ebsd2021:tema2
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| ebsd2021:tema2 [2021/06/28 16:10] – external edit 127.0.0.1 | ebsd2021:tema2 [2021/08/31 15:19] (current) – escola | ||
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| - | Tema 2 | + | **Tema 2: Geodesic flows in Hamiltonian dynamics** |
| + | |||
| + | **Symplectic form and symplectic manifold** | ||
| + | |||
| + | We start recalling some known facts on linear algebra. | ||
| + | Let $V$ be a vector space. | ||
| + | |||
| + | |||
| + | // | ||
| + | $\omega: | ||
| + | * bilinear: $\omega$ is linear on each coordinate. | ||
| + | * antisymmetric: | ||
| + | * non-degenerate: | ||
| + | |||
| + | In this case, we call $(V, | ||
| + | |||
| + | Symplectic bilinear forms have canonical representations: | ||
| + | if $\omega$ is symplectic, then there is a basis | ||
| + | $\{x_1, | ||
| + | $$ | ||
| + | \left\{ | ||
| + | \begin{array}{l} | ||
| + | \omega(x_i, | ||
| + | \omega(x_i, | ||
| + | \end{array}\right. | ||
| + | ,\ \ \forall i, | ||
| + | $$ | ||
| + | In particular, $V$ has even dimension, equal to $2n$. In this basis, $\omega$ takes the form | ||
| + | $$ | ||
| + | \omega(x, | ||
| + | \left[ | ||
| + | \begin{array}{ccc|ccc} | ||
| + | &&&&& | ||
| + | & | ||
| + | &&& | ||
| + | &&&&& | ||
| + | &{\rm -Id}&&& | ||
| + | &&&&& | ||
| + | \end{array}\right] | ||
| + | y. | ||
| + | $$ | ||
| + | |||
| + | Here is the prototype of a symplectic vector space: given $(E, | ||
| + | with inner product, let $V=E\times E$ and define $\omega: | ||
| + | $$ | ||
| + | \omega((x_1, | ||
| + | $$ | ||
| + | Then $(V, | ||
| + | for this example, in which case the symplectic bilinear map is defined in $\mathbb R^{2n}$. | ||
| + | |||
| + | |||
| + | With respect to the symplectic structure, there are some special subspaces. | ||
| + | |||
| + | //Isotropic and Lagrangian subspaces:// | ||
| + | a subspace $Y\subset V$, define | ||
| + | $$ | ||
| + | Y^\omega=\{x\in V: | ||
| + | $$ | ||
| + | It is easy to see that ${\rm dim}(Y)+{\rm dim}(Y^\omega)=2n$. | ||
| + | We call $Y$: | ||
| + | * // | ||
| + | * // | ||
| + | |||
| + | |||
| + | The next definition introduces the symplectic structure on manifolds. | ||
| + | Let $M$ be a $m$-dimensional differentiable manifold, and recall the definition of a symplectic | ||
| + | form (which is the choice of symplectic bilinear maps on each tangent space of $M$). | ||
| + | |||
| + | // | ||
| + | |||
| + | |||
| + | In particular, $m=2n$ is even. The simplest example of a symplectic manifold is $(\mathbb R^{2n}, | ||
| + | $$ | ||
| + | \omega=dx_1\wedge dp_1+\cdots+dx_n\wedge dp_n. | ||
| + | $$ | ||
| + | |||
| + | Compare this with Riemannian manifolds. A Riemannian manifold is a differentiable manifold | ||
| + | equipped with a Riemannian metric. The difference between metrics and two-forms is that the | ||
| + | first is symmetric, while the other is antisymmetric. This simple difference makes the two | ||
| + | contexts extremely different. | ||
| + | |||
| + | |||
| + | **$TM$ is a symplectic manifold** | ||
| + | |||
| + | We already know that $(TM, | ||
| + | |||
| + | //1--form $\Theta$ on $TM$:// Define the 1--form $\Theta$ on $TM$ taking | ||
| + | $\Theta_v: | ||
| + | $$ | ||
| + | \Theta_v(x, | ||
| + | $$ | ||
| + | |||
| + | |||
| + | Above, $TTM_v\cong TM_p\times TM_p$ via the horizontal and vertical coordinates. | ||
| + | |||
| + | **Lemma.** We have $d\Theta=\omega$. In particular, $\omega$ is closed. | ||
| + | |||
| + | |||
| + | **Hamiltonian vector fields** | ||
| + | |||
| + | Let $(M, | ||
| + | The derivative $dH$ is a 1--form. | ||
| + | |||
| + | // | ||
| + | vector field $X_H:M\to TM$ defined by | ||
| + | $$ | ||
| + | \omega_p(\cdot, | ||
| + | $$ | ||
| + | The flow generated by $X_H$ is called the // | ||
| + | |||
| + | |||
| + | In other words, the contraction 1--form $\omega(\cdot, | ||
| + | Existence and uniqueness follow from the non-degeneracy of $\omega$. | ||
| + | |||
| + | |||
| + | Let us express the Hamiltonian vector field in the prototypical example of $(\mathbb R^{2n}, | ||
| + | Let $H:\mathbb R^{2n}\to\mathbb R$ be a $C^1$ function. | ||
| + | We will show that $X_H$ satisfies the //Hamilton equations// | ||
| + | For $(v, | ||
| + | $$ | ||
| + | dH(v, | ||
| + | $$ | ||
| + | On the other expression, if $X_H=(X, | ||
| + | $$ | ||
| + | \omega((v, | ||
| + | $$ | ||
| + | Comparing the last two equations, we conclude that $X_i=\tfrac{\partial H}{\partial p_i}$ | ||
| + | and $Y_i=-\tfrac{\partial H}{\partial x_i}$ for $i=1, | ||
| + | the Hamilton equations | ||
| + | $$ | ||
| + | \left\{ | ||
| + | \begin{array}{l} | ||
| + | X=\tfrac{\partial H}{\partial p}\\ | ||
| + | \\ | ||
| + | Y =-\tfrac{\partial H}{\partial x} | ||
| + | \end{array} | ||
| + | \right. | ||
| + | $$ | ||
| + | characterize $X_H$. | ||
| + | |||
| + | |||
| + | The Halmiltonian vector field has some important invariance properties. | ||
| + | Let $\phi=\{\phi^t\}$ be flow generated by $X_H$. | ||
| + | |||
| + | **Theorem.** The following holds: | ||
| + | |||
| + | (1) $H\circ\phi^t=H$ for all $t\in\mathbb R$, hence $H$ is constant along flow lines. | ||
| + | |||
| + | (2) $\omega$ is preserved by $\phi$, i.e. | ||
| + | $\omega(d\phi^t v,d\phi^t w)=\omega(v, | ||
| + | and all $t\in\mathbb R$. | ||
| + | |||
| + | (3) $\phi$ preserves the volume form $\omega^n$. | ||
| + | |||
| + | |||
| + | **The geodesic flow is a Hamiltonian flow** | ||
| + | |||
| + | We already know that $(TM, | ||
| + | We claim that the geodesic flow $g:TM\to TM$ is the Hamiltonian flow | ||
| + | of the function $G: | ||
| + | $$ | ||
| + | G(v)=\tfrac{1}{2}\langle v, | ||
| + | $$ | ||
| + | To prove this, write $X_G=(X, | ||
| + | $$ | ||
| + | \omega(\xi, | ||
| + | $$ | ||
| + | If $x,y\in TM_v$, let $Z: | ||
| + | $Z' | ||
| + | $$ | ||
| + | dG_v(\xi)=\tfrac{d}{dt}|_{t=0}(G\circ Z)=\tfrac{d}{dt}|_{t=0}\tfrac{1}{2}\langle Z(t), | ||
| + | \langle v, | ||
| + | $$ | ||
| + | and so $(X, | ||
| + | |||
| + | |||
| ~~DISCUSSIONS~~ | ~~DISCUSSIONS~~ | ||
ebsd2021/tema2.1624907416.txt.gz · Last modified: 2021/06/28 16:10 by 127.0.0.1