-
Notifications
You must be signed in to change notification settings - Fork 0
/
Copy pathsurfaces.tex
843 lines (644 loc) · 33 KB
/
surfaces.tex
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
205
206
207
208
209
210
211
212
213
214
215
216
217
218
219
220
221
222
223
224
225
226
227
228
229
230
231
232
233
234
235
236
237
238
239
240
241
242
243
244
245
246
247
248
249
250
251
252
253
254
255
256
257
258
259
260
261
262
263
264
265
266
267
268
269
270
271
272
273
274
275
276
277
278
279
280
281
282
283
284
285
286
287
288
289
290
291
292
293
294
295
296
297
298
299
300
301
302
303
304
305
306
307
308
309
310
311
312
313
314
315
316
317
318
319
320
321
322
323
324
325
326
327
328
329
330
331
332
333
334
335
336
337
338
339
340
341
342
343
344
345
346
347
348
349
350
351
352
353
354
355
356
357
358
359
360
361
362
363
364
365
366
367
368
369
370
371
372
373
374
375
376
377
378
379
380
381
382
383
384
385
386
387
388
389
390
391
392
393
394
395
396
397
398
399
400
401
402
403
404
405
406
407
408
409
410
411
412
413
414
415
416
417
418
419
420
421
422
423
424
425
426
427
428
429
430
431
432
433
434
435
436
437
438
439
440
441
442
443
444
445
446
447
448
449
450
451
452
453
454
455
456
457
458
459
460
461
462
463
464
465
466
467
468
469
470
471
472
473
474
475
476
477
478
479
480
481
482
483
484
485
486
487
488
489
490
491
492
493
494
495
496
497
498
499
500
501
502
503
504
505
506
507
508
509
510
511
512
513
514
515
516
517
518
519
520
521
522
523
524
525
526
527
528
529
530
531
532
533
534
535
536
537
538
539
540
541
542
543
544
545
546
547
548
549
550
551
552
553
554
555
556
557
558
559
560
561
562
563
564
565
566
567
568
569
570
571
572
573
574
575
576
577
578
579
580
581
582
583
584
585
586
587
588
589
590
591
592
593
594
595
596
597
598
599
600
601
602
603
604
605
606
607
608
609
610
611
612
613
614
615
616
617
618
619
620
621
622
623
624
625
626
627
628
629
630
631
632
633
634
635
636
637
638
639
640
641
642
643
644
645
646
647
648
649
650
651
652
653
654
655
656
657
658
659
660
661
662
663
664
665
666
667
668
669
670
671
672
673
674
675
676
677
678
679
680
681
682
683
684
685
686
687
688
689
690
691
692
693
694
695
696
697
698
699
700
701
702
703
704
705
706
707
708
709
710
711
712
713
714
715
716
717
718
719
720
721
722
723
724
725
726
727
728
729
730
731
732
733
734
735
736
737
738
739
740
741
742
743
744
745
746
747
748
749
750
751
752
753
754
755
756
757
758
759
760
761
762
763
764
765
766
767
768
769
770
771
772
773
774
775
776
777
778
779
780
781
782
783
784
785
786
787
788
789
790
791
792
793
794
795
796
797
798
799
800
801
802
803
804
805
806
807
808
809
810
811
812
813
814
815
816
817
818
819
820
821
822
823
824
825
826
827
828
829
830
831
832
833
834
835
836
837
838
839
840
841
842
843
\csname @openrightfalse\endcsname
\chapter{Surfaces}
We assume that the reader is familiar with smooth surfaces and the related definitions
including intrinsic metric,
geodesics,
convex and saddle surfaces
as well as different types of curvature.
An introductory course in differential geometry should cover all necessary background material
[see \ncite{toponogov-curves-and-surfaces}, \ncite{petrunin-zamora}, or \S28--29 in \ncite{hilbert-cohn-vossen}].
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
{
\begin{wrapfigure}{r}{27 mm}
\vskip4mm
\centering
\includegraphics{mppics/pic-202}
\end{wrapfigure}
\subsection*{Convex hat}
\label{Convex hat}
\begin{pr}
Suppose that a plane $\Pi$ cuts from a smooth closed convex surface $\Sigma$ a disk $\Delta$.
Assume that the reflection of $\Delta$ with respect to $\Pi$ lies inside of $\Sigma$.
Show that $\Delta$ is \index{convex set}\emph{convex} with respect to the intrinsic metric of $\Sigma$;
that is,
if both ends of a minimizing geodesic in $\Sigma$
lie in $\Delta$,
then the entire geodesic lies in $\Delta$.
\end{pr}
}
\parit{Semisolution.}
Assume the contrary,
then there is a minimizing geodesic $\gamma\not\subset\Delta$ with ends $p$ and $q$ in $\Delta$.
Without loss of generality, we may assume that only one arc of $\gamma$ lies outside of $\Delta$.
Reflection of this arc with respect to $\Pi$ together with the remaining part of $\gamma$ forms another curve $\hat\gamma$ from $p$ to $q$;
it runs partly along $\Sigma$
and partly outside $\Sigma$,
but does not get inside $\Sigma$.
Note that
\[\length\hat\gamma=\length\gamma.\]
Denote by $\bar\gamma$ the closest point projection of $\hat\gamma$ on $\Sigma$.
Since $\Sigma$ is convex, the closest point projection decreases the length.
Therefore
the curve $\bar\gamma$ lies in $\Sigma$,
it has the same ends as $\gamma$,
and
\[\length\bar\gamma<\length\gamma.\]
This means that $\gamma$ is not length-minimizing
--- a contradiction.\qeds
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
{
\begin{wrapfigure}{r}{39 mm}
\vskip0mm
\centering
\includegraphics{mppics/pic-204}
\end{wrapfigure}
\subsection*{Involute of geodesic}
\label{Involute of geodesic}
\begin{pr}
Let $\Sigma$ be a smooth closed strictly convex surface
in $\RR^3$
and $\gamma\:[0,\ell]\z\to \Sigma$ a unit-speed minimizing geodesic.
Set $p\z=\gamma(0)$, $q=\gamma(\ell)$, and
$$p_t=\gamma(t)-t\cdot\gamma'(t),$$
where $\gamma'(t)$ denotes the velocity vector of $\gamma$ at~$t$.
\end{pr}
}
\vskip-\medskipamount
\textit{Show that for any $t\in (0,\ell)$,
one {}\emph{cannot see} $q$ from $p_t$;
that is, the line segment $[p_tq]$ intersects $\Sigma$ at a point distinct from $q$.}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Simple geodesic}
\label{Simple geodesic}
\begin{pr}
Let $\Sigma$ be a complete unbounded convex surface in $\mathbb R^3$.
Show that there is a two-sided infinite geodesic in $\Sigma$ with no self-intersections.
\end{pr}
Let us review a couple of statements
about Gauss curvature which might help to solve the problem \cite[see \S28 in][for more details]{hilbert-cohn-vossen}.
If $\Sigma$ is a convex surface in $\RR^3$ then its Gauss curvature is nonnegative.
Assume that a simply-connected region $\Omega$ in the surface $\Sigma$ is bounded by a closed broken geodesic $\gamma$.
Denote by $\kappa(\Omega)$ the integral of the Gauss curvature over $\Omega$.
For any point $p\in\Sigma$ consider the outer unit normal vector $n(p)\z\in\mathbb{S}^2$.
Then
\begin{align*}
\kappa(\Omega)&=\area[n(\Omega)]
\intertext{and by the Gauss--Bonnet formula}
\kappa(\Omega)&=2\cdot\pi-\sigma(\gamma),
\end{align*}
where $\sigma(\gamma)$ denotes the sum of the signed exterior angles of $\gamma$.
In particular, $|\sigma(\gamma)|\le2\cdot\pi$.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Geodesics for birds}
\label{liberman}
The \index{total curvature}\emph{total curvature} of a space curve $\gamma$ is defined as the integral of its curvature.
That is, if a curve $\gamma\:[a,b]\to\RR^3$ has unit speed parametrization,
then its total curvature equals
\[\int\limits_a^b|\gamma''(t)|\cdot dt,\]
the vector $\gamma''(t)$ is called the \index{curvature vector}\emph{curvature vector} and its length $|\gamma''(t)|$ is the \index{curvature}\emph{curvature} of $\gamma$ at time $t$.
The above definition makes sense for $C^{1,1}$ smooth curves,
that is, in the case when $\gamma'(t)$ is locally Lipschitz;
in this case the curvature $|\gamma''(t)|$ is defined almost everywhere.
The \index{geodesic}\emph{geodesics} in the following problem are defined as the curves locally minimizing the length;
that is, any sufficiently short arc of the curve containing a given value of the parameter is length-minimizing.
\begin{pr}
Let $f\:\RR^2\to\RR$ be a smooth $\ell$-Lipschitz function.
Let $W\subset \RR^3$ be the epigraph of $f$;
that is,
$$W=\set{(x,y,z)\in\RR^3}{z\ge f(x,y)}.$$
Equip $W$ with the induced intrinsic metric.
Show that any geodesic in $W$
has total curvature at most $2\cdot\ell$.
\end{pr}
Actually, geodesics in $W$ are $C^{1,1}$-smooth;
in particular, the formula for the total curvature mentioned above makes sense.
This is an easy exercise in real analysis which can be also taken for granted.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Immersed surface}
\label{Immersed surface}
\begin{pr}
Let $\Sigma$ be a smooth connected immersed surface in $\RR^3$ with strictly positive Gauss curvature and nonempty boundary $\partial\Sigma$.
Assume that the boundary $\partial\Sigma$ lies in a plane $\Pi$
and $\Sigma$ lies entirely on one side of~$\Pi$.
Prove that $\Sigma$ is an embedded disk.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Periodic asymptote}
\label{Asymptotic geodesic}
\begin{pr}
Let $\Sigma$ be a closed smooth surface with non-positive curvature at every point
and $\gamma$ a geodesic in $\Sigma$.
Assume that $\gamma$ is not periodic
and the curvature of $\Sigma$ vanishes at every point of $\gamma$.
Show that $\gamma$ does not have a periodic asymptote;
that is, there is no periodic geodesic $\delta$ such that the distance from $\gamma(t)$ to $\delta$ converges to $0$ as $t\to\infty$.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Saddle surface}
\label{Saddle surface}
Recall that a smooth surface $\Sigma$ in $\RR^3$
is \index{saddle surface}\emph{saddle} at a point $p$ if its principal curvatures at $p$ have opposite signs.
We say that $\Sigma$ is {}\emph{saddle} if it is saddle at all points.
\begin{pr}
Let $\Sigma$ be a saddle surface in $\RR^3$
homeomorphic to a disk.
Assume that the orthogonal projection to the $(x,y)$-plane
maps the boundary of $\Sigma$
injectively to a convex closed curve.
Show that this projection is injective on~$\Sigma$.
In particular, $\Sigma$ is the graph $z=f(x,y)$ of a function $f$ defined on a convex domain in the $(x,y)$-plane.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Asymptotic line}
\label{asymptotic-line}
The saddle surfaces are defined in the previous problem.
Recall that a smooth curve $\gamma$ on a smooth surface $\Sigma\subset \RR^3$ is called \index{asymptotic line}\emph{asymptotic} if $\gamma''(t)$ is tangent to the surface at $\gamma(t)$ for any $t$.
\begin{pr}
Let $\Sigma\subset \RR^3$ be the graph $z\z=f(x,y)$
of a smooth function $f$
and $\gamma$ a closed smooth asymptotic line in $\Sigma$.
Assume that $\Sigma$ is saddle in a neighborhood of $\gamma$.
Show that the projection of $\gamma$ to the $(x, y)$-plane cannot be star-shaped;
that is, there is no point $p$ in the plane such that each half-line from $p$ intersects the projection at exactly one point.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Minimal surface}
\label{min-surf}
Recall that a smooth surface in $\RR^3$ is called \index{minimal surface}\emph{minimal} if its mean curvature vanishes at all points.
The \index{mean curvature}\emph{mean curvature} at each point is defined as the sum of the principal curvatures at that point.
\begin{pr}
Let $\Sigma$ be a minimal surface in $\RR^3$ having its boundary on a unit sphere.
Assume that $\Sigma$ passes thru the center of the sphere.
Show that the area of $\Sigma$ is at least $\pi$.
\end{pr}
{
\begin{wrapfigure}[3]{r}{43 mm}
\vskip-4mm
\centering
\includegraphics{asy/gutter}
\end{wrapfigure}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Round gutter\hard}
\label{half-torus}
A round gutter is the surface shown on the picture.
}
More precisely, consider the torus $T$; a surface generated by revolving a circle in $\RR^3$ around an axis coplanar with the circle.
Let $\gamma\z\subset T$ be one of the circles in $T$ that locally separates positive and negative curvature on $T$;
a plane containing $\gamma$ is tangent to $T$ at all points of $\gamma$.
Then a neighborhood of $\gamma$ in $T$ is called
a \index{gutter}\emph{round gutter}
and the circle $\gamma$ is called its {}\emph{main latitude}.
\begin{pr}
Let $\Omega\subset \RR^3$ be a round gutter with the main latitude $\gamma$.
Assume that $\iota\:\Omega\z\to\RR^3$
is a smooth length-preserving embedding that is sufficiently close to the identity.
Show that $\gamma$ and $\iota(\gamma)$ are congruent;
that is, there is an isometric motion of $\RR^3$ sending $\gamma$ to $\iota(\gamma)$
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Non-contractible geodesics}
\label{torus}
\begin{pr}
Give an example of a non-flat metric
on the $2$-torus such that no closed geodesic is contractible.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Two disks}
\label{Two disks}
\begin{pr}
Let $\Sigma_1$ and $\Sigma_2$ be two smoothly embedded open disks in $\mathbb R^3$
that have a common closed smooth curve $\gamma$.
Show that there is a pair of points $p_1\in \Sigma_1$ and $p_2\in \Sigma_2$ with parallel tangent planes.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\subsection*{Second derivative bounds first\easy}
\label{Second derivative bounds first}
\begin{pr}
Let $f$ be a smooth function on the Lobachevsky plane with bounded Hessian.
Show that $f$ is Lipschitz.
\end{pr}
\section*{Semisolutions}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Involute of geodesic.}
Let $W$ be the closed unbounded set formed by $\Sigma$ and its exterior points.
Choose $t\in (0,\ell)$;
denote by $\gamma_t$ the concatenation of the line segment $[p_t\gamma(t)]$ and the arc $\gamma|_{[t,\ell]}$.
The key step is to show the following:
\begin{cl}{$({*})$} The curve $\gamma_t$ is a minimizing geodesic in the intrinsic metric induced on $W$.
\end{cl}
Try to prove it before reading further.
\medskip
Let $\Pi_t$ be the tangent plane to $\Sigma$ at $\gamma(t)$.
Consider the curve $\alpha(t)=p_t$.
Note that
$\alpha(t)\z\in\Pi_t$,
$\alpha'(t)\perp\Pi_t$,
and $\alpha'(t)$ points to the side of $\Pi_t$ opposite to $\Sigma$.
It follows that for any $x\in\Sigma$ the function
\[t\mapsto |x - p_t|
\quad\text{and, therefore,}\quad
t\mapsto |x - p_t|_W\] are non-decreasing;
here $|x - p_t|_W$ stands for the intrinsic distance from $x$ to $p_t$ in $W$.
\begin{wrapfigure}{r}{43 mm}
\vskip-6mm
\centering
\includegraphics{mppics/pic-205}
\end{wrapfigure}
On the other hand, by construction
\[|q - p_t|_W\le |q - p|_\Sigma;\]
therefore, from the above
\[|q - p_t|_W= |q - p|_\Sigma\]
for any $t$.
Hence $(*)$ follows.
Now assume that $q$ is visible from $p_t$ for some $t$;
that is, the line segment $[qp_t]$ intersects $\Sigma$ only at $q$.
From the above,
$\gamma_t$ coincides with the line segment $[qp_t]$.
On the other hand, $\gamma_t$ contains $\gamma(t)\in\Sigma$ --- a contradiction.\qeds
This problem is based on an observation used by Anatoliy Milka in the proof of the following generalization of the comparison theorem for convex surfaces \cite[Theorem 2]{milka-geod}.
\begin{pr}
Let $W$ be the closed unbounded set formed by a (not necessarily smooth) closed convex surface $\Sigma$ and its exterior points.
Suppose $\gamma_1\:[0,\ell_1]\to \Sigma$ and $\gamma_2\:[0,\ell_2]\to \Sigma$ are unit-speed minimizing geodesics that start at the same point $p$.
Set $x_i=\gamma_i(\ell_i)$ and $y_i=p+\ell_i\cdot\gamma_i'(0)$.
Show that
\[|x_1-x_2|_W\le |y_1-y_2|_W,\]
where $|\ - \ |_W$ stands for the intrinsic distance in $W$.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\begin{wrapfigure}{r}{43 mm}
\vskip-0mm
\centering
\includegraphics{mppics/pic-206}
\end{wrapfigure}
\parbf{Simple geodesic.}
Look at two combinatorial types of a self-intersection shown in the diagram.
One of them can and the other cannot appear as self-intersections of a geodesic on an unbounded convex surface.
Try to determine which is which before reading further.
\medskip
Let $\gamma$ be a two-sided infinite geodesic in $\Sigma$.
The following is the key statement in the proof.
\begin{cl}{$({*})$}
The geodesic $\gamma$ contains at most one simple loop.
\end{cl}
To prove $({*})$, we use the following observation.
\begin{cl}{$({*}{*})$}
The integral curvature $\omega$ of $\Sigma$ cannot exceed $2\cdot\pi$.
\end{cl}
Indeed, since $\Sigma$ is unbounded and convex,
it surrounds a half-line.
Consider a coordinate system with this half-line as the positive half of its $z$-axis.
In these coordinates, the surface $\Sigma$ is described as a graph $z=f(x,y)$ of a convex function $f$.
In particular, all outer normal vectors to $\Sigma$ have a negative $z$-coordinate;
in other words, they point to the southern hemisphere.
Therefore the area of the spherical image of $\Sigma$ is at most $2\cdot\pi$.
The area of this image is the integral of the Gauss curvature over $\Sigma$.
Hence $({*}{*})$ follows.
From the Gauss--Bonnet formula, we get the following conclusion.
If $\phi$ is the angle at the base of a simple geodesic loop then the integral curvature surrounded by the loop equals $\pi+\phi$.
In particular, $({*}{*})$ implies that $\phi\le\pi$; in other words, there are no \emph{concave loops}.
Now assume that $({*})$ does not hold, so that a geodesic has two simple loops.
Note that the disks bounded by the loops have to overlap,
otherwise the curvature of $\Sigma$ would exceed $2\cdot\pi$.
But if they overlap, then it is easy to show that the curve also contains a concave loop,
which contradicts the above observation.%
\footnote{This observation implies that the right picture on the above diagram cannot be realized by a geodesic.}
If a geodesic $\gamma$ has a self-intersection,
then it contains a simple loop.
From $({*})$, there is only one such loop;
it cuts a disk from $\Sigma$
and goes around it either clockwise or counterclockwise.
This way we divide all the self-intersecting geodesics
into two sets which we will call {}\emph{clockwise} and {}\emph{counterclockwise}.
Note that the geodesic $t\mapsto \gamma(t)$ is clockwise
if and only if
$t\z\mapsto \gamma(-t)$
is counterclockwise.
The sets of clockwise and counterclockwise are open and the space of all geodesics is connected.
It follows that there are geodesics that aren't clockwise nor counterclockwise.
Those geodesics have no self-intersections.\qeds
Note that the proof implies that a two-sided infinite geodesic can be found among geodesics containing a given point in $\Sigma$.
The problem is due to Stephan Cohn-Vossen \cite[Satz 9 in][]{convossen};
generalizations were obtained by
Vladimir Streltsov and Alexandr Alexandrov
\cite{streltsov-alexandrov}
and
by Victor Bangert \cite{bangert}.
The following problem is of the same style \cite{petrunin-self-crossing-geodesics}.
\begin{pr}
Let $\gamma$ be a closed geodesic on a closed surface of positive curvature $\Sigma$.
\begin{figure}[ht!]
\vskip-0mm
\centering
\includegraphics{mppics/pic-207}
\end{figure}
Show that $\gamma$ cannot look like one of the curves on the diagram.
In other words, $\gamma$ cannot subdivide $\Sigma$ into (1) one hexagon, one triangle, and three monogons, and (2) one pentagon, one quadrangle, and three monogons.
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Geodesics for birds.}
Choose a unit-speed geodesic in $W$, say
\[\gamma\:t\mapsto(x(t),y(t),z(t)).\]
We can assume that $\gamma$ is defined on a closed interval $[a,b]$.
The key step is to show the following:
\begin{cl}{$({*})$}
The function $t\mapsto z$ is concave.
\end{cl}
Parametrize the plane curve $t\mapsto (x(t),y(t))$ by the arc length $s$
and reparametrize $\gamma$ by $s$.
\begin{wrapfigure}{o}{35 mm}
\vskip-0mm
\centering
\includegraphics{mppics/pic-208}
\end{wrapfigure}
Note that the function $s\mapsto z$ is concave.
Indeed, suppose $s\mapsto z$ is not concave around $s_0$.
Then one could shorten $\gamma$ by increasing its $z$ component in a small interval around $s_0$ while keeping its endpoints fixed.
After the deformation, the curve still lies in $W$.
The latter contradicts that $\gamma$ is locally length-minimizing.
Finally, note that the concavity of $s\mapsto z$ is equivalent to the concavity of $t\mapsto z$.
Hence $({*})$ follows.
Since $f$ is smooth,
the curve $\gamma(t)$ is $C^{1,1}$;
that is, its first derivative $\gamma'(t)$ is a well-defined Lipschitz function.
It follows that its second derivative $\gamma''(t)$ is defined almost everywhere.
Since $z(t)$ is concave, we have $z''(t)\le 0$.
Since $f$ is $\ell$-Lipschitz, $z(t)$ is $\tfrac{\ell}{\sqrt{1+\ell^2}}$-Lipschitz.
It follows that
\[\int\limits_a^b |z''(t)|\cdot dt\le 2\cdot\tfrac{\ell}{\sqrt{1+\ell^2}}.\]
The curvature vector $\gamma''(t)$ is perpendicular to the surface.
Since the surface has slope at most $\ell$,
we get
\[|\gamma''(t)|\le |z''(t)|\cdot\sqrt{1+\ell^2}.\]
Hence
\[\int\limits_a^b |\gamma''(t)|\cdot dt\le 2\cdot\ell.\qedsin\]
\medskip
The statement holds for general $\ell$-Lischitz functions,
not necessarily smooth.
The given bound is optimal, the equality is attained by a two-side infinite geodesic on the graph of
\[f(x,y)=-\ell\cdot\sqrt{x^2+y^2}.\]
The problem is due to David Berg \cite{berg},
the same bound for convex $\ell$-Lipschitz surfaces was proved earlier by Vladimir Usov \cite{usov}.
The observation $({*})$
is called \index{Liberman’s lemma}\emph{Liberman’s lemma};
it was used earlier
to bound the total curvature
of a geodesic on a convex surface \cite{liberman}.\footnote{It is a part of the thesis of Joseph Liberman, defended a couple of months before he died in WWII.}
This lemma is often useful when working with geodesics on general convex surfaces.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Immersed surface.}
Let $\ell$ be a linear function that vanishes on $\Pi$
and is positive on $\Sigma$.
We will apply a Morse-type argument for the restriction of $\ell$ to $\Sigma$.
\medskip
Let $z_0$ be a maximum of $\ell$ on $\Sigma$;
set $s_0=\ell(z_0)$.
Given $s<s_0$, denote by $\Sigma_s$ the connected component of $z_0$ in $\Sigma\cap\ell^{-1}([s,s_0])$.
Note that
\begin{itemize}
\item $\Sigma_s$ is an embedded disk, and
\item $\partial\Sigma_s$ is a convex plane curve
\end{itemize}
for all $s$ sufficiently close to $s_0$.
Consider the set $A\subset [0,s_0)$ such that for any $a\in A$ these two conditions hold for any $s\in [a,s_0)$.
Observe that $A$ is open and closed in $[0,s_0)$.
Whence $A=[0,s_0)$; in particular, these conditions hold for $s=0$.
Since $\Sigma$ is connected, $\Sigma_0=\Sigma$.
Hence the result follows.\qeds
This problem is discussed in the lectures of Mikhael Gromov \cite[see \S$\tfrac12$~in][]{gromov-SGMC}.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Periodic asymptote.}
Arguing by contradiction, assume that there is a geodesic $\gamma$ on the surface $\Sigma$ with a periodic asymptote $\delta$.
Passing to a finite cover of $\Sigma$, we can ensure that the asymptote has no self-intersections.
In this case,
the restriction $\gamma|_{[a,\infty)}$
has no self-intersections
if $a$ is sufficiently large.
Cut $\Sigma$ along $\gamma([a,\infty))$ and then cut from the obtained surface an infinite triangle $\triangle$.
The triangle has two sides formed by both sides of cuts along $\gamma$;
let us denote these sides of $\triangle$ by $\gamma_-$ and $\gamma_+$.
Note that
\[\area\triangle<\area \Sigma<\infty,
\leqno(*)\]
and both sides $\gamma_\pm$
are infinite minimizing geodesics in $\triangle$.
Consider the Busemann function $f$ for $\gamma_+$ [defined on page~\pageref{page:Busemann function}];
denote by $\ell(t)$ the length of the level curve $f^{-1}(t)$.
Let $-\kappa(t)$ be the total curvature of the sup-level set $f^{-1}([t,\infty))$.
From the Gauss--Bonnet formula,
\[\ell'(t)=\kappa(t).\leqno({*}{*})\]
The level curve $f^{-1}(t)$ can be parametrized by a unit-speed curve, say $\theta_t\:[0,\ell(t)]\to \triangle$.
By the coarea formula we have
\[\kappa'(t)
=
-\int\limits_0^{\ell(t)} K_{\theta_t(\tau)}\cdot d\tau,
\]
where $K_x$ denotes the Gauss curvature of $\Sigma$ at the point $x$.
Since $K_{\theta_t(0)}\z=K_{\theta_t(\ell_t)}=0$ and the surface is smooth,
there is a constant $C$ such that $|K_{\theta_t(\tau)}|\le C\cdot \ell(t)^2$ for all $t$, $\tau$.
Therefore
\[\kappa'(t)\le C\cdot \ell(t)^3 \leqno(\asterism)\]
Together, $({*}{*})$ and $(\asterism)$ imply that there is $\eps>0$ such that
\[\ell(t)\ge \frac\eps{t-a}\]
for sufficiently large $t$.
By the coarea formula we get
\[\area\triangle=\int\limits_a^\infty\ell(t)\cdot dt=\infty;\]
the latter contradicts $(*)$.\qeds
I learned the problem from
Dmitri Burago
and Sergei Ivanov,
it originated from a discussion with
Keith Burns,
Michael Brin,
and Yakov Pesin.
Here is a motivation.
Let $\Sigma$ be a closed surface with non-positive curvature that is not flat.
The space $\Gamma$ of all unit-speed geodesics $\gamma\:\RR\z\to\Sigma$ can be identified with the unit tangent bundle $\UU\Sigma$.
In particular $\Gamma$ comes with a natural choice of measure.
Denote by $\Gamma_0\subset \Gamma$ the set of geodesics that run in the set of zero curvature all the time.
It is expected that $\Gamma_0$ has a vanishing measure.
In all known examples $\Gamma_0$ contains only periodic geodesics in only finitely many homotopy classes \cite[see also][]{hertz}.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Saddle surface.}
Denote by $\Sigma^\circ$ the interior of $\Sigma$.
Choose a plane $\Pi$.
Note that the intersection $\Pi\cap \Sigma^\circ$
locally looks either like a curve or like two curves intersecting transversally;
in the latter case, $\Pi$ is tangent to $\Sigma^\circ$ at the intersection point.
Further, note that $\Pi\cap \Sigma^\circ$ has no cycle.
Otherwise, $\Sigma$ would fail to be saddle at the point of the disk surrounded by that cycle maximizing the distance to $\Pi$.
If $\Sigma$ is not a graph then there is a point $p\in\Sigma$ with a vertical tangent plane;
denote this plane by $\Pi$.
The intersection $\Pi\cap\Sigma$ has a cross-point at~$p$.
Since the boundary of $\Sigma$ projects injectively to a closed convex curve in $(x,y)$-plane,
the intersection of $\Pi\cap\partial \Sigma$ has at most 2 points --- these are the only endpoints of $\Pi\cap\Sigma$.
It follows that the connected component of $p$ in $\Pi\cap\Sigma$ is a tree
with a vertex of degree 4 at $p$ and at most two end-points --- a contradiction.\qeds
The described idea can be used to prove the result of Richard Schoen and Shing-Tung Yau \cite{schoen-yau-2D} which gives a sufficient condition for a harmonic map between surfaces to be a diffeomorphism.
Unlike the original proof, it requires no calculations.
The proof above is based on the observation
that for any saddle surface $\Sigma$ and plane $\Pi$,
each connected component of $\Sigma\setminus \Pi$ is either unbounded or intersects the boundary curve.
This observation plays a central role in the proof of Sergei Bernstein \cite{bernshtein}
of the following problem:
\begin{pr}
Show that a smooth bounded function $f\:\RR^2\to\RR$ cannot have a strictly saddle graph.
\end{pr}
One could go further and define a \emph{generalized saddle surface} as an arbitrary (non-necessarily smooth) surface satisfying the observation above.
The geometry of these surfaces is far from being understood,
Samuil Shefel has a number of beautiful results about them,
\cite[see][and the references therein]{shefel, AKP-invitation}.
The statement of the problem holds for these generalized saddle surfaces, but
the proof is tricky \cite{petrunin-stadler}.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Asymptotic line.}
Denote by $\Pi_t$ the tangent plane to $\Sigma$ at $\gamma(t)$ and by $\ell_t$ the tangent line of $\gamma$ at time $t$.
Since $\gamma$ is asymptotic, the plane $\Pi_t$ rotates around $\ell_t$ as $t$ changes.
Since $\Sigma$ is saddle, the speed of rotation cannot vanish.%
\footnote{By the Beltrami--Enneper theorem, if $\gamma$ has unit speed, then the speed of rotation is $\pm\sqrt{-K}$, where $K$ is the Gauss curvature which cannot vanish on a saddle surface.}
Note that $\Pi_t$ is a graph of a linear function, say $h_t$, defined on the $(x, y)$-plane.
Denote by $\bar\ell_t$ the projection of $\ell_t$ to the $(x, y)$-plane.
The described rotation of $\Pi_t$ can be expressed algebraically:
the derivative $\tfrac{d}{dt}h_t(w)$ vanishes at the point $w$ if and only if $w\in \bar\ell_t$
and the derivative changes sign if $w$ changes the side of $\bar\ell_t$.
Denote by $\bar\gamma$ the projection of $\gamma$ to the $(x, y)$-plane.
If $\bar\gamma$ is star-shaped with respect to a point $w$, then $w$ cannot cross $\bar\ell_t$.
Therefore the function $t\mapsto h_t(w)$ is monotone on $\SSS^1$.
Observing that this function cannot be constant, we arrive at a contradiction.\qeds
This is a stripped version of Kovaleva's theorem \cite{kovaleva}, which was rediscovered by Dmitri Panov \cite{panov-curves,arnold}.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Minimal surface.}
Without loss of generality, we may assume that the sphere is centered at the origin of $\RR^3$.
Let $h$ be the restriction of the function $x\mapsto \tfrac12\cdot|x|^2$ to the surface $\Sigma$.
Direct calculations show that $\Delta_\Sigma h = 2$;
here $\Delta_\Sigma$ denoted Laplacian on $\Sigma$.
Applying the divergence theorem for the gradient $\nabla_\Sigma h$
in $\Sigma_r\z=\Sigma\cap B(0,r)$, we get
\[2\cdot \area\Sigma_r\le r\cdot\length [\partial\Sigma_r].\]
Set $a(r)=\area\Sigma_r$.
By the coarea formula, $a'(r)\ge\length [\partial\Sigma_r]$ for almost all $r$.
Therefore the function
\[f\:r\mapsto \frac{\area\Sigma_r}{r^2}
\]
is non-decreasing in the interval $(0,1)$.
Since $f(r)\to \pi$ as $r\to0$, the result follows.\qeds
We described a partial case of the so-called \index{monotonicity formula}\emph{monotonicity formula} for minimal surfaces.
The same argument shows that if $0$ is a double point
of $\Sigma$ then $\area\Sigma\z\ge 2\cdot \pi$.
This observation was used to prove
that the minimal disk bounded by a simple closed curve with total curvature $\le 4\cdot\pi$
is necessarily embedded.
It was proved by
Tobias Ekholm,
Brian White,
and Daniel Wienholtz
\cite{EWW};
an amusing variation of this proof
was obtained by
Stephan Stadler \cite{stadler-FM}.
This result also implies that any embedded circle of total curvature at most $4\cdot\pi$ is unknot.
The latter was proved independently by Istv{\'a}n F{\'a}ry \cite{fary-knot} and John Milnor \cite{milnor}.
Note that if we assume in addition that the surface is a disk,
then the statement holds for any saddle surface.
Indeed, denote by $S_r$ the sphere of radius $r$ concentrical with the unit sphere.
Then according to the problem ``A curve on a sphere'' [page \pageref{A curve in a sphere}],
\[\length[\partial\Sigma_r]\ge 2\cdot\pi\cdot r.\]
Then by the coarea formula, we get $\area\Sigma\ge \pi$.
On the other hand, there are saddle surfaces homeomorphic to the cylinder
having an arbitrarily small area in the ball.
If $\Sigma$ does not pass thru the center
and we only know the distance, say $r$,
from the center to $\Sigma$,
then the optimal bound is $\pi\cdot(1-r^2)$.
This question was open for about 40 years and proved by Simon Brendle and Pei-Ken Hung \cite{brende-hung};
their proof is based on a similar idea and is quite elementary.
Earlier Herbert Alexander,
David Hoffman,
and Robert Osserman
proved it for two cases: (1) for disks and (2) for arbitrary area minimizing surfaces, any dimension and codimension
\cite{alexander-osserman,alexander-hoffman-osserman}.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Round gutter.}
Without loss of generality, we can assume that the length of $\gamma$ is $2{\cdot}\pi$ and its intrinsic curvature is $1$ at all points.
Let $K$ be the convex hull of $\hat\Omega=\iota(\Omega)$.
Part of $\hat\Omega$ touches the boundary of $K$ and the rest lies in the interior of $K$.
Denote by $\hat\gamma$ the curve in $\hat\Omega$ dividing these two parts.
First note that the Gauss curvature of $\hat\Omega$ should vanish at the points of $\hat\gamma$;
in other words, $\hat\gamma=\iota(\gamma)$.
Indeed, since $\hat\gamma$ lies on the convex part,
the Gauss curvature at the points of $\hat\gamma$ should be non-negative.
On the other hand, $\hat\gamma$ bounds a flat disk in $\partial K$;
therefore its integral intrinsic curvature should be $2{\cdot}\pi$.
If the Gauss curvature is positive at a point of $\hat\gamma$,
then by the Gauss--Bonnet formula, the total intrinsic curvature of $\hat\gamma$ should be smaller than $2{\cdot}\pi$ --- a contradiction.
On the other hand, $\hat\gamma$ is an asymptotic line.
Indeed, if the direction of $\hat\gamma$ is not asymptotic at $t_0$,
then $\hat\gamma(t_0 \pm\eps)$ lies the interior of $K$ for some small $\eps>0$ --- a contradiction.
Therefore, as the space curve,
$\hat\gamma$ has to be a closed curve with constant curvature $1$.
Any such curve is congruent to a unit circle.\qeds
It is not known whether $\hat\Omega$ is congruent to $\Omega$ or not.
The solution presented above is based on my answer
to the question of Joseph O'Rourke \cite{rourke}.
Here are some related statements.
\begin{itemize}
\item A gutter is second-order rigid;
this was proved by Eduard Rembs
[see \ncite{rembs} and also page 135 in \ncite{efimov}].
\item Any second-order rigid surface does not admit analytic deformation
[proved by Nikolay Efimov; page 121 in \ncite{efimov}]
and for the surfaces of revolution, the assumption of analyticity can be removed
\cite[proved by Idzhad Sabitov, see][]{sabitov}.
\end{itemize}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Non-contractible geodesics.}
A torus of revolution is an example.
Indeed, it has a family of {}\emph{meridians} --- a family of circles that form closed geodesics.
Note that a geodesic on the torus is either a meridian
or it intersects meridians transversally.
In the latter case, all the meridians are crossed by the geodesic in the same direction.
Note that a contractible curve has to cross each meridian an equal number of times in both directions.
Therefore no geodesic of the torus is contractible.\qeds
I learned this problem
from the book of Mikhael Gromov \cite{gromov-MetStr},
where it is attributed to Y. Colin de Verdi\`ere.
The same argument can be used to show that a torus with a geodesic foliation has no contractible closed geodesics.
I do not know other examples of that type \cite{petrunin-torus}; namely, the following question is open:
\begin{pr}
Are there examples of Riemannian metrics on the 2-torus without closed null-homotopic geodesics and without a geodesic foliation?
\end{pr}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\parbf{Two disks.}
Choose a continuous map $h\:\Sigma_1\to \Sigma_2$
that is the identity on~$\gamma$.
Let us prove that for some $p_1\in \Sigma_1$ and $p_2=h(p_1)\in \Sigma_2$,
the tangent planes $\T_{p_1} \Sigma_1$ and $\T_{p_2} \Sigma_2$ are parallel;
this fact is stronger than the one required.
\medskip
Arguing by contradiction,
assume that such a point does not exist.
Then for each $p\in\Sigma_1$
there is a unique line $\ell_p\ni p$
parallel to both $\T_{p} \Sigma_1$ and $\T_{h(p)} \Sigma_2$.
Note that the lines $\ell_p$ form a tangent line distribution over $\Sigma_1$
and $\ell_p$ is tangent to $\gamma$ at all $p\in\gamma$.
Let $\Delta$ be the disk in $\Sigma_1$ bounded by $\gamma$.
Consider the doubling of $\Delta$ along $\gamma$;
it is diffeomorphic to $\mathbb S^2$.
The line distribution $\ell$ lifts to a line distribution on the doubling.
The latter contradicts the hairy ball theorem.\qeds
This proof was suggested nearly simultaneously
by Steven Sivek
and Damiano Testa \cite{two-disks}.
Note that the same proof works when $\Sigma_i$ are oriented open surfaces and $\gamma$ cuts a compact domain in each $\Sigma_i$.
There are examples of three disks $\Sigma_1$, $\Sigma_2$, and $\Sigma_3$
with a common closed curve $\gamma$ such that there is
no triple of points $p_i\in\Sigma_i$ with parallel tangent planes.
Such examples can be found among ruled surfaces \cite{three-disks}.
\parbf{Second derivative bounds first.}
Observe that the gradient $v=\nabla f$ is almost parallel;
that is, there is a constant $C$ such that $|\nabla_u v|\le C$ for any unit tangent vector $u$.
In particular, the parallel translation of $v(p)$ around a circle has to be close to $v(p)$.
If $|v(p)|$ is large, the latter contradicts the Gauss--Bonnet formula.
\medskip
I learned this problem from Christopher Criscitiello \cite{ccriscitiello}.