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The gradient of a scalar function


dotting gradient in spherical coordinates with displacement vectorDivergence in spherical coordinates$operatornamediv$ and $operatornamegrad$ in spherical coordinates. Formula from general relativity goes crazyWhy the gradient of the r vector is the identity map, geometrically speaking?Finding the Gradient of a Tensor FieldFinding the Gradient of a Vector Function by its ComponentsThe gradient on sphereDivergence in spherical coordinates starting from contractionTime derivative of scalar function that takes vector as argument













0












$begingroup$


I found this definition of gradient of scalar function $Phi$:



$nabla Phi = (g^ijpartial_j) vecg_i$



And I know:



Metric tensor of spherical coordinates



$g_11 = 1$



$g_22 = r^2$



$g_33 = r^2sintheta$



But I do not know how to use first definition. How can I find gradient of scalar function in spherical coordinates by using metric tensor










share|cite|improve this question









$endgroup$
















    0












    $begingroup$


    I found this definition of gradient of scalar function $Phi$:



    $nabla Phi = (g^ijpartial_j) vecg_i$



    And I know:



    Metric tensor of spherical coordinates



    $g_11 = 1$



    $g_22 = r^2$



    $g_33 = r^2sintheta$



    But I do not know how to use first definition. How can I find gradient of scalar function in spherical coordinates by using metric tensor










    share|cite|improve this question









    $endgroup$














      0












      0








      0





      $begingroup$


      I found this definition of gradient of scalar function $Phi$:



      $nabla Phi = (g^ijpartial_j) vecg_i$



      And I know:



      Metric tensor of spherical coordinates



      $g_11 = 1$



      $g_22 = r^2$



      $g_33 = r^2sintheta$



      But I do not know how to use first definition. How can I find gradient of scalar function in spherical coordinates by using metric tensor










      share|cite|improve this question









      $endgroup$




      I found this definition of gradient of scalar function $Phi$:



      $nabla Phi = (g^ijpartial_j) vecg_i$



      And I know:



      Metric tensor of spherical coordinates



      $g_11 = 1$



      $g_22 = r^2$



      $g_33 = r^2sintheta$



      But I do not know how to use first definition. How can I find gradient of scalar function in spherical coordinates by using metric tensor







      tensors spherical-coordinates gradient-flows






      share|cite|improve this question













      share|cite|improve this question











      share|cite|improve this question




      share|cite|improve this question










      asked Mar 17 at 21:11









      Ali OzAli Oz

      83




      83




















          1 Answer
          1






          active

          oldest

          votes


















          0












          $begingroup$

          You need the inverse of the tensor. Since it is diagonal, you have $g^11=1$, $g^22=1/r^2$ and $g^33=1/r^2sin^2theta$ (I think there is a typo in your last component).



          The first component of the gradient of $Phi$ would be
          $$
          g^11partialPhi/partial r+g^12partialPhi/partial theta+g^13partialPhi/partial phi=partialPhi/partial r.
          $$

          since the off-diagonal elements of the metric tensor are zero. The second component would be
          $$
          g^21partialPhi/partial r+g^22partialPhi/partial theta+g^23partialPhi/partial phi=frac1r^2partialPhi/partial theta.
          $$

          and the third
          $$
          g^31partialPhi/partial r+g^32partialPhi/partial theta+g^33partialPhi/partial phi=frac1r^2sin^2thetapartialPhi/partial phi.
          $$

          Observe that these are the components in the base $g_i$, which is orthogonal but not orthonormal. If you use unit vectors you get a slightly different expression.






          share|cite|improve this answer









          $endgroup$












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            1 Answer
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            active

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            0












            $begingroup$

            You need the inverse of the tensor. Since it is diagonal, you have $g^11=1$, $g^22=1/r^2$ and $g^33=1/r^2sin^2theta$ (I think there is a typo in your last component).



            The first component of the gradient of $Phi$ would be
            $$
            g^11partialPhi/partial r+g^12partialPhi/partial theta+g^13partialPhi/partial phi=partialPhi/partial r.
            $$

            since the off-diagonal elements of the metric tensor are zero. The second component would be
            $$
            g^21partialPhi/partial r+g^22partialPhi/partial theta+g^23partialPhi/partial phi=frac1r^2partialPhi/partial theta.
            $$

            and the third
            $$
            g^31partialPhi/partial r+g^32partialPhi/partial theta+g^33partialPhi/partial phi=frac1r^2sin^2thetapartialPhi/partial phi.
            $$

            Observe that these are the components in the base $g_i$, which is orthogonal but not orthonormal. If you use unit vectors you get a slightly different expression.






            share|cite|improve this answer









            $endgroup$

















              0












              $begingroup$

              You need the inverse of the tensor. Since it is diagonal, you have $g^11=1$, $g^22=1/r^2$ and $g^33=1/r^2sin^2theta$ (I think there is a typo in your last component).



              The first component of the gradient of $Phi$ would be
              $$
              g^11partialPhi/partial r+g^12partialPhi/partial theta+g^13partialPhi/partial phi=partialPhi/partial r.
              $$

              since the off-diagonal elements of the metric tensor are zero. The second component would be
              $$
              g^21partialPhi/partial r+g^22partialPhi/partial theta+g^23partialPhi/partial phi=frac1r^2partialPhi/partial theta.
              $$

              and the third
              $$
              g^31partialPhi/partial r+g^32partialPhi/partial theta+g^33partialPhi/partial phi=frac1r^2sin^2thetapartialPhi/partial phi.
              $$

              Observe that these are the components in the base $g_i$, which is orthogonal but not orthonormal. If you use unit vectors you get a slightly different expression.






              share|cite|improve this answer









              $endgroup$















                0












                0








                0





                $begingroup$

                You need the inverse of the tensor. Since it is diagonal, you have $g^11=1$, $g^22=1/r^2$ and $g^33=1/r^2sin^2theta$ (I think there is a typo in your last component).



                The first component of the gradient of $Phi$ would be
                $$
                g^11partialPhi/partial r+g^12partialPhi/partial theta+g^13partialPhi/partial phi=partialPhi/partial r.
                $$

                since the off-diagonal elements of the metric tensor are zero. The second component would be
                $$
                g^21partialPhi/partial r+g^22partialPhi/partial theta+g^23partialPhi/partial phi=frac1r^2partialPhi/partial theta.
                $$

                and the third
                $$
                g^31partialPhi/partial r+g^32partialPhi/partial theta+g^33partialPhi/partial phi=frac1r^2sin^2thetapartialPhi/partial phi.
                $$

                Observe that these are the components in the base $g_i$, which is orthogonal but not orthonormal. If you use unit vectors you get a slightly different expression.






                share|cite|improve this answer









                $endgroup$



                You need the inverse of the tensor. Since it is diagonal, you have $g^11=1$, $g^22=1/r^2$ and $g^33=1/r^2sin^2theta$ (I think there is a typo in your last component).



                The first component of the gradient of $Phi$ would be
                $$
                g^11partialPhi/partial r+g^12partialPhi/partial theta+g^13partialPhi/partial phi=partialPhi/partial r.
                $$

                since the off-diagonal elements of the metric tensor are zero. The second component would be
                $$
                g^21partialPhi/partial r+g^22partialPhi/partial theta+g^23partialPhi/partial phi=frac1r^2partialPhi/partial theta.
                $$

                and the third
                $$
                g^31partialPhi/partial r+g^32partialPhi/partial theta+g^33partialPhi/partial phi=frac1r^2sin^2thetapartialPhi/partial phi.
                $$

                Observe that these are the components in the base $g_i$, which is orthogonal but not orthonormal. If you use unit vectors you get a slightly different expression.







                share|cite|improve this answer












                share|cite|improve this answer



                share|cite|improve this answer










                answered Mar 17 at 22:33









                GReyesGReyes

                2,31315




                2,31315



























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