The Equations of the Surface and the Shift Tensor

In the preceding Chapter, we introduced some of the most fundamental objects in the analysis of surfaces without the help of coordinates in the ambient space. Perhaps the highlight of that Chapter was the emergence of the curvature tensor BαβB_{\alpha\beta} in the equation
αSβ=NBαβ.(2.79)\nabla_{\alpha}\mathbf{S}_{\beta}=\mathbf{N}B_{\alpha\beta}. \tag{2.79}
and its appearance in the Gauss equations
BαγBβδBβγBαδ=Rγδαβ(7.38)B_{\alpha\gamma}B_{\beta\delta}-B_{\beta\gamma}B_{\alpha\delta}=R_{\gamma \delta\alpha\beta} \tag{7.38}
which was demonstrated in the exercises. All of that was accomplished without ambient coordinates.
On the other hand, consistent with our experience with Euclidean spaces, our theoretical findings cannot be used to calculate any characteristics, including curvature, of any concrete surface due to the limited computational capabilities of geometric objects.
In this Chapter, we will remedy that shortcoming by introducing coordinates in the ambient space. This development will compel us to study the interplay between two coordinate systems: the surface coordinates SαS^{\alpha} and the ambient coordinates ZiZ^{i}. This interplay will yield variants of a new kind -- those that feature both surface and ambient indices -- which will invite us to extend the concept of a tensor to include two types of indices.
In this Chapter, our attention will be occupied by the shift tensor ZαiZ_{\alpha}^{i}, which describes the tangent space, and the components NiN^{i} of the unit normal, which describe the orthogonal space -- and, of course, the interplay between the two. The theory developed in this Chapter will be illustrated in the next Chapter with examples involving some of the most common surfaces, such as the sphere, the cylinder, and the torus.
Consider a two-dimensional surface embedded in a three-dimensional space and referred to surface coordinates SαS^{\alpha}. Furthermore, introduce an arbitrary coordinate system ZiZ^{i} in the ambient space.
With the help of the two coordinate systems, the surface can be described parametrically, i.e. by specifying the values of the ambient coordinates as functions of surface coordinates. For a two-dimensional surface in a three-dimensional space, a parametric specification requires three functions of two variables. These functions are called the equations of the surface and are denoted by the same symbols ZiZ^{i} as the ambient coordinates, i.e.
Z1=Z1(S1,S2)          (3.1)Z2=Z2(S1,S2)          (3.2)Z3=Z3(S1,S2).          (3.3)\begin{aligned}Z^{1} & =Z^{1}\left( S^{1},S^{2}\right)\ \ \ \ \ \ \ \ \ \ \left(3.1\right)\\Z^{2} & =Z^{2}\left( S^{1},S^{2}\right)\ \ \ \ \ \ \ \ \ \ \left(3.2\right)\\Z^{3} & =Z^{3}\left( S^{1},S^{2}\right) .\ \ \ \ \ \ \ \ \ \ \left(3.3\right)\end{aligned}
As usual, these equations can be captured by a single indicial identity,
Zi=Zi(S1,S2),(3.4)Z^{i}=Z^{i}\left( S^{1},S^{2}\right) ,\tag{3.4}
which, by collapsing the function arguments, can be written in an even more compact form
Zi=Zi(S).(3.5)Z^{i}=Z^{i}\left( S\right) .\tag{3.5}
Not surprisingly, the one operation that can be applied to the equation of the surface, i.e. differentiating with respect to SαS^{\alpha} resulting in the system
Zi(S)Sα,(3.6)\frac{\partial Z^{i}\left( S\right) }{\partial S^{\alpha}},\tag{3.6}
will give rise to an important object that will occupy much of our attention in the rest of our narrative.
Before proceeding with our analysis, however, let us consider a few classical examples of two-dimensional surfaces and one-dimensional planar curves.

3.2.1A sphere of radius RR

Refer a sphere of radius RR to the surface spherical coordinates θ,φ\theta,\varphi described in the previous Chapter.
(3.7)
If the ambient space is referred to Cartesian coordinates x,y,zx,y,z, aligned with the surface coordinates in the usual way, then the equations of the surface read
x(θ,φ)=Rsinθcosφ          (3.8)y(θ,φ)=Rsinθsinφ          (3.9)z(θ,φ)=Rcosθ.          (3.10)\begin{aligned}x\left( \theta,\varphi\right) & =R\sin\theta\cos\varphi\ \ \ \ \ \ \ \ \ \ \left(3.8\right)\\y\left( \theta,\varphi\right) & =R\sin\theta\sin\varphi\ \ \ \ \ \ \ \ \ \ \left(3.9\right)\\z\left( \theta,\varphi\right) & =R\cos\theta.\ \ \ \ \ \ \ \ \ \ \left(3.10\right)\end{aligned}
When the ambient space is referred to spherical coordinates r,θ1,φ1r,\theta _{1},\varphi_{1}, the equations of the surface appear in a particularly simple form
r(θ,φ)=R          (3.11)θ1(θ,φ)=θ          (3.12)φ1(θ,φ)=φ.          (3.13)\begin{aligned}r\left( \theta,\varphi\right) & =R\ \ \ \ \ \ \ \ \ \ \left(3.11\right)\\\theta_{1}\left( \theta,\varphi\right) & =\theta\ \ \ \ \ \ \ \ \ \ \left(3.12\right)\\\varphi_{1}\left( \theta,\varphi\right) & =\varphi.\ \ \ \ \ \ \ \ \ \ \left(3.13\right)\end{aligned}
The simplicity of these expressions indicates that spherical coordinates in the ambient space are a natural choice for describing the surface of a sphere. This simple example also illustrates the profound dependence of the equation of a surface on the choice of coordinates.

3.2.2A cylinder of radius RR

Refer a cylinder of radius RR to coordinates θ,z\theta,z illustrated in the following figure.
(3.14)
If the ambient space is referred to Cartesian coordinates x,y,z1x,y,z_{1}, the equations for the cylinder read
x(θ,z)=Rcosθ          (3.15)y(θ,z)=Rsinθ          (3.16)z1(θ,z)=z.          (3.17)\begin{aligned}x\left( \theta,z\right) & =R\cos\theta\ \ \ \ \ \ \ \ \ \ \left(3.15\right)\\y\left( \theta,z\right) & =R\sin\theta\ \ \ \ \ \ \ \ \ \ \left(3.16\right)\\z_{1}\left( \theta,z\right) & =z.\ \ \ \ \ \ \ \ \ \ \left(3.17\right)\end{aligned}
If the ambient space is referred to cylindrical coordinates r,θ1,z1r,\theta _{1},z_{1}, the equations become even simpler, i.e.
r(θ,z)=R          (3.18)θ1(θ,z)=θ          (3.19)z1(θ,z)=z.          (3.20)\begin{aligned}r\left( \theta,z\right) & =R\ \ \ \ \ \ \ \ \ \ \left(3.18\right)\\\theta_{1}\left( \theta,z\right) & =\theta\ \ \ \ \ \ \ \ \ \ \left(3.19\right)\\z_{1}\left( \theta,z\right) & =z.\ \ \ \ \ \ \ \ \ \ \left(3.20\right)\end{aligned}
Interestingly, note that the equations of a sphere in spherical coordinates are the same as the equations of a cylinder in cylindrical coordinates.

3.2.3A surface of revolution

A surface of revolution is formed by rotating a planar curve around a straight line (within the same plane) known as the axis of rotation. The curve that is being rotated may be referred to as the profile of the shape. Notice that both a sphere and a cylinder, as well as the upcoming torus, are examples of shapes of revolution.
  (3.21)
It is natural to choose the angle of rotation θ\theta to be one of the two surface coordinates. The other coordinate can be any parameter γ\gamma. If the ambient space is referred to Cartesian coordinates, then the shape of revolution about the zz-axis is given by
x(θ,γ)=G(γ)cosθ          (3.22)y(θ,γ)=G(γ)sinθ          (3.23)z(θ,γ)=H(γ),          (3.24)\begin{aligned}x\left( \theta,\gamma\right) & =G\left( \gamma\right) \cos \theta\ \ \ \ \ \ \ \ \ \ \left(3.22\right)\\y\left( \theta,\gamma\right) & =G\left( \gamma\right) \sin \theta\ \ \ \ \ \ \ \ \ \ \left(3.23\right)\\z\left( \theta,\gamma\right) & =H\left( \gamma\right) ,\ \ \ \ \ \ \ \ \ \ \left(3.24\right)\end{aligned}
where H(γ)H\left( \gamma\right) is the location of the point along the zz-axis and G(γ)G\left( \gamma\right) is the distance away from the zz-axis. If the ambient space is instead referred to cylindrical coordinates r,θ1,z1r,\theta_{1},z_{1}, we once again obtain equations of utmost simplicity, i.e.
r(θ,γ)=G(γ)          (3.25)θ1(θ,γ)=θ          (3.26)z1(θ,γ)=H(γ),          (3.27)\begin{aligned}r\left( \theta,\gamma\right) & =G\left( \gamma\right)\ \ \ \ \ \ \ \ \ \ \left(3.25\right)\\\theta_{1}\left( \theta,\gamma\right) & =\theta\ \ \ \ \ \ \ \ \ \ \left(3.26\right)\\z_{1}\left( \theta,\gamma\right) & =H\left( \gamma\right) ,\ \ \ \ \ \ \ \ \ \ \left(3.27\right)\end{aligned}
where H(γ)H\left( \gamma\right) is the location of the point along the zz-axis and G(γ)G\left( \gamma\right) is the distance away from the zz-axis. Finally, note that it is very common to choose
H(γ)=γ,(3.28)H\left( \gamma\right) =\gamma,\tag{3.28}
in which case γ\gamma corresponds exactly to the location of the point along the axis of rotation.

3.2.4A torus with radii RR and rr

A torus is the shape of revolution of a circle of radius rr whose center is the distance RR from from the rotation axis.
(3.29)
This simple profile corresponds to the functions
G(φ)=R+rcosφ          (3.30)H(φ)=rsinφ,          (3.31)\begin{aligned}G\left( \varphi\right) & =R+r\cos\varphi\ \ \ \ \ \ \ \ \ \ \left(3.30\right)\\H\left( \varphi\right) & =r\sin\varphi,\ \ \ \ \ \ \ \ \ \ \left(3.31\right)\end{aligned}
where we decided to use the letter φ\varphi instead of γ\gamma because of its interpretation as an angle.
(3.32)
Thus, the equations of the torus read
x(θ,φ)=(R+rcosφ)cosθ          (3.33)y(θ,φ)=(R+rcosφ)sinθ          (3.34)z(θ,φ)=rsinφ,          (3.35)\begin{aligned}x\left( \theta,\varphi\right) & =\left( R+r\cos\varphi\right) \cos \theta\ \ \ \ \ \ \ \ \ \ \left(3.33\right)\\y\left( \theta,\varphi\right) & =\left( R+r\cos\varphi\right) \sin \theta\ \ \ \ \ \ \ \ \ \ \left(3.34\right)\\z\left( \theta,\varphi\right) & =r\sin\varphi,\ \ \ \ \ \ \ \ \ \ \left(3.35\right)\end{aligned}
where both θ\theta and φ\varphi vary from 00 to 2π2\pi.
A planar curve is a one-dimensional "surface" embedded in a two-dimensional Euclidean plane which we will typically refer to either Cartesian or polar coordinates.

3.3.1Planar curves in Cartesian coordinates

The most common type of curve that we encounter in our introductory Calculus courses is the graph of a function f(x)f\left( x\right) . For example, the curve corresponding to the function
f(x)=ex2cos10x(3.36)f\left( x\right) =e^{-x^{2}}\cos10x\tag{3.36}
is shown in the following figure.
(3.37)
Every curve that represents the graph of a function f(x)f\left( x\right) can also be represented parametrically by the equations
x(γ)=γ          (3.38)y(γ)=f(γ).          (3.39)\begin{aligned}x\left( \gamma\right) & =\gamma\ \ \ \ \ \ \ \ \ \ \left(3.38\right)\\y\left( \gamma\right) & =f\left( \gamma\right) .\ \ \ \ \ \ \ \ \ \ \left(3.39\right)\end{aligned}
Of course, not every planar curve corresponds to the graph of a function. A quintessential curve that is not the graph of a function is a circle. The following figure illustrates a circle of radius RR centered at a point with coordinates (x0,y0)\left( x_{0},y_{0}\right) .
(3.40)
It is described by the equations
x(θ)=x0+Rcosθ          (3.41)y(θ)=y0+Rsinθ          (3.42)\begin{aligned}x\left( \theta\right) & =x_{0}+R\cos\theta\ \ \ \ \ \ \ \ \ \ \left(3.41\right)\\y\left( \theta\right) & =y_{0}+R\sin\theta\ \ \ \ \ \ \ \ \ \ \left(3.42\right)\end{aligned}
where, once again, we used θ\theta instead of γ\gamma because of its interpretation as an angle.
For a more intricate example, consider the equations
x(γ)=cosγ+sin3γ          (3.43)y(γ)=cos4γ+sinγ          (3.44)\begin{aligned}x\left( \gamma\right) & =\cos\gamma+\sin3\gamma\ \ \ \ \ \ \ \ \ \ \left(3.43\right)\\y\left( \gamma\right) & =\cos4\gamma+\sin\gamma\ \ \ \ \ \ \ \ \ \ \left(3.44\right)\end{aligned}
that describe the curve in the following figure.
(3.45)
Interestingly, many curves that can be represented by a graph of a function are still more easily represented parametrically. One example is a cycloid, which represents the trajectory of a point on a wheel rolling without slippage along a straight line.
(3.46)
A cycloid that corresponds to a wheel of radius RR is specified by the equations
x(θ)=Rθ+Rsinθ          (3.47)y(θ)=R+Rcosθ.          (3.48)\begin{aligned}x\left( \theta\right) & =R\theta+R\sin\theta\ \ \ \ \ \ \ \ \ \ \left(3.47\right)\\y\left( \theta\right) & =R+R\cos\theta.\ \ \ \ \ \ \ \ \ \ \left(3.48\right)\end{aligned}

3.3.2Planar curves in polar coordinates

A general planar curve in polar coordinates r,θr,\theta is given by
r=r(γ)          (3.49)θ=θ(γ).          (3.50)\begin{aligned}r & =r\left( \gamma\right)\ \ \ \ \ \ \ \ \ \ \left(3.49\right)\\\theta & =\theta\left( \gamma\right) .\ \ \ \ \ \ \ \ \ \ \left(3.50\right)\end{aligned}
As we described in Chapter TBD of Introduction to Tensor Calculus, r(γ)r\left( \gamma\right) can assume negative values and θ(γ)\theta\left( \gamma\right) can assume any value whatsoever. When r(γ)r\left( \gamma\right) is negative, the point with coordinates (r,θ)\left( r,\theta\right) is plotted as (r,θ+π)\left( -r,\theta+\pi\right) . To repeat an example from that Chapter, the curve given by the equation
r(γ)=sin2γ          (3.51)θ(γ)=sinγ          (3.52)\begin{aligned}r\left( \gamma\right) & =\sin2\gamma\ \ \ \ \ \ \ \ \ \ \left(3.51\right)\\\theta\left( \gamma\right) & =\sin\gamma\ \ \ \ \ \ \ \ \ \ \left(3.52\right)\end{aligned}
is shown in the following figure.
(3.53)
For another example, the curve given by the equations
r(γ)=2+sin3γ          (3.54)θ(γ)=γ+cos2γ          (3.55)\begin{aligned}r\left( \gamma\right) & =2+\sin3\gamma\ \ \ \ \ \ \ \ \ \ \left(3.54\right)\\\theta\left( \gamma\right) & =\gamma+\cos2\gamma\ \ \ \ \ \ \ \ \ \ \left(3.55\right)\end{aligned}
has the following shape:
(3.56)
Polar coordinates have their own version of a graph, i.e. curves that may be described by specifying rr as a function of θ\theta
r=f(θ),(3.57)r=f\left( \theta\right) ,\tag{3.57}
which is equivalent to the parametric equations
r(γ)=f(γ)          (3.58)θ(γ)=γ.          (3.59)\begin{aligned}r\left( \gamma\right) & =f\left( \gamma\right)\ \ \ \ \ \ \ \ \ \ \left(3.58\right)\\\theta\left( \gamma\right) & =\gamma.\ \ \ \ \ \ \ \ \ \ \left(3.59\right)\end{aligned}
For example, the following spiral corresponds to
f(θ)=eθ/8(3.60)f\left( \theta\right) =e^{\theta/8}\tag{3.60}
where θ\theta varies form 4π-4\pi to 4π4\pi.
(3.61)
It is also possible, but less common, to specify θ\theta as a function of rr.
This wraps up the description of the most common surfaces and curves that will be used throughout the rest of our narrative as illustration of the relevant concepts.
We now turn our attention to the shift tensor ZαiZ_{\alpha}^{i} -- a central object in the analysis of embedded surfaces that represents the tangent space. Furthermore, the shift tensor helps relate corresponding surface and ambient quantities. In fact, we will approach the shift tensor by exploring the relationship between the surface basis Sα\mathbf{S}_{\alpha} and the ambient basis Zi\mathbf{Z}_{i}.
Recall that the ambient covariant basis Zi\mathbf{Z}_{i} is given by the equation
Zi=R(Z)Zi,(6.45)\mathbf{Z}_{i}=\frac{\partial\mathbf{R}\left( Z\right) }{\partial Z^{i}}, \tag{6.45}
where R(Z)\mathbf{R}\left( Z\right) is the position vector as a function of the ambient coordinates ZiZ^{i}. Similarly, the surface covariant basis Sα\mathbf{S}_{\alpha} is given by the equation
Sα=R(S)Sα,(2.22)\mathbf{S}_{\alpha}=\frac{\partial\mathbf{R}\left( S\right) }{\partial S^{\alpha}}, \tag{2.22}
where R(S)\mathbf{R}\left( S\right) is the surface restriction of the position vector R\mathbf{R} as a function of the surface coordinates SαS^{\alpha}.
As usual, in order to relate the derivatives
R(Z)Zi    and    R(S)Sα,(3.62)\frac{\partial\mathbf{R}\left( Z\right) }{\partial Z^{i}}\text{ \ \ \ and\ \ \ \ }\frac{\partial\mathbf{R}\left( S\right) }{\partial S^{\alpha}},\tag{3.62}
we must first relate the functions
R(Z)    and    R(S).(3.63)\mathbf{R}\left( Z\right) \text{\ \ \ \ and\ \ \ \ }\mathbf{R}\left( S\right) .\tag{3.63}
To find the correct relationship, imagine the position vector R\mathbf{R} corresponding to a specific surface point PP with surface coordinates SαS^{\alpha}. The vector R\mathbf{R} can be obtained in two alternative ways. The first is to evaluate the function R(S)\mathbf{R}\left( S\right) at the coordinates SαS^{\alpha}. The second is to determine the ambient coordinates ZiZ^{i} of the point PP by evaluating the equations of the surface Zi(S)Z^{i}\left( S\right) at SαS^{\alpha} and then to evaluate the function R(Z)\mathbf{R}\left( Z\right) at the resulting values of the coordinates ZiZ^{i}. This line of reasoning yields the identity
R(S)=R(Z(S)).(3.64)\mathbf{R}\left( S\right) =\mathbf{R}\left( Z\left( S\right) \right) .\tag{3.64}
Differentiating this identity by the chain rule with respect to SαS^{\alpha}, we have
R(S)Sα=R(Z)ZiZi(S)Sα,(3.65)\frac{\partial\mathbf{R}\left( S\right) }{\partial S^{\alpha}} =\frac{\partial\mathbf{R}\left( Z\right) }{\partial Z^{i}}\frac{\partial Z^{i}\left( S\right) }{\partial S^{\alpha}},\tag{3.65}
where we recognize two of the three elements, i.e.
R(S)Sα=Sα    and    R(Z)Zi=Zi.(3.66)\frac{\partial\mathbf{R}\left( S\right) }{\partial S^{\alpha}} =\mathbf{S}_{\alpha}\text{ \ \ \ and\ \ \ \ }\frac{\partial\mathbf{R}\left( Z\right) }{\partial Z^{i}}=\mathbf{Z}_{i}.\tag{3.66}
The third element,
Zi(S)Sα,(3.67)\frac{\partial Z^{i}\left( S\right) }{\partial S^{\alpha}},\tag{3.67}
is the shift tensor! It is denoted by the symbol ZαiZ_{\alpha}^{i}, i.e.
Zαi=Zi(S)Sα.(3.68)Z_{\alpha}^{i}=\frac{\partial Z^{i}\left( S\right) }{\partial S^{\alpha}}.\tag{3.68}
By convention, the Latin index is considered first and the Greek index is considered second. Therefore, we do not need a placeholder to help us track the order of the indices. Meanwhile, the precise meaning of the word tensor, when applied to an object featuring both ambient and surface indices, will be described in the next Section.
With the help of the symbol ZαiZ_{\alpha}^{i}, the relationship between the surface and the ambient bases reads
Sα=ZαiZi.(3.69)\mathbf{S}_{\alpha}=Z_{\alpha}^{i}\mathbf{Z}_{i}.\tag{3.69}
For each α\alpha, this identity represents the vector Sα\mathbf{S}_{\alpha} as a linear combination of the ambient basis vectors Zi\mathbf{Z}_{i}. Thus, ZαiZ_{\alpha}^{i} are the components of the surface basis element Sα\mathbf{S}_{\alpha} with respect to the ambient basis Zi\mathbf{Z}_{i}. It is for this reason that the shift tensor is said to represent the tangent space.
Recall that the ambient components UiU^{i} of a vector U\mathbf{U} are given by the dot product
Ui=ZiU.(6.45)U^{i}=\mathbf{Z}^{i}\cdot\mathbf{U.} \tag{6.45}
Therefore,
Zαi=ZiSα.(3.70)Z_{\alpha}^{i}=\mathbf{Z}^{i}\cdot\mathbf{S}_{\alpha}.\tag{3.70}
In other words, the elements of the shift tensor are the pairwise dot products of the ambient and surface bases. By index juggling, we easily obtain the equivalent identities
Ziα=ZiSα          (3.71)Zia=ZiSα          (3.72)Ziα=ZiSα.          (3.73)\begin{aligned}Z_{i\alpha} & =\mathbf{Z}_{i}\cdot\mathbf{S}_{\alpha}\ \ \ \ \ \ \ \ \ \ \left(3.71\right)\\Z_{i}^{a} & =\mathbf{Z}_{i}\cdot\mathbf{S}^{\alpha}\ \ \ \ \ \ \ \ \ \ \left(3.72\right)\\Z^{i\alpha} & =\mathbf{Z}^{i}\cdot\mathbf{S}^{\alpha}.\ \ \ \ \ \ \ \ \ \ \left(3.73\right)\end{aligned}
Although we will save the bulk of our discussion of specific surfaces until the next Chapter, let us give the shift tensor for a sphere of radius RR in both Cartesian and spherical ambient coordinates. As we stated earlier in this Chapter, for the ambient space is referred to Cartesian coordinates x,y,zx,y,z, the equations of the sphere read
x(θ,φ)=Rsinθcosφ          (3.8)y(θ,φ)=Rsinθsinφ          (3.9)z(θ,φ)=Rcosθ.          (3.10)\begin{aligned}x\left( \theta,\varphi\right) & =R\sin\theta\cos\varphi\ \ \ \ \ \ \ \ \ \ \left(3.8\right)\\y\left( \theta,\varphi\right) & =R\sin\theta\sin\varphi\ \ \ \ \ \ \ \ \ \ \left(3.9\right)\\z\left( \theta,\varphi\right) & =R\cos\theta. \ \ \ \ \ \ \ \ \ \ \left(3.10\right)\end{aligned}
The shift tensor ZαiZ_{\alpha}^{i} then corresponds to the 3×23\times2 matrix
[x(θ,φ)θx(θ,φ)φy(θ,φ)θy(θ,φ)φz(θ,φ)θz(θ,φ)φ]=R[cosθcosφsinθsinφcosθsinφsinθcosφsinθ0](3.74)\left[ \begin{array} {cc} \frac{\partial x\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial x\left( \theta,\varphi\right) }{\partial\varphi}\\ \frac{\partial y\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial y\left( \theta,\varphi\right) }{\partial\varphi}\\ \frac{\partial z\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial z\left( \theta,\varphi\right) }{\partial\varphi} \end{array} \right] =R\left[ \begin{array} {rr} \cos\theta\cos\varphi & -\sin\theta\sin\varphi\\ \cos\theta\sin\varphi & \sin\theta\cos\varphi\\ -\sin\theta & 0 \end{array} \right]\tag{3.74}
Meanwhile, for the ambient space referred to spherical coordinates r,θ1,φ1r,\theta_{1},\varphi_{1}, the equations of the surface read
r(θ,φ)=R          (3.11)θ1(θ,φ)=θ          (3.12)φ1(θ,φ)=φ,          (3.13)\begin{aligned}r\left( \theta,\varphi\right) & =R\ \ \ \ \ \ \ \ \ \ \left(3.11\right)\\\theta_{1}\left( \theta,\varphi\right) & =\theta\ \ \ \ \ \ \ \ \ \ \left(3.12\right)\\\varphi_{1}\left( \theta,\varphi\right) & =\varphi, \ \ \ \ \ \ \ \ \ \ \left(3.13\right)\end{aligned}
the shift tensor ZαiZ_{\alpha}^{i} corresponds to the matrix
[r(θ,φ)θr(θ,φ)φθ1(θ,φ)θθ1(θ,φ)φφ1(θ,φ)θφ1(θ,φ)φ]=[001001].(3.75)\left[ \begin{array} {cc} \frac{\partial r\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial r\left( \theta,\varphi\right) }{\partial\varphi}\\ \frac{\partial\theta_{1}\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial\theta_{1}\left( \theta,\varphi\right) }{\partial\varphi}\\ \frac{\partial\varphi_{1}\left( \theta,\varphi\right) }{\partial\theta} & \frac{\partial\varphi_{1}\left( \theta,\varphi\right) }{\partial\varphi} \end{array} \right] =\left[ \begin{array} {rr} 0 & 0\\ 1 & 0\\ 0 & 1 \end{array} \right] .\tag{3.75}
Once again, the equation
Sα=ZαiZi(3.69)\mathbf{S}_{\alpha}=Z_{\alpha}^{i}\mathbf{Z}_{i} \tag{3.69}
tells us that the elements of the shift tensor are the components of the surface covariant basis Sα\mathbf{S}_{\alpha} with respect to the ambient covariant basis Zi\mathbf{Z}_{i}. Thus, the columns of each 3×23\times2 matrix representing the shift tensor are the ambient components of the corresponding surface covariant basis vectors. For the surface coordinates θ,φ\theta,\varphi, the covariant basis Sα\mathbf{S}_{\alpha} on the sphere is shown in the following figure and you should confirm that the columns of the matrices above correctly represent these vectors.
(3.76)
In particular, when spherical coordinates r,θ1,φ1r,\theta_{1},\varphi_{1} are chosen in the ambient space, the surface covariant basis Sα\mathbf{S}_{\alpha} is represented by the last two vectors of the ambient basis Zi\mathbf{Z}_{i}, i.e.
S1=Z2          (3.77)S2=Z3,          (3.78)\begin{aligned}\mathbf{S}_{1} & =\mathbf{Z}_{2}\ \ \ \ \ \ \ \ \ \ \left(3.77\right)\\\mathbf{S}_{2} & =\mathbf{Z}_{3},\ \ \ \ \ \ \ \ \ \ \left(3.78\right)\end{aligned}
which corroborates the particularly simple form of the shift tensor.
The shift tensor ZαiZ_{\alpha}^{i} is our first example of a variant featuring both ambient and surface indices. Therefore, we must revisit the concept of a tensor as ZαiZ_{\alpha}^{i} forces us to contend with two simultaneous coordinate changes: one in the ambient space and one on the surface. This is the task to which we will now turn our attention.
From the identity
Zαi=ZiSα,(3.70)Z_{\alpha}^{i}=\mathbf{Z}^{i}\cdot\mathbf{S}_{\alpha}, \tag{3.70}
it is clear that the elements of the shift tensor ZαiZ_{\alpha}^{i} change with both the ambient and surface coordinates. This invites us to expand the concept of a tensor to include transformations under simultaneous changes of ambient and surface coordinates. Before we give the general definition, let us examine how the shift tensor behaves in those circumstances.
Let ZiZ^{i} and ZiZ^{i^{\prime}} be the unprimed and primed ambient coordinates related by the functions
Zi=Zi(Z)   and          (3.79)Zi=Zi(Z).          (3.80)\begin{aligned}Z^{i} & =Z^{i}\left( Z^{\prime}\right) \text{ \ \ and}\ \ \ \ \ \ \ \ \ \ \left(3.79\right)\\Z^{i^{\prime}} & =Z^{i^{\prime}}\left( Z\right) .\ \ \ \ \ \ \ \ \ \ \left(3.80\right)\end{aligned}
At the same time, let SαS^{\alpha} and SαS^{\alpha^{\prime}} be the unprimed and primed surface coordinates related by the functions
Sα=Sα(S)   and          (3.81)Sα=Sα(S).          (3.82)\begin{aligned}S^{\alpha} & =S^{\alpha}\left( S^{\prime}\right) \ \ \text{ and}\ \ \ \ \ \ \ \ \ \ \left(3.81\right)\\S^{\alpha^{\prime}} & =S^{\alpha^{\prime}}\left( S\right) .\ \ \ \ \ \ \ \ \ \ \left(3.82\right)\end{aligned}
Also recall the definitions of the associated Jacobians, i.e.
Jii(Z)=Zi(Z)Zi and          (3.83)Jii(Z)=Zi(Z)Zi          (3.84)\begin{aligned}J_{i}^{i^{\prime}}\left( Z\right) & =\frac{\partial Z^{i^{\prime}}\left( Z\right) }{\partial Z^{i}}\text{ and}\ \ \ \ \ \ \ \ \ \ \left(3.83\right)\\J_{i^{\prime}}^{i}\left( Z^{\prime}\right) & =\frac{\partial Z^{i}\left( Z^{\prime}\right) }{\partial Z^{i^{\prime}}}\ \ \ \ \ \ \ \ \ \ \left(3.84\right)\end{aligned}
and
Jαα=Sα(S)Sα and          (2.12)Jαα=Sα(S)Sα.          (2.13)\begin{aligned}J_{\alpha^{\prime}}^{\alpha} & =\frac{\partial S^{\alpha}\left( S^{\prime }\right) }{\partial S^{\alpha^{\prime}}}\text{ and}\ \ \ \ \ \ \ \ \ \ \left(2.12\right)\\J_{\alpha}^{\alpha^{\prime}} & =\frac{\partial S^{\alpha^{\prime}}\left( S\right) }{\partial S^{\alpha}}. \ \ \ \ \ \ \ \ \ \ \left(2.13\right)\end{aligned}
In the primed coordinates, the shift tensor ZαiZ_{\alpha^{\prime}}^{i^{\prime}} is given by the equation
Zαi=ZiSα.(3.85)Z_{\alpha^{\prime}}^{i^{\prime}}=\mathbf{Z}^{i^{\prime}}\cdot\mathbf{S} _{\alpha^{\prime}}.\tag{3.85}
The ambient contravariant basis Zi\mathbf{Z}^{i} depends only on the choice of the ambient coordinates and, being a tensor, transforms according to the rule
Zi=ZiJii.(3.86)\mathbf{Z}^{i^{\prime}}=\mathbf{Z}^{i}J_{i}^{i^{\prime}}.\tag{3.86}
Similarly, the surface covariant basis Sα\mathbf{S}_{\alpha} depends only on the choice of the surface coordinates and, being a tensor, transforms according to the rule
Sα=SαJαα.(3.87)\mathbf{S}_{\alpha^{\prime}}=\mathbf{S}_{\alpha}J_{\alpha^{\prime}}^{\alpha}.\tag{3.87}
Therefore, for the shift tensor ZαiZ_{\alpha^{\prime}}^{i^{\prime}}, we have
Zαi=ZiSα=ZiJiiSαJαα=ZiSαJiiJαα=ZαiJiiJαα.(3.88)Z_{\alpha^{\prime}}^{i^{\prime}}=\mathbf{Z}^{i^{\prime}}\cdot\mathbf{S} _{\alpha^{\prime}}=\mathbf{Z}^{i}J_{i}^{i^{\prime}}\cdot\mathbf{S}_{\alpha }J_{\alpha^{\prime}}^{\alpha}=\mathbf{Z}^{i}\cdot\mathbf{S}_{\alpha} J_{i}^{i^{\prime}}J_{\alpha^{\prime}}^{\alpha}=Z_{\alpha}^{i}J_{i}^{i^{\prime }}J_{\alpha^{\prime}}^{\alpha}.\tag{3.88}
In summary,
Zαi=ZαiJiiJαα.(3.89)Z_{\alpha^{\prime}}^{i^{\prime}}=Z_{\alpha}^{i}J_{i}^{i^{\prime}} J_{\alpha^{\prime}}^{\alpha}.\tag{3.89}
In words, the shift tensor ZαiZ_{\alpha}^{i} exhibits the properties of a tensor with respect to changes of both ambient and surface coordinates.
Let us use this behavior as a blueprint for an expanded definition of a tensor. Consider a variant TjβiαT_{j\beta}^{i\alpha} with a representative collection of ambient and surface indices. Then TjβiαT_{j\beta}^{i\alpha} is an (absolute) tensor if its elements TjβiαT_{j^{\prime}\beta^{\prime} }^{i^{\prime}\alpha^{\prime}} in the primed coordinate systems are related to TjβiαT_{j\beta}^{i\alpha} by the equation
Tjβiα=TjβiαJiiJjjJααJββ.(3.90)T_{j^{\prime}\beta^{\prime}}^{i^{\prime}\alpha^{\prime}}=T_{j\beta}^{i\alpha }J_{i}^{i^{\prime}}J_{j^{\prime}}^{j}J_{\alpha}^{\alpha^{\prime}} J_{\beta^{\prime}}^{\beta}.\tag{3.90}
According to this definition, the shift tensor is indeed a tensor. Furthermore, all previously defined surface and ambient variants that are tensors in the original sense remain tensors in the sense of the new, more general definition. Of course, for tensors in the ambient space, we must limit our attention to their surface restrictions in order for the new definition to apply.
Finally, it is left as an exercise to demonstrate all of the common properties of tensors including the sum, product, and contraction properties, as well as the quotient theorem.
Consider a vector U\mathbf{U} in the tangent plane at a point PP on the surface. Like all vectors in the tangent plane, U\mathbf{U} can be decomposed with respect to the surface covariant basis Sα\mathbf{S}_{\alpha}, leading to the contravariant components UαU^{\alpha}, i.e.
U=UαSα.(3.91)\mathbf{U}=U^{\alpha}\mathbf{S}_{\alpha}.\tag{3.91}
However, like any vector whatsoever, whether it lies in the tangent plane or not, U\mathbf{U} can also be decomposed with respect to the ambient basis Zi\mathbf{Z}_{i} resulting in the ambient components UiU^{i}, i.e.
U=UiZi.(3.92)\mathbf{U}=U^{i}\mathbf{Z}_{i}.\tag{3.92}
The question is, how are UiU^{i} and UαU^{\alpha} related?
In order to answer this question, substitute the identity
Sα=ZαiZi(3.69)\mathbf{S}_{\alpha}=Z_{\alpha}^{i}\mathbf{Z}_{i} \tag{3.69}
into the equation
U=UαSα,(3.93)\mathbf{U}=U^{\alpha}\mathbf{S}_{\alpha},\tag{3.93}
which yields
U=UαZαiZi.(3.94)\mathbf{U}=U^{\alpha}Z_{\alpha}^{i}\mathbf{Z}_{i}.\tag{3.94}
This identity tells us that the combination UαZαiU^{\alpha}Z_{\alpha}^{i} represents the ambient coordinates of U\mathbf{U}. In other words,
Ui=UαZαi.(3.95)U^{i}=U^{\alpha}Z_{\alpha}^{i}.\tag{3.95}
In this identity, the shift tensor plays a role that can be more accurately described as "upshifting": translating the surface components of a tangent vector into its ambient components. It is left as an exercise, which should be attempted after Section 3.8, to show that for a tangent vector U\mathbf{U} with ambient components UiU^{i}, the surface components UαU^{\alpha} can be recovered by contraction with the shift tensor on the ambient index, i.e.
Uα=UiZiα.(3.96)U^{\alpha}=U^{i}Z_{i}^{\alpha}.\tag{3.96}
A curve embedded in a surface can be specified by the dependence of the surface coordinates SαS^{\alpha} of the points on the curve on a parameter γ\gamma, i.e.
Sα=Sα(γ).(3.97)S^{\alpha}=S^{\alpha}\left( \gamma\right) .\tag{3.97}
Our present goal is to express the length of the curve by an integral in terms of the functions Sα(γ)S^{\alpha}\left( \gamma\right) .
Recall from Chapter TBD of the Introduction to Tensor Calculus, that the length ss of a segment of a curve given by the vector equation
R=R(γ)(3.98)\mathbf{R}=\mathbf{R}\left( \gamma\right)\tag{3.98}
is expressed by the integral
s=γ0γ1R(γ)R(γ)dγ.(3.99)s=\int\limits_{\gamma_{0}}^{\gamma_{1}}\sqrt{\mathbf{R}^{\prime}\left( \gamma\right) \cdot\mathbf{R}^{\prime}\left( \gamma\right) }d\gamma.\tag{3.99}
Since the vector R(γ)\mathbf{R}^{\prime}\left( \gamma\right) is tangential to the curve it is also tangential to the surface in which the curve is embedded. Therefore, it can be expressed with respect to both ambient and surface covariant bases. As we learned in Chapter TBD of Introduction to Tensor Calculus, the contravariant components of R(γ)\mathbf{R}^{\prime}\left( \gamma\right) are
dZi(γ)dγ,(3.100)\frac{dZ^{i}\left( \gamma\right) }{d\gamma},\tag{3.100}
where
Zi=Zi(γ)(3.101)Z^{i}=Z^{i}\left( \gamma\right)\tag{3.101}
are the ambient equations of the curve. This conclusion follows from differentiating the identity
R(γ)=R(Z(γ))(3.102)\mathbf{R}\left( \gamma\right) =\mathbf{R}\left( Z\left( \gamma\right) \right)\tag{3.102}
with respect to γ\gamma, i.e.
R(γ)=RZidZidγ=dZidγZi.(3.103)\mathbf{R}^{\prime}\left( \gamma\right) =\frac{\partial\mathbf{R}}{\partial Z^{i}}\frac{dZ^{i}}{d\gamma}=\frac{dZ^{i}}{d\gamma}\mathbf{Z}_{i}.\tag{3.103}
With the help of the components of R(γ)\mathbf{R}^{\prime}\left( \gamma\right) , the geometric integral
s=γ0γ1R(γ)R(γ)dγ.(3.104)s=\int\nolimits_{\gamma_{0}}^{\gamma_{1}}\sqrt{\mathbf{R}^{\prime}\left( \gamma\right) \cdot\mathbf{R}^{\prime}\left( \gamma\right) }d\gamma.\tag{3.104}
can be converted into the arithmetic integral
s=γ0γ1ZijdZidγdZjdγdγ,(3.105)s=\int_{\gamma_{0}}^{\gamma_{1}}\sqrt{Z_{ij}\frac{dZ^{i}}{d\gamma}\frac {dZ^{j}}{d\gamma}}d\gamma,\tag{3.105}
as we established in Chapter TBD of Introduction to Tensor Calculus.
Similarly, the surface components of R(γ)\mathbf{R}^{\prime}\left( \gamma\right) are
dSα(γ)dγ,(3.106)\frac{dS^{\alpha}\left( \gamma\right) }{d\gamma},\tag{3.106}
as can be shown by differentiating the identity
R(γ)=R(S(γ))(3.107)\mathbf{R}\left( \gamma\right) =\mathbf{R}\left( S\left( \gamma\right) \right)\tag{3.107}
with respect to γ\gamma. We have
R(γ)=RSαdSαdγ=dSαdγSα.(3.108)\mathbf{R}^{\prime}\left( \gamma\right) =\frac{\partial\mathbf{R}}{\partial S^{\alpha}}\frac{dS^{\alpha}}{d\gamma}=\frac{dS^{\alpha}}{d\gamma} \mathbf{S}_{\alpha}.\tag{3.108}
Therefore, the length of the curve is also given by the formula
s=γ0γ1SαβdSαdγdSβdγdγ.(3.109)s=\int_{\gamma_{0}}^{\gamma_{1}}\sqrt{S_{\alpha\beta}\frac{dS^{\alpha} }{d\gamma}\frac{dS^{\beta}}{d\gamma}}d\gamma.\tag{3.109}
Thus, as we might have expected, the length of a curve on a surface can be calculated by referring to its equation within the surface and the surface covariant metric tensor, while ignoring how either object is embedded in the larger ambient space.
The connection between the surface and the ambient basis, i.e.
Sα=ZαiZi,(3.69)\mathbf{S}_{\alpha}=Z_{\alpha}^{i}\mathbf{Z}_{i}, \tag{3.69}
immediately leads to the connection between the surface and the ambient metric tensors. Indeed, since
Sαβ=SαSβ,(2.28)S_{\alpha\beta}=\mathbf{S}_{\alpha}\cdot\mathbf{S}_{\beta}, \tag{2.28}
we have
Sαβ=SαSβ=ZiZαiZjZβj=ZijZαiZβj.(3.110)S_{\alpha\beta}=\mathbf{S}_{\alpha}\cdot\mathbf{S}_{\beta}=\mathbf{Z} _{i}Z_{\alpha}^{i}\cdot\mathbf{Z}_{j}Z_{\beta}^{j}=Z_{ij}Z_{\alpha} ^{i}Z_{\beta}^{j}.\tag{3.110}
In summary,
Sαβ=ZijZαiZβj.(3.111)S_{\alpha\beta}=Z_{ij}Z_{\alpha}^{i}Z_{\beta}^{j}.\tag{3.111}
The right side of this identity may be described as having each of the subscripts of ZijZ_{ij} operated on by the shift tensor.
The pivotal identity
Sαβ=ZijZαiZβj(3.111)S_{\alpha\beta}=Z_{ij}Z_{\alpha}^{i}Z_{\beta}^{j} \tag{3.111}
can be written in a number of other useful forms. Since
ZijZαi=Zjα,(3.112)Z_{ij}Z_{\alpha}^{i}=Z_{j\alpha},\tag{3.112}
the first alternative form reads
Sαβ=ZjαZβj.(3.113)S_{\alpha\beta}=Z_{j\alpha}Z_{\beta}^{j}.\tag{3.113}
If you prefer to see the index ii in important identities, you may rewrite the same identity as
Sαβ=ZiαZβi.(3.114)S_{\alpha\beta}=Z_{i\alpha}Z_{\beta}^{i}.\tag{3.114}
Finally, by raising the index α\alpha, we arrive at
δβα=ZiαZβi,(3.115)\delta_{\beta}^{\alpha}=Z_{i}^{\alpha}Z_{\beta}^{i},\tag{3.115}
which is perhaps the most elegant form of the same identity. This identity is usually written with the two sides reversed, i.e.
ZiαZβi=δβα.(3.116)Z_{i}^{\alpha}Z_{\beta}^{i}=\delta_{\beta}^{\alpha}.\tag{3.116}
Interestingly, the identity that relates the surface and the ambient metric tensors SαβS_{\alpha\beta} and ZijZ_{ij} features neither object explicitly.
We ought to remark on the identity
ZiαZβi=δβα(3.116)Z_{i}^{\alpha}Z_{\beta}^{i}=\delta_{\beta}^{\alpha} \tag{3.116}
from the Linear Algebra point of view. Both ZiαZ_{i}^{\alpha} and ZβiZ_{\beta }^{i} correspond to 3×23\times2 matrices. If ZiαZ_{i}^{\alpha} corresponds to a matrix AA and ZβiZ_{\beta}^{i} corresponds to the matrix BB, then the contraction ZiαZβiZ_{i}^{\alpha}Z_{\beta}^{i} corresponds to the product ATBA^{T}B. Since δβα\delta_{\beta}^{\alpha} corresponds to the 2×22\times2 identity matrix , the matrix equation ATB=IA^{T}B=I has the following "shape":
[][]=[1001].(3.117)\begin{array} {c} \left[ \begin{array} {ccc} \blacksquare & \blacksquare & \blacksquare\\ \blacksquare & \blacksquare & \blacksquare \end{array} \right] \\ \end{array} \left[ \begin{array} {cc} \blacksquare & \blacksquare\\ \blacksquare & \blacksquare\\ \blacksquare & \blacksquare \end{array} \right] =\left[ \begin{array} {cc} 1 & 0\\ 0 & 1 \end{array} \right] .\tag{3.117}
Since each of the matrices is rank 22, it is quite feasible that the product results in the 2×22\times2 identity matrix.
On the other hand, if the same two matrices were multiplied in the opposite order, i.e. BATBA^{T}, the shape of the resulting identity would be
[][]=[].(3.118)\left[ \begin{array} {cc} \blacksquare & \blacksquare\\ \blacksquare & \blacksquare\\ \blacksquare & \blacksquare \end{array} \right] \begin{array} {c} \left[ \begin{array} {ccc} \blacksquare & \blacksquare & \blacksquare\\ \blacksquare & \blacksquare & \blacksquare \end{array} \right] \\ \end{array} =\left[ \begin{array} {ccc} \blacksquare & \blacksquare & \blacksquare\\ \blacksquare & \blacksquare & \blacksquare\\ \blacksquare & \blacksquare & \blacksquare \end{array} \right] .\tag{3.118}
The rank of the product still cannot be greater than 22 and therefore the resulting matrix cannot be the 3×33\times3 identity matrix. Since BATBA^{T} corresponds to the contraction ZαiZjαZ_{\alpha}^{i}Z_{j}^{\alpha}, we conclude that the latter cannot equal δji\delta_{j}^{i}, i.e.
ZαiZjαδji.(3.119)Z_{\alpha}^{i}Z_{j}^{\alpha}\neq\delta_{j}^{i}.\tag{3.119}
However, we will soon discover that ZαiZjαZ_{\alpha}^{i}Z_{j}^{\alpha} satisfies the analogous identity
ZαiZjα=δjiNiNj(3.161)Z_{\alpha}^{i}Z_{j}^{\alpha}=\delta_{j}^{i}-N^{i}N_{j} \tag{3.161}
which involves the components NiN^{i} of the unit normal N\mathbf{N} studied below.
Having related the ambient and the surface metric tensors, let us now relate the surface Christoffel symbol Γβγα\Gamma_{\beta\gamma}^{\alpha} to its ambient counterpart Γjki\Gamma_{jk}^{i}. Our analysis will yield an attractive identity that offers a practical way of calculating the surface Christoffel symbol Γβγα\Gamma_{\beta\gamma}^{\alpha} in many situations.
Recall that the surface Christoffel symbol is given by
Γαβγ=SγSαSβ(2.56)\Gamma_{\alpha\beta}^{\gamma}=\mathbf{S}^{\gamma}\cdot\frac{\partial \mathbf{S}_{\alpha}}{\partial S^{\beta}} \tag{2.56}
while the ambient Christoffel symbol is given by
Γijk=ZkZiZj.(6.45)\Gamma_{ij}^{k}=\mathbf{Z}^{k}\cdot\frac{\partial\mathbf{Z}_{i}}{\partial Z^{j}}. \tag{6.45}
The key to connecting these identities is of course the relationship
Sα=ZiZαi(3.69)\mathbf{S}_{\alpha}=\mathbf{Z}_{i}Z_{\alpha}^{i} \tag{3.69}
which expresses the surface basis Sα\mathbf{S}_{\alpha} in terms of the ambient basis Zi\mathbf{Z}_{i}.
Substituting Sγ=ZkZkγ\mathbf{S}^{\gamma}=\mathbf{Z}^{k}Z_{k}^{\gamma} and Sα=ZiZαi\mathbf{S}_{\alpha}=\mathbf{Z}_{i}Z_{\alpha}^{i} in the equation
Γαβγ=SγSαSβ,(2.56)\Gamma_{\alpha\beta}^{\gamma}=\mathbf{S}^{\gamma}\cdot\frac{\partial \mathbf{S}_{\alpha}}{\partial S^{\beta}}, \tag{2.56}
we find
Γαβγ=ZkZkγ(ZiZαi)Sβ.(3.120)\Gamma_{\alpha\beta}^{\gamma}=\mathbf{Z}^{k}Z_{k}^{\gamma}\cdot\frac {\partial\left( \mathbf{Z}_{i}Z_{\alpha}^{i}\right) }{\partial S^{\beta}}.\tag{3.120}
By the product rule,
Γαβγ=ZkZkγZiSβZαi+ZkZkγZiZαiSβ.(3.121)\Gamma_{\alpha\beta}^{\gamma}=\mathbf{Z}^{k}Z_{k}^{\gamma}\cdot\frac {\partial\mathbf{Z}_{i}}{\partial S^{\beta}}Z_{\alpha}^{i}+\mathbf{Z}^{k} Z_{k}^{\gamma}\cdot\mathbf{Z}_{i}\frac{\partial Z_{\alpha}^{i}}{\partial S^{\beta}}.\tag{3.121}
It is left as an exercise to show that
Zi(S)Sβ=ΓijmZβjZm.(3.122)\frac{\partial\mathbf{Z}_{i}\left( S\right) }{\partial S^{\beta}} =\Gamma_{ij}^{m}Z_{\beta}^{j}\mathbf{Z}_{m}.\tag{3.122}
and therefore
ZkZkγZiSβZαi=ZkZkγΓijmZβjZmZαi=ΓijkZαiZβjZkγ.(3.123)\mathbf{Z}^{k}Z_{k}^{\gamma}\cdot\frac{\partial\mathbf{Z}_{i}}{\partial S^{\beta}}Z_{\alpha}^{i}=\mathbf{Z}^{k}Z_{k}^{\gamma}\cdot\Gamma_{ij} ^{m}Z_{\beta}^{j}\mathbf{Z}_{m}Z_{\alpha}^{i}=\Gamma_{ij}^{k}Z_{\alpha} ^{i}Z_{\beta}^{j}Z_{k}^{\gamma}.\tag{3.123}
Meanwhile,
ZkZkγZiZαiSβ=ZkγδikZαiSβ=ZiγZαiSβ.(3.124)\mathbf{Z}^{k}Z_{k}^{\gamma}\cdot\mathbf{Z}_{i}\frac{\partial Z_{\alpha}^{i} }{\partial S^{\beta}}=Z_{k}^{\gamma}\delta_{i}^{k}\frac{\partial Z_{\alpha }^{i}}{\partial S^{\beta}}=Z_{i}^{\gamma}\frac{\partial Z_{\alpha}^{i} }{\partial S^{\beta}}.\tag{3.124}
Combining the above equations, we find
Γαβγ=ΓijkZαiZβjZkγ+ZiγZαiSβ.(3.125)\Gamma_{\alpha\beta}^{\gamma}=\Gamma_{ij}^{k}Z_{\alpha}^{i}Z_{\beta}^{j} Z_{k}^{\gamma}+Z_{i}^{\gamma}\frac{\partial Z_{\alpha}^{i}}{\partial S^{\beta }}.\tag{3.125}
The first term in this attractive identity can be described as the shift of the ambient Christoffel symbol onto the surface.
Finally, note that when the ambient space is referred to affine coordinates where Γjki=0\Gamma_{jk}^{i}=0, the above identity simplifies to the equation
Γαβγ=ZiγZαiSβ,(3.126)\Gamma_{\alpha\beta}^{\gamma}=Z_{i}^{\gamma}\frac{\partial Z_{\alpha}^{i} }{\partial S^{\beta}},\tag{3.126}
which is often used for practical calculations of the surface Christoffel symbol.
Denote the components of the unit normal N\mathbf{N} by NiN^{i}, i.e.
N=NiZi,(3.127)\mathbf{N}=N^{i}\mathbf{Z}_{i},\tag{3.127}
or
Ni=ZiN.(3.128)N^{i}=\mathbf{Z}^{i}\cdot\mathbf{N}.\tag{3.128}
Later in this Chapter, we will demonstrate that, up to sign, the components NiN^{i} are given by the explicit formula
Ni=12εijkεβγZjβZkγ.(3.170)N^{i}=\frac{1}{2}\varepsilon^{ijk}\varepsilon_{\beta\gamma}Z_{j}^{\beta} Z_{k}^{\gamma}. \tag{3.170}
For the time being, however, we would like see how much we can learn about NiN^{i} without this formula.
Recall that at each point on the surface, there are two unit normals that point in the opposite directions. Correspondingly, the components NiN^{i} can have two opposite sets of values depending on the choice of normal. In any given situation, the choice of normal is made a priori, either arbitrarily or according to some geometric rationale. Once the choice is made, the normal N\mathbf{N} may be considered unique and therefore an invariant. The components NiN^{i} are then uniquely determined as well and represent a tensor with respect to changes in the ambient coordinates.
Let us now determine the identities for the components NiN^{i} that correspond to the unit-length and orthogonality conditions
NN=1(2.4)\mathbf{N}\cdot\mathbf{N}=1 \tag{2.4}
and
NSα=0.(3.129)\mathbf{N}\cdot\mathbf{S}_{\alpha}=0.\tag{3.129}
Of course, the component form of the unit-length condition reads
NiNi=1.(3.130)N_{i}N^{i}=1.\tag{3.130}
In order to convert the orthogonality condition to component form, note that since N=NiZi\mathbf{N}=N^{i}\mathbf{Z}_{i}, we have
NSα=NiZiSα.(3.131)\mathbf{N}\cdot\mathbf{S}_{\alpha}=N^{i}\mathbf{Z}_{i}\cdot\mathbf{S}_{\alpha }.\tag{3.131}
Since
ZiSα=Ziα,(3.132)\mathbf{Z}_{i}\cdot\mathbf{S}_{\alpha}=Z_{i\alpha},\tag{3.132}
we have
NiZiSα=NiZiα.(3.133)N^{i}\mathbf{Z}_{i}\cdot\mathbf{S}_{\alpha}=N^{i}Z_{i\alpha}.\tag{3.133}
Thus, in component form, the orthogonality condition reads
NiZiα=0.(3.134)N^{i}Z_{i\alpha}=0.\tag{3.134}
It is left as an exercise to argue that, collectively, the equations
NiNi=1 and NiZiα=0(3.135)N_{i}N^{i}=1\text{ and }N^{i}Z_{i\alpha}=0\tag{3.135}
determine NiN^{i} up to sign.
Earlier in this Chapter, we considered a tangent vector U\mathbf{U} with surface components UαU^{\alpha} and showed that its ambient components UiU^{i} are given by the equation
Ui=UαZαi.(3.136)U^{i}=U^{\alpha}Z_{\alpha}^{i}.\tag{3.136}
This time, consider a vector U\mathbf{U} with components UiU^{i}, i.e. U=UiZi\mathbf{U}=U^{i}\mathbf{Z}_{i}, that is not tangent to the surface. The combination
UiZiα(3.137)U^{i}Z_{i}^{\alpha}\tag{3.137}
still makes sense from the tensor notation point of view. As our experience shows, feasible tensor combinations are almost always worthwhile. What, then, is the geometric interpretation of the vector with surface components
UiZiα?(3.138)U^{i}Z_{i}^{\alpha}?\tag{3.138}
In this Section, we will demonstrate that it is the orthogonal projection of U\mathbf{U} onto the tangent plane.
In Chapter 2, we showed that the surface components VαV^{\alpha} of the orthogonal projection V\mathbf{V} of U\mathbf{U} onto the tangent plane are given by the dot product
SαU.(3.139)\mathbf{S}^{\alpha}\cdot\mathbf{U}.\tag{3.139}
Substituting U=UiZi\mathbf{U}=U^{i}\mathbf{Z}_{i}, we find
SαU=SαUiZi.(3.140)\mathbf{S}^{\alpha}\cdot\mathbf{U}=\mathbf{S}^{\alpha}\cdot U^{i} \mathbf{Z}_{i}.\tag{3.140}
Since
SαZi=Ziα,(3.141)\mathbf{S}^{\alpha}\cdot\mathbf{Z}_{i}=Z_{i}^{\alpha},\tag{3.141}
we find
SαU=UiZiα.(3.142)\mathbf{S}^{\alpha}\cdot\mathbf{U}=U^{i}Z_{i}^{\alpha}.\tag{3.142}
Thus, the combination UiZiαU^{i}Z_{i}^{\alpha} indeed represents the components VαV^{\alpha} of the orthogonal projection of U\mathbf{U} onto the tangent plane. As a result, the shift tensor ZiαZ_{i}^{\alpha} may be thought of geometrically as the orthogonal projection operator onto the tangent plane, as it relates the ambient components of a vector U\mathbf{U} to the surface components of its orthogonal projection V\mathbf{V}.
Let us now relate the ambient components of U\mathbf{U} to the ambient components of V\mathbf{V}. At the end of the previous Section, we mentioned that the ambient coordinates ViV^{i} of a tangent vector V\mathbf{V} are obtained by contracting its surface components VαV^{\alpha} with the shift tensor, i.e.
Vi=VαZαi.(3.143)V^{i}=V^{\alpha}Z_{\alpha}^{i}.\tag{3.143}
Since, as we have just established, Vα=UjZjαV^{\alpha}=U^{j}Z_{j}^{\alpha}, we have
Vi=ZαiZjαUj.(3.144)V^{i}=Z_{\alpha}^{i}Z_{j}^{\alpha}U^{j}.\tag{3.144}
Alternatively, we could have arrived at this relationship by starting with the identity
V=(SαU)Sα(3.145)\mathbf{V}=\left( \mathbf{S}^{\alpha}\cdot\mathbf{U}\right) \mathbf{S} _{\alpha}\tag{3.145}
derived in Chapter 2. Then, upon substituting the expansions
V=ViZi,    U=UjZj,    Sα=ZαiZi,(3.146)\mathbf{V}=V^{i}\mathbf{Z}_{i}\text{, \ \ \ }\mathbf{U}=U^{j}\mathbf{Z} _{j}\text{, \ \ \ }\mathbf{S}_{\alpha}=Z_{\alpha}^{i}\mathbf{Z}_{i},\tag{3.146}
we find
ViZi=(SαUjZj)ZαiZi.(3.147)V^{i}\mathbf{Z}_{i}=\left( \mathbf{S}^{\alpha}\cdot U^{j}\mathbf{Z} _{j}\right) Z_{\alpha}^{i}\mathbf{Z}_{i}.\tag{3.147}
Since
SαZj=Zjα,(3.148)\mathbf{S}^{\alpha}\cdot\mathbf{Z}_{j}=Z_{j}^{\alpha},\tag{3.148}
we have
ViZi=UjZjαZαiZi.(3.149)V^{i}\mathbf{Z}_{i}=U^{j}Z_{j}^{\alpha}Z_{\alpha}^{i}\mathbf{Z}_{i}.\tag{3.149}
Equating the components of the vectors on either side, we once again arrive at the relationship
Vi=ZαiZjαUj.(3.144)V^{i}=Z_{\alpha}^{i}Z_{j}^{\alpha}U^{j}. \tag{3.144}
Thus, the combination
ZαiZjα(3.150)Z_{\alpha}^{i}Z_{j}^{\alpha}\tag{3.150}
may be thought of as the operator of orthogonal projection onto the tangent plane. It should be noted that compactness of ZαiZjαZ_{\alpha}^{i}Z_{j}^{\alpha} is quite remarkable. Recall from Linear Algebra that the problem of finding the orthogonal projection onto a linear subspace is solved by the technique of least squares. If AA is the rectangular matrix, then the operator of orthogonal projection onto the column space of AA is given by the combination
A(ATA)1AT.(3.151)A\left( A^{T}A\right) ^{-1}A^{T}.\tag{3.151}
The combination ZαiZjαZ_{\alpha}^{i}Z_{j}^{\alpha} includes all of the same elements -- however, the complexity of the operations is absorbed by the indicial notation. In particular, the matrix (ATA)1\left( A^{T}A\right) ^{-1} corresponds to the contravariant metric tensor SαβS^{\alpha\beta} which makes its presence felt via the placement of the surface index in the shift tensor ZjαZ_{j}^{\alpha} as a superscript.
In Chapter 2, we showed that the orthogonal projection W\mathbf{W} of a vector U\mathbf{U} onto the normal direction N\mathbf{N}, i.e. away from the tangent plane, is given by
W=(UN)N.(2.53)\mathbf{W}=\left( \mathbf{U}\cdot\mathbf{N}\right) \mathbf{N.} \tag{2.53}
Let us convert this identity to component form.
The dot product UN\mathbf{U}\cdot\mathbf{N} is given by UjNjU^{j}N_{j}. If WiW^{i} are the ambient components of W\mathbf{W}, then the above equation reads
WiZi=UjNjNiZi.(3.152)W^{i}\mathbf{Z}_{i}=U^{j}N_{j}N^{i}\mathbf{Z}_{i}.\tag{3.152}
Equating the components, we find
Wi=NiNjUj,(3.153)W^{i}=N^{i}N_{j}U^{j},\tag{3.153}
which is the relationship that we set out to find. Whereas the combination
ZαiZjα(3.154)Z_{\alpha}^{i}Z_{j}^{\alpha}\tag{3.154}
represented the operator of orthogonal projection onto the tangent plane, the combination
NiNj(3.155)N^{i}N_{j}\tag{3.155}
represents the operator of orthogonal projection away from the tangent plane. A good question to consider, then, is what does the sum
ZαiZjα+NiNj(3.156)Z_{\alpha}^{i}Z_{j}^{\alpha}+N^{i}N_{j}\tag{3.156}
represent? This question will be answered in the following Section.
Recall the identity
U=(SαU)Sα+(UN)N.(2.55)\mathbf{U}=\left( \mathbf{S}^{\alpha}\cdot\mathbf{U}\right) \mathbf{S} _{\alpha}+\left( \mathbf{U}\cdot\mathbf{N}\right) \mathbf{N.} \tag{2.55}
from Chapter 2 which states that a vector U\mathbf{U} at a point P P\ on a surface is the sum of its orthogonal projection V=(SαU)Sα\mathbf{V}=\left( \mathbf{S}^{\alpha}\cdot\mathbf{U}\right) \mathbf{S}_{\alpha} onto the tangent plane and its orthogonal projection W=(UN)N\mathbf{W}=\left( \mathbf{U} \cdot\mathbf{N}\right) \mathbf{N} away from the tangent plane. In component form, the above identity reads
Ui=ZαiZjαUj+NiNjUj.(3.157)U^{i}=Z_{\alpha}^{i}Z_{j}^{\alpha}U^{j}+N^{i}N_{j}U^{j}.\tag{3.157}
Substituting the combination δjiUj\delta_{j}^{i}U^{j} for UiU^{i} on the left, we find
δjiUj=ZαiZjαUj+NiNjUj.(3.158)\delta_{j}^{i}U^{j}=Z_{\alpha}^{i}Z_{j}^{\alpha}U^{j}+N^{i}N_{j}U^{j}.\tag{3.158}
Since the above identity holds for any UjU^{j}, we arrive at the relationship
δji=ZαiZjα+NiNj(3.159)\delta_{j}^{i}=Z_{\alpha}^{i}Z_{j}^{\alpha}+N^{i}N_{j}\tag{3.159}
known as the projection formula. It is usually written with the Kronecker delta on the right, i.e.
ZαiZjα+NiNj=δji.(3.160)Z_{\alpha}^{i}Z_{j}^{\alpha}+N^{i}N_{j}=\delta_{j}^{i}.\tag{3.160}
Other useful forms of the projection formula read
ZαiZjα=δjiNiNj(3.161)Z_{\alpha}^{i}Z_{j}^{\alpha}=\delta_{j}^{i}-N^{i}N_{j}\tag{3.161}
and
NiNj=δjiZαiZjα.(3.162)N^{i}N_{j}=\delta_{j}^{i}-Z_{\alpha}^{i}Z_{j}^{\alpha}.\tag{3.162}
Earlier in this Chapter, we remarked that the combination ZαiZjαZ_{\alpha}^{i} Z_{j}^{\alpha} cannot equal δji\delta_{j}^{i}. The projection formula refines that insight and identifies precisely the relationship of ZαiZjαZ_{\alpha}^{i} Z_{j}^{\alpha} to δji\delta_{j}^{i}.
As our experience so far has shown, we can work quite effectively with the components NiN^{i} of the unit normal even though they have only been specified implicitly by the orthogonality condition
ZiαNi=0(3.134)Z_{i}^{\alpha}N^{i}=0 \tag{3.134}
and the normalization condition
NiNi=1.(3.130)N_{i}N^{i}=1. \tag{3.130}
Of course, these conditions actually give us a practical way of calculating NiN^{i}. It is left as an exercise to show that if AA is the 3×23\times2 matrix that represents the shift tensor ZiαZ_{i}^{\alpha}, then NiN^{i} corresponds to a unit vector from the one-dimensional null space of ATA^{T}. Thus, an explicit expression for NiN^{i} is not needed. However, it is an intriguing challenge to find such an expression and we will do so in this Section.
The inspiration for the expression comes from the concept of the cross product. Note that the elements S1\mathbf{S}_{1} and S2\mathbf{S}_{2} of the surface covariant basis represent two linearly independent vectors in the tangent plane. Therefore, their cross product
S1×S2(3.163)\mathbf{S}_{1}\times\mathbf{S}_{2}\tag{3.163}
is orthogonal to the plane and is therefore collinear with N\mathbf{N}. Thus, all that is left to do is to find a vector of unit length that is a scalar multiple of S1×S2\mathbf{S}_{1}\times\mathbf{S}_{2}.
The ambient components of S1\mathbf{S}_{1} and S2\mathbf{S}_{2} are found in the elements of the shift tensor ZαiZ_{\alpha}^{i}. Specifically, the components of S1\mathbf{S}_{1} are Z1iZ_{1}^{i} and those of S2\mathbf{S}_{2} are Z2jZ_{2}^{j}. Thus, as was described in Chapter TBD of Introduction to Tensor Calculus, the covariant components UiU_{i} of U=S1×S2\mathbf{U} =\mathbf{S}_{1}\times\mathbf{S}_{2} are given by the equation
Ui=εijkZ1jZ2k.(3.164)U_{i}=\varepsilon_{ijk}Z_{1}^{j}Z_{2}^{k}.\tag{3.164}
It is left as a straightforward exercise to confirm that UiU_{i} satisfies the orthogonality condition
ZiαUi=0.(3.165)Z^{i\alpha}U_{i}=0.\tag{3.165}
However, in order to be geometrically meaningful, UiU^{i} must be a tensor. Meanwhile, the expression εijkZ1jZ2k\varepsilon_{ijk}Z_{1}^{j}Z_{2}^{k} uses literal subscripts 11 and 22, which are disallowed by the rules of the tensor notation and thus UiU^{i}, as defined, is not a tensor. Fortunately, this difficulty is easy to overcome.
It is left as an exercise that the expression εijkZ1jZ2k\varepsilon_{ijk}Z_{1}^{j} Z_{2}^{k} is skew-symmetric with respect to exchanging the values of the literal indices, i.e.
εijkZ1jZ2k=εijkZ2jZ1k(3.166)\varepsilon_{ijk}Z_{1}^{j}Z_{2}^{k}=-\varepsilon_{ijk}Z_{2}^{j}Z_{1}^{k}\tag{3.166}
Therefore, the difference
εijkZ1jZ2kεijkZ2jZ1k(3.167)\varepsilon_{ijk}Z_{1}^{j}Z_{2}^{k}-\varepsilon_{ijk}Z_{2}^{j}Z_{1}^{k}\tag{3.167}
is twice UiU_{i} and therefore also represents a vector that is collinear with N\mathbf{N}. With the help of the permutation symbol eαβe^{\alpha\beta}, this difference can be written in the form
εijkeαβZαjZβk.(3.168)\varepsilon_{ijk}e^{\alpha\beta}Z_{\alpha}^{j}Z_{\beta}^{k}.\tag{3.168}
Next, replace the permutation symbol eαβe^{\alpha\beta} with the Levi-Civita symbol εαβ=eαβ/S\varepsilon^{\alpha\beta}=e^{\alpha\beta}/\sqrt{S} in order to arrive at the tensor expression
εijkεαβZαjZβk(3.169)\varepsilon_{ijk}\varepsilon^{\alpha\beta}Z_{\alpha}^{j}Z_{\beta}^{k}\tag{3.169}
Now, the only remaining questions are those of length and sign. It is left as an exercise to show that the length of the vector with components above is 22. Thus, scaling the expression above by 1/21/2 we arrive at
Ni=12εijkεβγZjβZkγ.(3.170)N^{i}=\frac{1}{2}\varepsilon^{ijk}\varepsilon_{\beta\gamma}Z_{j}^{\beta} Z_{k}^{\gamma}.\tag{3.170}
Of course, depending on our a priori choice of N\mathbf{N}, the above formula may deliver the components of N-\mathbf{N} rather than N\mathbf{N}. Finally, we must note that the variant on the right side of the above formula is a tensor only under orientation-preserving transformations of both ambient and surface coordinates.
Exercise 3.1Show that the equations of the surface Zi(θ,φ)Z^{i}\left( \theta,\varphi\right) for a sphere of radius RR in cylindrical ambient coordinates r,θ1,zr,\theta_{1},z read
r(θ,φ)=Rsinθ          (3.171)θ1(θ,φ)=φ          (3.172)z(θ,φ)=Rcosθ          (3.173)\begin{aligned}r\left( \theta,\varphi\right) & =R\sin\theta\ \ \ \ \ \ \ \ \ \ \left(3.171\right)\\\theta_{1}\left( \theta,\varphi\right) & =\varphi\ \ \ \ \ \ \ \ \ \ \left(3.172\right)\\z\left( \theta,\varphi\right) & =R\cos\theta\ \ \ \ \ \ \ \ \ \ \left(3.173\right)\end{aligned}
Exercise 3.2Show that the equations of the surface Zi(θ,z)Z^{i}\left( \theta,z\right) for a cylinder of radius RR in spherical ambient coordinates r,θ1,φr,\theta_{1},\varphi read
r(θ,z)=R2+z2          (3.174)θ1(θ,z)=arctanRz          (3.175)φ(θ,z)=θ          (3.176)\begin{aligned}r\left( \theta,z\right) & =\sqrt{R^{2}+z^{2}}\ \ \ \ \ \ \ \ \ \ \left(3.174\right)\\\theta_{1}\left( \theta,z\right) & =\arctan\frac{R}{z}\ \ \ \ \ \ \ \ \ \ \left(3.175\right)\\\varphi\left( \theta,z\right) & =\theta\ \ \ \ \ \ \ \ \ \ \left(3.176\right)\end{aligned}
Exercise 3.3In the text, we showed that the shift tensor ZαiZ_{\alpha}^{i} is a tensor with the help of the identity
Zαi=ZiSα.(3.70)Z_{\alpha}^{i}=\mathbf{Z}^{i}\cdot\mathbf{S}_{\alpha}. \tag{3.70}
However, it is important to be able to demonstrate its tensor property on the basis of its definition
Zαi=Zi(S)Sα.(3.68)Z_{\alpha}^{i}=\frac{\partial Z^{i}\left( S\right) }{\partial S^{\alpha}}. \tag{3.68}
Do so in three steps. First, consider changes only of ambient coordinates. First justify and then use the identity
Zi(S)=Zi(Z(S))(3.177)Z^{i^{\prime}}\left( S\right) =Z^{i^{\prime}}\left( Z\left( S\right) \right)\tag{3.177}
to show that
Zαi=ZαiJi.i.(3.178)Z_{\alpha}^{i^{\prime}}=Z_{\alpha}^{i}J_{i.}^{i^{\prime}}.\tag{3.178}
Second, consider changes of only surface coordinates and use the identity
Zi(S)=Zi(S(S))(3.179)Z^{i}\left( S^{\prime}\right) =Z^{i}\left( S\left( S^{\prime}\right) \right)\tag{3.179}
to show that
Zαi=ZαiJαα.(3.180)Z_{\alpha^{\prime}}^{i}=Z_{\alpha}^{i}J_{\alpha^{\prime}}^{\alpha}.\tag{3.180}
Finally, consider simultaneous changes of ambient and surface coordinates. Use the identity
Zi(S)=Zi(Z(S(S)))(3.181)Z^{i^{\prime}}\left( S^{\prime}\right) =Z^{i^{\prime}}\left( Z\left( S\left( S^{\prime}\right) \right) \right)\tag{3.181}
to show that
Zαi=ZαiJiiJαα.(3.182)Z_{\alpha^{\prime}}^{i^{\prime}}=Z_{\alpha}^{i}J_{i}^{i^{\prime}} J_{\alpha^{\prime}}^{\alpha}.\tag{3.182}
Exercise 3.4Suppose that the elements of ZiαZ_{i\alpha} are organized into a 3×23\times2 matrix AA. Show that the 3×13\times1 matrix consisting of the elements of NiN^{i} belongs to the null space of ATA^{T}. This observation gives a practical way of calculating the components NiN^{i}.
Exercise 3.5Show that the length of the vector with components
εijkεαβZαjZβk(3.183)\varepsilon_{ijk}\varepsilon^{\alpha\beta}Z_{\alpha}^{j}Z_{\beta}^{k}\tag{3.183}
is 22. In other words, show that if
Ui=εijkεαβZαjZβk,(3.184)U_{i}=\varepsilon_{ijk}\varepsilon^{\alpha\beta}Z_{\alpha}^{j}Z_{\beta}^{k},\tag{3.184}
then
UiUi=4.(3.185)U_{i}U^{i}=4.\tag{3.185}
Exercise 3.6Let
Pji=ZαiZjα.(3.186)P_{j}^{i}=Z_{\alpha}^{i}Z_{j}^{\alpha}.\tag{3.186}
Show that
Pki=PjiPkj.(3.187)P_{k}^{i}=P_{j}^{i}P_{k}^{j}.\tag{3.187}
Notice that in the language of matrices, the above identity reads P2=PP^{2}=P which represents the Linear Algebra definition of a projection matrix.
Exercise 3.7Similarly, let
Pji=NiNj(3.188)P_{j}^{i}=N^{i}N_{j}\tag{3.188}
and show that
PjiPkj=Pki.(3.189)P_{j}^{i}P_{k}^{j}=P_{k}^{i}.\tag{3.189}
Thus, the matrix PP corresponding to PjiP_{j}^{i} also satisfies the Linear Algebra definition of a projection matrix.
Exercise 3.8Show that the derivatives of the ambient covariant basis with respect to the surface coordinates are given by the formula
Zi(S)Sβ=ΓijmZβjZm.(3.122)\frac{\partial\mathbf{Z}_{i}\left( S\right) }{\partial S^{\beta}} =\Gamma_{ij}^{m}Z_{\beta}^{j}\mathbf{Z}_{m}. \tag{3.122}
Exercise 3.9Derive the identity
Γαβγ=ΓijkZαiZβjZkγ+ZiγZαiSβ(3.125)\Gamma_{\alpha\beta}^{\gamma}=\Gamma_{ij}^{k}Z_{\alpha}^{i}Z_{\beta}^{j} Z_{k}^{\gamma}+Z_{i}^{\gamma}\frac{\partial Z_{\alpha}^{i}}{\partial S^{\beta }} \tag{3.125}
from the intrinsic definitions of the Christoffel symbols
Γβγα=12Sαω(SωβSγ+SωγSβSβγSω)(2.57)\Gamma_{\beta\gamma}^{\alpha}=\frac{1}{2}S^{\alpha\omega}\left( \frac{\partial S_{\omega\beta}}{\partial S^{\gamma}}+\frac{\partial S_{\omega\gamma}}{\partial S^{\beta}}-\frac{\partial S_{\beta\gamma}}{\partial S^{\omega}}\right) \tag{2.57}
and
Γjki=12Zim(ZmjZk+ZmkZjZjkZm).(6.45)\Gamma_{jk}^{i}=\frac{1}{2}Z^{im}\left( \frac{\partial Z_{mj}}{\partial Z^{k}}+\frac{\partial Z_{mk}}{\partial Z^{j}}-\frac{\partial Z_{jk}}{\partial Z^{m}}\right) . \tag{6.45}
Exercise 3.10Notice the striking similarity between the definition of the surface Christoffel symbol
Γαβγ=SγSαSβ(2.56)\Gamma_{\alpha\beta}^{\gamma}=\mathbf{S}^{\gamma}\cdot\frac{\partial \mathbf{S}_{\alpha}}{\partial S^{\beta}} \tag{2.56}
and the formula
Γαβγ=ZiγZαiSβ(3.190)\Gamma_{\alpha\beta}^{\gamma}=Z_{i}^{\gamma}\frac{\partial Z_{\alpha}^{i} }{\partial S^{\beta}}\tag{3.190}
valid for affine ambient coordinates. Derive the latter equation from the former by assuming affine coordinates in the ambient space from the start.
Exercise 3.11Use the explicit expression for NiN^{i} to prove the projection formula
ZαiZjα+NiNj=δji.(3.191)Z_{\alpha}^{i}Z_{j}^{\alpha}+N^{i}N_{j}=\delta_{j}^{i}.\tag{3.191}
This is an important, albeit time-consuming, exercise that you should take your time working out.
Exercise 3.12Show that the length of one cycle of the cycloid is 8r8r.
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