On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁

One primary objective in submanifold geometry is to discover fascinating and significant classical examples of ₁. In this paper, which relies on the theory we established in [Adv. Math. 405 (2022), 08514, 50 pages, arXiv:2101.11780] and utilizing the approach we provided for constructing constant -m...

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Опубліковано в: :Symmetry, Integrability and Geometry: Methods and Applications
Дата:2025
Автори: Chiu, Hung-Lin, Lai, Sin-Hua, Liu, Hsiao-Fan
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Опубліковано: Інститут математики НАН України 2025
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Цитувати:On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁. Hung-Lin Chiu, Sin-Hua Lai and Hsiao-Fan Liu. SIGMA 21 (2025), 011, 25 pages

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Chiu, Hung-Lin
Lai, Sin-Hua
Liu, Hsiao-Fan
author_facet Chiu, Hung-Lin
Lai, Sin-Hua
Liu, Hsiao-Fan
citation_txt On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁. Hung-Lin Chiu, Sin-Hua Lai and Hsiao-Fan Liu. SIGMA 21 (2025), 011, 25 pages
collection DSpace DC
container_title Symmetry, Integrability and Geometry: Methods and Applications
description One primary objective in submanifold geometry is to discover fascinating and significant classical examples of ₁. In this paper, which relies on the theory we established in [Adv. Math. 405 (2022), 08514, 50 pages, arXiv:2101.11780] and utilizing the approach we provided for constructing constant -mean curvature surfaces, we have identified intriguing examples of such surfaces. Notably, we present a complete description of rotationally invariant surfaces of constant p-mean curvature and shed light on the geometric interpretation of the energy with a lower bound.
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fulltext Symmetry, Integrability and Geometry: Methods and Applications SIGMA 21 (2025), 011, 25 pages On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 Hung-Lin CHIU ab, Sin-Hua LAI c and Hsiao-Fan LIU de a) Department of Mathematics, National Tsing Hua University, Hsinchu, Taiwan E-mail: hlchiu@math.nthu.edu.tw b) National Center for Theoretical Sciences, Taipei, Taiwan c) Fundamental Education Center, National Chin-Yi University of Technology, Taichung, Taiwan E-mail: shlai@ncut.edu.tw d) Department of Applied Mathematics and Data Science, Tamkang University, New Taipei City, Taiwan E-mail: hfliu@mail.tku.edu.tw e) Department of Applied Mathematics, National Chung Hsing University, Taiwan Received April 15, 2024, in final form February 04, 2025; Published online February 18, 2025 https://doi.org/10.3842/SIGMA.2025.011 Abstract. One primary objective in submanifold geometry is to discover fascinating and significant classical examples ofH1. In this paper which relies on the theory we established in [Adv. Math. 405 (2022), 08514, 50 pages, arXiv:2101.11780] and utilizing the approach we provided for constructing constant p-mean curvature surfaces, we have identified intriguing examples of such surfaces. Notably, we present a complete description of rotationally invari- ant surfaces of constant p-mean curvature and shed light on the geometric interpretation of the energy E with a lower bound. Key words: Heisenberg group; Pansu sphere; p-minimal surface; Codazzi-like equation; ro- tationally invariant surface 2020 Mathematics Subject Classification: 53A10; 53C42; 53C22; 34A26 1 Introduction This article is an extension of the previous paper [5], in which we studied the constant p-mean curvature surfaces in the Heisenberg group H1. In [5], we focused on the foundation of the theory and paid more attention to the investigation of p-minimal surfaces. However, in the present article, instead of theory, we mainly focus on the examples, including an approach to construct constant p-mean curvature surfaces. Recall that the Heisenberg group H1 is the space R3 with the associated group multiplication (x1, y1, z1) ◦ (x2, y2, z2) = (x1 + x2, y1 + y2, z1 + z2 + y1x2 − x1y2), which is a 3-dimensional Lie group. The space of all left-invariant vector fields is spanned by the following three vector fields: e̊1 = ∂ ∂x + y ∂ ∂z , e̊2 = ∂ ∂y − x ∂ ∂z and T = ∂ ∂z . The Heisenberg dilation (scaling) by the factor δ > 0 is the map Dδ : H1 → H1 defined by Dδ(x, y, z) = ( δx, δy, δ2z ) for any (x, y, z) ∈ H1 (see [6]). mailto:hlchiu@math.nthu.edu.tw mailto:shlai@ncut.edu.tw mailto:hfliu@mail.tku.edu.tw https://doi.org/10.3842/SIGMA.2025.011 2 H.-L. Chiu, S.-H. Lai and H.-F. Liu The standard contact bundle on H1 is the subbundle ξ of the tangent bundle TH1 spanned by e̊1 and e̊2. It is also defined to be the kernel of the contact form Θ = dz + xdy − ydx. The CR structure on H1 is the endomorphism J : ξ → ξ defined by J (̊e1) = e̊2 and J (̊e2) = −e̊1. One can view H1 as a pseudo-hermitian manifold with (J,Θ) as the standard pseudo-hermitian structure. There is a naturally associated connection ∇ if we regard all these left-invariant vector fields e̊1, e̊2, and T as parallel vector fields. A naturally associated metric on H1 is the adapted metric gΘ, which is defined by gΘ = dΘ(·, J ·) + Θ2. It is equivalent to defining the metric regarding e̊1, e̊2, and T as an orthonormal frame field. We sometimes use ⟨·, ·⟩ to denote the adapted metric. In this paper, we use the adapted metric to measure the lengths, angles of vectors, and so on. Suppose Σ is a surface in the Heisenberg group H1. There is a one-form I on Σ induced from the adapted metric gΘ. This induced metric is defined on the whole surface Σ and is called the first fundamental form of Σ. The intersection TΣ∩ξ is integrated to be a singular foliation on Σ called the characteristic foliation. Each leaf is called a characteristic curve. A point p ∈ Σ is called a singular point if the tangent plane TpΣ coincides with the contact plane ξp; otherwise, p is called a regular (or non-singular) point. Generically, a point p ∈ Σ is a regular point, and the set of all regular points is called the regular part of Σ. In this paper, we always assume that the surface Σ is of class C2, but of class C∞ on the regular part. On the regular part, we can choose a unit vector field e1 such that e1 defines the characteristic foliation. The vector e1 is determined up to a sign. Let e2 = Je1. Then {e1, e2} forms an orthonormal frame field of the contact bundle ξ. We usually call the vector field e2 a horizontal normal vector field. Then the p-mean curvature H of the surface Σ is defined by ∇e1e2 = −He1. The p-mean curvature H is only defined on the regular part of Σ. If H = c, which is a constant on the whole regular part, we call the surface a constant p-mean curvature surface. In particular, if c = 0, it is a p-minimal surface. There also exists a function α defined on the regular part such that αe2+T is tangent to the surface Σ. We call this function the α-function of Σ. It is uniquely determined up to a sign, which depends on the choice of the characteristic direction e1. Define ê1 = e1 and ê2 = αe2+T√ 1+α2 , then {ê1, ê2} forms an orthonormal frame field of the tangent bundle TΣ. Notice that ê2 is uniquely determined and independent of the choice of the characteristic direction e1. In [3, 4], it was shown that these three invariants, I, e1, and α, form a complete set of invariants for constant p-mean curvature surfaces with H = c in H1. Namely, for any two surfaces with the same constant p-mean curvature having the same I, α, e1, they are differed only by a Heisenberg symmetry. In particular, if Σ ⊂ H1 is a constant p-mean curvature surface with H = c, then in terms of a compatible coordinate system (U ;x, y), which means e1 = ∂ ∂x , the integrability condition (see [5]) is reduced to −ax + a bx b = cα( 1 + α2 )1/2 , −bx b = 2α+ ααx 1 + α2 , αxx + 6ααx + 4α3 + c2α = 0, (1.1) where the two functions a and b are a representation of the first fundamental form I in the following sense that they describe the vector field ê2 = a(x, y) ∂ ∂x + b(x, y) ∂ ∂y . In other words, there exists the α satisfying the Codazzi-like equation αxx + 6ααx + 4α3 + c2α = 0, (1.2) which is a nonlinear ordinary differential equation. In [5], we normalized a and b such that they can be uniquely determined by the function α, and hence we obtained the result that the On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 3 existence of a constant p-mean curvature surface (without singular points) is equivalent to the ex- istence of a solution to a nonlinear second-order ODE (1.2), which is a kind of Liénard equations (cf. [7]). They are one-to-one correspondences in some sense. For a detailed description, see [5, Theorems 1.1, 1.3 and 6.3]. This result tells us that the investigation of the geometry of con- stant p-mean curvature surfaces in H1 is equal to the study of the solution of the equation (1.2). More specifically, we obtained a complete set of solutions (see [5, Theorems 1.2 and 1.4] or Theorem 2.1) and used the types of the solutions to the equation to characterize the constant p-mean curvature surfaces as several classes, which are vertical, special type I, special type II and general type (see [5, Definitions 5.1 and 5.2] for p-minimal cases and see Definitions 2.2 and 2.3 for the cases with c ̸= 0 in the present article). After the process of normalization, we obtained a complete set of invariants from the normal form of the α-function. It is worth of our mention that these invariants in some sense measure how different a constant p-mean curvature surface is from the model case, which is the horizontal plane in the p-minimal case, and the Pansu sphere in the case c > 0. We first study rotationally invariant surfaces in H1 with constant p-mean curvature H = c using the Codazzi-like equation (1.2). In [8], M. Ritoré and C. Rosales made an investigation on such kinds of surfaces by a first-order ODE system. In the present paper, we shall study them again from the point of view of our theory established in the previous paper [5] and the present one. Let Σ(s, θ) be a rotationally invariant surface in H1 with H = c, generated by the curve γ(s) = (x(s), 0, t(s)), x(s) ≥ 0, on the xt-plane, that is, Σ is parametrized by Σ(s, θ) = (x(s) cos θ, x(s) sin θ, t(s)), where x′2 + t′2 = 1. Here ′ means taking a derivative with respect to s. Recall the energy E = xt′√ x2x′2 + t′2 + λx2, (1.3) which was introduced in [8] and was shown to be a constant. Here 2λ = c and notice that our p-mean curvature differs from the one defined in [8] by a sign. Hence, we have Theorems A and B as follows. Theorem A. A curve γ = (x, t) is the generating curve of a rotationally invariant surface Σ in H1 with H = c ̸= 0 if and only if γ = (x, t) is defined by x2 = k c2 +r cos (cs̃), t = − s̃ c− r 2 sin (cs̃), up to a constant, for some horizontal arc-length parameter s̃ and some k, r ∈ R such that k ≥ 1 and r = 2 c2 √ k − 1. In addition, we have k = 2cE + 2. If r = 0, then Σ is a cylinder. If r ̸= 0, then, in terms of normal coordinates ( s̄, θ̄ ) , the two invariants for Σ are ζ1(θ̄) = −2Eθ̄ cr , up to a constant, which is linear on θ̄, ζ2(θ̄) = −2cE + 2 c2r , which is a constant. Theorem B. A curve γ = (x, t) is the generating curve of a rotationally invariant p-minimal surface Σ in H1 if and only if either t is a constant, and hence Σ is a part of the horizontal plane, or γ = (x, t) is defined by x2 = s̃2 + c2, t = ms̃, up to a constant, for some horizontal arc-length parameter s̃ and some c2,m ∈ R, m ̸= 0. In addition, we have E = m. In terms of normal coordinates (s̄, θ̄), the two invariants for Σ are ζ1(θ̄) = Eθ̄, up to a constant, which is linear on θ̄, ζ2(θ̄) = c2, which is a constant. 4 H.-L. Chiu, S.-H. Lai and H.-F. Liu For more interesting examples, in Section 4, we provide an approach to construct a constant p-mean curvature surface. This approach is an analog of the one we performed in the previ- ous paper [5] for p-minimal surfaces. Actually, in [5], we deformed the horizontal plane along a curve C(θ) = (x1(θ), x2(θ), x3(θ)) to obtain a p-minimal surface. More specifically, in [5, Sec- tion 9], depending on a parametrized curve C(θ) = (x1(θ), x2(θ), x3(θ)) for θ ∈ R, we deformed the graph u = 0 to obtain a p-minimal surface parametrized by Y (r, θ) = (x1(θ) + r cos θ, x2(θ) + r sin θ, x3(θ) + rx2(θ) cos θ − rx1(θ) sin θ), for r ∈ R. It is easy to check that Y is an immersion if and only if either Θ ( C′(θ) ) −( x′2(θ) cos θ−x′1(θ) sin θ )2 ̸= 0 or r + ( x′2(θ) cos θ − x′1(θ) sin θ ) ̸= 0 for all θ. In particular, the surface Y defines a p-minimal surface of special type I if the curve C satisfies x′3(θ) + x1(θ)x ′ 2(θ)− x2(θ)x ′ 1(θ)− ( x′2(θ) cos θ − x′1(θ) sin θ )2 = 0, for all θ. In addition, the corresponding ζ1-invariant [5, formula (9.9)] reads ζ1(θ) = x′2(θ) cos θ − x′1(θ) sin θ − ∫ [ x′1(θ) cos θ + x′2(θ) sin θ ] dθ. (1.4) Similarly, the surface Y defines a p-minimal surface of general type if the curve C satisfies x′3(θ) + x1(θ)x ′ 2(θ)− x2(θ)x ′ 1(θ)− ( x′2(θ) cos θ − x′1(θ) sin θ )2 ̸= 0, for all θ. In addition, the corresponding ζ1- and ζ2-invariant read ζ1(θ) = x′2(θ) cos θ − x′1(θ) sin θ − ∫ [ x′1(θ) cos θ + x′2(θ) sin θ ] dθ, ζ2(θ) = x′3(θ) + x1(θ)x ′ 2(θ)− x2(θ)x ′ 1(θ)− ( x′2(θ) cos θ − x′1(θ) sin θ )2 . (1.5) In Section 4, we construct a constant p-mean curvature surface by perturbing the Pansu sphere along a given curve C(θ). In Section 2.1, we see that the Pansu sphere (2.2) can be parametrized by X(s, θ) = cos θ − sin θ 0 sin θ cos θ 0 0 0 1 x(s) y(s) t(s)  = x(s) cos θ − y(s) sin θ x(s) sin θ + y(s) cos θ t(s)  , where x(s) = 1 2λ sin(2λs), y(s) = − 1 2λ cos(2λs) + 1 2λ , t(s) = 1 4λ2 sin(2λs)− 1 2λ s+ π 4λ2 , with X(0, θ) = ( 0, 0, π 4λ2 ) and X ( π λ , θ ) = ( 0, 0,− π 4λ2 ) as the North pole and South pole, respec- tively. We deform it along C(θ) = (x1(θ), x2(θ), x3(θ)) to obtain a constant p-mean curvature surface Y (s, θ) as follows Y (s, θ) = (x1(θ) + (x(s) cos θ − y(s) sin θ), x2(θ) + (x(s) sin θ + y(s) cos θ), x3(θ) + t(s) + x2(θ)(x(s) cos θ − y(s) sin θ)− x1(θ)(x(s) sin θ + y(s) cos θ)). We also give a condition for Y to be an immersion. The coordinate system (s, θ) for Y is a compatible one. We have (see (4.4)) α = λ A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs( B(θ)− 1 2λ ) cos 2λs+A(θ) sin 2λs+D(θ) , (1.6) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 5 where A(θ) = x′2(θ) cos θ − x′1(θ) sin θ, B(θ) = x′2(θ) sin θ + x′1(θ) cos θ, D(θ) = λΘ(C′(θ)) + ( 1 2λ −B(θ) ) , V (θ) = ( A(θ), 1 2λ −B(θ) ) . It is obvious that V (θ) = 0 implies α = 0, and hence Y is a cylinder. For nonzero V (θ), we then define ∥V (θ)∥ = √ [A(θ)]2 + [ 1 2λ −B(θ) ]2 and write G(θ) = D(θ) ∥V (θ)∥ , V (θ) ∥V (θ)∥ = (sin ζ(θ), cos ζ(θ)), for some function ζ(θ). From (1.6), we thus have α = λ sin ( 2λs+ ζ(θ) ) G(θ)− cos ( 2λs+ ζ(θ) ) . Finally, we normalize the α-function to obtain the two invariants for Y , stated in Theorem 4.1. We list it here as the third main result of the present paper. Theorem C. If V = 0, then α = 0. If V ̸= 0, we consider the new coordinates s̃ = s + Γ(θ), θ̃ = Ψ(θ), where Γ(θ) = θ 2λ − ∫ D(θ)dθ, Ψ(θ) = 2λ ∫ ∥V (θ)∥ dθ, then the coordinate system ( s̃, θ̃ ) is normal. In terms of the normal coordinates, the invariants of Y are given by ζ1 ( θ̃ ) = ζ(θ)− 2λΓ(θ), ζ2 ( θ̃ ) = G(θ), (1.7) where θ = Ψ−1 ( θ̃ ) . In Section 5, we use formula (1.4), (1.5) and (1.7) to construct various examples of surfaces of constant p-mean curvature including degenerate p-minimal surfaces of special type I. 2 Solutions to the Codazzi-like equation The Codazzi-like equation for a surface in H1 with constant p-mean curvature H = c > 0 is αxx + 6ααx + 4α3 + c2α = 0. (2.1) Theorem 2.1 ([5]). Besides the following three special solutions to (2.1), α(x) = 0, − c 2 tan(cx+ cK1), α(x) = − c 2 tan ( c 2 x− c 2 K2 ) , we have the general solution to (2.1) of the form α(x) = c 2 sin ( cx+ c1 ) c2 − cos ( cx+ c1 ) , which depends on constants K1, K2, c1, and c2. 6 H.-L. Chiu, S.-H. Lai and H.-F. Liu Note that all the solutions are a periodic function with α ( x+ 2π c ) = α(x) for all x. We give some remarks as follows. (1) In terms of the following identities − tan ( θ + π 2 ) = cot θ = sin 2θ 1− cos 2θ , − tan 2θ = − sin 2θ cos 2θ = sin 2θ 0− cos 2θ , we see that the two nontrivial special solutions in Theorem 2.1 correspond to the general solution in Theorem 2.1 with c2 = 0 and c2 = 1, respectively. (2) From the following identity sin (θ + π) c2 − cos (θ + π) = sin θ −c2 − cos θ , we can assume without loss of generality that c2 ≥ 0 in the general solution. Due to Theorem 2.1, we are able to use the types of the solutions to (2.1) to classify the constant p-mean curvature surfaces into several classes, which are vertical, special type I, special type II and general type. In terms of compatible coordinates (x, y), the function α(x, y) is a solution to the Codazzi-like equation (2.1) for any given y. By Theorem 2.1, the function α(x, y) hence has one of the following forms of special types 0, c 2 sin(cx+ c1) 0− cos(cx+ c1) , c 2 sin (cx+ c1) 1− cos ( cx+ c1) , and general types c 2 sin (cx+c1) c2−cos (c(x+c1) , where, instead of constants, both c1 and c2 are now functions of y. Notice that it is convenient at some point to assume that c2(y) ≥ 0 for all y. We now use the types of the function α(x, y) to define the types of constant p-mean curvature surfaces as follows. Definition 2.2. Locally, we say that a constant p-mean curvature surface is (1) vertical if α vanishes (i.e., α(x, y) = 0 for all x, y); (2) of special type I if α = c 2 sin (cx+c1(y)) 1−cos (cx+c1(y)) ; (3) of special type II if α = c 2 sin(cx+c1(y)) 0−cos(cx+c1(y)) ; (4) of general type if α = c 2 sin (cx+c1(y)) c2(y)−cos (cx+c1(y)) with c2(y) /∈ {0, 1} for all y. We further divide constant p-mean curvature surfaces of general type into three classes as follows. Definition 2.3. A constant p-mean curvature surface of general type is (1) of type I if c2(y) > 1 for all y; (2) of type II if 0 < c2(y) < 1 for all y, and −c1+cos−1 c2 c < x < 2π−c1−cos−1 c2 c ; (3) of type III if 0 < c2(y) < 1 for all y, and either −c1 c ≤ x < −c1+cos−1 c2 c or 2π−c1−cos−1 c2 c < x ≤ −c1+2π c , where cos−1 is the inverse of the function cos : [0, π] → [−1, 1]. We notice that the type is invariant under the action of a Heisenberg rigid motion and the regular part of a constant p-mean curvature surface Σ ⊂ H1 is a union of these types of surfaces. The corresponding paths of each type of α are shown on the phase plane (see Figure 1). We express some basic facts as follows. On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 7 c2 > 1 c2 = 1 c2 = 0 3 α α′ Direction Field of a first order system:α'=v,v'=-6αv-4α3-(1.5)2α Figure 1. Direction field for c = 1.5. � If α vanishes, then it is part of a vertical cylinder. � The two concave downward parabolas in red represent α = c 2 sin (cx+ c1) 1− cos (cx+ c1) , c 2 sin (cx+ c1) 0− cos (cx+ c1) , respectively. The one for α = c 2 sin (cx+c1) 1−cos (cx+c1) is above the one for α = c 2 sin (cx+c1) 0−cos (cx+c1) . For surfaces of special type I, we have that α ( π−c1 c ) = 0, α′ (π−c1 c ) = − c2 4 and α →  ∞, if x → −c1 c from the right, −∞, if x → 2π − c1 c from the left, and, for surfaces of special type II in which α has period π, we have that α ( −c1 c ) = α ( π − c1 c ) = 0, α′ ( −c1 c ) = α′ ( π − c1 c ) = −c2 2 and α →  ∞, if x → π − 2c1 2c from the right, −∞, if x → 3π − 2c1 2c from the left. � The closed curves in orange on the phase plane correspond to the family of solutions α(x) = c 2 sin (cx+ c1) c2 − cos (cx+ c1) , 8 H.-L. Chiu, S.-H. Lai and H.-F. Liu where c1, c2 are constants and c2 > 1, which are of type I. There exist zeros for α-function at x = −c1 c , π−c1 c , at which we have that α′ ( −c1 c ) = 1 2 c2 c2 − 1 > 0, α′ ( π − c1 c ) = −1 2 c2 c2 + 1 < 0. There are no singular points for surfaces of type I. � The curves in between the two red concave downward parabolas are of type II. The α- function of type II has a zero at x = π−c1 c , and α′ ( π − c1 c ) = −1 2 c2 c2 + 1 < 0. For surfaces of type II, it can be checked that α →  ∞, if x → −c1 + cos−1 c2 c from the right, −∞, if x → −c1 + 2π − cos−1 c2 c from the left. � The curves beneath the lower concave downward parabola are of type III. There exists a zero for α-function at x = −c1 c , and α′ ( −c1 c ) = 1 2 c2 c2 − 1 < 0. For surfaces of type III, we have α →  −∞, if x → −c1 + cos−1 c2 c from the left, ∞, if x → −c1 + 2π − cos−1 c2 c from the right. 2.1 The Pansu sphere Lemma 2.4 (Pansu sphere). A Pansu sphere given in [1] by f(z) = 1 2λ2 ( λ|z| √ 1− λ2|z|2 + cos−1(λ|z|) ) , |z| ≤ 1 λ , (2.2) of constant p-mean curvature c = 2λ has its α-function of special type I. In fact, we have α = λ sin(2λs) (1− cos(2λs)) , a = −λ√ 1 + α2 , b = 2λ2 √ 1 + α2(1− cos 2λs) . Proof. We parametrize a Pansu sphere by X(s, θ) = cos θ − sin θ 0 sin θ cos θ 0 0 0 1 x(s) y(s) t(s)  = x(s) cos θ − y(s) sin θ x(s) sin θ + y(s) cos θ t(s)  , (2.3) where x(s) = 1 2λ sin(2λs), y(s) = − 1 2λ cos(2λs) + 1 2λ , t(s) = 1 4λ2 sin(2λs)− 1 2λ s+ π 4λ2 , (2.4) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 9 with X(0, θ) = ( 0, 0, π 4λ2 ) and X ( π λ , θ ) = ( 0, 0,− π 4λ2 ) as the North pole and South pole, re- spectively. We then have e1 := Xs, which means that X(s, θ) defines a compatible coordinate system. Moreover, e2 = Je1, where e1 = Xs = ( x′(s) cos θ − y′(s) sin θ, x′(s) sin θ + y′(s) cos θ, t′(s) ) = ( x′(s) cos θ − y′(s) sin θ )̊ e1 + ( x′(s) sin θ + y′(s) cos θ )̊ e2, e2 = − ( x′(s) sin θ + y′(s) cos θ )̊ e1 + ( x′(s) cos θ − y′(s) sin θ )̊ e2. We note that α is a function satisfying αe2 + T = AXs + BXθ, (2.5) for some functions A and B. Direct calculation shows that Xθ = (−x(s) sin θ − y(s) cos θ)̊e1 + (x(s) cos θ − y(s) sin θ)̊e2 + (x2(s) + y2(s))T. Therefore, (2.5) implies −α ( x′(s) sin θ + y′(s) cos θ ) = A ( x′(s) cos θ − y′(s) sin θ ) + B(−x(s) sin θ − y(s) cos θ), α ( x′(s) cos θ − y′(s) sin θ ) = A ( x′(s) sin θ + y′(s) cos θ ) + B(x(s) cos θ − y(s) sin θ), 1 = B ( x2(s) + y2(s) ) . (2.6) The last equation of (2.6) yields B = 1 x2(s)+y2(s) , and hence b = B√ 1 + α2 = 2λ2 √ 1 + α2(1− cos 2λs) . The first two equations of (2.6) indicate −α (( x′2 ) + ( y′2 )) = B ( −xx′ − yy′ ) , which implies α = xx′ + yy′ x2 + y2 . (2.7) In what follows, we claim the above α is one of special solutions. Notice that (2.4) shows x2 + y2 = 1 4λ2 (2− 2 cos(2λs)), and hence (2.7) can be rewritten as α = 1 2 ( lnx2 + y2 )′ = λ sin(2λs) (1− cos(2λs)) . Substituting b and α into (2.6), we have a = A√ 1+α2 = −λ√ 1+α2 . ■ Given a α-function, we have shown [5] that the first fundamental form (a, b) is determined up to two functions h(y) and k(y) as follows. Proposition 2.5. For any α(x, y) = c 2 sin (cx+c1(y)) c2(y)−cos (cx+c1(y)) , the explicit formula for the induced metric on a constant p-mean curvature surface with c as its p-mean curvature and this α as its α-function is given by a = ( − c 2 + c 2c2 (c2 − cos (cx+ c1)) + h(y) |c2 − cos (cx+ c1)| ) 1( 1 + α2 )1/2 , and b = ( ek(y) |c2 − cos (cx+ c1)| ) 1( 1 + α2 )1/2 , for some functions h(y) and k(y). 10 H.-L. Chiu, S.-H. Lai and H.-F. Liu 2.2 The normalization As we normalize the induced metric a and b to be close as much as possible to the metric induced on the horizontal p-minimal plane, we would like to normalize a and b so that they look like the induced metric of the Pansu sphere. Indeed, from the transformation law [5, formula (2.20)], it is easy to see that there exist another compatible coordinates (x̃, ỹ), called normal coordinates such that ã = − c 2( 1 + α2 )1/2 , (2.8) b̃ = c2 2 |c2 − cos (cx+ c1)| ( 1 + α2 )1/2 , (2.9) where c = 2λ. Such normal coordinates are uniquely determined up to a translation. We thus have the following theorem. Theorem 2.6. In normal coordinates (x, y), the functions c1(y) and c2(y) in the expression α(x) = c 2 sin (cx+c1) c2−cos (cx+c1) are unique in the following sense: up to a translation on y, c2(y) is unique, and c1(y) is unique up to a constant. We denote these two unique functions by ζ1(y) = c1(y), ζ2(y) = c2(y). Therefore, the set {ζ1(y), ζ2(y)} constitutes a complete set of invariants for those surfaces (α not vanishing). It is worth our attention that, for the surfaces with c2 > 1, the denominator of the formula for α is never zero. That means the surfaces won’t extend to a surface with singular points. Moreover, if the surface is closed, it must be a closed constant p-mean curvature surface without singular points, which means the surface is of type of torus. This indicates that it is possible to find a Wente-type torus in this class of surfaces. 2.3 The structure of the singular sets In this subsection, we study the structure of the singular set. For the general type, we choose a normal coordinate system (s, θ) such that α = λ sin (2λs+ ζ1(θ)) ζ2(θ)− cos (2λs+ ζ1(θ)) , and a = − λ√ 1 + α2 , b = 2λ2 |ζ2(θ)− cos (2λs+ ζ1(θ))| √ 1 + α2 . Then the singular set is the graph of the function x(θ) = cos−1(ζ2(θ))−ζ1(θ) 2λ . The induced metric I (or the first fundamental form) on the regular part reads I = ds⊗ ds− a b ds⊗ dθ − a b dθ ⊗ ds+ ( 1 + a2 ) b2 dθ ⊗ dθ. Now we use the metric to compute the length of the singular set {( cos−1(ζ2(θ))−ζ1(θ) 2λ , θ )} , where θ belongs to some open interval. Case ζ2(θ) ̸= 1. Let γ(θ) = ( cos−1(ζ2(θ))−ζ1(θ) 2λ , θ ) , which is a parametrization of the singular set. Then the square of the velocity at θ is ∣∣γ′(θ)∣∣2 = [q′(θ)]2 − 2aq′(θ) b + a2 + 1 b2 = [a− bq′(θ)]2 + 1 b2 > 0 for all θ, (2.10) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 11 where q′(θ) = [ cos−1(ζ2(θ))− ζ1(θ) 2λ ]′ = −ζ ′ 2(θ) 2λ √ 1− ζ22 (θ) − ζ ′ 1(θ) 2λ . Formula (2.10) shows that the parametrized curve γ(θ) of the singular set has a positive length. Case ζ2(θ) = 1. We parametrize the singular set by γ(θ) = ( cos−1(1−ϵ)−ζ1(θ) 2λ , θ ) for ϵ > 0. It is easy to see γ′(θ) = (−ζ′1(θ) 2λ , 1 ) . When ε → 0, the metric I = ds⊗ ds− a b ds⊗ dθ − a b dθ ⊗ ds+ ( 1 + a2 ) b2 dθ ⊗ dθ degenerates to Ĩ = ds⊗ ds. Then the square of the velocity at θ is ∣∣γ′(θ)∣∣2 = [ζ′1(θ)] 2 4λ2 . Thus, if ζ1(θ) = c1 and ζ2(θ) = 1, the length of the parametrized curve γ(θ) of the singular set is zero. This result coincides with the singular set for the Pansu sphere being isolated. We conclude the above discussion with the following theorem, an analog of [5, Theorem 1.7]. Theorem 2.7. The singular set of a constant p-mean surface with H = c ̸= 0 is either (1) an isolated point; or (2) a smooth curve. In addition, an isolated singular point only happens on the surfaces of special type I with ζ1 = const, namely, a part of the Pansu sphere containing one of the poles as the isolated singular point. Theorem 2.7 together with [5, Theorem 1.7] are just special cases of [2, Theorem 3.3]. How- ever, we give a computable proof of this result for constant p-mean surfaces. We also have the description of how a characteristic leaf goes through a singular curve, which is called a “go through” theorem in [2]. Suppose p0 is a point in a singular curve. From the above basic facts, we see that a characteristic curve γ always reaches the singular point p0 going a finite distance. From the opposite direction, suppose γ̃ is another characteristic curve that reaches p0. Then the union of γ, p0 and γ̃ forms a smooth curve (we also refer the reader to the proof of [5, Theorem 1.8], they are similar). We thus have the following theorem. Theorem 2.8. Let Σ ⊂ H1 be a constant p-mean surface with H = c ̸= 0. Then the character- istic foliation is smooth around the singular curve in the following sense that each leaf can be extended smoothly to a point on the singular curve. Making use of Theorem 2.8, we have the following result. Theorem 2.9. Let Σ be a constant p-mean surface of type II (III) with H = c ̸= 0. If it can be smoothly extended through the singular curve, then the other side of the singular curve is of type III (II). Therefore, we see that a surface of general type II is always pasted together with a surface of general type III at a singular curve and vice versa. 3 Rotationally invariant surfaces in H1 Let Σ(s, θ) be a rotationally invariant surface in H1 generated by a curve γ(s) = (x(s), 0, t(s)) on the xt-plane, that is, Σ is parametrized by Σ(s, θ) = (x(s) cos θ, x(s) sin θ, t(s)), where x′2 + t′2 = 1. Here ′ means taking a derivative with respect to s. 12 H.-L. Chiu, S.-H. Lai and H.-F. Liu 3.1 The computation of H, α, a and b Now we consider the horizontal (see [3, Definition 1.1]) generating curve γ̃(s) = (x(s) cos θ(s), x(s) sin θ(s), t(s)). Lemma 3.1. γ̃ is horizontal if and only if t′ + x2θ′ = 0. Proof. Note that at the point γ̃(s), e̊1 = ∂ ∂x1 + y1 ∂ ∂z = ∂ ∂x1 + x(s) sin θ(s) ∂ ∂z , e̊2 = ∂ ∂y1 − x1 ∂ ∂z = ∂ ∂y1 − x(s) cos θ(s) ∂ ∂z , and direct computations imply γ̃′(s) = ( x′ cos θ − xθ′ sin θ )̊ e1 + ( x′ sin θ + xθ′ cos θ )̊ e2 + ( t′ + x2θ′ ) T, and hence γ̃′(s) ∈ ξ if and only if t′ + x2θ′ = 0. ■ Let s̃ be the horizontal arc-length of γ̃(s). We can thus re-parametrize the surface Σ(s, θ) to be Σ(s̃, θ̃) = ( x(s) cos θ(s) cos θ̃ − x(s) sin θ(s) sin θ̃, x(s) cos θ(s) sin θ̃ + x(s) sin θ(s) cos θ̃, t(s) ) , with a compatible coordinate system e1 = ∂ ∂s̃ = Σs ∂s ∂s̃ , where Σs = ( x′ cosϕ− xθ′ sinϕ )̊ e1 + ( x′ sinϕ+ xθ′ cosϕ )̊ e2. Moreover, we see |γ̃|′2 = x2x′2+t′2 x2 , so that we may choose s̃ such that ∣∣dγ̃(s̃) ds̃ ∣∣ = 1, that is, ds̃ ds = |γ̃′(s)| = √ x2x′2 + t′2 x . (3.1) Manipulating Σ to be Σ ( s̃, θ̃ ) = ( x(s) cos ( θ(s) + θ̃ ) , x(s) sin ( θ(s) + θ̃ ) , t(s) ) , ( denote ϕ = θ(s) + θ̃ ) and obtain Σs̃ = ds ds̃ ( x′ cosϕ− xθ′ sinϕ )̊ e1 + ds ds̃ ( x′ sinϕ+ xθ′ cosϕ )̊ e2, Σθ̃ = −x sinϕe̊1 + x cosϕe̊2 + x2 ∂ ∂z . Then e1 = Σs̃ = x√ x2x′2 + t′2 ( x′ cosϕ− xθ′ sinϕ )̊ e1 + ds ds̃ ( x′ sinϕ+ xθ′ cosϕ )̊ e2, (3.2) e2 = Je1 = x√ x2x′2 + t′2 ( x′ cosϕ− xθ′ sinϕ )̊ e2 − ds ds̃ ( x′ sinϕ+ xθ′ cosϕ )̊ e1. (3.3) The fact that αe2+T√ 1+α2 ∈ TΣ implies αe2+T = a √ 1 + α2Σs̃+ b √ 1 + α2Σθ̃. Using (3.2), (3.3) and comparing the coefficients of e̊1, e̊2, and T , respectively, one sees a = t′ x √ 1 + α2 √ x2x′2 + t′2 , b = 1 x2 √ 1 + α2 , α = x′√ x2x′2 + t′2 , (3.4) and hence, from the first equation of the integrability conditions (1.1), we have H = − x3 ( x′t′′ − x′′t′ ) + t′3 x { x2x′2 + t′2 }3/2 . (3.5) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 13 3.2 Another understanding of energy E In this subsection, we assume moreover that the rotationally invariant surface Σ is of constant p-mean curvature. We consider the relation between the integrability condition and the energy discussed in Ritoré and Rosales’ paper [8]. The integrability condition as̃ − a b bs̃ + cα√ 1+α2 = 0 indicates that∫ ( as̃ b − a b2 bs̃ + cα b √ 1 + α2 ) ds̃ (3.6) is a constant. Then we have (3.6) computed as a b + c ∫ x2x′√ x2x′2 + t′2 ds̃ = a b + c ∫ xx′ds = a b + λx2, up to a constant, which clearly says that a b +λx2 is constant. The constant a b +λx2 interprets the energy E based on Ritoré’s discussion. Indeed, we have E = a b + λx2 = xt′√ x2x′2 + t′2 + λx2 = ts̃ + λx2, (3.7) that is, ts̃ = E − λx2. One sees t = Es̃− λ ∫ x2ds̃. (3.8) 3.3 The Coddazi-like equation For later use, we calculate 1 + α2 = 1+x2x′2 x2x′2+t′2 and convert α to be of the general form α = x′√ x2x′2 + t′2 = xs̃ x . (3.9) Note that α satisfies the Coddazi-like equation αs̃s̃ + 6ααs̃ + 4α3 + c2α = 0, where c = 2λ. Then this ODE immediately shows xs̃s̃s̃ x + 3 xs̃xs̃s̃ x2 + c2 xs̃ x = 0. (3.10) The equation (3.10) is manipulated to be ( xxs̃s̃ + (xs̃) 2 + c2 2 x 2 ) s̃ = 0, which gives( x2 ) s̃s̃ + c2x2 = k, for some constant k. (3.11) Let u = x2, then (3.11) becomes a second-order inhomogeneous constant coefficient ODE us̃s̃ + c2u = k. (3.12) (I) Suppose c ̸= 0, the homogeneous ODE us̃s̃ + c2u = 0 has the general solution uh given by uh = k1 sin(cs̃) + k2 cos(cs̃) = r cos(cs̃− c1), (3.13) where r = √ k21 + k22 and r sin c1 = k1. One also notes that up = k c2 is a particular solution to (3.12), and hence x2 = u = k c2 + r cos(cs̃− c1). (3.14) 14 H.-L. Chiu, S.-H. Lai and H.-F. Liu (II) When c = 0, it is clear that (3.11) becomes ( x2 ) s̃s̃ = k, which implies x2 = ks̃2 + 2k1s̃+ k2, (3.15) for some constants k, k1 and k2. Example 3.2. If k = 0, k1 = 0, then (3.15) yields x = √ k2. On the other hand, (3.16) suggests 0 = t′3√ k2t′3 = 1√ k2 > 0, which is a contradiction. We conclude that there are no such kinds of p-minimal surfaces (k = 0, k1 = 0) which are rotationally symmetric. In this case, α vanishes so that it corresponds a vertical cylinder surface which is absolutely not p-minimal. 3.4 The relation between k and E Assume that c = 2λ ̸= 0. We write (3.5) as −2λ = x3 ( x′t′′ − x′′t′ ) + t′3 x { x2x′2 + t′2 }3/2 = x2 ( t′ x′ )′ x′2{ x2x′2 + t′2 }3/2 + 1 x4 ( xt′√ x2x′2 + t′2 )3 = I1 + I2, (3.16) where I1 = x2 ( t′ x′ )′ x′2{ x2x′2 + t′2 }3/2 , I2 = 1 x4 ( xt′√ x2x′2 + t′2 )3 . From (3.14), taking a derivative with respect to s, we have x′ = −cr sin (cs̃− c1) √ x2x′2 + t′2 2x2 . (3.17) On the other hand, (3.7) implies t′ = ( E − λx2 )√x2x′2 + t′2 x . (3.18) By means of (3.14), (3.17),(3.18) and (3.1), after direct computations, we have I1 = x2 ( t′ x′ )′ x′2{ x2x′2 + t′2 }3/2 = ( 2x ( E − λx2 ) −cr sin (cs̃− c1) )′( c2r2 sin2 (cs̃− c1) ( x2x′2 + t′2 ) 4x4 ) = 1 4x2 ( −2x2x′ ( 4λx2x′ − 2x′ ( E − λx2 ))(x2 − ( E − λx2 )2 x4x′2 ) + 2 ( E − λx2 )( c2x2 − k )) , and from (3.7), we have I2 = 1 x4 ( xt′√ x2x′2 + t′2 )3 = 1 x4 ( E − λx2 )3 . Therefore, −2λ = I1 + I2 = 1 4x4 (( −4c− 2Ec2 − 2c+ ck ) x4 + ( 8λE2 + 4E − 2Ek ) x2 ) , which implies k = 2cE + 2. On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 15 3.5 Horizontal generating curves for c ̸= 0 In this subsection, we will show that k, and hence the energy E, has a lower bound. A horizontal generating curve of a rotationally invariant constant p-mean curvature surface is a geodesic curve, which is parametrized by γ̃(s̃) =  1 c sin(cs̃) + x0 −1 c cos(cs̃) + 1 c + y0( 1 c2 + cy0 c2 ) sin(cs̃) + x0 c cos(cs̃)− s̃ c + π c2 − x0 c + t0  (3.19) for some (x0, y0, t0), where s̃ is a horizontal arc length parameter. Suppose that γ(s) = (x(s), 0, t(s)) with x ≥ 0 is the corresponding generating curve, we have x2 = ( 1 c sin(cs̃) + x0 )2 + ( −1 c cos(cs̃) + 1 c + y0 )2 = 2 x0 c sin(cs̃)− 2 ( 1 + cy0 c2 ) cos(cs̃) + x20 + ( 1 + cy0 c )2 + 1 c2 = r cos(cs̃− c1) + k c2 , where k = 1 + (cx0) 2 + (1 + cy0) 2 ≥ 1, r = √( 2 x0 c )2 + ( 2 ( 1 + cy0 c2 ))2 = 2 c2 √ (cx0)2 + (1 + cy0)2 = 2 c2 √ k − 1, and c1 is a real number such that sin c1 = 2 x0 c r , cos c1 = − 2( 1+cy0 c2 ) r . 3.6 The invariants ζ1 and ζ2 for surfaces with c ̸= 0 If r = 0, then k = 1, x0 = 0, y0 = −1 c . Thus, (3.19) implies γ̃(s̃) = ( 1 c sin(cs̃),−1 c cos(cs̃),− s̃ c + π c2 + t0 ) , which generates a cylinder. We assume from now on that r ̸= 0. Taking the derivative with respect to s̃ on both sides of (3.14) to have 2xxs̃ = −rc sin(cs̃ − c1). Together with (3.9), we have α of the general form as follows: α = xxs̃ x2 = −rλ sin(cs̃− c1) k c2 + r cos(cs̃− c1) = λ sin(cs̃− c1) c2 − cos(cs̃− c1) , where c2 = − k rc2 . In this subsection, we want to normalize a and b such that they have the forms looking as (2.8) and (2.9), respectively. Together with (3.4), (3.14) and (3.7), we have a = t′ x √ 1 + α2 √ x2x′2 + t′2 = ( E x2 − λ ) 1√ 1 + α2 , b = 1 x2 √ 1 + α2 = 1 k c2 + r cos(cs̃− c1) 1√ 1 + α2 . 16 H.-L. Chiu, S.-H. Lai and H.-F. Liu Thus we choose the normal coordinates { s̄, θ̄ } with s̄ = s̃ + Γ ( θ̃ ) , θ̄ = Ψ ( θ̃ ) , such that Γ′(θ̃) = −E, Ψ′(θ̃) = −2λ2r. Then we have ā = −λ√ 1 + ᾱ2 , b̄ = 2λ2( − k rc2 − cos(cs̃− c1) ) 1√ 1 + ᾱ2 , with ᾱ = λ sin(cs̃− c1) c2 − cos(cs̃− c1) = λ sin ( cs̄− c1 − Eθ̄ rλ ) c2 − cos ( cs̄− c1 − Eθ̄ rλ ) , that is, ζ1 ( θ̄ ) = −c1 − 2Eθ̄ cr , ζ2 ( θ̄ ) = c2 = − k rc2 = −2cE + 2 c2r . (3.20) If E = 0, then k = 2, thus the surface has the generating curve defined by x2 = 2 c2 + r cos (cs̃− c1) = r ( 2 c2r + cos (cs̃− c1) ) , t = −λ ( 2 c2 s̃+ r c sin (cs̃− c1) ) , with ζ1 ( θ̄ ) = −c1, ζ2 ( θ̄ ) = − 2 c2r < 0. Therefore, we see that x2 ≥ 0 ⇔ cos (cs̃− c1) ≥ ζ2 ( θ̄ ) , which means that the generating curve (x, t) is defined on the whole R if and only if ζ2 ( θ̄ ) ≤ −1. In particular, if ζ2 ( θ̄ ) = −1, it is the Pansu sphere. If E ̸= 0, then k = 2cE + 2 and (3.20) implies that ζ ′1 ( θ̄ ) = −2E cr > ζ2 ( θ̄ ) . (3.21) For any constants η1 and η2 with η1 > η2, we obtain the unique solution to the equation system −2E cr = η1, −2cE + 2 c2r = η2. 3.7 The allowed values of k and E with c = 0 In this subsection, we shall show what possible values can k and E attain. Assume that c = 2λ = 0. We write (3.5) as 0 = x3 ( x′t′′ − x′′t′ ) + t′3 x { x2x′2 + t′2 }3/2 = x2 ( t′ x′ )′ x′2{ x2x′2 + t′2 }3/2 + 1 x4 ( xt′√ x2x′2 + t′2 )3 = I1 + I2. Taking a derivative of (3.15) with respect to s, we get x′ = (ks̃+ k1) √ x2x′2 + t′2 x2 . (3.22) On the other hand, from (3.7), we have t′ = E √ x2x′2 + t′2 x . (3.23) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 17 By means of (3.15), (3.22),(3.23) and (3.1), a direct computation gives I1 = x2 ( t′ x′ )′ x′2{ x2x′2 + t′2 }3/2 = 1 x2 ( E ( x2 − E2 ) x2 − kE ) , and (3.7) implies I2 = 1 x4 ( xt′√ x2x′2 + t′2 )3 = 1 x4 E3. Therefore, 0 = I1 + I2 = E(1−k) x2 , which says that E = 0 or k = 1. (3.24) The equation (3.7) says that t and Es̃ are differed only by a constant. If E = 0, then t is constant, which gives us that Σ is a plane that is perpendicular to t-axis. 3.8 The invariants ζ1 and ζ2 for surfaces with c = 0 and E ̸= 0 If E = 0, the surface is a perpendicular plane to the t-axis. Therefore, in this subsection, we assume that E ̸= 0, and thus, from (3.24), we have k = 1. Then one rewrites α to be α = xxs̃ x2 = s̃+ k1 (s̃+ k1)2 + ( k2 − k21 ) . From (3.15), we have 1 x2 = α s̃+k1 > 0. We want to normalize a and b such that they have the form specified in [5, Theorem 1.3]. Together with (3.4) and (3.7), we have a = t′ x √ 1 + α2 √ x2x′2 + t′2 = ( E x2 ) 1√ 1 + α2 = Eb, b = 1 x2 √ 1 + α2 = α (s̃+ k1) √ 1 + α2 = |α| (|s̃+ k1|) √ 1 + α2 . Thus we choose the normal coordinates { s̄, θ̄ } with s̄ = s̃+Γ ( θ̃ ) , θ̄ = Ψ ( θ̃ ) such that Γ′(θ̃) = −E, Ψ′(θ̃) = 1. Then we have ā = 0, b̄ = |ᾱ| |s̃+ k1| √ 1 + ᾱ2 with ᾱ = s̃+ k1 (s̃+ k1)2 + ( k2 − k21 ) = s̄− Γ ( θ̃ ) + k1 (s̄− Γ ( θ̃ ) + k1)2 + ( k2 − k21 ) , that is, ζ1 ( θ̄ ) = k1 + Eθ̄, which is linear in θ̄, ζ2 ( θ̄ ) = k2 − k21, which is a constant, denoted as ζ2. From (3.15) and (3.7), we conclude that the generating curve is defined by x2 = (s̃+ k1) 2 + ζ2, t = Es̃, up to a constant. (3.25) 18 H.-L. Chiu, S.-H. Lai and H.-F. Liu Remark 3.3. We remark that for λ = 0, two kinds of p-minimal surfaces are presented depend- ing on the energy E. When E = 0, t in (3.16) is constant and then one obtains a plane that is perpendicular to the t-axis. On the other hand, if E ̸= 0, we have p-minimal surfaces generated by curves defined by (3.25). For λ ̸= 0, substituting (3.14) in (3.8), we see t = Es̃− λ ∫ ( k c2 + √ k21 + k22 cos(cs̃− c1) ) ds̃ = ( E − k 4λ ) s̃− √ k21 + k22 2 sin(2λs̃− c1) + const. In the case λ ̸= 0, we give the following two examples. Example 3.4. We choose k1, k2 in (3.13) so that √ k21 + k22 = − k c2 , and then (3.14) implies x = ± √ 2k 2λ sin ( λs̃− c1 2 ) . Moreover, if E = 0, then t = − k 4λ s̃+ k 8λ2 sin(2λs̃− c1), which is a scaling sphere. The other two integrability conditions (see [5, equation (2.13)]) are −bs̃ b = 2α+ ααs̃ 1 + α2 , aHs̃ + bHθ̃ = αs̃s̃ + 6ααs̃ + 4α3 + αH2 √ 1 + α2 . (3.26) We rewrite the first equation in (3.26) as 2α+ ααs̃ 1 + α2 + bs̃ b = 0. Integrating on both sides to see that∫ ( 2α+ ααs̃ 1 + α2 + bs̃ b ) ds̃ is a constant. More precisely, in terms of x, x′, t, t′, we write∫ 2 ( α+ ααs̃ 1 + α2 + bs̃ b ) ds̃ = ∫ ( 2 xs̃ x + ααs̃ 1 + α2 + bs̃ b ) ds̃ = ln ( bx2 √ 1 + α2 ) + const. The conclusion is that ln ( bx2 √ 1 + α2 ) is a constant, which also follows from (3.4). Suppose H is constant. The second equation of (3.26) is exactly αs̃s̃+6ααs̃+4α3+αH2 = 0. Using (3.9), this ODE becomes (3.10), which has been discussed previously. 4 The construction of constant p-mean curvature surfaces In this section, we construct constant p-mean curvature surfaces by perturbing the Pansu sphere in some way. Recall the parametrization of the Pansu sphere (2.3). For each fixed angle θ, the curve lθ defined by lθ(s) = (x(s) cos θ − y(s) sin θ, x(s) sin θ + y(s) cos θ, t(s)) is a geodesic with curvature 2λ. Let C be an arbitrary curve C : R → H1 given by C(θ) = (x1(θ), x2(θ), x3(θ)). For each fixed θ, we translate lθ by C(θ), so that the curve LC(θ)(lθ) is also a geodesic curve with curvature 2λ. Then the union of all these curves ΣC = ∪θLC(θ)(lθ) constitutes a constant p-mean curvature surface with a parametrization Y (s, θ) = (x1(θ) + (x(s) cos θ − y(s) sin θ ) , x2(θ) + (x(s) sin θ + y(s) cos θ), x3(θ) + t(s) + x2(θ)(x(s) cos θ − y(s) sin θ) − x1(θ)(x(s) sin θ + y(s) cos θ)). (4.1) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 19 By a straightforward computation, and notice that x′(s) cos θ − y′(s) sin θ = cos (2λs+ θ), x′(s) sin θ + y′(s) cos θ = sin (2λs+ θ), x(s) cos θ − y(s) sin θ = − 1 2λ (sin θ − sin (2λs+ θ)), x(s) sin θ + y(s) cos θ = 1 2λ (cos θ − cos (2λs+ θ)), x2(s) + y2(s) = 1 2λ2 (1− cos 2λs), we have Ys = ( x′(s) cos θ − y′(s) sin θ )̊ e1 + ( x′(s) sin θ + y′(s) cos θ )̊ e2|Y (s,θ) = cos (2λs+ θ)̊e1 + sin (2λs+ θ)̊e2, Yθ = ( x′1(θ)− x(s) sin θ − y(s) cos θ )̊ e1 + ( x′2(θ) + x(s) cos θ − y(s) sin θ )̊ e2 + ( Θ(C′(θ)) + 2x′2(θ) ( x(s) cos θ − y(s) sin θ ) − 2x′1(θ) ( x(s) sin θ + y(s) cos θ ) + x2(s) + y2(s) ) T = ( x′1(θ)− 1 2λ (cos θ − cos (2λs+ θ)) ) e̊1 + ( x′2(θ)− 1 2λ (sin θ − sin (2λs+ θ)) ) e̊2 + ( Θ(C′(θ))− x′2(θ) 1 λ (sin θ − sin (2λs+ θ))− x′1(θ) 1 λ (cos θ − cos (2λs+ θ)) + 1 2λ2 (1− cos 2λs) ) T. Therefore, Ys ∧ Yθ = [ x′2(θ) cos (2λs+ θ)− x′1(θ) sin (2λs+ θ) + sin 2λs 2λ ] e̊1 ∧ e̊2 + [cos (2λs+ θ) 〈 Yθ, T 〉 ]̊e1 ∧ T + [sin (2λs+ θ) 〈 Yθ, T 〉 ]̊e2 ∧ T = [ A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs ] e̊1 ∧ e̊2 + [cos (2λs+ θ) 〈 Yθ, T 〉 ]̊e1 ∧ T + [sin (2λs+ θ) 〈 Yθ, T 〉 ]̊e2 ∧ T, (4.2) where A(θ) = x′2(θ) cos θ − x′1(θ) sin θ, B(θ) = x′2(θ) sin θ + x′1(θ) cos θ,〈 Yθ, T 〉 = 1 λ [( B(θ)− 1 2λ ) cos 2λs+A(θ) sin 2λs+D(θ) ] , D(θ) = λΘ(C′(θ)) + ( 1 2λ −B(θ) ) . (4.3) From (4.2), we conclude that Y is an immersion if and only if either[ A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs ] ̸= 0 or 〈 Yθ, T 〉 ̸= 0. For the constructed surface Y in (4.1), we always assume it is defined on a region such that Y is an immersion and ΣC is the constant p-mean curvature surface defined by such an immersion Y . A point p ∈ ΣC is a singular point if and only if 〈 Yθ, T 〉 = 0. Thus at a singular point, we must have [ A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs ] ̸= 0. 20 H.-L. Chiu, S.-H. Lai and H.-F. Liu Now, we proceed to compute the invariants for Y . From the construction of Y , we see that (s, θ) is a compatible coordinate system and we are able to choose the characteristic direc- tion e1 = Ys, and hence e2 = Je1 = − sin (2λs+ θ)̊e1 + cos (2λs+ θ)̊e2. The α-function is a function defined on the regular part that satisfies αe2 + T = a √ 1 + α2Ys + b √ 1 + α2Yθ = a √ 1 + α2e1 + b √ 1 + α2Yθ for some functions a and b. This is equivalent to, comparing the alike terms, −α sin (2λs+ θ) = a √ 1 + α2 cos (2λs+ θ) + b √ 1 + α2 ( x′1(θ)− 1 2λ (cos θ − cos (2λs+ θ)) ) , α cos (2λs+ θ) = a √ 1 + α2 sin (2λs+ θ) + b √ 1 + α2 ( x′2(θ)− 1 2λ (sin θ − sin (2λs+ θ)) ) , 1 = b √ 1 + α2 〈 Yθ, T 〉 . We thus have a = −2λ ( x′1(θ) cos(2λs+ θ) + x′2(θ) sin(2λs+ θ) ) − (1− cos 2λs) 2λ √ 1 + α2⟨Yθ, T ⟩ , b = 1√ 1 + α2 〈 Yθ, T 〉 , α = x′2(θ) cos (2λs+ θ)− x′1(θ) sin (2λs+ θ) + sin 2λs 2λ〈 Yθ, T 〉 = λ A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs( B(θ)− 1 2λ ) cos 2λs+A(θ) sin 2λs+D(θ) . (4.4) Let V = ( A(θ), 1 2λ−B(θ) ) and ∥V ∥ = √ [A(θ)]2 + [ 1 2λ −B(θ) ]2 . If V = 0, then α = 0. If V ̸= 0, then we can write V ∥V ∥ = (sin ζ(θ), cos ζ(θ)), for some function ζ(θ). The functions α, a, and b can be further written as α = λ sin ζ(θ) cos 2λs+ cos ζ(θ) sin 2λs − cos ζ(θ) cos 2λs+ sin ζ(θ) sin 2λs+ D(θ) ∥V ∥ = λ sin ( 2λs+ ζ(θ) ) G(θ)− cos ( 2λs+ ζ(θ) ) , a = −2λ[sin ζ(θ) sin(2λs)− cos ζ(θ) cos 2λs]− 1 ∥V ∥ 2 √ 1 + α2 [D(θ) ∥V ∥ − cos(2λs+ ζ(θ)) ] = 2λ∥V ∥ cos(2λs+ ζ(θ))− 1 2∥V ∥ √ 1 + α2[G(θ)− cos(2λs+ ζ(θ))] , b = λ ∥V ∥√ 1 + α2 [D(θ) ∥V ∥ − cos(2λs+ ζ(θ)) ] = λ ∥V ∥√ 1 + α2[G(θ)− cos(2λs+ ζ(θ))] , where G(θ) = D(θ) ∥V ∥ = D(θ)√ (A(θ))2 + ( 1 2λ −B(θ) )2 . (4.5) On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 21 Next, we normalize the three invariants α, a, and b. Firstly, we choose another compatible coordinates (s̃ = s+ Γ(θ), θ̃ = Ψ(θ)), for some Γ(θ) and Ψ(θ). From the transformation law of the induced metric ã = a+ bΓ′(θ), b̃ = bΨ′(θ), this can be chosen so that Γ′(θ) = −2λ∥V (θ)∥G(θ) + 1 2λ = 1 2λ −D(θ), or equivalently, Γ(θ) = θ 2λ − ∫ D(θ)dθ. If we further choose Ψ such that θ̃ = Ψ(θ) = 2λ ∫ ∥V (θ)∥dθ, then in terms of the compatible coordinates ( s̃, θ̃ ) , the three invariants read ã = −λ√ 1 + α̃2 , b̃ = 2λ2 √ 1 + α̃2 { G ( Ψ−1 ( θ̃ )) − cos [ 2λs̃− 2λΓ ( Ψ−1 ( θ̃ )) + ζ ( Ψ−1 ( θ̃ ))]} , α̃ = λ sin ( 2λs̃− 2λΓ(θ) + ζ ( Ψ−1 ( θ̃ ))) G ( Ψ−1 ( θ̃ )) − cos [ 2λs̃− 2λΓ ( Ψ−1 ( θ̃ )) + ζ ( Ψ−1 ( θ̃ ))] , where D and G are defined in (4.3) and (4.5), respectively. We summarize the above discussion as a theorem in the following. Theorem 4.1. The coordinate system (s, θ) for Y in (4.1) is compatible. If V = 0, then α = 0. If V ̸= 0, then the new coordinate system ( s̃, θ̃ ) , where s̃ = s+ Γ(θ), θ̃ = Ψ(θ), with Γ(θ) = θ 2λ − ∫ D(θ)dθ, Ψ(θ) = 2λ ∫ ∥V (θ)∥dθ, is normal. In terms of the normal coordinates, the invariants of Y are given by ζ1 ( θ̃ ) = ζ ( Ψ−1 ( θ̃ )) − 2λΓ ( Ψ−1 ( θ̃ )) , ζ2 ( θ̃ ) = G ( Ψ−1 ( θ̃ )) . (4.6) Particularly, in order to have constant ζ1 ( θ̃ ) and nonzero constant ζ2 ( θ̃ ) , Theorem 4.1 sug- gests the constant p-mean curvature surfaces deformed by curves C(θ) = (x1(θ), x2(θ), x3(θ)) = ( r λ sin θ,− r λ cos θ, r(1− r) λ2 θ ) , (4.7) where r ̸= 1 2 . More precisely, we have the following proposition. Proposition 4.2. For any curve C(θ) defined as (4.7), the deformed surface Y (s, θ) has both constant invariants ζ1 ( θ̃ ) and ζ2 ( θ̃ ) ̸= 0. Proof. We argue by assuming ζ2 ( θ̃ ) = ζ2 is a constant, x1(θ) = r λ sin θ , and x2(θ) = − r λ cos θ for any r ̸= 1 2 . Then (4.3) implies A(θ) = 0, B(θ) = r λ , which leads to ∥V ∥ = |1−2r| 2λ . The second equation of (4.6) shows that D(θ) = ζ2∥V ∥, and hence ζ1 ( θ̃ ) = sin−1 ( A(θ) ∥V ∥ ) − 2λ ( θ 2λ − ∫ D(θ)dθ ) = −θ + ∫ ζ2|1− 2r|dθ = (ζ2|1− 2r| − 1)θ + const. In order to have ζ1 ( θ̃ ) being constant, we must have ζ2|1− 2r| = 1. It is clear to see that ζ2 ̸= 0 and r ̸= 0. The system (4.6) immediately shows D(θ) = 1 2λ , which gives x′3(θ) = r(1−r) λ2 , by (4.3). Namely, x3(θ) = r(1−r) λ2 θ + const. Moreover, the new coordinates can be obtained by θ̃ = Ψ(θ) = |1− 2r|θ + const and Γ(θ), up to a constant. ■ 22 H.-L. Chiu, S.-H. Lai and H.-F. Liu 5 Examples It is easy to see that the Pansu sphere can be obtained by deforming the following curves C1(θ) = (0, 0, const) or C2(θ) = ( 1 λ sin θ,− 1 λ cos θ, const ) . Using a similar idea as Theorem 4.1 and Proposition 4.2, we obtain curves C(θ) that result in constant p-mean curvature surfaces with constant ζ2 and linear ζ1 ( θ̃ ) in Sections 5.1 and 5.3. We collect C(θ) in Tables 1 and 2 as follows. Table 1. Examples of C(θ) for constant p-mean curvature surfaces. C(θ) constant ζ1 linear ζ1 ζ2 > 1 ( r λ sin θ,− r λ cos θ, r(1−r) λ2 θ ) 0 < r < 1, r ̸= 1 2 ζ2 = 1 |1−2r| m ̸= 1: (x1(θ), x2(θ), x3(θ)) x1(θ) = sin θ 2λ − sin((m−1)θ) 2λk(m−1) x2(θ) = − cos θ 2λ − cos((m−1)θ) 2λk(m−1) x3(θ) = 1+k2(m−1) 4λ2k2(m−1) θ − sin(mθ) 4λ2k(m−1) m = 1: ( sin θ 2λ − θ 2λk ,− cos θ 2λ , kθ−θ cos θ 4λ2k ) ζ1 = mθ + const and ζ2 = k > 0 ζ2 = 1 Pansu sphere 0 < ζ2 < 1 ( r λ sin θ,− r λ cos θ, r(1−r) λ2 θ ) r < 0 or r > 1 ζ2 = 1 |1−2r| ζ2 = 0 ( β 4λ , 0, β 4λ − θ 4λ2 ) β = ln | sec θ + tan θ| ζ1 = 0 ( cos θ, sin θ,− ( θ + θ 2λ2 )) ζ1 = −θ + const Table 2. Examples of C(θ) for p-minimal surfaces. C(θ) constant ζ1 linear ζ1 ζ2 > 0 type I (r sin θ,−r cos θ, z(θ)) z′(θ) + r2 > 0 ζ1 = −rθ ζ2 < 0 type II, III (r sin θ,−r cos θ, z(θ)) z′(θ) + r2 < 0 ζ1 = −rθ special type I degenerate case: ( −θ, 0, sin(2θ)−2θ 4 ) or entire graph: u = 0 special type II u = xy + g(y) 5.1 Examples of constant p-mean curvature surfaces Proposition 5.1. Given any curve C(θ) = ( 1 λ sin θ,− 1 λ cos θ, k − 1 2λ2 θ + const ) , the deformed surface Y (s, θ) has the invariants ζ1 ( θ̃ ) = (k − 1)θ̃ + const and ζ2 ( θ̃ ) = k, where k ∈ R. On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 23 Remark 5.2. It is easy to see that the surfaces obtained by curves given in Proposition 5.1 are not rotationally symmetric since ζ ′1 = k − 1 < ζ2 by (3.21). Proposition 5.3. For any constant k > 0 and m, there exist constant p-mean curvature sur- faces Y (s, θ) defined as (4.1) with invariants ζ1(θ) = mθ + const and ζ2 = k. Proof. It suffices to solve the system (4.6). In order to obtain a surface with linear ζ1(θ) = mθ for any given nonzero constant ζ2 = k, we assume A(θ) = 1 2λk sin(mθ) and 1 2λ −B(θ) = 1 2λk cos(mθ). (5.1) It results in ∥V ∥ = 1 2λk , and ζ1(θ) = sin−1 ( A(θ) ∥V ∥ ) − 2λ ( θ 2λ − ∫ D(θ) dθ ) = mθ − θ + 2λ ∫ ζ2(θ)∥V ∥ dθ = mθ − θ + 2λk ∫ 1 2λk dθ = mθ + const. Next we solve for x′1(θ) and x′2(θ) from (4.3), that is, 1 2λk sin(mθ) = x′2(θ) cos θ − x′1(θ) sin θ, 1 2λ − 1 2λk cos(mθ) = x′2(θ) sin θ + x′1(θ) cos θ. It is easy to see that x′1(θ) = 1 2λ cos(θ)− 1 2λk cos((m− 1)θ), x′2(θ) = 1 2λ sin(θ) + 1 2λk sin((m− 1)θ), and hence for m ̸= 1, x1(θ) = 1 2λ sin(θ)− 1 2λk(m− 1) sin((m− 1)θ) + const, x2(θ) = − 1 2λ cos(θ)− 1 2λk(m− 1) cos((m− 1)θ) + const. (5.2) The equation (4.3) also suggests x′3(θ) = 1 + k2(m− 1) 4λ2k2(m− 1) − m cos(mθ) 4λ2k(m− 1) , and then we have x3(θ) = 1 + k2(m− 1) 4λ2k2(m− 1) θ − sin(mθ) 4λ2k(m− 1) + const. (5.3) Therefore, deforming such curves C(θ) = (x1(θ), x2(θ), x3(θ)) defined by (5.2) and (5.3) gives surfaces with nonzero ζ2 = k and linear ζ1(θ) = mθ + const for all m ̸= 1. When m = 1, direct computations from (5.1) imply x1(θ) = 1 2λ sin(θ)− θ 2λk + const, x2(θ) = − 1 2λ cos(θ) + const, x3(θ) = kθ − θ cos θ 4λ2k . ■ Example 5.4. If C(θ) = (x1(θ), x2(θ), x3(θ)) = ( 1 4λ ln | sec θ + tan θ|+ c3, c4, c5 4λ ln | sec θ + tan θ| − 1 4λ2 θ + c6 ) , then ζ1 ( θ̃ ) = 0, ζ2 ( θ̃ ) = 0. 24 H.-L. Chiu, S.-H. Lai and H.-F. Liu 5.2 Basic properties of surfaces of special type I For p-minimal surfaces of special type I, we have the first fundamental form, in terms of normal coordinates (x, y), I = dx⊗ dx+ ( 1 + α2 α4 ) dy ⊗ dy, so that I degenerates along the curve where α blows up. Recall that the parametrization of the surface Y is Y (r, θ) = (x(θ) + r cos θ, y(θ) + r sin θ, z(θ) + ry(θ) cos θ − rx(θ) sin θ). We have Yr = (cos θ, sin θ, y(θ) cos θ − x(θ) sin θ), Yθ = ( x′(θ)− r sin θ, y′(θ) + r cos θ, ∗ ) , where ∗ = z′(θ) + ry′(θ) cos θ − y(θ) sin θ − x′(θ) sin θ − x(θ) cos θ. Then Yr × Yθ = ∣∣∣∣∣∣ i j k cos θ sin θ y(θ) cos θ − x(θ) sin θ x′(θ)− r sin θ y′(θ) + r cos θ ∗ ∣∣∣∣∣∣ = ρ ( sin θ ( y′(θ) cos θ − x′(θ) sin θ ) − y(θ), − cos θ ( y′(θ) cos θ − x′(θ) sin θ ) + x(θ), 1 ) , where ρ = r + ( y′(θ) cos θ − x′(θ) sin θ ) . For p-minimal surfaces of special type I, we have α = 1 r + ( y′(θ) cos θ − x′(θ) sin θ ) . Therefore, Yr and Yθ are linearly dependent along the curve when α blows up. For constant p-mean curvature surfaces of special type I, (4.2) and (4.3) immediately imply that Ys ∧ Yθ = 0 if and only if 0 = A(θ) cos 2λs+ ( 1 2λ −B(θ) ) sin 2λs, −D(θ) = − ( 1 2λ −B(θ) ) cos 2λs+A(θ) sin 2λs, that is,( cos 2λs sin 2λs sin 2λs − cos 2λs )( A(θ)/∥V ∥( 1 2λ −B(θ) ) /∥V ∥ ) = ( 0 −G(θ) ) . This implies that Ys ∧ Yθ = 0 holds if and only if G(θ) = ±1, namely, it happens only on the surface Y of special type I at points where the function α blows up. 5.3 Examples of p-minimal surfaces In what follows, we give some p-minimal surfaces of special type II (i.e., ζ2 < 0 and linear ζ1). We first recall in [5] that C(θ) = (x(θ), y(θ), z(θ)) satisfying ζ1(θ) = −Γ(θ) + y′(θ) cos θ − x′ sin θ, ζ2(θ) = z′(θ) + x(θ)y′(θ)− y(θ)x′(θ)− ( y′(θ) cos θ − x′(θ) sin θ )2 , where Γ(θ) = ∫ x′(θ) cos θ + y′(θ) sin θdθ, will result in a p-minimal surface. For any nonzero r ∈ R, if x(θ) = r sin θ and y(θ) = −r cos θ, then Γ(θ) = rθ (up to a constant), ζ1(θ) = −rθ, and ζ2(θ) = z′(θ) + r2. We choose z(θ) such that z′(θ) + r2 < 0 to have negative ζ2. On Invariants of Constant p-Mean Curvature Surfaces in the Heisenberg Group H1 25 Acknowledgements The first author’s research was supported in part by NSTC 112-2115-M-007-009-MY3. The second author’s research was supported in part by NSTC 110-2115-M-167-002-MY2 and NSTC 112-2115-M-167-002-MY2. The third author’s research was supported in part by NSTC 112- 2628-M-032-001-MY4. We all thank the anonymous referees for carefully reading our manuscript and their insightful comments and suggestions for improving the article. References [1] Cheng J.-H., Chiu H.-L., Hwang J.-F., Yang P., Umbilicity and characterization of Pansu spheres in the Heisenberg group, J. Reine Angew. Math. 738 (2018), 203–235, arXiv:1406.2444. [2] Cheng J.-H., Hwang J.-F., Malchiodi A., Yang P., Minimal surfaces in pseudohermitian geometry, Ann. Sc. Norm. Super. Pisa Cl. Sci. 4 (2005), 129–177, arXiv:math.DG/0401136. [3] Chiu H.-L., Huang Y.-C., Lai S.-H., An application of the moving frame method to integral geometry in the Heisenberg group, SIGMA 13 (2017), 097, 27 pages, arXiv:1509.00950. [4] Chiu H.-L., Lai S.-H., The fundamental theorem for hypersurfaces in Heisenberg groups, Calc. Var. Partial Differential Equations 54 (2015), 1091–1118. [5] Chiu H.-L., Liu H.-F., A characterization of constant p-mean curvature surfaces in the Heisenberg group H1, Adv. Math. 405 (2022), 08514, 50 pages, arXiv:2101.11780. [6] Dragomir S., Tomassini G., Differential geometry and analysis on CR manifolds, Progr. Math., Vol. 246, Birkhäuser, Boston, MA, 2006. [7] Polyanin A.D., Zaitsev V.F., Handbook of exact solutions for ordinary differential equations, 2nd ed., Chapman & Hall/CRC, Boca Raton, FL, 2003. [8] Ritoré M., Rosales C., Rotationally invariant hypersurfaces with constant mean curvature in the Heisenberg group Hn, J. Geom. Anal. 16 (2006), 703–720, arXiv:math.DG/0504439. https://doi.org/10.1515/crelle-2015-0044 https://arxiv.org/abs/1406.2444 http://www.numdam.org/item/ASNSP_2005_5_4_1_129_0/ http://www.numdam.org/item/ASNSP_2005_5_4_1_129_0/ https://arxiv.org/abs/math.DG/0401136 https://doi.org/10.3842/SIGMA.2017.097 https://arxiv.org/abs/1509.00950 https://doi.org/10.1007/s00526-015-0818-1 https://doi.org/10.1007/s00526-015-0818-1 https://doi.org/10.1016/j.aim.2022.108514 https://arxiv.org/abs/2101.11780 https://doi.org/10.1007/0-8176-4483-0 https://doi.org/10.1007/BF02922137 https://arxiv.org/abs/math.DG/0504439 1 Introduction 2 Solutions to the Codazzi-like equation 2.1 The Pansu sphere 2.2 The normalization 2.3 The structure of the singular sets 3 Rotationally invariant surfaces in H_1 3.1 The computation of H, alpha, a and b 3.2 Another understanding of energy E 3.3 The Coddazi-like equation 3.4 The relation between k and E 3.5 Horizontal generating curves for c neq 0 3.6 The invariants zeta_1 and zeta_2 for surfaces with c neq 0 3.7 The allowed values of k and E with c=0 3.8 The invariants zeta_1 and zeta_2 for surfaces with c=0 and E neq 0 4 The construction of constant p-mean curvature surfaces 5 Examples 5.1 Examples of constant p-mean curvature surfaces 5.2 Basic properties of surfaces of special type I 5.3 Examples of p-minimal surfaces References
id nasplib_isofts_kiev_ua-123456789-212880
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 1815-0659
language English
last_indexed 2026-03-21T18:31:18Z
publishDate 2025
publisher Інститут математики НАН України
record_format dspace
spelling Chiu, Hung-Lin
Lai, Sin-Hua
Liu, Hsiao-Fan
2026-02-13T13:50:02Z
2025
On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁. Hung-Lin Chiu, Sin-Hua Lai and Hsiao-Fan Liu. SIGMA 21 (2025), 011, 25 pages
1815-0659
2020 Mathematics Subject Classification: 53A10; 53C42; 53C22; 34A26
arXiv:2309.14697
https://nasplib.isofts.kiev.ua/handle/123456789/212880
https://doi.org/10.3842/SIGMA.2025.011
One primary objective in submanifold geometry is to discover fascinating and significant classical examples of ₁. In this paper, which relies on the theory we established in [Adv. Math. 405 (2022), 08514, 50 pages, arXiv:2101.11780] and utilizing the approach we provided for constructing constant -mean curvature surfaces, we have identified intriguing examples of such surfaces. Notably, we present a complete description of rotationally invariant surfaces of constant p-mean curvature and shed light on the geometric interpretation of the energy with a lower bound.
The first author’s research was supported in part by NSTC 112-2115-M-007-009-MY3. The second author’s research was supported in part by NSTC 110-2115-M-167-002-MY2 and NSTC 112-2115-M-167-002-MY2. The third author’s research was supported in part by NSTC 1122628-M-032-001-MY4. We all thank the anonymous referees for carefully reading our manuscript and their insightful comments and suggestions for improving the article.
en
Інститут математики НАН України
Symmetry, Integrability and Geometry: Methods and Applications
On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
Article
published earlier
spellingShingle On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
Chiu, Hung-Lin
Lai, Sin-Hua
Liu, Hsiao-Fan
title On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
title_full On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
title_fullStr On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
title_full_unstemmed On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
title_short On Invariants of Constant -Mean Curvature Surfaces in the Heisenberg Group ₁
title_sort on invariants of constant -mean curvature surfaces in the heisenberg group ₁
url https://nasplib.isofts.kiev.ua/handle/123456789/212880
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