Abstract:Abstract. This paper considers 4-dimensional manifolds upon which there is a Lorentz metric h and a symmetric connection Γ and which are originally assumed unrelated. It then derives sufficient conditions on h and Γ (expressed through the curvature tensor of Γ) for Γ to be the Levi-Civita connection of some (local) Lorentz metric g and calculates the relationship between g and h. Some examples are provided which help to assess the strength of the sufficient conditions derived.
“…To see this note that g ′ need not have Lorentz signature (−, +, +, +) but, if this is insisted upon, the curvature classification scheme, including the nature (timelike, spacelike or null) of F and * F in class B, r in class C and F in class D is the same whether taken for (the common curvature tensor) Riem with g or Riem with g ′ . In this sense it is a classification of Riem, independent of the metric generating Riem [6].…”
Section: Notation and Preliminary Remarksmentioning
Abstract. A study is made of 4-dimensional Lorentz manifolds which are projectively related, that is, whose Levi-Civita connections give rise to the same (unparameterised) geodesics. A brief review of some relevant recent work is provided and a list of new results connecting projective relatedness and the holonomy type of the Lorentz manifold in question is given. This necessitates a review of the possible holonomy groups for such manifolds which, in turn, requires a certain convenient classification of the associated curvature tensors. These reviews are provided.
“…To see this note that g ′ need not have Lorentz signature (−, +, +, +) but, if this is insisted upon, the curvature classification scheme, including the nature (timelike, spacelike or null) of F and * F in class B, r in class C and F in class D is the same whether taken for (the common curvature tensor) Riem with g or Riem with g ′ . In this sense it is a classification of Riem, independent of the metric generating Riem [6].…”
Section: Notation and Preliminary Remarksmentioning
Abstract. A study is made of 4-dimensional Lorentz manifolds which are projectively related, that is, whose Levi-Civita connections give rise to the same (unparameterised) geodesics. A brief review of some relevant recent work is provided and a list of new results connecting projective relatedness and the holonomy type of the Lorentz manifold in question is given. This necessitates a review of the possible holonomy groups for such manifolds which, in turn, requires a certain convenient classification of the associated curvature tensors. These reviews are provided.
“…where, as mentioned earlier, Ru denotes the covector at p with components R ′ ab u b and similarly for Rz, Rx and Ry. Recalling that in this notation, ẽa are, respectively, the covectors with components u a , z a , x a and y a , one can substitute these expansions into (19) and (20) and equate coefficients of the e ′ a e ′ b in an obvious way. One finds that several of these vanish and certain others are forced to be equal.…”
Section: Now If In Additionmentioning
confidence: 99%
“…To see this, consider the following example (see and cf. [19,20,21]). Let U be the open subset of R 4 given by x 0 > 0 and let ϕ : U → R be given by ϕ(x 0 , x 1 , x 2 , x 3 )=log x 0 .…”
mentioning
confidence: 99%
“…Then, with a closed 1-form ψ defined on U by the components ψ a = (1 − e ϕ ) −1 ϕ a , define another connection ∇ ′ on U by (52). Then ∇ ′ is the desired connection on U because it is known that ∇ ′ is not a metric connection [19,20]]. Thus, knowledge of the total (unparametrised) geodesic structure of space-time does not determine whether the connection is metric or not.…”
This paper discusses the extent to which one can determine the spacetime metric from a knowledge of a certain subset of the (unparametrised) geodesics of its Levi-Civita connection, that is, from the experimental evidence of the equivalence principle. It is shown that, if the space-time concerned is known to be vacuum, then the Levi-Civita connection is uniquely determined and its associated metric is uniquely determined up to a choice of units of measurement, by the specification of these geodesics. It is further demonstrated that if two space-times share the same unparametrised geodesics and only one is assumed vacuum then their Levi-Civita connections are again equal (and so the other metric is also a vacuum metric) and the first result above is recovered.
“…Finding the metric has been studied extensively [5,6,8,9,10,11,12,13,14,16,19,20,21,23,24,25,26,27,28]. These works provide a mixture of somewhat general algorithms and studies of existence and uniqueness.…”
The fundamental theorem of Riemannian geometry is inverted for analytic Christoffel symbols. The inversion formula, henceforth dubbed Ricardo's formula, is obtained without ancillary assumptions. Even though Ricardo's formula can mathematically give the full answer, it is argued that the solution should be taken only up to a constant conformal factor. A procedure to obtain the Christoffel symbols out of unparameterized geodesics is sketched. Thus, a complete framework to obtain the metric out of measurements is presented. The framework is suitable for analysis of experiments testing the geometrical nature of gravity.
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