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After reading about the pushforward and pullback, I don't really have a concrete grasp of them, so I think these simple questions might clear things up for me; I appreciate any hints or solutions.

Let $(s,t)$ be coordinates on $\mathbb{R}^2$ and $(x,y,z)$ be coordinates on $\mathbb{R}^3$. Let $g:\mathbb{R}^2\to\mathbb{R}^3$ be defined by $g(s,t)=(\sin(t),st^2,s^3-1)$.

Let $X_p\in T_p\mathbb{R}^2$ be given by $X_p=\frac{\partial}{\partial s}|_p - \frac{\partial}{\partial t}|_p$, compute the push-forward $g_*X_p$.

Let $\omega$ be the smooth $1$-form $\omega=dx+xdy+y^2dz$; find the pullback $g^*\omega$.

From what I understand, if $\varphi:M\to N$ then $d\varphi_p:T_p M\to T_{\varphi(p)}N$ and is given by $d\varphi_p(X)(f)=X(f\circ \varphi)$ where $X\in TM (T_pM?)$ and $f\in C^\infty (N)$. I think that $d\varphi=\varphi_*$? And I reckon that in this case $M=\mathbb{R}^2$, $N=\mathbb{R}^3$, and $\varphi=g$ but I'm not sure what $f$ equals (what does $g_*X_p$ act on?).... do we even need to act on an $f$ to find $g_*X$? Sorry I'm a bit lost.

Squirtle
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1 Answers1

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Let's work out some computations: first, the push-forward of the vector field $X = \frac{\partial }{\partial s} - \frac{\partial }{\partial t}$, denoted $g_* X$. To do so, we need to find the push forward of the two vector fields $\frac{\partial}{\partial s}$ and $\frac{\partial}{\partial t}$. This is given by $$ g_* \left( \frac{\partial}{\partial s} \right) = \frac{\partial x}{\partial s} \frac{\partial}{\partial x} + \frac{\partial y}{\partial s} \frac{\partial}{\partial y} + \frac{\partial z}{\partial s}\frac{\partial }{\partial z} = t^2 \frac{\partial}{\partial y} + 3s^2 \frac{\partial}{\partial z}, $$ and $$ g_* \left( \frac{\partial}{\partial t} \right) = \frac{\partial x}{\partial t} \frac{\partial}{\partial x} + \frac{\partial y}{\partial t}\frac{\partial}{\partial y} + \frac{\partial z}{\partial t} \frac{\partial}{\partial z} = \cos(t) \frac{\partial}{\partial x} + 2st \frac{\partial}{\partial y}. $$ Then, $$ g_* X = g_* \left( \frac{\partial}{\partial s} \right) - g_* \left( \frac{\partial}{\partial t} \right) = -\cos(t) \frac{\partial}{\partial x} + (t^2 -2st) \frac{\partial}{\partial y} + 3s^2 \frac{\partial}{\partial z}. $$ A remark: in $g_* X$, I should have written this without reference to $s$ and $t$ (that is, solve the equations $x=\sin(t)$ and $y=st^2$ and $z=s^3-1$ for $s$ and $t$ in terms of $x,y,z$), however it was not clear to me how to do that here.

Next, let's find the pullback $g^{*}\omega$: this will be a 1-form on $\mathbb{R}^2$ and hence should be of the form $a(s,t) ds + b(s,t) dt$. To figure out what these functions $a(s,t)$ and $b(s,t)$ are, let us rewrite each `component' of the form $\omega$ in terms of $s$ and $t$: $$ dx = \frac{\partial x}{\partial s} ds + \frac{\partial x}{\partial t} dt = \cos(t) dt $$ $$ dy = \frac{\partial y}{\partial s} ds + \frac{\partial y}{\partial t} dt = t^2 ds + 2st dt $$ $$ dz = \frac{\partial z}{\partial s} ds + \frac{\partial z}{\partial t} dt = 3s^2 ds $$ Putting all of this together, we find that \begin{align*} g^* \omega &= \cos(t) dt + \sin(t) (t^2 ds + 2st dt) + s^2 t^4 (3s^2 ds) \\ &= (t^2 \sin(t) + s^4 t^4 ) ds + (\cos(t) + 2st \sin(t) ) dt. \end{align*}

If you find that you need practice with computations when dealing with manifolds and differential geometry (e.g. push forwards, pullbacks, Lie derivatives, etc.), I recommend looking at an exercise-heavy book such as Gadea & Masque's "Analysis and Algebra on Differentiable Manifolds, A Workbook for Students and Teachers". I found this one to be very helpful when learning this material for the first time.

msteve
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  • If you should have expressed s and t in terms of x,y,z then could you? – Squirtle Jan 09 '15 at 04:48
  • It's not clear to me how to solve for $s$ and $t$ in terms of $x,y,z$ given the equation $x=\sin(t)$, $y=st^2$, and $z =s^3 - 1$. If I could solve this, then that would be what to substitute in to the push forward. – msteve Jan 09 '15 at 04:52
  • Actually, I suppose it would not be that bad, you could do something like $s = (1+z)^{1/3}$ and $t = \sqrt{\frac{y}{(1+z)^{1/3}}}$, though I suppose I have not taken into account the equation $x = \sin(t)$... – msteve Jan 09 '15 at 05:10
  • After thinking about it more.... one does $not$ need to express the numbers $t,s$ in terms of $x,y,z$, because..... they are just... numbers. – Squirtle Jan 09 '15 at 22:33
  • They are not numbers but smooth functions, since $g_* X$ is a vector field on $\mathbb{R}^2$: we can write it as $g_* X = f_1(x,y,z) \frac{\partial}{\partial x} + f_2(x,y,z) \frac{\partial}{\partial y} + f_3(x,y,z) \frac{\partial}{\partial z}$ for some smooth functions $f_1,f_2,f_3$ on $\mathbb{R}^3$. Once we evaluate the vector field at some point $g(p)$, then it is an element of the vector space $T_{g(p)} \mathbb{R}^3$ and hence it can be written as $g_* X {g(p)} = f_1(g(p)) \frac{\partial}{\partial x} \bigg|{g(p)} + \ldots + f_3(g(p)) \frac{\partial}{\partial z} \bigg|_{g(p)}$. – msteve Jan 09 '15 at 23:48