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<article xmlns:xlink="http://www.w3.org/1999/xlink">
  <front>
    <journal-meta />
    <article-meta>
      <title-group>
        <article-title>The Schouten Curvature for a Nonholonomic Distribution in Sub-Riemannian Geometry and Jacobi Fields</article-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author">
          <string-name>Victor R. Krym</string-name>
          <email>vkrym12@rambler.ru</email>
          <xref ref-type="aff" rid="aff0">0</xref>
        </contrib>
        <aff id="aff0">
          <label>0</label>
          <institution>DAMTP, Centre for Mathematical Sciences</institution>
          ,
          <addr-line>Wilberforce Road, Cambridge CB3 0WA</addr-line>
          ,
          <country country="UK">United Kingdom</country>
        </aff>
      </contrib-group>
      <fpage>213</fpage>
      <lpage>227</lpage>
      <abstract>
        <p>The paper shows that if the distribution is de ned on a manifold with the special smooth structure and does not depend on the vertical coordinates, then the Schouten curvature tensor coincides with the Riemannian curvature tensor. The Schouten curvature tensor is used to write the Jacobi equation for the distribution. This leads to studies on second-order optimality conditions for the horizontal geodesics in subRiemannian geometry. Conjugate points are de ned by the solutions of the Jacobi equation. If a geodesic passed a point conjugated with its beginning then this geodesic ceases to be optimal.</p>
      </abstract>
      <kwd-group>
        <kwd>Sub-Riemannian geometry</kwd>
        <kwd>Schouten curvature</kwd>
        <kwd>Jacobi</kwd>
        <kwd>elds</kwd>
        <kwd>Nonholonomic distributions</kwd>
      </kwd-group>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>-</title>
      <p>Distribution on a smooth manifold N is a family of subspaces A(x) TxN ,
x 2 N . General theory of the variational calculus with nonholonomic restrictions
'(t; x; x_ ) = 0 was published by G.A. Bliss [2]. If the restrictions are linear for
velocities, !x(x_ ) = 0, where ! is a 1-form, we get distributions [25, 26].</p>
      <p>The Romanian mathematician Vranceanu rst introduced the term of the
nonholonomic structure on a Riemannian manifold in 1928 [27]. The Dutch
mathematician Schouten de ned the connection and appropriate curvature
tensor for horizontal vector elds on a distribution in [23, 22]. The soviet
geometrician Vagner extended this construction and built the general curvature tensor
compatible with the Schouten tensor satisfying common requirements for the
curvature in 1937, Kazan [24]. These results were published by Gorbatenko,
Tomsk, in 1985 [6] with modern notations.</p>
      <p>The Schouten curvature tensor is di erent from the Riemannian curvature.
In this paper we prove that if the distribution is de ned on a manifold with the
Copyright c by the paper's authors. Copying permitted for private and academic purposes.</p>
      <p>In: S. Belim et al. (eds.): OPTA-SCL 2018, Omsk, Russia, published at http://ceur-ws.org
special smooth structure and does not depend on the \vertical" coordinates then
these two tensors are identical. This curvature tensor is necessary to write the
Jacobi equation for a distribution.</p>
      <p>We study also second-order optimality conditions for the horizontal geodesics
in sub-Riemannian geometry. If a geodesic passed a point conjugated with its
beginning then this geodesic ceases to be optimal. Conjugate points are de ned
by means of the solutions of the Jacobi equation. In this paper we discuss several
examples of conjugate points in sub-Riemannian geometry.
2</p>
    </sec>
    <sec id="sec-2">
      <title>Variations and Equations of Variations</title>
      <p>Let : [t0; T ] ! N be a C1-smooth horizontal path, !( 0) = 0, where ! is a
1form. Horizontal variation of is a 1-parametric family of maps ( ; ) : [t1; t2] !
N , j j &lt; ", if there are continuous vector elds X = @@t , Y = @@ , the central
line is just (t; 0) = (t) and the eld X is horizontal, X(t; ) 2 A( (t; )) and
n
X !
k=1</p>
      <p>
        j;k=1
= m+1; : : :; n:
(
        <xref ref-type="bibr" rid="ref1">1</xref>
        )
The vector eld Y ( ; 0) along is denoted as Y . These equations are of the form
(Y 0; Y ) = 0, = m+1; : : :; n. This is a system of n m di erential equations.
Since the rank of the matrix (!k ) is n m, the horizontal projection of the
eld Y is arbitrary and the vertical components Y are de ned by the initial
conditions.
3
3.1
      </p>
    </sec>
    <sec id="sec-3">
      <title>The Accessory Problem of G.A. Bliss (Example)</title>
      <p>The Lagrange Problem
Let us consider the 2-dimensional distribution A on R3 de ned by the 1-form
! = x2dx1 + dx3. The energy functional is J (x( )) = 12 R0T (x_ 1)2 + (x_ 2)2 dt, the
metric tensor for this distribution is the identity matrix. The Lagrangian of the
variational problem is L = 12 (x_ 1)2 + (x_ 2)2 + l!( 0). The horizontal geodesics
starting from the origin in R3 for l 6= 0 are
8 x1(t) = 1l
&gt;
&gt;&gt;&gt; x2(t) = 1l v1
&lt;
&gt;
&gt;
&gt;
&gt;
:
v2 + v2 cos lt + v1 sin lt ;</p>
      <p>v1 cos lt + v2 sin lt ;
+2v1v2 cos 2lt + (v12</p>
      <p>
        v22) sin 2lt :
x3(t) = 41l2 2lt(v12 + v22) + 2v1v2
4v1v2 cos lt
4v12 sin lt+
(
        <xref ref-type="bibr" rid="ref2">2</xref>
        )
Note that x_ 1(0) = v1 and x_ 2(0) = v2. These geodesics are shown at Fig. 1 for
(
        <xref ref-type="bibr" rid="ref3">3</xref>
        )
l = 1. These geodesics are optimal for the interval [0; 2 =jlj). If jltj &gt; 2 , then
the geodesic ceased to be optimal.
      </p>
      <p>Z T Xn</p>
      <p>t0 i;j=1
=0
t0
= L(t; x; x_ ) 0</p>
      <p>
        +2
T
t0
where (t0) = ddt0 , (T ) = ddT , 0 (t0) = dd2t20 , 0 (T ) = dd2T2 , = @@ at = 0.
This functional should be minimized for variables satisfying the equations of
variations along [2]. Since the distribution A is de ned by the 1-form ! =
x2dx1 + dx3 in our example, the constrains (
        <xref ref-type="bibr" rid="ref1">1</xref>
        ) in the accessory problem are
This is the equation of variations along . Since the Lagrangian in our example
is L = 21 (x_ 1)2 + (x_ 2)2 + l(x2x_ 1 + x_ 3), the Lagrangian for the accessory problem
is = 12 ( _1)2 + ( _2)2 + l 2 _1 + ( _3 + x2 _1 + 2x_ 1). The generalized momenta
p1 = _1 + l 2 + x2, p2 = _2 and p3 = . The generalized forces f1 = 0,
f2 = l _1 + x_ 1 and f3 = 0. The Euler|Lagrange equations for the accessory
problem are 1 +l _2 + x_ 2 = 0, 2 = l _1 + x_ 1 and _ = 0. Applying the geodesics
(
        <xref ref-type="bibr" rid="ref2">2</xref>
        ) we get
8 1 + l _2 +
&gt;&lt;&gt; 2 l _1
      </p>
      <p>_3 + 1l v1
&gt;&gt;: _ = 0:
v1 sin lt + v2 cos lt = 0
v1 cos lt v2 sin lt = 0
v1 cos lt + v2 sin lt _1 + v1 cos lt
v2 sin lt 2 = 0
This is the system of linear homogeneous di erential equations for the variables
; . To nd points conjugate with the starting point t0 = 0 one should nd
the solutions of these equations which are zero (0) = 0 at the initial point but
0(0) 6= 0. The solutions have the form</p>
      <p>
        ( 1; 2; 3)T = P (a1; a2; )T ;
where a1, a2, are constants and P is the following part of the fundamental
matrix of the system (
        <xref ref-type="bibr" rid="ref6">6</xref>
        ):
0 sin lt
      </p>
      <p>BB 1 clos lt
P = BBB l</p>
      <p>B 2v1lt 4v1 sin lt+
B +v1 sin 2lt 2v2 cos lt+
@ +v2 cos 2lt+v2
2l2
cos lt 1</p>
      <p>l
sin lt</p>
      <p>l
2v2lt v2 sin 2lt+
+v1 cos 2lt+v1
2v1 cos lt
2l2
(v1lt
(v1lt
v2) cos lt (v1 + v2lt) sin lt + v2 1</p>
      <p>l2
v2) sin lt + (v1 + v2lt) cos lt v1 CC</p>
      <p>
        l2 CC :
(v12+v22)lt 4v12 sin lt+(v12 v22+2v1v2lt) sin 2lt+ CC
+2(v1lt +2(v22v)1vv12c+o(svl22t 2vv121)lvt2)lctossin2lltt+2v1v2+ AC
2l3
If t1 is a point conjugated with the initial point then there is the solution of (
        <xref ref-type="bibr" rid="ref6">6</xref>
        )
satisfying (t1) = 0. To nd such a solution we should calculate the determinant
det P =
2t lt cos
2 sin
      </p>
      <p>
        sin(
lt
2
lt
2
lt
2
)(v12 + v22)=l4:
Since det P (t1) = 0 we get two series of conjugate points. For the conjugate
points of rst series sin l2t = 0 and tk = 2 k=l, k 2 Z. The rst conjugate point
of this series is t1 = 2 =l (Fig. 1). The appropriate Jacobi eld is de ned by (
        <xref ref-type="bibr" rid="ref7">7</xref>
        )
with the parameters
a1 = v2;
For the conjugate points of second series lt cos l2t 2 sin l2t = 0. Approximately
tn ( + 2 n)=l, n 2 N. The rst conjugate point of this series is t1 8:99=l
(Fig. 2). The appropriate Jacobi eld is de ned by (
        <xref ref-type="bibr" rid="ref7">7</xref>
        ) with the parameters
a1
4:49v2=l;
a2
4:49v1=l;
(
        <xref ref-type="bibr" rid="ref10">10</xref>
        )
8:99.
      </p>
      <p>
        The equations (
        <xref ref-type="bibr" rid="ref2">2</xref>
        ) de ne the exponential map for the geodesics with the
initial velocity vector v = (v1; v2) and Lagrange multiplier l: x(t) = expl0(tv).
This exponential map was studied in [9] and its di erential was found. Let us
consider the family of paths
y(t; ) = expl0+
(t(v + b));
(
        <xref ref-type="bibr" rid="ref11">11</xref>
        )
where b = (b1; b2). This is the variation of the geodesic x( ). Let us nd the
derivatives
(l t sin lt +
cos lt
)v2 + ( sin lt
      </p>
      <p>l t cos lt)v1
( sin lt
l t cos lt)v2 + ( l t sin lt</p>
      <p>cos lt + )v1
b1l sin lt</p>
      <p>b2l cos lt + b2l =l2;
= ( sin 2lt
l t cos 2lt</p>
      <p>l t)v22+
=0
(( 2l t sin 2lt
2 cos 2lt + 2l t sin lt + 4 cos lt
2 )v1
b2l sin 2lt + b1l cos 2lt</p>
      <p>2b1l cos lt + 2b2l2t + b1l)v2+
(
sin 2lt + l t cos 2lt + 4 sin lt
2l t cos lt
l t)v12+
(b1l sin 2lt + b2l cos 2lt
4b1l sin lt
2b2l cos lt + 2b1l2t + b2l)v1 =(2l3):
some</p>
      <p>
        and b. For the conjugate points of rst series this is
The rank of exponential geodesic map is not its maximum rank at a conjugate
=0
(t1) = 0 for
8 (2 v1)=l2 = 0
&lt; (2 v2)=l2 = 0
: (2 ( (v12 + v2 )
2
l(b2v2 + b1v1)))=l3 = 0:
(
        <xref ref-type="bibr" rid="ref12">12</xref>
        )
Therefore = 0 and b2 = b1v1=v2. This means that the Lagrange multiplier l
is xed and b?v matching (
        <xref ref-type="bibr" rid="ref9">9</xref>
        ).
=0
be solved numerically. For the point t1 8:99=l the solution is b1 4:49v2 =l,
b2 4:49v1 =l, 6= 0 matching (
        <xref ref-type="bibr" rid="ref10">10</xref>
        ). With this solution in mind we can draw
the geodesic variation with these parameters. This variation is shown on Fig. 2
for l = 1. The endpoints of the geodesics are close to each other at t1 8:99=l
as should be expected for a conjugate point.
(t) = 0 should
4
      </p>
    </sec>
    <sec id="sec-4">
      <title>The Schouten Curvature and the Schouten{Vranceanu</title>
    </sec>
    <sec id="sec-5">
      <title>Connection</title>
      <p>
        Let us consider the distribution A of dimension m on a smooth manifold N
of dimension n. The coordinates xk, k = 1; : : :; n, on an open and su ciently
small domain U N can be chosen so as to maximize the projection of the
distribution A on the rst m coordinates. Then the basis of the distribution A
can be chosen as
n
X
=m+1
k = 1; : : :; m;
(
        <xref ref-type="bibr" rid="ref13">13</xref>
        )
the potentials of the distribution. We assume that they are C1-smooth. The
m
distribution A can be de ned also by di erential 1-forms ! = P As dxs + dx ,
s=1
= m+1; : : :; n. Here and further Latin indexes are in the range 1; : : :; m and
m
Greek indexes are in the range m+1; : : :; n. The Lie brackets [ei; ej ] = P cikj ek +
k=1
n
P cij @ . According to the choice (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ) the only non-zero components are
=m+1
Fij = cij . The tensor Fij is the tensions tensor.
      </p>
      <p>
        For any point x 2 N the quadratic form h ; ix is de ned on A(x). The metric
tensor in the basis (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ) is
      </p>
      <p>gij (x) = hei; ej ix:</p>
      <p>To de ne covariant di erentiation r on the distribution, we must introduce a
symmetric Riemannian connection. The property of being Riemannian is de ned
in a standard way:
while the symmetry condition must be modi ed as</p>
      <p>XhY; Zi = hrX Y; Zi + hY; rX Zi;
rX Y</p>
      <p>rY X = pr([X; Y ]);
m
where pr = P ek dxk is the (horizontal) projection on the distribution. To
k=1
make this projection invariant with respect to transformations of coordinates, we
must impose the following constraints on the smooth structure of the manifold:
@@yxk = 0, k = 1; : : :; m, = m+1; : : :; n, and @@xy ; =m+1;:::;n is the identity
matrix [13, 14, 16]. The coordinates x will be called verticals. The di erentials
of the transfer maps hU hV 1 for all charts hU : U ! Rn, U; V N , admissible
in this smooth structure are the block matrices</p>
      <p>
        0 1
(
        <xref ref-type="bibr" rid="ref14">14</xref>
        )
(
        <xref ref-type="bibr" rid="ref15">15</xref>
        )
(
        <xref ref-type="bibr" rid="ref16">16</xref>
        )
(
        <xref ref-type="bibr" rid="ref17">17</xref>
        )
      </p>
      <p>
        Since the connection r is Riemannian and pr-symmetric (
        <xref ref-type="bibr" rid="ref15">15</xref>
        ), (
        <xref ref-type="bibr" rid="ref16">16</xref>
        ) we get
2hrX Y; Zi = (XhY; Zi
hY; pr[X; Z]i) + (Y hZ; Xi
hX; pr[Y; Z]i)
Due to (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ) pr[ei; ej ] = 0. Let us assume that the metric tensor of the distribution
does not depend on the vertical coordinates x . Then the equation (
        <xref ref-type="bibr" rid="ref18">18</xref>
        ) matches
the Levi-Civita connection on a manifold: rei ej = Pm
k=1 ikj ek and
(ZhX; Y i
      </p>
      <p>
        hZ; pr[X; Y ]i): (
        <xref ref-type="bibr" rid="ref18">18</xref>
        )
(
        <xref ref-type="bibr" rid="ref19">19</xref>
        )
Theorem 1. For a distribution of dimension m on a manifold with the smooth
structure (
        <xref ref-type="bibr" rid="ref17">17</xref>
        ) the vectors of the basis (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ) change over the coordinate
transformations just as the coordinate basis of a manifold of the same dimension. If the
distribution and its metric tensor do not depend on the vertical coordinates then
the Riemannian and pr-symmetric connection r matches the Riemannian and
symmetric connection of a manifold with metric (
        <xref ref-type="bibr" rid="ref14">14</xref>
        ).
      </p>
      <p>
        For any point x 2 N and any three vectors u; v; w 2 A(x) the curvature map
of distribution A at point x is de ned by the Schouten tensor [23, 22, 6]
R(u; v)w = ru~rv~w~
rv~ru~w~
rpr[u~;v~]w~
pr (1
pr)[u~; v~]; w~ ;
(
        <xref ref-type="bibr" rid="ref20">20</xref>
        )
where u~, v~, w~ are horizontal vector elds on a neighbourhood of x such that
u~(x) = u, v~(x) = v, w~(x) = w. The curvature does not depend on the way of
expansion of u; v; w to vector elds. Assume that w~ does not depend on vertical
coordinates x and consider R(ei; ej )ek for the basis (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ). The horizontal projection
of the Lie derivative on the vertical vector eld is zero: pr (1 pr)[ei; ej ]; ek = 0,
because ek does not depend on x and the result of di erentiation of the Lie
bracket [ei; ej ] on ek has the zero horizontal projection. Therefore the equation
(
        <xref ref-type="bibr" rid="ref20">20</xref>
        ) can be simpli ed: R(ei; ej )ek = rei rej ek rej rei ek rpr[ei;ej]ek. The
term rpr[ei;ej]ek = 0 since pr[ei; ej ] = 0. The corresponding term in Riemannian
geometry is also zero for any coordinate vector elds since [@i; @j ] = 0. Final
equation for the curvature of distribution in the basis (
        <xref ref-type="bibr" rid="ref13">13</xref>
        ) matches the equation
for the curvature of a manifold: Rijkl = hR(ek; el)ej ; eii and
ksj lis :
(
        <xref ref-type="bibr" rid="ref21">21</xref>
        )
Theorem 2. Let the distribution be de ned on a manifold with the smooth
structure (
        <xref ref-type="bibr" rid="ref17">17</xref>
        ). If the distribution and its metric tensor do not depend on the vertical
coordinates then its Schouten tensor matches the Riemannian curvature tensor
of a manifold with metric (
        <xref ref-type="bibr" rid="ref14">14</xref>
        ).
\Look inside": we cannot distinguish a distribution from a manifold locally. We
know that a distribution is involved in our physics because the equations of
motion of a charged particle are just the equations of horizontal geodesics [8,
15]. The potentials Aj for a 4-dimensional distribution on a 5-manifold are just
the 4-potentials of the electromagnetic eld. The existence of these potentials is
con rmed by the Aharonov|Bohm e ect [1]. The Maxwell equations and the
Dirac equation use this 4-potential and there is a problem how to nd soliton-like
solution for the 4-potential satisfying these equations [4, 5]. If the distribution
and its metric tensor do not depend on the vertical coordinates we say that the
distribution satis es the cyclicity condition.
5
      </p>
    </sec>
    <sec id="sec-6">
      <title>The Equations of Geodesics</title>
      <p>Let the distribution A on a manifold N n be de ned by the di erential 1-forms
m
! = P As dxs + dx , = m+1; : : :; n. The geodesics equations for a
distribus=1
tion with the cyclicity condition are [10]
where dDt { covariant derivative, (a0; l) { the Lagrange multipliers, which cannot
be altogether zero. A geodesic is called normal (or regular), i there is the
only one set of multipliers (a0; l) with a0 = 1 for . Operator F^ is the tensions
tensor Fij = @jAi @iAj with the second index raised by the inverse metric
tensor of the distribution.</p>
      <p>Example 1. Let the 2-dimensional distribution in R3 be de ned by ! =
0 2y
y2dx+dz. The tensions tensor F = 2y 0 . Non-trivial abnormal geodesics
appear at y = 0. It can be any absolutely continuous function x = x(t) with
z = const due to !( 0) = 0. Since any path with backward movements cannot
be optimal, we can choose parametrization so that
8 x = x0 + ct
&lt;</p>
      <p>y = 0
: z = const
:
N.N. Petrov [19{21] and R. Montgomery [18] proved independently that if this
path is short enough it is a solution to the minimization problem for some length
functional.</p>
      <p>Example 2. Let the 2-dimensional distribution in R3 be de ned by ! =
f (x)g(y)dx xdy + dz, where f , g are some su ciently smooth functions. The
tensions tensor is</p>
      <p>F =</p>
      <p>
        0
f (x)g0(y) 1
f (x)g0(y) + 1
0
:
21y dy. Hence, z(t) = z0
the abnormal geodesics
If the equation f (x)g0(y) + 1 = 0 has a continuous solution for all y 2 [y0; y1]
with some y0, y1, then this is an abnormal geodesic. Since x = f 1( 1=g0(y)),
we assume that g0 : [y0; y1] ! R is a di eomorphism to its image and there
is the inverse function f 1 continuous in the domain of 1=g0. Let us choose
g(y) = y2=2 and f (x) = x, then x = 1=y. If y = y0 + ct, then x = 1=(y0 + ct)
where c = const 6= 0 and t 6= y0=c. The coordinate z = z(t) is de ned by the
horizontality condition dz = xdy 12 xy2dx = y1 dy + y2 d( y1 ) = y1 dy + 21y dy =
12 ln jy0 + ctj. We proved that this distribution admits
(
        <xref ref-type="bibr" rid="ref23">23</xref>
        )
(
        <xref ref-type="bibr" rid="ref24">24</xref>
        )
8&gt;&lt; x = y0 1+ t
      </p>
      <p>
        y = y0 + t
&gt;: z = z0 21 ln jy0 + tj
; t 6=
y0; y0; z0 2 R:
(
        <xref ref-type="bibr" rid="ref25">25</xref>
        )
It is an open question whether some of these abnormal geodesics are solutions
of the minimization problem for some length functional on the distribution.
      </p>
      <p>Further we consider regular geodesics only.</p>
    </sec>
    <sec id="sec-7">
      <title>The Jacobi Equation</title>
      <p>l</p>
      <p>I(Y; Z) =
Let us assume that both the distribution and the metric tensor of the
distribution are independent of vertical coordinates (the cyclicity condition). Hence
the Lagrange multipliers are time-independent (constant). The Jacobi equation
for this class of distributions can be written in geometric covariant form. The
distribution is assumed to be totally nonholonomic. The Hilbert condition [2]
for geodesics is always ful lled in this theory (all geodesics are non-singular).</p>
      <p>Consider the minimization problem for the energy functional J ( ) =
12 RtT0 h 0; 0i dt for horizontal paths with xed endpoints and time. This is the
Lagrange problem. We shall omit the subscript and the summation sign in
n n
sums involving Lagrange multipliers such as P l ! and P l F .
=m+1 =m+1</p>
      <p>By de nition, a two-parameter variation of a geodesic is a two-parameter
family of curves (t; ; ) such that (t; 0; 0) (t) [2]. A geodesic and its
variation are assumed to be C2-smooth. In addition, we assume that the
@3 @3
third derivatives @ @t@ and @t@ @ do exist for all admissible t, , and are
continuous along . In the paper [11], it was shown that the second variation of
T</p>
      <p>+
t0
=0 =
=0
Z T D DY
t0
dt
;</p>
      <p>DZ E
dt</p>
      <p>R(Y; 0) 0; Z</p>
      <p>dt
Z T
t0
l (rY F )( 0; Z) + F
; Z</p>
      <p>
        dt (
        <xref ref-type="bibr" rid="ref26">26</xref>
        )
is called the index form of a geodesic with Lagrange multipliers l. The vector
elds Y ( ; 0; 0) and Z( ; 0; 0) along will be denoted by the same letters Y , Z.
If one of the elds Y or Z is vertical, then I(Y; Z) = 0.
      </p>
      <p>The metric tensor of a distribution is positively de nite in sub-Riemannian
geometry. Therefore the functional I(Y; Y ) &gt; 0 for variations of geodesics which
are su ciently short. It is one of the necessary conditions of optimality. The
optimality may be lost if I(Y; Y ) = 0 and it will be lost if I(Y; Y ) &lt; 0. To nd
critical variations we should consider the minimization problem for the functional
If the distribution is integrable in some sence, i.e. the sequence of commutators (the
ag of the distribution) does not span the whole tangent bundle of the manifold,
then some vertical coordinates of Jacobi elds are dependend and the fundamental
matrix of the Jacobi equation is degenerated for all points.</p>
      <sec id="sec-7-1">
        <title>I(Y; Y ) with the constrains (Y 0; Y ) = 0 (1). Hence we should minimize</title>
        <p>Consider the variation Y 7! Y + Y and collect linear for Y terms. We get
Z T D DY
t0
dt
;</p>
        <p>D Y E
dt</p>
        <p>R(Y; 0) 0; Y
l (r Y F )( 0; Y ) + (rY F )( 0; Y ) + F
; Y
+ F
; Y</p>
        <p>dt+
dt
D Y
dt
Assuming that the vector eld Y is C1-smooth and that the derivative DdYt is
absolutely continuous, we have</p>
        <p>
          I (Y ) =
1 Z T
De nition 1. A pair (Y~ ; ), where Y~ is a vector eld along a geodesic with
Lagrange multipliers l, will be called a Jacobi eld if Y~ satis es the variations
equations (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) and its horizontal projection Y = pr Y~ satis es the nonholonomic
Jacobi equation
        </p>
        <p>
          D DY
dt dt
The F^ operator is the tensions tensor F with the second index raised by the
inverse metric tensor of the distribution. We assume that both the distribution
and the metric tensor of the distribution are independent of vertical coordinates
(the cyclicity condition). Hence the Lagrange multipliers (both l and ) are
time-independent. The equations (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ), (29) together with 0 = 0 are a system of
linear homogeneous di erential equations with the variables (Y~ ; ). The set of
solutions of this system is a linear space. Therefore there are two types of Jacobi
elds. For the rst type 0 (zero vector). For the second type of Jacobi elds
6= 0.
        </p>
        <p>A horizontal vector eld Y along a geodesic with Lagrange multipliers l
will be called a horizontal Jacobi eld i it satis es (29) with some multipliers
.</p>
        <p>De nition 2. Points t1; t2 2 [t0; T ], t1 6= t2, are said to be conjugated along
a horizontal geodesic if there exists a nontrivial Jacobi eld Y (with some )
along which vanishes at these points: Y (t1) = 0 and Y (t2) = 0.</p>
        <p>A smooth variation ( ; ) : [t0; T ] (
its longitudinal lines are geodesics.</p>
        <p>; ) ! N is a geodesic variation i all
; ) ! N is a geodesic variation then the
is a horizontal Jacobi eld along each
lonl( )(rY F^)X
,
Theorem 3. Let be a geodesic with the origin x0 = (t0) and endpoint x1 =
(T ). The point x1 = explx0 (u) is conjugated with the point x0 along i the
rank of the di erential d(u;l) expx0 is not its maximum, i.e. i (u; l) is a critical
point of the mapping (u; l) 7! explx0 (u).</p>
        <p>Proof. The Jacobi equation which appears in the Bliss accessory problem is the
result of the linearisation of geodesics equations
8</p>
        <p>
          0 = X
&lt; DdXt + lF^X = 0 :
: !(X) = 0
(30)
The fundamental matrix in the Bliss problem matches the matrix of the
differential d(u;l) expx0 , because this di erential satis es the linearised geodesics
equations as the result of di erentiation of a solution of a di erential equation
by initial conditions [17, p. 289], [7]. Since we consider distributions with the
cyclicity condition the index form I(Y; Z) depends on the horizontal projections
of elds Y , Z only. Hence the horizontal projection of a Jacobi eld in the
Bliss problem satis es (29). Therefore we can consider a (horizontal) solution
of the equation (29) and nd its vertical components by means of the
variations equation (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ). The fundamental matrix of the obtained solution matches
the fundamental matrix of the Bliss problem and therefore the di erential
matrix d(u;l) expx0 .
        </p>
        <p>In the next part of this paper we consider Jacobi elds of the rst type.
The Jacobi elds of rst type ( 0).
Lemma 2. If Y; Z are horizontal Jacobi elds along a geodesic with Lagrange
multipliers l, then f = hY; Z0i hY 0; Zi lF (Y; Z) is a constant function.
Proof. f 0 = hY 0; Z0i + hY; Z00i hY 00; Zi hY 0; Z0i l(r 0 F )(Y; Z) lF (Y 0; Z)
lF (Y; Z0) = hY; R(Z; 0) 0 + l(rZ F^) 0 + lF^Z0i + hR(Y; 0) 0 + l(rY F^) 0 +
lF^Y 0; Zi l(r 0 F )(Y; Z) lF (Y 0; Z) lF (Y; Z0) = l(rZ F )( 0; Y )
l(rY F )(Z; 0) l(r 0 F )(Y; Z) = ldF ( 0; Y; Z) = 0.</p>
        <p>Hence the Jacobi elds preserve the de nite antisymmetric form. Note that
the vector eld X = 0 is a horizontal Jacobi eld. Indeed due to the geodesics
equations X0 = lF^X, therefore X00 = l(rX F^)X lF^X0, and this is the
equation (29) (the curvature contribution R(X; X)X = 0).</p>
        <p>Applying Lemma 2 to an arbitrary horizontal Jacobi eld Y and 0 we obtain
hY; 00i hY 0; 0i lF (Y; 0) = C. Since is a horizontal geodesic, 00 = lF^ 0
and hY 0; 0i = const.</p>
        <p>Lemma 3. A geodesic : [t0; T ] ! N may contain only a
points which are conjugated to t0.
nite number of
The proof is similar to that given in [3, p. 149].</p>
        <p>
          If a (regular) geodesic : [t0; T ] ! N is a solution to the minimization
problem for the functional J , then the functional I (Y ) is non-negative for any
vector eld Y along satisfying (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ).
        </p>
        <p>
          Theorem 4. Let : [t0; T ] ! N be a geodesic and the semi-interval (t0; T ] does
not contain points conjugated with t0. Then the functional I (Y ) is positively
de nite for all vector elds Y along satisfying (
          <xref ref-type="bibr" rid="ref1">1</xref>
          ) wich are zero at the endpoints
of .
        </p>
        <p>Theorem 5. Let the cyclicity condition be satis ed for a distribution. Suppose
that the metric tensor of a distribution is positive de nite, a (regular) geodesic
connects two given points x0 and x1, and there are no points on the semi-interval
(t0; T ] that are conjugated to t0. Then, on the path , the energy functional
attains its weak local minimum in the problem with xed endpoints.</p>
      </sec>
      <sec id="sec-7-2">
        <title>The proof is given in [12].</title>
        <p>7</p>
      </sec>
    </sec>
    <sec id="sec-8">
      <title>Conclusion</title>
      <p>Hence we propose the Jacobi equation for horizontal geodesics on a distribution
in sub-Riemannian geometry which involves the curvature tensor of a
distribution and its tensions tensor. The classical variational theory treats this equation
as a sum of derivatives of the given functional. We established the
geometric sense of these sums in terms of well-de ned geometric objects. The Jacobi
equation (29) is applicable to regular geodesics. Since there are also abnormal
geodesics in the sub-Riemannian geometry, we discussed two examples of such
geodesics. There is one more way where geodesics may loss its optimality: it is
the case when two given points can be connected by more than one geodesic.
We could not discuss this case here yet it should be always noted.</p>
    </sec>
  </body>
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