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Acceleration (differential geometry)

In mathematics and physics, acceleration is the rate of change of velocity of a curve with respect to a given linear connection. This operation provides us with a measure of the rate and direction of the "bend".

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In mathematics and physics, acceleration is the rate of change of velocity of a curve with respect to a given linear connection. This operation provides us with a measure of the rate and direction of the "bend".12

Formal definition

Let be given a differentiable manifold M {\displaystyle M} , considered as spacetime (not only space), with a connection Γ {\displaystyle \Gamma } . Let γ : R M {\displaystyle \gamma \colon \mathbb {R} \to M} be a curve in M {\displaystyle M} with tangent vector, i.e. (spacetime) velocity, γ ˙ ( τ ) {\displaystyle {\dot {\gamma }}(\tau )} , with parameter τ {\displaystyle \tau } .

The (spacetime) acceleration vector of γ {\displaystyle \gamma } is defined by γ ˙ γ ˙ {\displaystyle \nabla _{\dot {\gamma }}{\dot {\gamma }}} , where {\displaystyle \nabla } denotes the covariant derivative associated to Γ {\displaystyle \Gamma } .

It is a covariant derivative along γ {\displaystyle \gamma } , and it is often denoted by

γ ˙ γ ˙ = γ ˙ d τ . {\displaystyle \nabla _{\dot {\gamma }}{\dot {\gamma }}={\frac {\nabla {\dot {\gamma }}}{d\tau }}.}

With respect to an arbitrary coordinate system ( x μ ) {\displaystyle (x^{\mu })} , and with ( Γ λ μ ν ) {\displaystyle (\Gamma ^{\lambda }{}_{\mu \nu })} being the components of the connection (i.e., covariant derivative μ := / x μ {\displaystyle \nabla _{\mu }:=\nabla _{\partial /\partial x^{\mu }}} ) relative to this coordinate system, defined by

/ x μ x ν = Γ λ μ ν x λ , {\displaystyle \nabla _{\partial /\partial x^{\mu }}{\frac {\partial }{\partial x^{\nu }}}=\Gamma ^{\lambda }{}_{\mu \nu }{\frac {\partial }{\partial x^{\lambda }}},}

for the acceleration vector field a μ := ( γ ˙ γ ˙ ) μ {\displaystyle a^{\mu }:=(\nabla _{\dot {\gamma }}{\dot {\gamma }})^{\mu }} one gets:

a μ = v ρ ρ v μ = d v μ d τ + Γ μ ν λ v ν v λ = d 2 x μ d τ 2 + Γ μ ν λ d x ν d τ d x λ d τ , {\displaystyle a^{\mu }=v^{\rho }\nabla _{\rho }v^{\mu }={\frac {dv^{\mu }}{d\tau }}+\Gamma ^{\mu }{}_{\nu \lambda }v^{\nu }v^{\lambda }={\frac {d^{2}x^{\mu }}{d\tau ^{2}}}+\Gamma ^{\mu }{}_{\nu \lambda }{\frac {dx^{\nu }}{d\tau }}{\frac {dx^{\lambda }}{d\tau }},}

where x μ ( τ ) := γ μ ( τ ) {\displaystyle x^{\mu }(\tau ):=\gamma ^{\mu }(\tau )} is the local expression for the path γ {\displaystyle \gamma } , and v ρ := ( γ ˙ ) ρ {\displaystyle v^{\rho }:=({\dot {\gamma }})^{\rho }} .

The concept of acceleration is a covariant derivative concept. In other words, in order to define acceleration an additional structure on M {\displaystyle M} must be given.

Using abstract index notation, the acceleration of a given curve with unit tangent vector ξ a {\displaystyle \xi ^{a}} is given by ξ b b ξ a {\displaystyle \xi ^{b}\nabla _{b}\xi ^{a}} .3

See also

See also

Notes

Notes

  1. Friedman, M. (1983). Foundations of Space-Time Theories. Princeton: Princeton University Press. p. 38. ISBN 0-691-07239-6.
  2. Benn, I.M.; Tucker, R.W. (1987). An Introduction to Spinors and Geometry with Applications in Physics. Bristol and New York: Adam Hilger. p. 203. ISBN 0-85274-169-3.
  3. Malament, David B. (2012). Topics in the Foundations of General Relativity and Newtonian Gravitation Theory. Chicago: University of Chicago Press. ISBN 978-0-226-50245-8.
References

References

  • Friedman, M. (1983). Foundations of Space-Time Theories. Princeton: Princeton University Press. ISBN 0-691-07239-6.
  • Dillen, F. J. E.; Verstraelen, L.C.A. (2000). Handbook of Differential Geometry. Vol. 1. Amsterdam: North-Holland. ISBN 0-444-82240-2.
  • Pfister, Herbert; King, Markus (2015). Inertia and Gravitation. The Fundamental Nature and Structure of Space-Time. Vol. The Lecture Notes in Physics. Volume 897. Heidelberg: Springer. doi:10.1007/978-3-319-15036-9. ISBN 978-3-319-15035-2.