- Commit
- bedd7677dae474f49f56fa3698f3c2862477e94a
- Parent
- cafddd125eb9bb578ba4fc32e2d3f0157dc8546a
- Author
- Pablo <pablo-escobar@riseup.net>
- Date
Fixed multiple typos in the third section
Riemannian Geometry course project on the manifold H¹(I, M) of class H¹ curves on a Riemannian manifold M and its applications to the geodesics problem
Fixed multiple typos in the third section
1 file changed, 30 insertions, 29 deletions
Status | File Name | N° Changes | Insertions | Deletions |
Modified | sections/applications.tex | 59 | 30 | 29 |
diff --git a/sections/applications.tex b/sections/applications.tex @@ -19,7 +19,7 @@ instance: any piece-wise smooth function \(H : I \times (-\epsilon, \epsilon) \to M\) determines a variation \(\{ \gamma_t \}_t\) given by \(\gamma_t(s) = H(s, t)\). This is representative of the theory that lies ahead, in the sense that most of the results we'll discuss in the following are minor refinements -to the classical theory. Instead, the value of the theory we will develop in +of the classical theory. Instead, the value of the theory we will develop in here lies in its conceptual simplicity: instead of relying in ad-hoc methods we can now use the standard tools of calculus to study the critical points of the energy functional \(E\). @@ -29,7 +29,7 @@ a smooth function \(E \in C^\infty(H^1(I, M))\) we can study its classical ``critical points'' -- i.e. curves \(\gamma\) with a variation \(\{ \gamma_t \}_t\) such that \(\left.\frac\dd\dt\right|_{t = 0} E(\gamma_t) = 0\) -- by looking at its derivative. The first variation of energy thus becomes a -particular case of the formula for \(d E\), and the second variation of energy +particular case of a formula for \(d E\), and the second variation of energy becomes a particular case of a formula for the Hessian of \(E\) at a critical point. Without further ado, we prove\dots @@ -136,7 +136,7 @@ We begin with a technical lemma. X & \mapsto X_0 & X & \mapsto X_1 \end{align*} - are surjective maps for all \(\gamma \in H^1(\gamma^* TM)\). + are surjective maps for all \(\gamma \in H^1(I, M)\). \end{proof} We can now show\dots @@ -195,9 +195,8 @@ of \(E\!\restriction_{\Omega_{p q} M}\) and \(E\!\restriction_{\Lambda M}\). \(\dot\gamma(0) = \dot\gamma(1)\) and \(X_0 = X_1\). This establishes that the geodesics are indeed critical points of the restrictions of \(E\). - Suppose \(\gamma \in \Omega_{p q} M\) is a critical point of - \(E\!\restriction_{\Omega_{p q} M}\) and let \(Y, Z \in H^1(\gamma^* TM)\) be - such that + Suppose \(\gamma \in \Omega_{p q} M\) is a critical point and let \(Y, Z \in + H^1(\gamma^* TM)\) be such that \begin{align*} \frac\nabla\dt Y & = \partial \gamma & Y_0 & = 0 & @@ -216,10 +215,10 @@ of \(E\!\restriction_{\Omega_{p q} M}\) and \(E\!\restriction_{\Lambda M}\). \] and \[ - 0 - = d E_\gamma X + \langle \partial \gamma, \partial \gamma - Z \rangle_0 = \left\langle \partial \gamma, \frac\nabla\dt X \right\rangle_0 - = \langle \partial \gamma, \partial \gamma - Z \rangle_0, + = d E_\gamma X + = 0, \] which implies \(\norm{\partial \gamma - Z}_0^2 = 0\). In other words, \(\partial \gamma = Z \in H^1(\gamma^* TM)\) and therefore \(\frac\nabla\dt @@ -315,11 +314,12 @@ technical lemma, whose proof amounts to an uninspiring exercise in analysis -- see lemma 2.4.6 of \cite{klingenberg}. \begin{lemma}\label{thm:inclusion-submnfds-is-compact} - Let \(\Omega_{p q}^0 M \subset C^0(I, M)\) be the space of curves joining - \(p\) to \(q\). Then the inclusion \(\Omega_{p q} M \longhookrightarrow - \Omega_{p q}^0 M\) is continuous and compact. Likewise, if \(\Lambda^0 M - \subset C^0(I, M)\) is the space of free loops then the inclusion \(\Lambda M - \longhookrightarrow \Lambda^0 M\) is continuous and compact. + Let \(\Omega_{p q}^0 M \subset C^0(I, M)\) be the space of continuous curves + joining \(p\) to \(q\). Then the inclusion \(\Omega_{p q} M + \longhookrightarrow \Omega_{p q}^0 M\) is continuous and compact. Likewise, + if \(M\) is compact and \(\Lambda^0 M \subset C^0(I, M)\) is the space of + continuous free loops then the inclusion \(\Lambda M \longhookrightarrow + \Lambda^0 M\) is continuous and compact. \end{lemma} As a first consequence, we prove\dots @@ -408,9 +408,9 @@ As a first consequence, we prove\dots \cdot \norm{X}_0 \end{equation} - Given a bounded sequence \((X_n)_n \subset \Omega_{p q} M\), it follow from - lemma~\ref{thm:inclusion-submnfds-is-compact} that \((X_n)_n\) - is relatively compact as a \(C^0\)-sequence. From + Given a bounded sequence \((X_n)_n \subset T_\gamma \Omega_{p q} M\), it + follow from lemma~\ref{thm:inclusion-submnfds-is-compact} that \((X_n)_n\) is + relatively compact as a \(C^0\)-sequence. From (\ref{eq:compact-operator-quota}) we then get that \((K_\gamma X_n)_n\) is relatively compact as an \(H^1\)-sequence, as desired. The same argument holds for \(\Lambda M\) if \(M\) is compact -- so that we can once more apply @@ -439,7 +439,8 @@ essential for stating Morse's index theorem. M = \ker A_\gamma\) and \(T_\gamma^+ \Omega_{p q} M\) is the proper Hilbert subspace given by the closure of the subspace spanned by eigenvectors with positive eigenvalues. The same holds for critical points \(\gamma\) of - \(E\!\restriction_{\Lambda M}\) and \(T_\gamma \Lambda M\). + \(E\!\restriction_{\Lambda M}\) and \(T_\gamma \Lambda M\) if \(M\) is + compact. \end{corollary} \begin{definition}\label{def:morse-index} @@ -483,7 +484,7 @@ however, is the following consequence of Morse's theorem. \begin{enumerate} \item If there are no conjugate points of \(\gamma\) then there exists a neighborhood \(U \subset \Omega_{p q} M\) of \(\gamma\) such that - \(E(\eta) > E(\gamma)\) for all \(\eta \in U\) with \(\eta \ne 0\). + \(E(\eta) > E(\gamma)\) for all \(\eta \in U\) with \(\eta \ne \gamma\). \item Let \(k > 0\) be the sum of the multiplicities of the conjugate points of \(\gamma\) in the interior of \(I\). Then there exists an @@ -493,15 +494,15 @@ however, is the following consequence of Morse's theorem. \] of the unit ball \(B^k = \{v \in \RR^k : \norm{v} < 1\}\) with \(i(0) = \gamma\), \(E(i(v)) < E(\gamma)\) and \(\ell(i(v)) < \ell(\gamma)\) for - all \(v \in B^k \setminus \{ 0 \}\). + all nonzero \(v \in B^k\). \end{enumerate} \end{theorem} \begin{proof} First of all notice that given \(\eta \in U_\gamma\) with \(\eta = - \exp_\gamma(X)\), \(X \in H^1(\gamma^* TM)\), the Taylor series for - \(E(\eta)\) is given by \(E(\eta) = E(\gamma) + \frac{1}{2} d^2 E_\gamma(X, - X) + \cdots\). More precisely, + \exp_\gamma(X)\), \(X \in H^1(W_\gamma)\), the Taylor series for \(E(\eta)\) + is given by \(E(\eta) = E(\gamma) + \frac{1}{2} d^2 E_\gamma(X, X) + + \cdots\). More precisely, \begin{equation}\label{eq:energy-taylor-series} \frac{\abs{E(\eta) - E(\gamma) - \frac12 d^2 E_\gamma(X, X)}}{\norm{X}_1^2} \to 0 @@ -510,7 +511,7 @@ however, is the following consequence of Morse's theorem. Let \(\gamma\) be as in \textbf{(i)}. Since \(\gamma\) has no conjugate points, it follows from Morses's index theorem that \(T_\gamma^- \Omega_{p q} - M = 0\). Furthermore, by noting that any piece-wise smooth \(X \in \ker + M = 0\). Furthermore, by noticing that any piece-wise smooth \(X \in \ker A_\gamma\) is Jacobi field vanishing at \(p\) and \(q\) one can also show \(T_\gamma^0 \Omega_{p q} M = 0\). Hence \(T_\gamma \Omega_{p q} M = T_\gamma^+ \Omega_{p q} M\) and therefore \(d^2 E\!\restriction_{\Omega_{p q} @@ -534,16 +535,16 @@ however, is the following consequence of Morse's theorem. = E(\gamma) - \frac{1}{2} \delta^2 \sum_j \lambda_j \cdot v_j + \cdots \] we find that \(E(i(v)) < E(\gamma)\) for sufficiently small \(\delta\). In - particular, \(\ell(i(v)) \le E(i(v))^2 < E(\gamma)^2 = \ell(\gamma)\). + particular, \(\ell(i(v))^2 \le E(i(v)) < E(\gamma) = \ell(\gamma)^2\). \end{proof} We should point out that part \textbf{(i)} of theorem~\ref{thm:jacobi-darboux} is weaker than the classical formulation of the Jacobi-Darboux theorem -- such as in theorem 5.5.3 of \cite{gorodski} for example -- in two aspects. First, we -do not compare the length of curves in question. This could be amended by -showing that the length functional \(\ell : H^1(I, M) \to \RR\) is smooth and -that its Hessian \(d^2 \ell_\gamma\) is given by \(C \cdot d^2 E_\gamma\) for -some \(C > 0\). +do not compare the length of curves \(\gamma\) and \(\eta \in U\). This could +be amended by showing that the length functional \(\ell : H^1(I, M) \to \RR\) +is smooth and that its Hessian \(d^2 \ell_\gamma\) is given by \(C \cdot d^2 +E_\gamma\) for some \(C > 0\). Secondly, unlike the classical formulation we only consider curves in an \(H^1\)-neighborhood of \(\gamma\) -- instead of a neighborhood of \(\gamma\)