scholarly journals THE QUANTUM GRAVITY WITH TORSION AND GHOST-FREE DE SITTER GRAVITY (Ⅰ)——GRAVITATIONAL FIELD WITH HOESION UNDER LINEAR COVARIANT GAUGE CONDITION

1984 ◽  
Vol 33 (10) ◽  
pp. 1377
Author(s):  
YAN MU-LIN ◽  
GUO HAN-YING
Keyword(s):  
Gravitational Field ◽  
Quantum Gravity ◽  
Gauge Condition ◽  
De Sitter ◽  
Covariant Gauge

“Prehistoric” Quantum Gravity

2020 ◽  
pp. 41-70
Author(s):  
Dean Rickles
Keyword(s):  
General Relativity ◽  
Quantum Theory ◽  
Gravitational Field ◽  
Quantum Gravity ◽  
Philosophical Nature

In this chapter we examine the very earliest work on the problem of quantum gravity (understood very liberally). We show that, even before the concept of the quantization of the gravitational field in 1929, there was a fairly lively investigation of the relationships between gravity and quantum stretching as far back as 1916, and certainly no suggestion that such a theory would not be forthcoming. Indeed, there are, rather, many suggestions explicitly advocating that an integration of quantum theory and general relativity (or gravitation, at least) is essential for future physics, in order to construct a satisfactory foundation. We also see how this belief was guided by a diverse family of underlying agendas and constraints, often of a highly philosophical nature.

scholarly journals Geodesic Effect Near an Elliptical Orbit

2012 ◽  
Vol 2012 ◽  
pp. 1-8
Author(s):  
Alina-Daniela Vîlcu
Keyword(s):  
Gravitational Field ◽  
Elliptical Orbit ◽  
Newtonian Mechanics ◽  
The Sun ◽  
Classical Approach ◽  
De Sitter ◽  
Lagrange Equations ◽  
The Earth ◽  
Elliptical Motion

Using a differential geometric treatment, we analytically derived the expression for De Sitter (geodesic) precession in the elliptical motion of the Earth through the gravitational field of the Sun with Schwarzschild's metric. The expression obtained in this paper in a simple way, using a classical approach, agrees with that given in B. M. Barker and R. F. O'Connell (1970, 1975) in a different setting, using the tools of Newtonian mechanics and the Euler-Lagrange equations.

scholarly journals Exact Solutions in Poincaré Gauge Gravity Theory

Universe ◽  
2019 ◽  
Vol 5 (5) ◽  
pp. 127 ◽  
Author(s):  
Yuri N. Obukhov
Keyword(s):  
Gravitational Field ◽  
Gravity Models ◽  
Field Potentials ◽  
De Sitter ◽  
Field Equations ◽  
Yang Mills ◽  
Gravitational Field Equations ◽  
Poincaré Symmetry ◽  
Gauge Gravity ◽  
Vacuum Solutions

In the framework of the gauge theory based on the Poincaré symmetry group, the gravitational field is described in terms of the coframe and the local Lorentz connection. Considered as gauge field potentials, they give rise to the corresponding field strength which are naturally identified with the torsion and the curvature on the Riemann–Cartan spacetime. We study the class of quadratic Poincaré gauge gravity models with the most general Yang–Mills type Lagrangian which contains all possible parity-even and parity-odd invariants built from the torsion and the curvature. Exact vacuum solutions of the gravitational field equations are constructed as a certain deformation of de Sitter geometry. They are black holes with nontrivial torsion.

XLV.—The Internal and External Fields of a Particle in a Gravitational Field

1949 ◽  
Vol 62 (4) ◽  
pp. 427-433
Author(s):  
G. L. Clark
Keyword(s):  
Gravitational Field ◽  
Energy Tensor ◽  
External Fields ◽  
De Sitter ◽  
Volume Integral ◽  
Interaction Terms ◽  
Minor Alteration ◽  
Stress Components ◽  
System Of Particles ◽  
A Minor

SummaryThe gravitational field of a system of particles was investigated by de Sitter as far back as 1916. A minor alteration to the analysis was made by Eddington and Clark in 1938. The amended value of the potential g44 is the same as that derived by Einstein, Infeld and Hoffmann without making use of the energy-tensor; this agreement suggests that the revised de Sitter argument is correct. In this paper we show that this is not the case, for the de Sitter analysis completely overlooked any possible interaction terms in the stress components of the energy-tensor. We find the value of these terms, pmn, and show that the agreement mentioned above is due to the fact that the volume integral of pu vanishes.

PERTURBATIVE FINITENESS OF 2D INDUCED QUANTUM GRAVITY

1992 ◽  
Vol 07 (05) ◽  
pp. 437-440 ◽  
Author(s):  
S.D. ODINTSOV ◽  
I.L. SHAPIRO
Keyword(s):  
Quantum Gravity ◽  
Effective Action ◽  
General Type ◽  
Full Agreement ◽  
Exactly Solvable ◽  
Covariant Gauge ◽  
Generally Covariant

The divergences structure of the local 2D induced quantum gravity in the generally covariant gauge of the general type is considered. It is shown that for the particular choice of this gauge the effective action is perturbatively finite. This fact is in full agreement with the fact that the theory is exactly solvable.

DIMENSION EMERGENCE, HOLOGRAPHY AND QUANTUM GRAVITY

2011 ◽  
Vol 26 (21) ◽  
pp. 3679-3696
Author(s):  
YU-LEI FENG ◽  
LI-XIN XU ◽  
YU-TING WANG
Keyword(s):  
Quantum Mechanics ◽  
Gravitational Field ◽  
Quantum Gravity ◽  
Quantum System ◽  
Alternative Interpretation ◽  
Reduction Mechanism ◽  
Dimensional Theory ◽  
Shift Vector ◽  
Higher Dimensional ◽  
Holography Principle

In this paper, we try to give an alternative interpretation of the holography principle. We argue that the space or time may be regarded as emerging from quantum mechanics as an evolutive parameter. The lower D-dimensional theory is related to a corresponding (D+1)-theory by a mysterious quantum system. Then from the higher-dimensional theory, under a new dimension reduction mechanism we obtain the corresponding results. We also try to incorporate the gauge field into the reduction, roughly identifying Aμ with Nμ which is the shift vector in the ADM-like decomposition of space–time metric. In the end, we extend to the gravitational field, and obtain a relation [Formula: see text] with a cutoff factor κ, from a different view.

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