Bibliographies thématiques / Gravity Tensor

Littérature scientifique sur le sujet « Gravity Tensor »

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Publié le 11 mars 2023

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Articles de revues sur le sujet "Gravity Tensor"

POPŁAWSKI, NIKODEM J. « ON THE NONSYMMETRIC PURELY AFFINE GRAVITY ». Modern Physics Letters A 22, n^o 36 (30 novembre 2007) : 2701–20. http://dx.doi.org/10.1142/s0217732307025662.

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We review the vacuum purely affine gravity with the nonsymmetric connection and metric. We also examine dynamical effects of the second Ricci tensor and covariant second-rank tensors constructed from the torsion tensor in the gravitational Lagrangian.

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Gogberashvili, M. Y. « Tensor-tensor model of gravity ». Theoretical and Mathematical Physics 113, n^o 3 (décembre 1997) : 1572–81. http://dx.doi.org/10.1007/bf02634517.

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Bergshoeff, Eric, Wout Merbis, Alasdair J. Routh et Paul K. Townsend. « The third way to 3D gravity ». International Journal of Modern Physics D 24, n^o 12 (octobre 2015) : 1544015. http://dx.doi.org/10.1142/s0218271815440150.

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Consistency of Einstein’s gravitational field equation [Formula: see text] imposes a “conservation condition” on the [Formula: see text]-tensor that is satisfied by (i) matter stress tensors, as a consequence of the matter equations of motion and (ii) identically by certain other tensors, such as the metric tensor. However, there is a third way, overlooked until now because it implies a “nongeometrical” action: one not constructed from the metric and its derivatives alone. The new possibility is exemplified by the 3D “minimal massive gravity” model, which resolves the “bulk versus boundary” unitarity problem of topologically massive gravity with Anti-de Sitter asymptotics. Although all known examples of the third way are in three spacetime dimensions, the idea is general and could, in principle, apply to higher dimensional theories.

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Torres, Diego F., et Héctor Vucetich. « Hyperextended scalar-tensor gravity ». Physical Review D 54, n^o 12 (15 décembre 1996) : 7373–77. http://dx.doi.org/10.1103/physrevd.54.7373.

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Chiba, Takeshi. « 1/R gravity and scalar-tensor gravity ». Physics Letters B 575, n^o 1-2 (novembre 2003) : 1–3. http://dx.doi.org/10.1016/j.physletb.2003.09.033.

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Nieto, J. A. « Alternative self-dual gravity in eight dimensions ». Modern Physics Letters A 31, n^o 26 (17 août 2016) : 1650147. http://dx.doi.org/10.1142/s0217732316501479.

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We develop an alternative Ashtekar formalism in eight dimensions. In fact, using a MacDowell–Mansouri physical framework and a self-dual curvature symmetry, we propose an action in eight dimensions in which the Levi-Civita tenor with eight indices plays a key role. We explicitly show that such an action contains number of linear, quadratic and cubic terms in the Riemann tensor, Ricci tensor and scalar curvature. In particular, the linear term is reduced to the Einstein–Hilbert action with cosmological constant in eight dimensions. We prove that such a reduced action is equivalent to the Lovelock action in eight dimensions.

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VERDAGUER, ENRIC. « METRIC FLUCTUATIONS IN DE SITTER SPACETIME IN STOCHASTIC GRAVITY ». International Journal of Modern Physics D 20, n^o 05 (20 mai 2011) : 851–60. http://dx.doi.org/10.1142/s0218271811019189.

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Stochastic gravity extends semiclassical gravity by allowing for a systematic and self-consistent description of the metric fluctuations produced by the quantum fluctuations of the stress tensor. The effect of minimally coupled scalar fields with arbitrary mass in de Sitter spacetime is discussed, assuming that these fields are in the Bunch–Davies de Sitter invariant vacuum. The matter field fluctuations are described by the noise kernel which is obtained from the symmetrized two-point correlation of the stress tensor operator. The noise kernel is computed in terms of de Sitter invariant bi-tensors. It turns out that in a de Sitter background the two-point function of the linearized Einstein tensor, which is gauge invariant, is directly related to the noise kernel.

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Peng, Jun-Jin, et Hui-Fa Liu. « A new formula for conserved charges of Lovelock gravity in AdS space–times and its generalization ». International Journal of Modern Physics A 35, n^o 20 (2 juillet 2020) : 2050102. http://dx.doi.org/10.1142/s0217751x2050102x.

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Within the framework of the Lovelock gravity theory, we propose a new rank-four divergenceless tensor consisting of the Riemann curvature tensor and inheriting its algebraic symmetry characters. Such a tensor can be adopted to define conserved charges of the Lovelock gravity theory in asymptotically anti-de Sitter (AdS) space–times. Besides, inspired with the case of the Lovelock gravity, we put forward another general fourth-rank tensor in the context of an arbitrary diffeomorphism invariant theory of gravity described by the Lagrangian constructed out of the curvature tensor. On basis of the newly-constructed tensor, we further suggest a Komar-like formula for the conserved charges of this generic gravity theory.

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Heisenberg, Lavinia. « Scalar-vector-tensor gravity theories ». Journal of Cosmology and Astroparticle Physics 2018, n^o 10 (29 octobre 2018) : 054. http://dx.doi.org/10.1088/1475-7516/2018/10/054.

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Moffat, J. W. « Scalar–tensor–vector gravity theory ». Journal of Cosmology and Astroparticle Physics 2006, n^o 03 (6 mars 2006) : 004. http://dx.doi.org/10.1088/1475-7516/2006/03/004.

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Thèses sur le sujet "Gravity Tensor"

Davies, Trevor Bamidelé. « Quadratic scalar-tensor gravity ». Thesis, University of Aberdeen, 2017. http://digitool.abdn.ac.uk:80/webclient/DeliveryManager?pid=234075.

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This thesis develops novel analytic models of scalar-tensor theories with quadratic coupling. In this framework, the coupling strength between scalar and matter is regulated in a way that allows the vacuum expectation value to vanish for low matter densities while becoming non-vanishingly large in the high-density regime. This results in significant deviations from the predictions of General Relativity in the strong-gravity regime. In astrophysics, we addressed the core-collapse supernova problem to account for the apparently missing energy required to explain the observed powerful explosions. We assumed a small, massless scalar gravitational field, thus allowing General Relativity to be recovered in the weak-gravity asymptotic limit. The non-trivial effects coming from the coupling function in the presence of a high-density field were analyzed at the instant of neutron star formation. Our results show that the scalar gravitational field evolves from a cosmological value to a new equilibrium via a Higgs-like mechanism. Additionally, the calculations associated with the gravitational binding energy shift and relevant relaxation timescale are explicitly shown. The full theory space of the model was also investigated for positive values of the coupling parameter. We studied a mechanism to address the stalled shock issue in core-collapse scenarios, which involved the application of sufficiently large positive values to the coupling parameter. Our results show that pulsating neutron stars act like optical cavities in which resonant scalar waves are parametrically amplified. It implies that the surface of a neutron star acts like an anti-phase reflector, releasing traveling scalar gravitational waves similar to an optical laser. In cosmology, the same framework was applied to a generic Friedman-Robertson-Walker universe involving general metric coupling and scalar potential functions. In cosmology, the same framework was applied to a generic Friedman-Robertson-Walker universe involving general metric coupling and scalar potential functions. We developed a mechanism which allowed the scalar field to be dynamically trapped, thus generating a potential capable of driving primordial inflation. Our results show that a trapped scalar field produces non-trivial dynamical consequences when applied to standard cosmology. Additionally, our analytic solutions for the generic inflationary behaviour, produce acceptable duration and e-foldings, thus recovering the Hubble parameter which is consistent with the present-day value. A feature of our cosmological model is that the universe can undergo several accelerating or decelerating phases, even though the scalar potential and metric coupling are monotonic functions overall. As this is important for the current dark energy problem, the quasi-static motion of the gravitational field induced by the scalar potential in the early universe, is investigated for a small value of the scalar field with normalized metric at the present time. Our results show that a variable Lambda Cold Dark Matter universe emerges naturally from the quadratic model.

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Wands, David Graham. « Cosmology of scalar-tensor gravity ». Thesis, University of Sussex, 1993. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.335537.

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Delepouve, Thibault. « Quartic Tensor Models ». Thesis, Université Paris-Saclay (ComUE), 2017. http://www.theses.fr/2017SACLS085/document.

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Les modèles de tenseurs sont des mesures de probabilité sur des espaces de tenseurs aléatoires. Ils généralisent les modèles de matrices et furent développés pour l’étude de la géométrie aléatoire en dimension arbitraire. De plus, ils sont fortement liés aux théories de gravité quantique car, en plus des modèles standards très simples, ils incluent les théories de champs sur groupes, qui constituent l’approche « intégrale fonctionnelle » de la gravité quantique à boucle. Dans cette thèse, nous étudions le cas restreint des modèles tensoriels quartiques, pour lesquels un plus grand nombre de résultats mathématiques rigoureux ont pu être démontrés. Grâce à la transformation de champ intermédiaire, les modèles quartiques peuvent être ré-écrits sous forme de modèles de matrices multiples, et leurs développements perturbatifs peuvent être indexés par des cartes combinatoires. En utilisant divers développement en cartes, nous démontrons d’importants résultats d’analycité ainsi que des bornes pour les cumulants du modèle tensoriel standard le plus général et de rang arbitraire, ainsi que du plus simple modèle renormalisable de rang 3. Ensuite, nous introduisons une nouvelle famille de modèles, les modèles améliorés, dont le développement perturbatif se comporte de manière nouvelle, différente du comportement « melonique » qui caractérise les modèles tensoriels précédemment étudiés
Tensor models are probability measures for random tensors. They generalise matrix models and were developed to study random geometry in arbitrary dimension. Moreover, they are strongly connected to quantum gravity theories as, additionally to the standard bare-bones models, they encompass the field theoretical approach to loop quantum gravity known as group field theory.In the present thesis, we focus on the restricted case of quartic tensor models, for which a far greater number of rigorous mathematical results have been proven. Quartic models can be re-written as multi-matrix models using the intermediate field representation, and their perturbative expansions can be written as series expansions over combinatorial maps. Using a variety of map expansions, we prove analyticity results and useful bounds for the cumulants of various tensor models : the most general standard quartic model at any rank and the simplest renormalisable tensor field theory at rank 3. Then, we introduce a new class of models, the enhanced models, which perturbative expansions display new behaviour, different to the so called melonic behaviour that characterise most known tensor models so far

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Da, Silva Caroline Dos Santos. « Cosmic strings and scalar tensor gravity ». Thesis, Durham University, 1999. http://etheses.dur.ac.uk/4577/.

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This thesis is concerned with the study of cosmic strings. We studied the values for the Higgs mass and string coupling for which the gravitational effect of an infinite cosmic string in the context of the Einstein theory is not only locally but also globally weak. We conclude this happens for strings formed at scales less or equal to the Planck one with Higgs mass being less or equal to the boson vectorial mass. Then we examined the metric of an isolated self-gravitating abelian-Higgs vortex in dilatonic gravity for arbitrary coupling of the vortex fields to the dilaton. We looked for solutions in both massless and massive dilaton gravity. We compared our results to existing metrics for strings in Einstein and .Jordan-Brans-Dicke theories. We explored the generalisation of Bogomolnyi arguments for our vortices and commented on the effects on test particles. We then included the presence of an axion field and examined the metric of an isolated self-gravitating axionic-dilatonic string. Finally we studied dilatonic strings through black hole solutions in string theory. We concluded that the horizon of non-extreme charged black holes supports the long-range fields of the Nielsen-Olesen string that can be considered as black hole hair and whose gravitational effect is in general the production of a conical deficit into the metric of the black hole background. We also concluded that the effect of the dilaton on the horizon of these black holes is to generate an additional charge.

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Oreta, Timothy. « Vector-Galileon-Tensor theories of gravity ». Master's thesis, University of Cape Town, 2016. http://hdl.handle.net/11427/20925.

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A detailed study of the cosmological evolution in a particular vector-tensor theory of gravity with a potential and a Galileon-motivated interaction terms is presented. The evolution of vector field self interactions that are relatively related to Galileon fields throughout the expansion history of the universe is considered and a classification of the parameters M (mass term) and H (Hubble parameter) according to the behaviour of the field in each cosmological epoch is carried out. In particular, we obtain conditions for the parameters so that the field grows exponentially or oscillates with decreasing amplitude. We also obtain an autonomous system for the inflationary case. The general features of the phasemaps are given and the critical point is appropriately characterised. It is not possible to obtain an autonomous system for radiation and matter dominated epochs hence, we consider other analytical methods. We obtain eigenvalues and hence, phasemaps. The general features of the phasemaps are given and the point to which the trajectories on the phasemaps converge is appropriately characterised. Therefore, we show that it is possible to obtain a wide variety of behaviours or interesting phenomenologies for the cosmological evolution of vector field self-interactions that are relatively related to Galileon fields by choosing suitable values for the parameters M and H of given conditions.

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Bourhrous, Hassan. « CMB tensor anisotropies in f(R) gravity ». Master's thesis, University of Cape Town, 2014. http://hdl.handle.net/11427/4866.

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Dartois, Stephane. « Random Tensor models : Combinatorics, Geometry, Quantum Gravity and Integrability ». Thesis, Sorbonne Paris Cité, 2015. http://www.theses.fr/2015USPCD104/document.

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Dans cette thèse nous explorons différentes facettes des modèles de tenseurs aléatoires. Les modèles de tenseurs aléatoires ont été introduits en physique dans le cadre de l'étude de la gravité quantique. En effet les modèles de matrices aléatoires, qui sont un cas particuliers de modèles de tenseurs, en sont une des origines. Ces modèles de matrices sont connus pour leur riche combinatoire et l'incroyable diversité de leurs propriétés qui les font toucher tous les domaines de l'analyse, la géométrie et des probabilités. De plus leur étude par les physiciens ont prouvé leur efficacité en ce qui concerne l'étude de la gravité quantique à deux dimensions. Les modèles de tenseurs aléatoires incarnent une généralisation possible des modèles de matrices. Comme leurs cousins, les modèles de matrices, ils posent questions dans les domaines de la combinatoire (comment traiter les cartes combinatoires d dimensionnelles ?), de la géométrie (comment contrôler la géométrie des triangulations générées ?) et de la physique (quel type d'espace-temps produisent-ils ? Quels sont leurs différentes phases ?). Cette thèse espère établir des pistes ainsi que des techniques d'études de ces modèles. Dans une première partie nous donnons une vue d'ensemble des modèles de matrices. Puis, nous discutons la combinatoire des triangulations en dimensions supérieures ou égales à trois en nous concentrant sur le cas tridimensionnelle (lequel est plus simple à visualiser). Nous définissons ces modèles et étudions certaines de leurs propriétés à l'aide de techniques combinatoires permettant de traiter les cartes d dimensionnelles. Enfin nous nous concentrons sur la généralisation de techniques issues des modèles de matrices dans le cas d'une famille particulières de modèles de tenseurs aléatoires. Ceci culmine avec le dernier chapitre de la thèse donnant des résultats partiels concernant la généralisation de la récurrence topologique de Eynard et Orantin à cette famille de modèles de tenseurs
In this thesis manuscript we explore different facets of random tensor models. These models have been introduced to mimic the incredible successes of random matrix models in physics, mathematics and combinatorics. After giving a very short introduction to few aspects of random matrix models and recalling a physical motivation called Group Field Theory, we start exploring the world of random tensor models and its relation to geometry, quantum gravity and combinatorics. We first define these models in a natural way and discuss their geometry and combinatorics. After these first explorations we start generalizing random matrix methods to random tensors in order to describes the mathematical and physical properties of random tensor models, at least in some specific cases

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Wu, Chun-Hsien. « Quantum fluctuations of the stress tensor / ». Thesis, Connect to Dissertations & ; Theses @ Tufts University, 2002.

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Thesis (Ph.D.)--Tufts University, 2002.
Adviser: L. H. Ford. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 161-165). Access restricted to members of the Tufts University community. Also available via the World Wide Web;

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Schiappacasse, Enrico D. « Beyond Semiclassical Gravity| Quantum Stress Tensor Fluctuations in the Vacuum ». Thesis, Tufts University, 2018. http://pqdtopen.proquest.com/#viewpdf?dispub=10812605.

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Large vacuum fluctuations of a quantum stress tensor can be described by the asymptotic behavior of its probability distribution. Here we focus on stress tensor operators which have been averaged with a sampling function in time. The Minkowski vacuum state is not an eigenstate of the time-averaged operator, but can be expanded in terms of its eigenstates. We calculate the probability distribution and the cumulative probability distribution for obtaining a given value in a measurement of the time-averaged operator taken in the vacuum state. In these calculations, we use the normal ordered square of the time derivative of a massless scalar field in Minkowski spacetime as an example of a stress tensor operator. We analyze the rate of decrease of the tail of the probability distribution for different temporal sampling functions, such as compactly supported functions and the Lorentzian function. We find that the tails decrease relatively slowly, as exponentials of fractional powers, in agreement with previous work using the moments of the distribution. Our results lead additional support to the conclusion that large vacuum stress tensor fluctuations are more probable than large thermal fluctuations, and may have observable effects.

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Holden, Damien James. « Generalised Brans-Dicke cosmology ». Thesis, University of Portsmouth, 2002. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.247071.

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Livres sur le sujet "Gravity Tensor"

Faraoni, Valerio. Cosmology in scalar-tensor gravity. Dordrecht : Kluwer Academic Publishers, 2004.

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Faraoni, Valerio. Cosmology in Scalar-Tensor Gravity. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0.

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J, Azzam M. O., Mann J. A et Lewis Research Center, dir. Effect of gravity on surface tension. [Cleveland, Ohio] : National Aeronautics and Space Administration, Lewis Research Center, 1998.

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Aharon, I. Hydrodynamic stability of multicomponent droplet gasification in reduced gravity. [Washington, DC : National Aeronautics and Space Administration, 1995.

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Aharon, I. Hydrodynamic stability of multicomponent droplet gasification in reduced gravity. [Washington, DC : National Aeronautics and Space Administration, 1995.

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Free surface flows under compensated gravity conditions. Berlin : Springer, 2007.

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United States. National Aeronautics and Space Administration., dir. Annual report on numerical studies of the surface tension effect of cryogenic liquid helium. Huntsville, Ala : University of Alabama in Huntsville, 1994.

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Faraoni, Valerio. Cosmology in Scalar-Tensor Gravity. Springer London, Limited, 2004.

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Faraoni, Valerio. Cosmology in Scalar-Tensor Gravity. Springer Netherlands, 2012.

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Chapitres de livres sur le sujet "Gravity Tensor"

Faraoni, Valerio. « Scalar-Tensor Gravity ». Dans Cosmology in Scalar-Tensor Gravity, 1–53. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_1.

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Coley, A. A. « Scalar Tensor Theories of Gravity ». Dans Astrophysics and Space Science Library, 96–105. Dordrecht : Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0327-7_8.

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Faraoni, Valerio. « Effective Energy-Momentum Tensors and Conformal Frames ». Dans Cosmology in Scalar-Tensor Gravity, 55–81. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_2.

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Faraoni, Valerio. « Gravitational Waves in Scalar-Tensor Cosmology ». Dans Cosmology in Scalar-Tensor Gravity, 83–92. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_3.

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Faraoni, Valerio. « Exact Solutions of Scalar-Tensor Cosmology ». Dans Cosmology in Scalar-Tensor Gravity, 93–114. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_4.

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Faraoni, Valerio. « The Early Universe ». Dans Cosmology in Scalar-Tensor Gravity, 115–25. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_5.

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Faraoni, Valerio. « Perturbations ». Dans Cosmology in Scalar-Tensor Gravity, 127–41. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_6.

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Faraoni, Valerio. « Nonminimal Coupling ». Dans Cosmology in Scalar-Tensor Gravity, 143–95. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_7.

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Faraoni, Valerio. « The Present Universe ». Dans Cosmology in Scalar-Tensor Gravity, 197–228. Dordrecht : Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-1989-0_8.

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Lynden-Bell, D. « A Local Stress Tensor for Gravity Fields ». Dans Gravity and the Quantum, 209–19. Cham : Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-51700-1_15.

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Actes de conférences sur le sujet "Gravity Tensor"

Rivasseau, Vincent, et Nicolas Delporte. « The Tensor Track V : Holographic Tensors ». Dans Corfu Summer Institute 2017 "Schools and Workshops on Elementary Particle Physics and Gravity". Trieste, Italy : Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.318.0218.

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Mims, John H., et James Mataragio. « Airborne Full Tensor Gravity ». Dans Symposium on the Application of Geophysics to Engineering and Environmental Problems 2010. Environment and Engineering Geophysical Society, 2010. http://dx.doi.org/10.4133/1.3445466.

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H. Mims, John, et James Mataragio. « Airborne Full Tensor Gravity ». Dans 23rd EEGS Symposium on the Application of Geophysics to Engineering and Environmental Problems. European Association of Geoscientists & Engineers, 2010. http://dx.doi.org/10.3997/2214-4609-pdb.175.sageep051.

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Mickus, K., et J. Hinojosa. « Gravity Gradient Tensor Determined from Vertical Gravity Measurements ». Dans 61st EAGE Conference and Exhibition. European Association of Geoscientists & Engineers, 1999. http://dx.doi.org/10.3997/2214-4609.201407963.

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Esposito-Farèse, Gilles. « Tests of Scalar-Tensor Gravity ». Dans PHI IN THE SKY : The Quest for Cosmological Scalar Fields. AIP, 2004. http://dx.doi.org/10.1063/1.1835173.

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Kokkotas, K. D. « Stellar Dynamics in Scalar-Tensor Gravity ». Dans RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS : 7th International Conference of the Hellenic Astronomical Society. AIP, 2006. http://dx.doi.org/10.1063/1.2348058.

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Yokoyama, Jun’ichi. « Birth of the Inflationary Universe and Tensor Fluctuations ». Dans Second LeCosPA International Symposium : Everything about Gravity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813203952_0010.

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Routh, Partha S., Greg J. Jorgensen et Jerry L. Kisabeth. « Base of the salt imaging using gravity and tensor gravity data ». Dans SEG Technical Program Expanded Abstracts 2001. Society of Exploration Geophysicists, 2001. http://dx.doi.org/10.1190/1.1816386.

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BARTOLO, N., et M. PIETRONI. « QUINTESSENCE IN TENSOR-SCALAR THEORIES OF GRAVITY ». Dans Proceedings of the Third International Workshop on Particle Physics and the Early Universe. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792129_0013.

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Rivasseau, Vincent. « Quantum gravity and renormalization : The tensor track ». Dans THE 8TH INTERNATIONAL CONFERENCE ON PROGRESS IN THEORETICAL PHYSICS (ICPTP 2011). AIP, 2012. http://dx.doi.org/10.1063/1.4715396.

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Rapports d'organisations sur le sujet "Gravity Tensor"

Wieberg, Scott. Integration of Full Tensor Gravity and Z-Axis Tipper Electromagnetic Passive Low Frequency EM Instruments for Simultaneous Data Acquisition - Final Technical Report. Office of Scientific and Technical Information (OSTI), décembre 2016. http://dx.doi.org/10.2172/1338618.

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Biek, Robert F., Peter D. Rowley et David B. Hacker. Utah’s Ancient Mega-Landslides : Geology, Discovery, and Guide to Earth’s Largest Terrestrial Landslides. Utah Geological Survey, décembre 2022. http://dx.doi.org/10.34191/c-132.

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Southwest Utah contains what may be the largest landslide complex on land in the world. This complex includes three ancient side-by-side gigantic slides that cover an area roughly the size of Yellowstone National Park with a volume of slide debris that would nearly fill the Grand Canyon to its rim. Geologists call it the Marysvale gravity slide complex— “Marysvale” for the namesake volcanic field that partly failed catastrophically three separate times, and “gravity slide” to call attention to a special class of extremely large and geologically complex landslides several tens to thousands of square miles in extent. Here we refer to them simply as mega-landslides or slides—they are larger and far more interesting than geologists could ever have imagined.

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ARMY ENGINEER DISTRICT VICKSBURG MS. Tensas Basin, Red River Backwater Area. Black River, Louisiana Tensas-Cocodrie Pumping Plant, Gravity Drainage Structure, and Upper Weir Foundation Report. Fort Belvoir, VA : Defense Technical Information Center, août 1996. http://dx.doi.org/10.21236/ada315879.

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