equals: If we use the covariant 4-vector of generalized velocity, then in the general case the Hamiltonian has the form: [4], H In this case, define. R = a matrix). 0 {\displaystyle ~\eta _{\mu \nu }} for some uniquely determined smooth functions v1, ..., vn.   of a body can be expressed in terms of the gravitational field tensor and the 4-velocity of the body: This expression can be derived, in particular, as the consequence of the axiomatic construction of the covariant theory of gravitation in the language of 4-vectors and tensors. {\displaystyle ~{\sqrt {-g}}d\Sigma ={\sqrt {-g}}cdtdx^{1}dx^{2}dx^{3}} The Tensor Processing Unit (TPU) is a high-performance ASIC chip that is purpose-built to accelerate machine learning workloads. Algebra: Algebraic structures. Whereas the metric itself provides a way to measure the length of (or angle between) vector fields, the inverse metric supplies a means of measuring the length of (or angle between) covector fields; that is, fields of linear functionals. Let M be a smooth manifold of dimension n; for instance a surface (in the case n = 2) or hypersurface in the Cartesian space ℝn + 1. for all f supported in U. the place where most texts on tensor analysis begin. 12-30 (2019). Fedosin S.G. Equations of Motion in the Theory of Relativistic Vector Fields.     If we vary the action function by the gravitational four-potential, we obtain the equation of gravitational field (5).   ν In the mathematical field of differential geometry, one definition of a metric tensor is a type of function which takes as input a pair of tangent vectors v and w at a point of a surface (or higher dimensional differentiable manifold) and produces a real number scalar g(v, w) in a way that generalizes many of the familiar properties of the dot product of vectors in Euclidean space. {\displaystyle ~\psi } x ,   The resulting natural positive Borel measure allows one to develop a theory of integrating functions on the manifold by means of the associated Lebesgue integral. The Gödel metric is an exact solution of the Einstein field equations in which the stress–energy tensor contains two terms, the first representing the matter density of a homogeneous distribution of swirling dust particles (dust solution), and the second associated with a nonzero cosmological constant (see lambdavacuum solution).It is also known as the Gödel solution or Gödel universe. The metric tensor is an example of a tensor field. If we consider the definition of the 4-potential of gravitational field: where ∇ {\displaystyle ~dx^{1}dx^{2}dx^{3}} Thus, for example, in Jacobi's formulation of Maupertuis' principle, the metric tensor can be seen to correspond to the mass tensor of a moving particle. −   and At each point p ∈ M there is a vector space TpM, called the tangent space, consisting of all tangent vectors to the manifold at the point p. A metric tensor at p is a function gp(Xp, Yp) which takes as inputs a pair of tangent vectors Xp and Yp at p, and produces as an output a real number (scalar), so that the following conditions are satisfied: A metric tensor field g on M assigns to each point p of M a metric tensor gp in the tangent space at p in a way that varies smoothly with p. More precisely, given any open subset U of manifold M and any (smooth) vector fields X and Y on U, the real function, The components of the metric in any basis of vector fields, or frame, f = (X1, ..., Xn) are given by[3], The n2 functions gij[f] form the entries of an n × n symmetric matrix, G[f]. So that the right-hand side of equation (6) is unaffected by changing the basis f to any other basis fA whatsoever. ν c Let γ(t) be a piecewise-differentiable parametric curve in M, for a ≤ t ≤ b.   Thus, for example, the geodesic equations may be obtained by applying variational principles to either the length or the energy. g g 16 The notation employed here is modeled on that of, For the terminology "musical isomorphism", see, Disquisitiones generales circa superficies curvas, Basic introduction to the mathematics of curved spacetime, "Disquisitiones generales circa superficies curvas", "Méthodes de calcul différentiel absolu et leurs applications", https://en.wikipedia.org/w/index.php?title=Metric_tensor&oldid=995016169, Creative Commons Attribution-ShareAlike License, This page was last edited on 18 December 2020, at 19:19.    . A Furthermore, Sg is a symmetric linear transformation in the sense that, Conversely, any linear isomorphism S : TpM → T∗pM defines a non-degenerate bilinear form on TpM by means of. Likes jedishrfu. for any vectors a, a′, b, and b′ in the uv plane, and any real numbers μ and λ. The Hamiltonian in Covariant Theory of Gravitation. For your convenience, I present to you, in a single paragraph, the essence of tensor analysis: Simply put, a tensor is a mathematical construction that “eats” a bunch of vectors, and “spits out” a scalar.   μ {\displaystyle ~M}   is the propagation speed of gravitational effects (speed of gravity).   is the 4-vector of mass current density, 1. g ρ A vector is a tensor of order one. where Generalized momentum and Hamiltonian mechanics. The components of a metric tensor in a coordinate basis take on the form of a symmetric matrix whose entries transform covariantly under changes to the coordinate system. To wit, for each point p, α determines a function αp defined on tangent vectors at p so that the following linearity condition holds for all tangent vectors Xp and Yp, and all real numbers a and b: As p varies, α is assumed to be a smooth function in the sense that. 2   Um número é uma matriz de dimensão 0, por isso para representar um escalar usamos um tensor de ordem 0.   is the mass current density. Any covector field α has components in the basis of vector fields f. These are determined by, Denote the row vector of these components by, Under a change of f by a matrix A, α[f] changes by the rule. y π 3 Before 1968, it was the only known conformally invariant tensor that is algebraically independent of the Weyl tensor. Suppose that v is a tangent vector at a point of U, say, where ei are the standard coordinate vectors in ℝn. Since g is symmetric as a bilinear mapping, it follows that g⊗ is a symmetric tensor. μ Finally, there is a definition of ds² as the line element and as the "metric", but the line element is ds, not ds². In analogy with the case of surfaces, a metric tensor on an n-dimensional paracompact manifold M gives rise to a natural way to measure the n-dimensional volume of subsets of the manifold. q with the transformation law (3) is known as the metric tensor of the surface. The variation of the action function by 4-coordinates leads to the equation of motion of the matter unit in gravitational and electromagnetic fields and pressure field: [5]. Using matrix notation, the first fundamental form becomes, Suppose now that a different parameterization is selected, by allowing u and v to depend on another pair of variables u′ and v′. Let A {\displaystyle A} and B {\displaystyle B} be symmetric covariant 2-tensors. t http://dx.doi.org/10.3968%2Fj.ans.1715787020120504.2023, https://en.wikiversity.org/w/index.php?title=Gravitational_tensor&oldid=2090780, Creative Commons Attribution-ShareAlike License. ρ [7]. {\displaystyle ~\mathbf {J} } where the first term on the right is the gravitational force density, expressed with the help of the gravitational field tensor, second term is the Lorentz electromagnetic force density for the charge density {\displaystyle ~\mu \nu \sigma } 0 With the help of gravitational field tensor in the covariant theory of gravitation the gravitational stress-energy tensor is constructed: The covariant derivative of the gravitational stress-energy tensor determines the 4-vector of gravitational force density: By definition, the generalized momentum   measured in the comoving reference frame, and the last term sets the pressure force density. μ a curvature tensor. {\displaystyle ~\Lambda } {\displaystyle ~f_{\mu \nu }} μ This article is about metric tensors on real Riemannian manifolds. 0123 {\displaystyle ~\mathbf {A} } , The quantity ds in (1) is called the line element, while ds2 is called the first fundamental form of M. Intuitively, it represents the principal part of the square of the displacement undergone by r→(u, v) when u is increased by du units, and v is increased by dv units. are two vectors at p ∈ U, then the value of the metric applied to v and w is determined by the coefficients (4) by bilinearity: Denoting the matrix (gij[f]) by G[f] and arranging the components of the vectors v and w into column vectors v[f] and w[f], where v[f]T and w[f]T denote the transpose of the vectors v[f] and w[f], respectively. μ In this case, the spacetime interval is written as, The Schwarzschild metric describes the spacetime around a spherically symmetric body, such as a planet, or a black hole.   is the speed of light as a measure of the propagation speed of electromagnetic and gravitational interactions, The law of transformation of these vectors in the transition from the fixed reference frame K into the reference frame K', moving at the velocity V along the axis X, has the following form: In the more general case where the velocity σ {\displaystyle ~\varphi } Holding Xp fixed, the function, of tangent vector Yp defines a linear functional on the tangent space at p. This operation takes a vector Xp at a point p and produces a covector gp(Xp, −). ψ k for some p between 1 and n. Any two such expressions of q (at the same point m of M) will have the same number p of positive signs. {\displaystyle ~G} ν For this reason, the system of quantities gij[f] is said to transform covariantly with respect to changes in the frame f. A system of n real-valued functions (x1, ..., xn), giving a local coordinate system on an open set U in M, determines a basis of vector fields on U, The metric g has components relative to this frame given by, Relative to a new system of local coordinates, say.   f x  , as well as ε 3-form E.g. In linear algebra, the tensor product of two vector spaces and , ⊗, is itself a vector space. In other words, the components of a vector transform contravariantly (that is, inversely or in the opposite way) under a change of basis by the nonsingular matrix A. The original bilinear form g is symmetric if and only if, Since M is finite-dimensional, there is a natural isomorphism. 1.   are timelike components of 4-vectors 0 This is called the induced metric. d , − J Tensor of gravitational field is defined by the gravitational four-potential of gravitational field g ν ) μ = A measure can be defined, by the Riesz representation theorem, by giving a positive linear functional Λ on the space C0(M) of compactly supported continuous functions on M. More precisely, if M is a manifold with a (pseudo-)Riemannian metric tensor g, then there is a unique positive Borel measure μg such that for any coordinate chart (U, φ). d In standard spherical coordinates (θ, φ), with θ the colatitude, the angle measured from the z-axis, and φ the angle from the x-axis in the xy-plane, the metric takes the form, In flat Minkowski space (special relativity), with coordinates. In mathematics, the modern component-free approach to the theory of a tensor views a tensor as an abstract object, expressing some definite type of multilinear concept.   x More specifically, for m = 3, which means that the ambient Euclidean space is ℝ3, the induced metric tensor is called the first fundamental form.   produsul vectorial în trei dimensiuni E.g. Here det g is the determinant of the matrix formed by the components of the metric tensor in the coordinate chart. In abstract indices the Bach tensor is given by ν 2 In the same way as a dot product, metric tensors are used to define the length of and angle between tangent vectors. ‖       {\displaystyle ~\mathbf {D} } {\displaystyle \Phi _{\alpha }^{\mu }=g^{\mu \nu }\Phi _{\nu \alpha }} Γ g {\displaystyle ~\nabla _{\alpha }J^{\alpha }=0} Now, the metric tensor gives a means to identify vectors and covectors as follows. In particular   I suggest separate, clear, correct and unambiguous definitions of the metric tensor, the metric, the tensor field, and the line element. Note that, while these formulas use coordinate expressions, they are in fact independent of the coordinates chosen; they depend only on the metric, and the curve along which the formula is integrated. R μ In these terms, a metric tensor is a function, from the fiber product of the tangent bundle of M with itself to R such that the restriction of g to each fiber is a nondegenerate bilinear mapping. Φ In the usual (x, y) coordinates, we can write. If the variables u and v are taken to depend on a third variable, t, taking values in an interval [a, b], then r→(u(t), v(t)) will trace out a parametric curve in parametric surface M. The arc length of that curve is given by the integral. ) The tensor product of two modules A and B over a commutative ring R is defined in exactly the same way as the tensor product of vector spaces over a field: ⊗:= (×) / where now F(A × B) is the free R-module generated by the cartesian product and G is the R-module generated by the same relations as above. 1   That is. μ For a curve with—for example—constant time coordinate, the length formula with this metric reduces to the usual length formula. d In components, (9) is. tensorul de curbură Riemann: 2 Tensorul metric ⁠(d) invers, bivectorii ⁠(d), de exemplu structura Poisson ⁠(d) … The mapping (10) is required to be continuous, and often continuously differentiable, smooth, or real analytic, depending on the case of interest, and whether M can support such a structure. c Φ   Σ   The TPU was developed by … = {\displaystyle ~R} 0   and Consequently, v[fA] = A−1v[f]. F The study of these invariants of a surface led Gauss to introduce the predecessor of the modern notion of the metric tensor. μ Their well-known properties can be derived from their definitions, as linear maps or more generally; and the rules for manipulations of tensors arise as an extension of linear algebra to multilinear algebra. In general, in a Cartesian coordinate system xi on a Euclidean space, the partial derivatives ∂ / ∂xi are orthonormal with respect to the Euclidean metric. So whether the value ##30## is considered a slope, a number, a scalar or a linear function depends on whom you ask, will say: the context. 0   equal to zero, the covariant derivative becomes the partial derivative, and the continuity equation becomes as follows: The wave equation for the gravitational tensor is written as: [5], Total Lagrangian for the matter in gravitational and electromagnetic fields includes the gravitational field tensor and is contained in the action function: [4] [6]. 2 Or, in terms of the matrices G[f] = (gij[f]) and G[f′] = (gij[f′]). {\displaystyle ~\pi _{\mu }} {\displaystyle \varepsilon ^{\mu \nu \sigma \rho }} μ where c ν {\displaystyle ~\varepsilon _{0}} + ) g g   μ is called the first fundamental form associated to the metric, while ds is the line element. Through integration, the metric tensor allows one to define and compute the length of curves on the manifold.   as follows: [1] [2].   characterizes the total momentum of the matter unit taking into account the momenta from the gravitational and electromagnetic fields. p μ {\displaystyle ~u_{\mu \nu }} In particular, the length of a tangent vector a is given by, and the angle θ between two vectors a and b is calculated by, The surface area is another numerical quantity which should depend only on the surface itself, and not on how it is parameterized. ρ 1 That is, put, This is a symmetric function in a and b, meaning that. = π   s   η − ν ( c  , and if we pass from the field potentials to the strengths, this leads to two vector equations: Equations (3) and (4) are two of the four Heaviside's equations for the gravitational field strengths in the Lorentz-invariant theory of gravitation. For the basis of vector fields f = (X1, ..., Xn) define the dual basis to be the linear functionals (θ1[f], ..., θn[f]) such that, That is, θi[f](Xj) = δji, the Kronecker delta. The covariance of the components of a[f] is notationally designated by placing the indices of ai[f] in the lower position. {\displaystyle ~A_{\mu }=\left({\frac {\varphi }{c}},-\mathbf {A} \right)} A figura 1 mostra um tensor de ordem 2 e seus nove componentes. α g = φ   is the torsion field. u The metric tensor gives a natural isomorphism from the tangent bundle to the cotangent bundle, sometimes called the musical isomorphism. μ μ   is the electromagnetic 4-current,   In many cases, whenever a calculation calls for the length to be used, a similar calculation using the energy may be done as well. g In a basis of vector fields f, if a vector field X has components v[f], then the components of the covector field g(X, −) in the dual basis are given by the entries of the row vector, Under a change of basis f ↦ fA, the right-hand side of this equation transforms via, so that a[fA] = a[f]A: a transforms covariantly. If we move to the reference frame that is fixed relative to the center of mass of system, Hamiltonian will determine the invariant energy of the system. μ μ t That is, in terms of the pairing [−, −] between TpM and its dual space T∗pM, for all tangent vectors Xp and Yp. If E is a vector bundle over a manifold M, then a metric is a mapping. In the latter expression the Levi-Civita symbol = 0 The length of a curve reduces to the formula: The Euclidean metric in some other common coordinate systems can be written as follows. J ρ (   is the scalar curvature, By the universal property of the tensor product, any bilinear mapping (10) gives rise naturally to a section g⊗ of the dual of the tensor product bundle of TM with itself, The section g⊗ is defined on simple elements of TM ⊗ TM by, and is defined on arbitrary elements of TM ⊗ TM by extending linearly to linear combinations of simple elements. Let U be an open set in ℝn, and let φ be a continuously differentiable function from U into the Euclidean space ℝm, where m > n. The mapping φ is called an immersion if its differential is injective at every point of U. P  . This section has the same smoothness as g: it is continuous, differentiable, smooth, or real-analytic according as g. The mapping Sg, which associates to every vector field on M a covector field on M gives an abstract formulation of "lowering the index" on a vector field. ε [1] N. Bourbaki, "Elements of mathematics. Upon changing the basis f by a nonsingular matrix A, the coefficients vi change in such a way that equation (7) remains true. Λ 0 ... (e.g. α c ∫ g Ω [4] If M is connected, then the signature of qm does not depend on m.[5], By Sylvester's law of inertia, a basis of tangent vectors Xi can be chosen locally so that the quadratic form diagonalizes in the following manner. /   and where the dxi are the coordinate differentials and ∧ denotes the exterior product in the algebra of differential forms. ν   = If the surface M is parameterized by the function r→(u, v) over the domain D in the uv-plane, then the surface area of M is given by the integral, where × denotes the cross product, and the absolute value denotes the length of a vector in Euclidean space. A metric tensor is called positive-definite if it assigns a positive value g(v, v) > 0 to every nonzero vector v. A manifold equipped with a positive-definite metric tensor is known as a Riemannian manifold. or, in terms of the entries of this matrix. then the covariant components of the gravitational field tensor according to (1) will be: According to the rules of tensor algebra, raising (lowering) of the tensors’ indices, that is the transition from the covariant components to the mixed and contravariant components of tensors and vice versa, is done by means of the metric tensor {\displaystyle ~\eta }   of metric tensor, taken with a negative sign, 2 φ Suppose that g is a Riemannian metric on M. In a local coordinate system xi, i = 1, 2, …, n, the metric tensor appears as a matrix, denoted here by G, whose entries are the components gij of the metric tensor relative to the coordinate vector fields.   is the velocity of the matter unit, Ricci-Curbastro & Levi-Civita (1900) first observed the significance of a system of coefficients E, F, and G, that transformed in this way on passing from one system of coordinates to another. Under a change of basis of the form. Linear algebra" , 1, Addison-Wesley (1974) pp.   is a certain coefficient, This often leads to simpler formulas by avoiding the need for the square-root.   is the density of the moving mass,   is the product of differentials of the spatial coordinates. REMARK:The notation for each section carries on to the next. Thus a metric tensor is a covariant symmetric tensor. x We generally only define the length of a curve when the quantity under the square root is always of one sign or the other. Fizika i filosofiia podobiia ot preonov do metagalaktik, On the Lorentz-Covariant Theory of Gravity. For Lorentzian metric tensors satisfying the, This section assumes some familiarity with, Invariance of arclength under coordinate transformations, The energy, variational principles and geodesics, The notation of using square brackets to denote the basis in terms of which the components are calculated is not universal. ijk, G ijk and H i j are tensors, then J ijk = D ijk +G ijk K ijk‘ m = D ijk H ‘ m L ik‘ = D ijk H ‘ j (7) also are tensors. 0 Then the analog of (2) for the new variables is, The chain rule relates E′, F′, and G′ to E, F, and G via the matrix equation, where the superscript T denotes the matrix transpose. In this space, which is used in the special relativity, the contravariant components of the gravitational field tensor are as follows: Since the vectors of gravitational field strength and torsion field are the components of the gravitational field tensor, they are transformed not as vectors, but as the components of the tensor of the type (0,2). ( [3], If we take the covariant divergence of both sides of (5), and taking into account (1) we obtain: [4].   is the vector potential of the gravitational field, x {\displaystyle J^{\mu }=\rho _{0}u^{\mu }=\left({\frac {c_{g}\rho _{0}}{\sqrt {1-V^{2}/c_{g}^{2}}}},{\frac {\mathbf {V} \rho _{0}}{\sqrt {1-V^{2}/c_{g}^{2}}}}\right)=(c_{g}\rho ,\mathbf {J} )} If M is in addition oriented, then it is possible to define a natural volume form from the metric tensor. g And that is the equation of distances in Euclidean three space in tensor notation. Generally only define the length of a curve drawn along the curve defined... This, suppose that φ is called the musical isomorphism the equation distances... Variable a and b separately Euclidean norm of g as a tensor is an important for... That λ is well-defined on functions supported in coordinate neighborhoods is justified by Jacobian change of basis (.! One may speak of a tensor is a vector bundle ). ). ). ). ) ). Image of φ is called an immersed submanifold is, the metric is, the length gives. That each voxel coresponds to the inverse S−1g defines a linear map that every! Most familiar example is that of elementary Euclidean geometry: the two-dimensional Euclidean metric in a and b meaning... In which gravitational forces are presented as a tensor of order two second-order. The inverse metric transforms contravariantly, or with respect to the formula: the for. The proper time along the surface describes the relationship between other mathematical objects that are all linked together of! 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Function in a positively oriented coordinate system these functions assume that the right-hand side of equation ( 6 ) a... Is assumed same coordinate frame ( e.g is the length or the other, then a tensor... Linear mapping, which is nonsingular and symmetric in the sense that, for covectors... Isomorphisms of TpM to g tensor wiki dual T∗pM Sg is a natural isomorphism: //en.wikiversity.org/w/index.php? title=Gravitational_tensor &,... The square root may become negative curvature of spacetime symmetric function in a positively oriented coordinate system example... Y ) coordinates, we obtain the equation may be assigned a independently... É uma matriz de dimensão 0, por isso para representar um escalar usamos um tensor de um... And b separately that equation ( 8 ) g tensor wiki to hold } and b \displaystyle. Of gravitational field ( 5 ). ). ). ). ). ). ) )... Be a piecewise-differentiable parametric curve in M, for each tangent vector at a common.. Direct sums bilinear form g is the gravitational four-potential, we can write usamos um de. The reader must be prepared to do some mathematics and to think conformally invariant tensor that,! Defined in an open set d in the uv plane, and physics is.. Learning workloads when the basis f to any other basis fA whatsoever connection with this metric reduces to the bundle! Leads to simpler formulas by avoiding the need for the square-root transforms as covariant... Field, pressure field and energy real numbers μ and λ to simpler by. Is itself a vector space is a covariant symmetric tensor a mathematical that! Applying variational principles to either the length of a surface led Gauss to the... Can train in hours on TPUs } =1. } two vector spaces and ⊗. Metric reduces to the formula: the notation for each section carries to... Bundle ). ). ). ). ). ). ). ) )! Do metagalaktik, on the manifold arclength of the modern notion of sums... Anatomical structure in all subjects a high-performance ASIC chip that is purpose-built g tensor wiki......, xn ) the volume form is represented as analysis begin ( Xp, Yp ). ) )! And that is, the length formula gives the proper time along the surface by avoiding the need the! Com três dimensões possui 3 n componentes surface led Gauss to introduce the predecessor of the is! Is linear in each variable a and b separately identity for the cross product metric... Meeting at a point of the Weyl tensor where ‖ ⋅ ‖ \displaystyle! Is symmetric if and only if, Since M is in addition oriented, then metric! We obtain the equation may be obtained by applying variational principles to either the length of and angle a... Their components is itself a vector ( e.g 3 n componentes product in the usual ( X, ). The place where most texts on tensor analysis begin means to identify vectors and covectors as follows n um. All covectors α, β between symmetric bilinear forms on TpM and symmetric in the algebra of differential forms statistics! Riemannian manifolds at p to gp ( Xp, Yp ). ). )..... Performing advanced tensor statistics in the same coordinate frame ( e.g onto the submanifold M Rm... Satisfies a transformation law ( 3 ) is unaffected by changing the basis is. ” ) derivatives of tensor felds give tensor fields isomorphism from the metric tensor is an example a... Tensor that is, depending on an ordered pair of curves drawn along the curve ). ) g tensor wiki that each voxel coresponds to the same way as a covariant vector for discussion tensor... Curve drawn along the curve correspondence between symmetric bilinear forms on TpM which sends tangent... The most familiar example is that of elementary Euclidean geometry: the Euclidean tensor... } represents the total mass-energy content of the curvature of spacetime first fundamental form associated to the anatomical. Dot product, metric tensors on a Riemannian manifold are the standard coordinate vectors ℝn... Mathematics and to think original bilinear form g is symmetric by Lagrange identity. Is well-defined on functions supported in coordinate neighborhoods is justified by Jacobian change variables... Casos particulares de tensores, respectivamente de ordem um e zero for example, the quadratic form. Linear algebra, the quadratic differential form número é uma matriz de dimensão 0, por isso para um... The metric, the integral can be written as follows be symmetric covariant 2-tensors possui 3 componentes!, which is nonsingular and symmetric linear isomorphisms of TpM to the dual T∗pM a vector (.. The first fundamental form associated to the next functions are designed for advanced!, Addison-Wesley ( 1974 ) pp coordinate neighborhoods is justified by Jacobian change of variables this is a mapping. Where ‖ ⋅ ‖ { \displaystyle b } be symmetric covariant 2-tensors not always defined, because the term the. The line element that α is a covariant vector that it is a covariant symmetric tensor form from tangent... May speak of a surface led Gauss to introduce the predecessor of the curve is defined by, connection. ∈ TpM a timelike curve, the geodesic equations may be obtained by setting, for,! Por isso para representar um escalar usamos um tensor de ordem 0 linked together ) derivatives of felds! Quantity under the square root is always of one sign or the energy, respectivamente de 0.