Prove that $U^sigma nabla_sigma U^mu = g^mununabla_nu ln V$A question about Killing vector and Riemann curvature tensorA question about Riemann curvature tensor and metric tensorGeodesics on the cylinder and Levi-Civita connectionExpression of $R_ijk^s$ in terms of coefficients $Gamma_ij^k$ of the Riemannian connectionInertial frames: from General Relativity to Special RelativityVariation of the Spin Connection with respect to the VierbeinCovariant derivative of tensor densitiesProve the geodesic on 2-sphere is the great circleProof of the Symmetry LemmaWhat is the curvature form $Omega$ associated with the Levi-Civita connection for the complexified $n$-sphere with respect to the standard metric?
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Prove that $U^sigma nabla_sigma U^mu = g^mununabla_nu ln V$
A question about Killing vector and Riemann curvature tensorA question about Riemann curvature tensor and metric tensorGeodesics on the cylinder and Levi-Civita connectionExpression of $R_ijk^s$ in terms of coefficients $Gamma_ij^k$ of the Riemannian connectionInertial frames: from General Relativity to Special RelativityVariation of the Spin Connection with respect to the VierbeinCovariant derivative of tensor densitiesProve the geodesic on 2-sphere is the great circleProof of the Symmetry LemmaWhat is the curvature form $Omega$ associated with the Levi-Civita connection for the complexified $n$-sphere with respect to the standard metric?
$begingroup$
Let $U^mu$ be a vector in 4-dimensional Minkowski space with norm $-1$ and $K^mu = V(x)U^mu$ a vector proportional to it. We can write $V(x) = sqrt-K_nu K^nu$.
(This setup comes from physics where $U^mu$ is a four-velocity, $K^mu$ is a normalized time-like Killing vector for an observer at infinity and $V(x)$ is called the redshift factor.)
Then, define $a^mu$ (the four-acceleration) by $U^sigma nabla_sigma U^mu$, where $nabla$ is the Christoffel connection.
According to Sean Carroll, Spacetime and Geometry, p. 247, $a_mu = nabla_muln V$. Why?
Attempt:
beginalignnabla_muln V &= frac 12V^2nabla_muleft(-K_nu K^nuright)\
&=-frac 12V^2left((nabla_mu K_nu)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left((nabla_mu g_rhonuK^rho)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left(K_rhonabla_mu K^rho + K_nunabla_mu K^nuright)\
&=-frac K_nunabla_mu K^nuV^2\
&= -frac 1VU_nunabla_muleft(VU^nuright)\
&= -U_nunabla_mu U^nu - frac 1 VU_nu U^nunabla_mu Vendalign
differential-geometry semi-riemannian-geometry
$endgroup$
add a comment |
$begingroup$
Let $U^mu$ be a vector in 4-dimensional Minkowski space with norm $-1$ and $K^mu = V(x)U^mu$ a vector proportional to it. We can write $V(x) = sqrt-K_nu K^nu$.
(This setup comes from physics where $U^mu$ is a four-velocity, $K^mu$ is a normalized time-like Killing vector for an observer at infinity and $V(x)$ is called the redshift factor.)
Then, define $a^mu$ (the four-acceleration) by $U^sigma nabla_sigma U^mu$, where $nabla$ is the Christoffel connection.
According to Sean Carroll, Spacetime and Geometry, p. 247, $a_mu = nabla_muln V$. Why?
Attempt:
beginalignnabla_muln V &= frac 12V^2nabla_muleft(-K_nu K^nuright)\
&=-frac 12V^2left((nabla_mu K_nu)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left((nabla_mu g_rhonuK^rho)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left(K_rhonabla_mu K^rho + K_nunabla_mu K^nuright)\
&=-frac K_nunabla_mu K^nuV^2\
&= -frac 1VU_nunabla_muleft(VU^nuright)\
&= -U_nunabla_mu U^nu - frac 1 VU_nu U^nunabla_mu Vendalign
differential-geometry semi-riemannian-geometry
$endgroup$
add a comment |
$begingroup$
Let $U^mu$ be a vector in 4-dimensional Minkowski space with norm $-1$ and $K^mu = V(x)U^mu$ a vector proportional to it. We can write $V(x) = sqrt-K_nu K^nu$.
(This setup comes from physics where $U^mu$ is a four-velocity, $K^mu$ is a normalized time-like Killing vector for an observer at infinity and $V(x)$ is called the redshift factor.)
Then, define $a^mu$ (the four-acceleration) by $U^sigma nabla_sigma U^mu$, where $nabla$ is the Christoffel connection.
According to Sean Carroll, Spacetime and Geometry, p. 247, $a_mu = nabla_muln V$. Why?
Attempt:
beginalignnabla_muln V &= frac 12V^2nabla_muleft(-K_nu K^nuright)\
&=-frac 12V^2left((nabla_mu K_nu)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left((nabla_mu g_rhonuK^rho)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left(K_rhonabla_mu K^rho + K_nunabla_mu K^nuright)\
&=-frac K_nunabla_mu K^nuV^2\
&= -frac 1VU_nunabla_muleft(VU^nuright)\
&= -U_nunabla_mu U^nu - frac 1 VU_nu U^nunabla_mu Vendalign
differential-geometry semi-riemannian-geometry
$endgroup$
Let $U^mu$ be a vector in 4-dimensional Minkowski space with norm $-1$ and $K^mu = V(x)U^mu$ a vector proportional to it. We can write $V(x) = sqrt-K_nu K^nu$.
(This setup comes from physics where $U^mu$ is a four-velocity, $K^mu$ is a normalized time-like Killing vector for an observer at infinity and $V(x)$ is called the redshift factor.)
Then, define $a^mu$ (the four-acceleration) by $U^sigma nabla_sigma U^mu$, where $nabla$ is the Christoffel connection.
According to Sean Carroll, Spacetime and Geometry, p. 247, $a_mu = nabla_muln V$. Why?
Attempt:
beginalignnabla_muln V &= frac 12V^2nabla_muleft(-K_nu K^nuright)\
&=-frac 12V^2left((nabla_mu K_nu)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left((nabla_mu g_rhonuK^rho)K^nu + K_nunabla_mu K^nuright)\
&=-frac 12V^2left(K_rhonabla_mu K^rho + K_nunabla_mu K^nuright)\
&=-frac K_nunabla_mu K^nuV^2\
&= -frac 1VU_nunabla_muleft(VU^nuright)\
&= -U_nunabla_mu U^nu - frac 1 VU_nu U^nunabla_mu Vendalign
differential-geometry semi-riemannian-geometry
differential-geometry semi-riemannian-geometry
asked Mar 21 at 13:36
RodrigoRodrigo
2,9751231
2,9751231
add a comment |
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