Chapter 4: Problem 7
Let \(f: M \rightarrow N, g: N \rightarrow K\), and \(h=g: f: M \rightarrow K\). Show that \(h_{*}=g_{*} f_{*}\).
Chapter 4: Problem 7
Let \(f: M \rightarrow N, g: N \rightarrow K\), and \(h=g: f: M \rightarrow K\). Show that \(h_{*}=g_{*} f_{*}\).
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Get started for freeA rod of weight \(P\), tilted at an angle of \(60^{\circ}\) to the plane of a table, begins to fall with initial velocity zero (Figure 74). Find the constraint force of the table at the initial moment, considering the table as (a) absolutely smooth and (b) absolutely rough. (In the first case, the holonomic constraint holds the end of the rod on the plane of the table, and in the second case, at a given point.)
Suppose that a particle moves in the field of the uniform helical line \(x=\cos \varphi\). \(y=\sin \varphi_{z} z=c \varphi\). Find the law of conservation corresponding to this helical symmetry.
Show that \(S O(3)\) is embedded in \(R^{9}\), and at the same time, that \(S O(3)\) is a manifold.
Show that the vector \(f_{* x} v\) does not depend on the curve \(\boldsymbol{\varphi}\), but only on the vector \(\boldsymbol{v}\).
Extend Noether's theorem to non-autonomous lagrangian systems. Hint. Let \(M_{1}=M \times \mathbb{R}\) be the extended configuration space (the direct product of the configuration manifold \(M\) with the time axis \(\mathbb{R}\) ). Define a function \(L_{1}: T M_{1} \rightarrow \mathbb{R}\) by $$ L \frac{d t}{d z} \text { : } $$ i.e., in lucal coordinates \(q, t\) on \(M_{1}\) we define it by the formula $$ L_{1}\left(\mathbf{q}, t, \frac{d \mathbf{q}}{d \tau}, \frac{d t}{d \tau}\right)=L\left(\mathbf{q}, \frac{d \mathbf{q} / d \tau}{d t, d \tau}, t\right) \frac{d t}{d \tau} $$ We apply Noether's theorem to the lagrangian system \(\left(M_{2}, L_{1}\right)\). If \(L_{1}\) admits the transformations \(h^{s}: M_{1} \rightarrow M_{1}\). we obtain a first integral \(l_{1}: T M_{1} \rightarrow \mathbb{R}\). Since \(\int L d t=\int L_{1} d \tau_{\text {. this reduces }}\) to a first integral \(I: T M \times\) of \(\rightarrow \mathbb{R}\) of the viginal system. If. in local coordinates \((\boldsymbol{q}, t)\) on \(M_{1}\), we have \(I_{1}=I_{1}(\mathbf{q}, t, d \mathbf{q} / d \tau, d l / d \tau)\), then \(I(\mathbf{q}, \mathbf{q}, t)=l_{1}\left(\mathbf{q}, I_{1}, \dot{\mathbf{q}}, 1\right)\). In particular, if \(L\) does not depend on time, \(L_{1}\) admits translations along time, \(h^{s}(q, t)=\) (q. \(t+5\) ). The corresponding first integral \(l\) is the energy integral.
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