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Livres sur le sujet « Gravity Tensor »

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Auteur : Grafiati

Publié le 11 mars 2023

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1

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

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2

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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3

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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4

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

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5

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

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6

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

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7

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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8

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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9

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

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10

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

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11

Faraoni, Valerio. Cosmology in Scalar-Tensor Gravity (Fundamental Theories of Physics). Springer, 2004.

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12

Mercati, Flavio. Cotton-Squared Theory. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198789475.003.0010.

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This chapter analyzes a non-viable theory of gravity based on a Jacobi-type action with a conformally invariant potential term based on the square of the Cotton tensor. This theory has striking similarities with Maxwell’s electromagnetism, of which it represents the generalization to spin 2, but unfortunately it is not dynamically consistent, leaving SD as the only viable spatially conformally invariant relational theory of gravity.

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13

Blaha, Stephen. Unification of the Seven Boson Interactions based on the Riemann-Christoffel Curvature Tensor : Modified Galactic Scale Gravity, Explicit Quark Confinement, Interactions between Interactions. Pingree-Hill Publishing, 2016.

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14

Tender Gravity. Boreal Books, 2022.

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15

Kachelriess, Michael. Spin-1 and spin-2 fields. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198802877.003.0007.

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Massive and massless spin-1 and spin-2 fields, their field equations and propagators are studied. The connection between local gauge symmetry and the coupling to a conserved current is derived in the massless case. The dynamical stress tensor is defined as source of gravity, and its local conservation is shown. The basic ideas of large extra dimensions is outlined in an appendix.

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16

Tensorial Methods and Renormalization in Group Field Theories. Springer, 2014.

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17

Bubble generation in a continuous liquid flow under gravity conditions. [Cleveland, Ohio] : National Aeronautics and Space Administration, Glenn Research Center, 1999.

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18

Thermocapillary flow with evaporation and condensation at low gravit. [Washington, DC : National Aeronautics and Space Administration, 1995.

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19

Carrozza, Sylvain. Tensorial Methods and Renormalization in Group Field Theories. Springer, 2016.

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20

Carrozza, Sylvain. Tensorial Methods and Renormalization in Group Field Theories. Springer London, Limited, 2014.

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21

Shaibani, Aziz. Weakness of the Neck Muscles. Oxford University Press, 2018. http://dx.doi.org/10.1093/med/9780190661304.003.0010.

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The neck is furnished by tens of muscles for flexion, extension, lateral bending, and rotation. It carries a 10-pound head for at least two-thirds of every day. These muscles are under delicate central control, and they are subject to different central and peripheral malfunctions. Differential involvement of the neck flexors’ Vs extensors helps with the diagnosis of various neuromuscular disorders. Weakness of the cervical extensors leads to head drop, a troubling condition that is caused by many neuromuscular disorders. Movement disorders such as cervical dystonia and Parkinson disease lead to head drop, causing confusion with neuromuscular causes such as myasthenia gravis (MG) and amyotrophic lateral sclerosis (ALS). Head protrusion of the elderly (camptocormia) is a different entity.

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22

Bridges, John C. Evolution of the Martian Crust. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.18.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Mars, which has a tenth of the mass of Earth, has cooled as a single lithospheric plate. Current topography gravity maps and magnetic maps do not show signs of the plate tectonics processes that have shaped the Earth’s surface. Instead, Mars has been shaped by the effects of meteorite bombardment, igneous activity, and sedimentary—including aqueous—processes. Mars also contains enormous igneous centers—Tharsis and Elysium, with other shield volcanoes in the ancient highlands. In fact, the planet has been volcanically active for nearly all of its 4.5 Gyr history, and crater counts in the Northern Lowlands suggest that may have extended to within the last tens of millions of years. Our knowledge of the composition of the igneous rocks on Mars is informed by over 100 Martian meteorites and the results from landers and orbiters. These show dominantly tholeiitic basaltic compositions derived by melting of a relatively K, Fe-rich mantle compared to that of the Earth. However, recent meteorite and lander results reveal considerable diversity, including more silica-rich and alkaline igneous activity. These show the importance of a range of processes including crystal fractionation, partial melting, and possibly mantle metasomatism and crustal contamination of magmas. The figures and plots of compositional data from meteorites and landers show the range of compositions with comparisons to other planetary basalts (Earth, Moon, Venus). A notable feature of Martian igneous rocks is the apparent absence of amphibole. This is one of the clues that the Martian mantle had a very low water content when compared to that of Earth.The Martian crust, however, has undergone hydrothermal alteration, with impact as an important heat source. This is shown by SNC analyses of secondary minerals and Near Infra-Red analyses from orbit. The associated water may be endogenous.Our view of the Martian crust has changed since Viking landers touched down on the planet in 1976: from one almost entirely dominated by basaltic flows to one where much of the ancient highlands, particularly in ancient craters, is covered by km deep sedimentary deposits that record changing environmental conditions from ancient to recent Mars. The composition of these sediments—including, notably, the MSL Curiosity Rover results—reveal an ancient Mars where physical weathering of basaltic and fractionated igneous source material has dominated over extensive chemical weathering.

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