I am studying Riemannian Geometry in my own. And I was going through the proof of Hopf Rinow from the book of Carmo . I have a few doubts if one could help.
In one side it has been proved that if $exp_p$ is defined on all of $T_pM$ then there exists a length minimizing geodesics between $p$ and $q$. Since geodesics are locally length minimizing by definition, I am not clear how to get exactly the idea how far it minimizes.
In this direction of the proof which is essentially same in this pdf https://www.mathi.uni-heidelberg.de/~lee/Sven05.pdf
where we are exactly using the assumption that $exp_p$ is defined on all of $T_pM$?
- Here in the proof we are taking $x_0=exp_p(\delta v)$ and I guess it's coming from the fact that every geodesics starting from $p$ in normal nbd of the from $ exp_p(sv)$ for some unit tangent vector in $T_pM$.
However in Prop.5.11 of Lee's book in normal nbd geodesics from $p$ is given by $\gamma_V(t)=(tV^1,..,tV^n)$ . So I am very much confused about what is exactly the expression of geodesics starting from the point $p$ in normal neighborhoods .
Any help would definitely help my understanding in the subject.