25 research outputs found
Emergence of gravity from spinfoams
We find a nontrivial regime of spinfoam quantum gravity that reproduces
classical Einstein equations. This is the double scaling limit of small Immirzi
parameter (gamma), large spins (j) with physical area (gamma times j) constant.
In addition to quantum corrections in the Planck constant, we find new
corrections in the Immirzi parameter due to the quantum discreteness of
spacetime. The result is a strong evidence that the spinfoam covariant
quantization of general relativity possesses the correct classical limit.Comment: 9 pages, shorter version of "Regge gravity from spinfoams
Regge gravity from spinfoams
We consider spinfoam quantum gravity for general triangulations in the regime
, namely in the combined classical limit of large areas
and flipped limit of small Barbero-Immirzi parameter , where
is the Planck length. Under few working hypotheses we find that the flipped
limit enforces the constraints that turn the spinfoam theory into an effective
Regge-like quantum theory with lengths as variables, while the classical limit
selects among the possible geometries the ones satisfying the Einstein
equations. Two kinds of quantum corrections appear in terms of powers of
and . The result also suggests that the
Barbero-Immirzi parameter may run to smaller values under coarse-graining of
the triangulation.Comment: 18 pages, presentation substantially improve
Fractal Space-Time from Spin-Foams
In this paper we perform the calculation of the spectral dimension of
spacetime in 4d quantum gravity using the Barrett-Crane (BC) spinfoam model. We
realize this considering a very simple decomposition of the 4d spacetime
already used in the graviton propagator calculation and we introduce a boundary
state which selects a classical geometry on the boundary. We obtain that the
spectral dimension of the spacetime runs from to 4, across a
phase, when the energy of a probe scalar field decreases from
high to low energy. The spectral dimension at the Planck
scale depends on the areas spectrum used in the calculation.
For three different spectra , and we find respectively dimension , 2.45 and 2.08.Comment: 5 pages, 2 figure
Coherent spin-networks
In this paper we discuss a proposal of coherent states for Loop Quantum
Gravity. These states are labeled by a point in the phase space of General
Relativity as captured by a spin-network graph. They are defined as the gauge
invariant projection of a product over links of Hall's heat-kernels for the
cotangent bundle of SU(2). The labels of the state are written in terms of two
unit-vectors, a spin and an angle for each link of the graph. The heat-kernel
time is chosen to be a function of the spin. These labels are the ones used in
the Spin Foam setting and admit a clear geometric interpretation. Moreover, the
set of labels per link can be written as an element of SL(2,C). Therefore,
these states coincide with Thiemann's coherent states with the area operator as
complexifier. We study the properties of semiclassicality of these states and
show that, for large spins, they reproduce a superposition over spins of
spin-networks with nodes labeled by Livine-Speziale coherent intertwiners.
Moreover, the weight associated to spins on links turns out to be given by a
Gaussian times a phase as originally proposed by Rovelli.Comment: 15 page
Coherent states for FLRW space-times in loop quantum gravity
We construct a class of coherent spin-network states that capture proprieties
of curved space-times of the Friedmann-Lama\^itre-Robertson-Walker type on
which they are peaked. The data coded by a coherent state are associated to a
cellular decomposition of a spatial (const.) section with dual graph given
by the complete five-vertex graph, though the construction can be easily
generalized to other graphs. The labels of coherent states are complex SL(2,
\mathbbm{C}) variables, one for each link of the graph and are computed
through a smearing process starting from a continuum extrinsic and intrinsic
geometry of the canonical surface. The construction covers both Euclidean and
Lorentzian signatures; in the Euclidean case and in the limit of flat space we
reproduce the simplicial 4-simplex semiclassical states used in Spin Foams.Comment: 10 pages, 1 figure, published versio
Compatibility of radial, Lorenz and harmonic gauges
We observe that the radial gauge can be consistently imposed \emph{together}
with the Lorenz gauge in Maxwell theory, and with the harmonic traceless gauge
in linearized general relativity. This simple observation has relevance for
some recent developments in quantum gravity where the radial gauge is
implicitly utilized.Comment: 9 pages, minor changes in the bibliograph
Spinfoams in the holomorphic representation
We study a holomorphic representation for spinfoams. The representation is
obtained via the Ashtekar-Lewandowski-Marolf-Mour\~ao-Thiemann coherent state
transform. We derive the expression of the 4d spinfoam vertex for Euclidean and
for Lorentzian gravity in the holomorphic representation. The advantage of this
representation rests on the fact that the variables used have a clear
interpretation in terms of a classical intrinsic and extrinsic geometry of
space. We show how the peakedness on the extrinsic geometry selects a single
exponential of the Regge action in the semiclassical large-scale asymptotics of
the spinfoam vertex.Comment: 10 pages, 1 figure, published versio
Asymptotics of LQG fusion coefficients
The fusion coefficients from SO(3) to SO(4) play a key role in the definition
of spin foam models for the dynamics in Loop Quantum Gravity. In this paper we
give a simple analytic formula of the EPRL fusion coefficients. We study the
large spin asymptotics and show that they map SO(3) semiclassical intertwiners
into semiclassical intertwiners. This non-trivial
property opens the possibility for an analysis of the semiclassical behavior of
the model.Comment: 14 pages, minor change