-Thompson's preon theory.

The project to embed topological order in loop quantum gravity is called quantum graphity, and Tomasz Konopka, Fotini Markopoulou and Simone Severini have argued that loop quantum gravity's spin networks are equivalent to Wen and Levin's string net condensation, and give rise directly to U(1) gauge charge and electrons. In the quantum graphity model, points in spacetime are represented by nodes on a graph connected by links that can be on or off. This indicates whether or not the two points are directly connected as if they are next to each other in spacetime. When they are on the links have additional state variables which are used to define the random dynamics of the graph under the influence of quantum fluctuations and temperature. At high temperature the graph is in Phase I where all the points are randomly connected to each other and no concept of spacetime as we know it exists. As the temperature drops and the graph cools, it is conjectured to undergo a phase transition to a Phase II where spacetime forms. It will then look like a spacetime manifold on large scales with only near-neighbour points being connected in the graph. The hypothesis of quantum graphity is that this geometrogenesis models the condensation of spacetime in the big bang.

LQG and group field theory

Einstein's theory of spacetime, general relativity, describes spacetime as a continuum, whereas loop quantum gravity describes the quanta of spacetime as discrete. There is some analogy to fluids, which can often be approximated as continuous, even if they are actually made of discrete atoms. Daniele Oriti has proposed group field theory as an approach to derive a classical, continuous spacetime from a discrete atomic manner in analogy to mechanisms found in condensed matter physics, and suggests that spin networks can undergo a condensation that is analogous to a Bose Einstein condensate as an example of a transition from discrete to continuous.

Problems

While there has been a recent proposal relating to observation of naked singularities, and doubly special relativity, as a part of a program called loop quantum cosmology, as of now there is no experimental observation for which loop quantum gravity makes a prediction not made by the Standard Model or general relativity. This problem plagues all current theories of quantum gravity (except those that have been proven wrong).

Making predictions from the theory of LQG has been extremely difficult computationally, also a recurring problem with modern theories in physics.

Another problem is that a crucial free parameter in the theory known as the Immirzi parameter can only be computed by demanding agreement with Bekenstein and Hawking's calculation of the black hole entropy. Loop quantum gravity predicts that the entropy of a black hole is proportional to the area of the event horizon, but does not obtain the Bekenstein-Hawking formula S = A/4 unless the Immirzi parameter is chosen to give this value. A prediction directly from theory would be preferable.

Presently, no semiclassical limit recovering general relativity has been shown to exist.