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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?













1












$begingroup$


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










share|cite|improve this question









$endgroup$
















    1












    $begingroup$


    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










    share|cite|improve this question









    $endgroup$














      1












      1








      1





      $begingroup$


      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










      share|cite|improve this question









      $endgroup$




      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






      share|cite|improve this question













      share|cite|improve this question











      share|cite|improve this question




      share|cite|improve this question










      asked Mar 21 at 13:36









      RodrigoRodrigo

      2,9751231




      2,9751231




















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