| View Poll Results: Which paper(s) will contribute most significantly to future research? | |||
| A positive formalism for quantum theory in the generalized boundary formulation |
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0 | 0% |
| Gravitational origin of the weak interaction's chirality |
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2 | 15.38% |
| On the Architecture of Spacetime Geometry |
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5 | 38.46% |
| Black Hole Entropy from complex Ashtekar variables |
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4 | 30.77% |
| Asymptotic silence in loop quantum cosmology |
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1 | 7.69% |
| Primordial tensor power spectrum in holonomy corrected Omega-LQC |
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1 | 7.69% |
| A "Helium Atom" of Space: Dynamical Instability of the Isochoric Pentahedron |
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2 | 15.38% |
| Pentahedral volume, chaos, and quantum gravity |
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2 | 15.38% |
| The Matter Bounce Scenario in Loop Quantum Cosmology |
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2 | 15.38% |
| Holonomy-flux spinfoam amplitude |
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1 | 7.69% |
| The spin connection of twisted geometry |
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5 | 38.46% |
| An Extension of the Quantum Theory of Cosmological Perturbations to the Planck Era |
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2 | 15.38% |
| Schwinger-Dyson Equations in Group Field Theories of Quantum Gravity |
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0 | 0% |
| Horizon entanglement entropy and universality of the graviton coupling |
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2 | 15.38% |
| Emergent Isotropy-Breaking in Quantum Cosmology |
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0 | 0% |
| Pure connection formalism for gravity: Feynman rules and the graviton-graviton scattering |
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1 | 7.69% |
| Geometric asymptotics for spin foam lattice gauge gravity on arbitrary triangulations |
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1 | 7.69% |
| A new perspective on cosmology in Loop Quantum Gravity |
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4 | 30.77% |
| Interpretation of the triad orientations in loop quantum cosmology |
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2 | 15.38% |
| Multiple Choice Poll. Voters: 13. You may not vote on this poll | |||
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Our picks for fourth quarter 2012 MIP (most important QG paper) |
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| Mar6-13, 04:59 PM | #18 |
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Our picks for fourth quarter 2012 MIP (most important QG paper)
Cordial thanks! to Adpc, Atyy, Chronos, Demystifier, Devils, Erkant, Julcab12, Nonlinear, and Skydive Phil. It can be instructive to see what others have identified as especially significant research. I often find myself taking a second look at a paper others of us pick, to better understand its potential importance.
Here's how the votes currently stack up: Four votes: http://arxiv.org/abs/1212.5183 On the Architecture of Spacetime Geometry Eugenio Bianchi, Robert C. Myers http://arxiv.org/abs/1212.4060 Black Hole Entropy from complex Ashtekar variables Ernesto Frodden, Marc Geiller, Karim Noui, Alejandro Perez http://arxiv.org/abs/1211.2166 The spin connection of twisted geometry Hal M. Haggard, Carlo Rovelli, Francesca Vidotto, Wolfgang Wieland Two votes: http://lanl.arxiv.org/abs/1212.1930 A "Helium Atom" of Space: Dynamical Instability of the Isochoric Pentahedron Christopher E. Coleman-Smith, Berndt Müller http://arxiv.org/abs/1211.7311 Pentahedral volume, chaos, and quantum gravity Hal M. Haggard http://arxiv.org/abs/1211.6269 The Matter Bounce Scenario in Loop Quantum Cosmology Edward Wilson-Ewing http://arxiv.org/abs/1211.1354 An Extension of the Quantum Theory of Cosmological Perturbations to the Planck Era Ivan Agullo, Abhay Ashtekar, William Nelson http://arxiv.org/abs/1211.0522 Horizon entanglement entropy and universality of the graviton coupling Eugenio Bianchi http://arxiv.org/abs/1210.4504 A new perspective on cosmology in Loop Quantum Gravity Emanuele Alesci, Francesco Cianfrani http://arxiv.org/abs/1210.0418 Interpretation of the triad orientations in loop quantum cosmology Claus Kiefer, Christian Schell Plus six that I didn't list here, each of which only got ONE vote, so far. |
| Mar15-13, 12:52 PM | #19 |
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Keeping the first quarter 2013 list up to date in view of the upcoming MIP poll, here are a few Loop and allied papers of special interest. For compactness I've omitted the abstracts of papers listed earlier. 17 papers so far. The list is provisional and may be shortened.
http://arxiv.org/abs/1303.3576 Cosmology from Group Field Theory Steffen Gielen, Daniele Oriti, Lorenzo Sindoni (Submitted on 14 Mar 2013) We identify a class of condensate states in the group field theory (GFT) approach to quantum gravity that can be interpreted as macroscopic homogeneous spatial geometries. We then extract the dynamics of such condensate states directly from the fundamental quantum GFT dynamics, following the procedure used in ordinary quantum fluids. The effective dynamics is a non-linear and non-local extension of quantum cosmology. We also show that any GFT model with a kinetic term of Laplacian type gives rise, in a semi-classical (WKB) approximation and in the isotropic case, to a modified Friedmann equation. This is the first concrete, general procedure for extracting an effective cosmological dynamics directly from a fundamental theory of quantum geometry. 5 pages http://arxiv.org/abs/1303.2773 BTZ Black Hole Entropy in Loop Quantum Gravity and in Spin Foam Models J.Manuel Garcia-Islas (Submitted on 12 Mar 2013) We present a comparison of the calculation of BTZ black hole entropy in loop quantum gravity and in spin foam models. We see that both give the same answer. 6 pages, 3 figures http://arxiv.org/abs/1303.1687 Quantum states of the bouncing universe Jean Pierre Gazeau, Jakub Mielczarek, Wlodzimierz Piechocki (Submitted on 7 Mar 2013) In this paper we study quantum dynamics of the bouncing cosmological model. We focus on the model of the flat Friedman-Robertson-Walker universe with a free scalar field. The bouncing behavior, which replaces classical singularity, appears due to the modification of general relativity along the methods of loop quantum cosmology. We show that there exist a unitary transformation that enables to describe the system as a free particle with Hamiltonian equal to canonical momentum. We examine properties of the various quantum states of the Universe: boxcar state, standard coherent state, and soliton-like state, as well as Schrödinger's cat states constructed from these states. Characteristics of the states such as quantum moments and Wigner functions are investigated. We show that each of these states have, for some range of parameters, a proper semiclassical limit fulfilling the correspondence principle. Decoherence of the superposition of two universes is described and possible interpretations in terms of triad orientation and Belinsky-Khalatnikov-Lifshitz conjecture are given. Some interesting features regarding the area of the negative part of the Wigner function have emerged. 18 pages, 19 figures http://arxiv.org/abs/1303.0752 Inclusion of matter in inhomogeneous loop quantum cosmology Daniel Martín-de Blas, Mercedes Martín-Benito, Guillermo A. Mena Marugán (Submitted on 4 Mar 2013) We study the hybrid quantization of the linearly polarized Gowdy T3 model with a massless scalar field with the same symmetries as the metric. For simplicity, we quantize its restriction to the model with local rotational symmetry. Using this hybrid approach, the homogeneous degrees of freedom of the geometry are quantized ŕ la loop, leading to the resolution of the cosmological singularity. A Fock quantization is employed both for the matter and the gravitational inhomogeneities. Owing to the inclusion of the massless scalar field this system allows us to modelize flat Friedmann-Robertson-Walker cosmologies filled with inhomogeneities propagating in one direction, providing a perfect scenario to study the quantum back-reaction of the inhomogeneities on the polymeric homogeneous and isotropic background. 4 pages http://arxiv.org/abs/1303.0195 Living in Curved Momentum Space J. Kowalski-Glikman http://arxiv.org/abs/1302.7142 Holonomy Operator and Quantization Ambiguities on Spinor Space Etera R. Livine http://arxiv.org/abs/1302.7037 Loop Quantization of Shape Dynamics Tim Koslowski http://arxiv.org/abs/1302.5265 The loop quantum gravity black hole Rodolfo Gambini, Jorge Pullin http://arxiv.org/abs/1302.3833 Loop Quantum Cosmology Ivan Agullo, Alejandro Corichi http://arxiv.org/abs/1302.1781 Self-Energy in the Lorentzian ERPL-FK Spin Foam Model of Quantum Gravity Aldo Riello http://arxiv.org/abs/1302.0724 Death and resurrection of the zeroth principle of thermodynamics Hal M. Haggard, Carlo Rovelli http://arxiv.org/abs/1302.0254 The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations Ivan Agullo, Abhay Ashtekar, William Nelson http://arxiv.org/abs/1301.6210 Embedding loop quantum cosmology without piecewise linearity Jonathan Engle http://arxiv.org/abs/1301.5859 Hamiltonian spinfoam gravity Wolfgang M. Wieland http://arxiv.org/abs/1301.3480 Gauge networks in noncommutative geometry Matilde Marcolli, Walter D. van Suijlekom http://arxiv.org/abs/1301.2245 Quantum-Reduced Loop Gravity: Cosmology Emanuele Alesci, Francesco Cianfrani http://arxiv.org/abs/1301.1264 Inflation as a prediction of loop quantum cosmology Linda Linsefors, Aurelien Barrau |
| Mar15-13, 01:11 PM | #20 |
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Hmmm, My choice is #2 On the Architecture of Spacetime Geometry. It has the most promising title imo.
![]() Sorry to have skewed the results
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| Mar22-13, 11:27 PM | #21 |
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Thanks for registering your choice, nitsuJ--however you arrived at your decision, I think it's a good pick!
In preparation for the upcoming MIP poll, here are a few Loop and allied papers of special interest. For compactness I've omitted the abstracts of papers listed earlier. The list of 19 papers is provisional and may be shortened. http://arxiv.org/abs/1303.4989 Loop Quantum Gravity and the The Planck Regime of Cosmology Abhay Ashtekar (Submitted on 20 Mar 2013) The very early universe provides the best arena we currently have to test quantum gravity theories. The success of the inflationary paradigm in accounting for the observed inhomogeneities in the cosmic microwave background already illustrates this point to a certain extent because the paradigm is based on quantum field theory on the curved cosmological space-times. However, this analysis excludes the Planck era because the background space-time satisfies Einstein's equations all the way back to the big bang singularity. Using techniques from loop quantum gravity, the paradigm has now been extended to a self-consistent theory from the Planck regime to the onset of inflation, covering some 11 orders of magnitude in curvature. In addition, for a narrow window of initial conditions, there are departures from the standard paradigm, with novel effects, such as a modification of the consistency relation involving the scalar and tensor power spectra and a new source for non-Gaussianities. Thus, the genesis of the large scale structure of the universe can be traced back to quantum gravity fluctuations in the Planck regime. This report provides a bird's eye view of these developments for the general relativity community. 23 pages, 4 figures. Plenary talk at the Conference: Relativity and Gravitation: 100 Years after Einstein in Prague. To appear in the Proceedings to be published by Edition Open Access. Summarizes results that appeared in journal articles [2-13] http://arxiv.org/abs/1303.4752 Imaginary action, spinfoam asymptotics and the 'transplanckian' regime of loop quantum gravity Norbert Bodendorfer, Yasha Neiman (Submitted on 19 Mar 2013) It was recently noted that the on-shell Einstein-Hilbert action with York-Gibbons-Hawking boundary term has an imaginary part, proportional to the area of the codimension-2 surfaces on which the boundary normal becomes null. We extend this result to first-order formulations of gravity, by generalizing a previously proposed boundary term to closed boundaries. As a side effect, we settle the issue of the Holst modification vs. the Nieh-Yan density by demanding a well-defined variational principle. We then set out to find the imaginary action in the large-spin 4-simplex limit of the Lorentzian EPRL/FK spinfoam. It turns out that the spinfoam's effective action indeed has the correct imaginary part, but only if the Barbero-Immirzi parameter γ is set to ± i after the quantum calculation. An interpretation and a connection to other recent results is discussed. In particular, we propose that the large-spin limit of loop quantum gravity can be viewed as a high-energy 'transplanckian' regime. 22 pages, 5 figures http://arxiv.org/abs/1303.4636 Spin foams Jonathan Engle (Submitted on 19 Mar 2013) The spin foam framework provides a way to define the dynamics of canonical loop quantum gravity in a spacetime covariant way, by using a path integral over histories of quantum states which can be interpreted as 'quantum space-times'. This chapter provides a basic introduction to spin foams aimed principally at beginning graduate students and, where possible, at broader audiences. 32 pages, 14 figures, 2 tables, to appear as a chapter of "The Springer Handbook of Spacetime," edited by A. Ashtekar and V. Petkov (Springer-Verlag 2013) http://arxiv.org/abs/1303.3576 Cosmology from Group Field Theory Steffen Gielen, Daniele Oriti, Lorenzo Sindoni http://arxiv.org/abs/1303.2773 BTZ Black Hole Entropy in Loop Quantum Gravity and in Spin Foam Models J.Manuel Garcia-Islas http://arxiv.org/abs/1303.0752 Inclusion of matter in inhomogeneous loop quantum cosmology Daniel Martín-de Blas, Mercedes Martín-Benito, Guillermo A. Mena Marugán http://arxiv.org/abs/1303.0195 Living in Curved Momentum Space J. Kowalski-Glikman http://arxiv.org/abs/1302.7142 Holonomy Operator and Quantization Ambiguities on Spinor Space Etera R. Livine http://arxiv.org/abs/1302.7037 Loop Quantization of Shape Dynamics Tim Koslowski http://arxiv.org/abs/1302.5265 The loop quantum gravity black hole Rodolfo Gambini, Jorge Pullin http://arxiv.org/abs/1302.3833 Loop Quantum Cosmology Ivan Agullo, Alejandro Corichi http://arxiv.org/abs/1302.1781 Self-Energy in the Lorentzian ERPL-FK Spin Foam Model of Quantum Gravity Aldo Riello http://arxiv.org/abs/1302.0724 Death and resurrection of the zeroth principle of thermodynamics Hal M. Haggard, Carlo Rovelli http://arxiv.org/abs/1302.0254 The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations Ivan Agullo, Abhay Ashtekar, William Nelson http://arxiv.org/abs/1301.6210 Embedding loop quantum cosmology without piecewise linearity Jonathan Engle http://arxiv.org/abs/1301.5859 Hamiltonian spinfoam gravity Wolfgang M. Wieland http://arxiv.org/abs/1301.3480 Gauge networks in noncommutative geometry Matilde Marcolli, Walter D. van Suijlekom http://arxiv.org/abs/1301.2245 Quantum-Reduced Loop Gravity: Cosmology Emanuele Alesci, Francesco Cianfrani http://arxiv.org/abs/1301.1264 Inflation as a prediction of loop quantum cosmology Linda Linsefors, Aurelien Barrau |
| Mar24-13, 05:32 PM | #22 |
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It would be nice if the voters justified their choice. My criteria are that the paper should explain the connection of quantum mechanics to general relativity in an unambiguous way. And if GR is a quantum phenomenon what does that say about QM of matter (can it shed some light).
It is not clear to me if any of the papers does that, but they express GR (without matter) in a statistical manner with emphasis on black hole entropy which seems like a very narrow goal. Even LQC looks very artificial. At least in string theory you can see the connection much better. |
| Mar24-13, 05:41 PM | #23 |
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Recognitions:
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BTW, Myers is a string theorist. |
| Mar27-13, 11:28 AM | #24 |
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Here, for the upcoming first quarter 2013 MIP poll, I've listed 20 Loop and allied QG papers of special interest. For compactness I've omitted the abstracts shown earlier. The list is provisional and may be shortened. http://arxiv.org/abs/1303.6157 Loop quantum dynamics of the gravitational collapse Yaser Tavakoli, Joao Marto, Andrea Dapor (Submitted on 25 Mar 2013) We consider a quantum description for a spherically symmetric gravitational collapse of a massless scalar field. The effective scenario from loop quantum gravity is applied to a homogeneous interior spacetime. The classical singularity that arises at the final stage of our collapsing system is resolved and replaced by a quantum bounce. Our main purpose is to investigate the evolution of trapped surfaces during the collapse in semiclassical regime. We show that, in this regime, there exists a threshold scale below which no horizon can form as collapse evolves towards the bounce. By employing the matching conditions at the boundary shell, quantum effects are carried out to the exterior region, leading to an improved Vaidya geometry. In addition, the effective mass loss emerging in this model predicts an outward energy flux from the interior quantum geometry regime. 11 pages, 5 figures http://arxiv.org/abs/1303.5612 A Gravitational Entropy Proposal Timothy Clifton, George F R Ellis, Reza Tavakol (Submitted on 22 Mar 2013) We propose a thermodynamically motivated measure of gravitational entropy based on the Bel-Robinson tensor, which has a natural interpretation as the effective super-energy-momentum tensor of free gravitational fields. The specific form of this measure differs depending on whether the gravitational field is Coulomb-like or wave-like, and reduces to the Bekenstein-Hawking value when integrated over the interior of a Schwarzschild black hole. For scalar perturbations of a Robertson-Walker geometry we find that the entropy goes like the Hubble weighted anisotropy of the gravitational field, and therefore increases as structure formation occurs. This is in keeping with our expectations for the behaviour of gravitational entropy in cosmology, and provides a thermodynamically motivated arrow of time for cosmological solutions of Einstein's field equations. It is also in keeping with Penrose's Weyl curvature hypothesis. 17 pages http://arxiv.org/abs/1303.4989 Loop Quantum Gravity and the The Planck Regime of Cosmology Abhay Ashtekar http://arxiv.org/abs/1303.4752 Imaginary action, spinfoam asymptotics and the 'transplanckian' regime of loop quantum gravity Norbert Bodendorfer, Yasha Neiman http://arxiv.org/abs/1303.4636 Spin foams Jonathan Engle http://arxiv.org/abs/1303.3576 Cosmology from Group Field Theory Steffen Gielen, Daniele Oriti, Lorenzo Sindoni http://arxiv.org/abs/1303.2773 BTZ Black Hole Entropy in Loop Quantum Gravity and in Spin Foam Models J.Manuel Garcia-Islas http://arxiv.org/abs/1303.0752 Inclusion of matter in inhomogeneous loop quantum cosmology Daniel Martín-de Blas, Mercedes Martín-Benito, Guillermo A. Mena Marugán http://arxiv.org/abs/1303.0195 Living in Curved Momentum Space J. Kowalski-Glikman http://arxiv.org/abs/1302.7142 Holonomy Operator and Quantization Ambiguities on Spinor Space Etera R. Livine http://arxiv.org/abs/1302.5265 The loop quantum gravity black hole Rodolfo Gambini, Jorge Pullin http://arxiv.org/abs/1302.3833 Loop Quantum Cosmology Ivan Agullo, Alejandro Corichi http://arxiv.org/abs/1302.1781 Self-Energy in the Lorentzian ERPL-FK Spin Foam Model of Quantum Gravity Aldo Riello http://arxiv.org/abs/1302.0724 Death and resurrection of the zeroth principle of thermodynamics Hal M. Haggard, Carlo Rovelli http://arxiv.org/abs/1302.0254 The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations Ivan Agullo, Abhay Ashtekar, William Nelson http://arxiv.org/abs/1301.6210 Embedding loop quantum cosmology without piecewise linearity Jonathan Engle http://arxiv.org/abs/1301.5859 Hamiltonian spinfoam gravity Wolfgang M. Wieland http://arxiv.org/abs/1301.3480 Gauge networks in noncommutative geometry Matilde Marcolli, Walter D. van Suijlekom http://arxiv.org/abs/1301.2245 Quantum-Reduced Loop Gravity: Cosmology Emanuele Alesci, Francesco Cianfrani http://arxiv.org/abs/1301.1264 Inflation as a prediction of loop quantum cosmology Linda Linsefors, Aurelien Barrau |
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