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The flat model: vanishing connection and curvature, translation Killing fields and straight geodesics
Statement
Let be the flat model of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart with its inertial chart , and let be its metric-selected connection, whose existence and uniqueness are supplied by Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields. Let be a real parameter.
(a) Vanishing connection. In the inertial chart all Christoffel symbols of vanish identically:
(b) Vanishing curvature. The curvature operator of vanishes identically, ; consequently the curvature components, the Ricci tensor, the scalar curvature and the Einstein tensor vanish identically,
(c) Translation Killing fields. Each coordinate field is a Killing field of (Killing fields of a Lorentzian metric); in particular the time orientation field is a unit timelike Killing field.
(d) Straight geodesics. A smooth curve on an interval with nonempty interior (Geodesic of an affine connection) is a geodesic of if and only if there are such that
For such a geodesic the speed is constant, ; the maximal geodesic with and has domain . If and , the geodesic is a future timelike worldline (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold) and, for any , the parameter is proper time up to an additive constant, with the physical four-velocity , (Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent clause 3).
(e) Inertial-chart velocity reading. Let be a geodesic as in (d) with , and . Define ; this is strictly increasing, and on define . Then for its spatial component , and the coordinate velocity is the constant vector . With from the Euclidean inner product (The Euclidean inner product on ), timelikeness gives .
Facts & Assumptions
Given: The flat model of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart with its metric-selected connection , the inertial chart , a real parameter , and a smooth curve .
In a chart, the Christoffel symbols of the metric-selected connection are ; equivalently, metric compatibility and torsion freedom are the identities and (Christoffel symbols of an affine connection, Torsion freedom and metric compatibility in chart components, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields).
In a chart with Christoffel symbols , the curvature components are , and , , (Tensoriality of the curvature, its coordinate formula and its point-normal metric formula clause (b), The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (c)).
In coordinates, a smooth curve is a geodesic if and only if on every parameter subinterval lying in the chart, where (Coordinate geodesic equation, Geodesic of an affine connection).
A smooth vector field on has a unique maximal local flow , , whose fibres are the maximal integral curves; if is defined for all and all it is a global flow (The fundamental theorem on flows, Local and global flows generated by a vector field, Complete vector fields).
For a smooth vector field , the Lie derivative of the metric is , where is the flow of ; is a Killing field exactly when (Killing fields of a Lorentzian metric, The Lie derivative of a tensor field).
On a future-directed timelike geodesic with affine parameter and constant speed , the parameter is proper time, and satisfies (Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent clause 3, Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold).
In the Euclidean norm satisfies (The Euclidean inner product on ).
Proof
(The connection vanishes.) In the inertial chart all metric components are the constants by The flat model spacetime: the Minkowski metric on R^4 and its inertial chart clause (a), so each partial derivative vanishes identically. The formula of [L1] gives at every point of , proving (a).
(The coordinate fields are Killing.) Fix and consider the map in the identity chart, where is the -th standard basis vector. The curve has coordinate derivative at every parameter, so it is an integral curve of ; it is defined for all . By uniqueness of maximal integral curves in [L4], the maximal local flow of is this global flow . In the inertial chart the differential of is the identity of the chart basis and the metric components are the constants , so the components of the pulled-back field are for all ; hence for every . By [L5], , so is a Killing field. In particular is Killing, and by clause (c) of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart, so it is unit timelike. This proves (c).
(The curvature vanishes.) Substituting into the coordinate formula of [L2] gives ; since , and are obtained from and by the contractions and products displayed in [L2], and is the constant matrix , all of them vanish identically. The curvature operator vanishes because its components in the chart vanish, and a smooth tensor field all of whose components in one chart vanish is the zero field. This proves (b).
(Geodesics are straight lines.) Let be the coordinate expression of a smooth curve. By [L3] and step 1.1, is a geodesic if and only if for on every parameter subinterval, that is, if and only if for some ; then the maximal interval is all of , because the affine expression extends to and is again a solution. The speed is constant for every geodesic by clause 3 of Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed, and inserting the affine expression gives the value . This proves the first two claims of (d).
(Future timelike geodesics and proper time.) Suppose with . By clause (c) of The flat model spacetime: the Minkowski metric on R^4 and its inertial chart, is a future timelike curve, and by [L6] the parameter is proper time, with for . This proves the third claim of (d); for (e), write , so that is constant; from and we have , hence [L7] gives .
Remarks
- Flatness is a computation, not a definition. The model is called flat in The flat model spacetime: the Minkowski metric on R^4 and its inertial chart; its curvature vanishing is proved here from the constant components, and no converse statement (that a flat Lorentzian manifold is isometric to this model) is asserted.
- Maximality. The geodesics of step 2.2 are complete as curves of the flat model; this completeness is special to the model and is not inherited by metrics only locally isometric to it.
- Use. Clause (b) supplies the curvature computation for the flat vacuum model on this page; clause (d) supplies the kinematic reading of that model and the kinetic input of the weak-field bridge.
Depends on
The flat model spacetime: the Minkowski metric on R^4 and its inertial chart
Metric compatibility, torsion freedom and the metric-selected connection class
Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
Christoffel symbols of an affine connection
Torsion freedom and metric compatibility in chart components
Tensoriality of the curvature, its coordinate formula and its point-normal metric formula
The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors
Coordinate geodesic equation
Geodesic of an affine connection
Killing fields of a Lorentzian metric
The Lie derivative of a tensor field
Local and global flows generated by a vector field
Complete vector fields
The fundamental theorem on flows
A smooth vector field is a smooth section of the tangent bundle
Proper time is well defined and reparametrization invariant; the four-velocity is its proper-time tangent
Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold
Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed
The Euclidean inner product on
Dependency tree · 2 levels
Sources
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Ch. 3: the geodesic equation (3.47) and the statement that in flat space geodesics are straight lines in inertial coordinates, printed pp. 70-71 (PDF pp. 77-78)
- H. S. Reall, Part III General Relativity (Cambridge, October 12, 2022 revision), section 2.1: vanishing Christoffel symbols and curvature of the flat metric in Cartesian coordinates, printed pp. 25-27 (PDF pp. 26-28)
- D. Tong, General Relativity (Cambridge Part III Mathematical Tripos, Michaelmas 2019), section 3.3.1: the geodesic equation and the statement that constant-velocity straight lines are the geodesics of the flat metric, printed pp. 119-121 (PDF pp. 126-128)