to e
∇˙γ˙γ=∓kγJ˙γ. We can interpret it as a trajectory
for a Kähler magnetic field ∓kγBJwith the Kähler
form BJ.
We here recall some properties of circles on
CHn(c). Congruency of circles guarantees that every
circle is a homogeneous curve, that is, it is an orbit of
one parameter family of isometries of CHn. Since
CHnis a typical example of Hadamard manifolds,
we can define its ideal boundary ∂CHnas the set of
asymptotic classes of geodesics, and have a compacti
fication CHn=CHnS∂CHn, [4, 5]. When a curve
γwhich is unbounded in both directions, that is, both
γ[0,∞)and γ−∞,0]are unbounded sets, we set
γ(∞) = limt→∞ γ(t), γ(∞) = limt→−∞ γ(t)if
they exist in ∂CHn. These are called points at infinity
of γ. We say a smooth curve γparameterized by its
arclength to be horocyclic if it satisfies the following
conditions, [6]:
i) Both γ(∞)and γ(−∞)exist and coincide with
each other;
ii) If it crosses with a geodesic βsatisfying β(∞) =
γ(∞), then they cross orthogonally.
We set a function ν: [0,∞)→Rby
ν(k) =
0,if k < √|c|
2,
(4k2+c)3/2
(3√3|c|k),if √|c|
2≤k≤p|c|,
1,if k > p|c|.
We take a horizontal lift ˆγof a circle γon CHn(c)
through a Hopf fibration ϖ:H2n+1
1(⊂Cn+1)→
CHn(c)of an antide Sitter space H2n+1
1and regard
it as a curve in Cn+1. When its geodesic curvature is
kγand complex torsion is τγ, by solving an ordinary
differential equation on ˆγ, we can get the following
feature of γ:
1) If kγ>p|c|or τγ< ν(kγ), it is bounded;
2) If it does not satisfies the condition in 1), it is
unbounded in both directions and has points at
infinity;
3) It is horocyclic if and only if p|c|/2 ≤kγ≤
p|c|and |τγ|=ν(kγ)hold;
4) When τγ=±1, it lies on a totally geodesic CH1,
and when τγ= 0, it lies on a totally geodesic
RH2.
The following figure shows the images of the moduli
spaces of unbounded and bounded circles on CHn(c).
-
6q
q
√|c|
2
p|c|
k
τ
unbounded
circles bounded circles
horocyclic circles
X
Xz
@
@I
Figure 1: moduli space of circles on CHn
3 Horocyclic circles are expressed
uniquely by trajectories
In this paper, we study whether circles in CHn(c)can
be seen as extrinsic shapes of some “nice” curves on
a homogeneous real hypersurface. Let M=T(r)
be a tube of radius raround totally geodesic com
plex hypersurface CHn−1in CHn(c). On this hy
persurface we have an almost contact metric structure
(ξ, η, ϕ, ⟨,⟩)induced by the complex structure J
on CHn. By taking a unit normal vector field Nof
Min CHn(c)and the induced metric ⟨,⟩, we set
the characteristic vector field ξby ξ=−JN, the 1
form ηby η(v) = ⟨v, ξ⟩, the (1,1)tensor field ϕby
ϕ(v) = Jv −η(v)N. The shape operator AMof M
satisfies AMξ=δMξand AMv=λMvfor arbitrary
tangent vector vorthogonal to ξ. Here, the principal
curvatures are given as δM=p|c|coth p|c|rand
λM=p|c|/2tanhp|c|r/2, [7, 8], for example.
If we denote by ∇and e
∇the Riemannian connec
tions on Mand on CHn(c), respectively, we have the
formulae of Gauss and Weingarten:
e
∇XY=∇XY+⟨AMX, Y ⟩N,
e
∇XN=−AMX,
for arbitrary vector fields X, Y tangent to M. Since
the complex structure Jis parallel with respect to e
∇,
these formulas guarantee
∇XϕY=η(Y)AMX− ⟨AMX, Y ⟩ξ, (2)
∇Xξ=ϕAMX. (3)
We define a 2form Fϕon Mby Fϕ(v, w) =
⟨v, ϕ(w)⟩. By use of (3), we find that it is closed. We
therefore call its constant multiple Fκ=κFϕ(κ∈R)
aSasakian magnetic field. A smooth curve σparam
eterized by its arclength is said to be a trajectory for
Fκif it satisfies the equation ∇˙γ˙γ=κϕ ˙γ. Since we
find that trajectories for the null magnetic field F0are
geodesics and that every trajectory is determined by
its initial unit tangent vector, we may say that trajec
tories are generalizations of geodesics and are sim
plest curve next to geodesics from the viewpoint of
WSEAS TRANSACTIONS on MATHEMATICS
DOI: 10.37394/23206.2023.22.102
Yusei Aoki, Toshiaki Adachi