Faster access than browser!Similarities between Brans–Dicke theory and Lagrangian (field theory)
Brans–Dicke theory and Lagrangian (field theory) have 13 things in common (in Unionpedia): Boundary value problem, Classical field theory, Einstein field equations, Equivalence principle, Gravitational constant, Metric tensor, Ricci curvature, Riemann curvature tensor, Scalar curvature, Scalar field, Spacetime, Stress–energy tensor, Tensor field.
Boundary value problem
In mathematics, in the field of differential equations, a boundary value problem is a differential equation together with a set of additional constraints, called the boundary conditions.
Boundary value problem and Brans–Dicke theory · Boundary value problem and Lagrangian (field theory) ·
Classical field theory
A classical field theory is a physical theory that predicts how one or more physical fields interact with matter through field equations.
Brans–Dicke theory and Classical field theory · Classical field theory and Lagrangian (field theory) ·
Einstein field equations
The Einstein field equations (EFE; also known as Einstein's equations) comprise the set of 10 equations in Albert Einstein's general theory of relativity that describe the fundamental interaction of gravitation as a result of spacetime being curved by mass and energy.
Brans–Dicke theory and Einstein field equations · Einstein field equations and Lagrangian (field theory) ·
Equivalence principle
In the theory of general relativity, the equivalence principle is any of several related concepts dealing with the equivalence of gravitational and inertial mass, and to Albert Einstein's observation that the gravitational "force" as experienced locally while standing on a massive body (such as the Earth) is the same as the pseudo-force experienced by an observer in a non-inertial (accelerated) frame of reference.
Brans–Dicke theory and Equivalence principle · Equivalence principle and Lagrangian (field theory) ·
Gravitational constant
The gravitational constant (also known as the "universal gravitational constant", the "Newtonian constant of gravitation", or the "Cavendish gravitational constant"), denoted by the letter, is an empirical physical constant involved in the calculation of gravitational effects in Sir Isaac Newton's law of universal gravitation and in Albert Einstein's general theory of relativity.
Brans–Dicke theory and Gravitational constant · Gravitational constant and Lagrangian (field theory) ·
Metric tensor
In the mathematical field of differential geometry, a metric tensor is a type of function which takes as input a pair of tangent vectors and at a point of a surface (or higher dimensional differentiable manifold) and produces a real number scalar in a way that generalizes many of the familiar properties of the dot product of vectors in Euclidean space.
Brans–Dicke theory and Metric tensor · Lagrangian (field theory) and Metric tensor ·
Ricci curvature
In differential geometry, the Ricci curvature tensor, named after Gregorio Ricci-Curbastro, represents the amount by which the volume of a small wedge of a geodesic ball in a curved Riemannian manifold deviates from that of the standard ball in Euclidean space.
Brans–Dicke theory and Ricci curvature · Lagrangian (field theory) and Ricci curvature ·
Riemann curvature tensor
In the mathematical field of differential geometry, the Riemann curvature tensor or Riemann–Christoffel tensor (after Bernhard Riemann and Elwin Bruno Christoffel) is the most common method used to express the curvature of Riemannian manifolds.
Brans–Dicke theory and Riemann curvature tensor · Lagrangian (field theory) and Riemann curvature tensor ·
Scalar curvature
In Riemannian geometry, the scalar curvature (or the Ricci scalar) is the simplest curvature invariant of a Riemannian manifold.
Brans–Dicke theory and Scalar curvature · Lagrangian (field theory) and Scalar curvature ·
Scalar field
In mathematics and physics, a scalar field associates a scalar value to every point in a space – possibly physical space.
Brans–Dicke theory and Scalar field · Lagrangian (field theory) and Scalar field ·
Spacetime
In physics, spacetime is any mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum.
Brans–Dicke theory and Spacetime · Lagrangian (field theory) and Spacetime ·
Stress–energy tensor
The stress–energy tensor (sometimes stress–energy–momentum tensor or energy–momentum tensor) is a tensor quantity in physics that describes the density and flux of energy and momentum in spacetime, generalizing the stress tensor of Newtonian physics.
Brans–Dicke theory and Stress–energy tensor · Lagrangian (field theory) and Stress–energy tensor ·
Tensor field
In mathematics and physics, a tensor field assigns a tensor to each point of a mathematical space (typically a Euclidean space or manifold).
Brans–Dicke theory and Tensor field · Lagrangian (field theory) and Tensor field ·
The list above answers the following questions
- What Brans–Dicke theory and Lagrangian (field theory) have in common
- What are the similarities between Brans–Dicke theory and Lagrangian (field theory)
Brans–Dicke theory and Lagrangian (field theory) Comparison
Brans–Dicke theory has 58 relations, while Lagrangian (field theory) has 90. As they have in common 13, the Jaccard index is 8.78% = 13 / (58 + 90).
References
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