PROCEEDINGS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 124, Number 10, October 1996
MULTIPLE GEOMETRICALLY DISTINCT CLOSED NONCOLLISION ORBITS OF FIXED ENERGY FOR N-BODY TYPE PROBLEMS WITH STRONG FORCE POTENTIALS ZHANG SHIQING (Communicated by James Glimm) Abstract. Using the equivariant Ljusternik-Schnirelmann theory, we prove that there are at least 2(N − 1)2N−2 geometrically distinct noncollision orbits with prescribed energy for a class of planar N-body type problems with strong force potentials.
1. Introduction In the last few years, variational methods have started to be used for studying the periodic solutions for singular Hamiltonian systems. Existence of periodic solutions with prescribed period for some classes of N-body problems has been proved in [2]–[6], [9], [11]. On the contrary, we know of only one paper ([1]) obtaining the results in the large concerning the existence of one periodic solution with prescribed energy, and except for the author’s preprint paper ([14]), there is no result in the large dealing with the existence of multiple geometrically distinct closed noncollision orbits. This is mainly because the N-body problems in Rk have S 1 ×O(k) symmetry, where O(k) is the rotational symmetry group of order k. In order to obtain multiple geometrically distinct trajectories, we must consider the effects of the group S 1 × O(k); this results in some problems in topology. Using the equivariant Ljusternik-Schnirelmann theory, we obtain the result in the large concerning multiple geometrically distinct closed noncollision orbits for a class of planar N-body problems with strong force potentials. The key observations of the proof about our results are that the variational functional satisfies the PalaisSmale condition and that we must construct a special set such that its S 1 × O(2) equivariant category is easily computed and the superbound of the functional on the set is also easily estimated. Many variational methods’ papers deal with N-body type problems, but assume conditions on the potential that exclude the actual N-body problem (i.e. gravitational potential). This paper is no exception, but in another paper ([14]), the author does deal with gravitational potentials. Received by the editors January 11, 1995. 1991 Mathematics Subject Classification. Primary 34C25, 34C15, 58F05. Key words and phrases. N-body type problems with fixed energy, geometrically distinct noncollision periodic orbits, equivariant Ljusternik-Schnirelmann theory. c
1996 American Mathematical Society
3039
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3040
ZHANG SHIQING
We set Ω = R2 \ {0} and consider a potential V of the form: 1 X (1.1) Vij (xi − xj ), V (x) = V (x1 , . . . , xN ) = 2 1≤i6=j≤N
where xi ∈ R , x = (x1 , . . . , xN ) ∈ (R ) and Vij ∈ C 1 (Ω, R) (i, j = 1, . . . , N ). Given mi > 0 (i = 1, . . . , N ) and h ∈ R, we seek periodic solutions of ( mi x ¨i + Vx0i (x1 , . . . , xN ) = 0, 1 ≤ i ≤ N, (Ph) P N 1 2 ˙ i | + V (x1 , . . . , xN ) = h, 1 ≤ i ≤ N. i=1 mi |x 2 2 N
2
Definition 1.1. If the solution x = (x1 , . . . , xN ) of (Ph) satisfies (i) xi ∈ C 2 (0, T ; R2 ), (ii) xi (t) 6= xj (t), ∀t ∈ [0, T ] and ∀1 ≤ i 6= j ≤ N , then we call x the noncollision periodic solution of (Ph). Definition 1.2. Let x and y be two periodic solutions of (Ph), neither of which can be brought into the other by the standard S 1 × O(2) action. Then we call x and y distinct in geometrics. Theorem 1.3. Assume V possesses the form of (1.1) and Vij and V satisfy (V 1) Vij (ξ) = Vji (ξ), ∀i 6= j, ∀ξ ∈ R2 , and V (u1 , . . . , uN ) = V (Ru1 , . . . , RuN ), ∀R ∈ O(2), ∀(u1 , . . . , uN ) ∈ (R2 )N . (V 2) There are α > 2 and a > b > 0 such that for any xi ∈ R2 and xi 6= xj a X mi mj b X mi mj (1.2) − ≤ V (x , . . . , x ) ≤ − . 1 N 2 |xi − xj |α 2 |xi − xj |α 1≤i6=j≤N
i6=j
(V 3)
c2 >
where c5 = c4 =
1 2/α c 2 4 N X
α−2 2
1 c5 , 9
2/α c4 +
2 c3 , α−2
4π 2 i2 mi ,
i=1
a X mi mj , 2 |i − j|α i6=j 2/α 2π 2 α α − 2 c2 = (bc1 )2/α , α−2 2 (α+2)/2 X c1 = 2−(α+2)/2 mi mj m−α/2 , c3 =
i6=j
m=
N X
mi .
i=1
Then for any h > 0, (Ph) has at least 2(N − 1)2N −2 geometrically distinct noncollision periodic solutions.
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GEOMETRICALLY DISTINCT NONCOLLISION ORBITS
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Corollary 1.4. In Theorem 1.3, let N = 3, m1 = 1, m2 = ε 1, m3 = 1/4, α → 2, and a = b = 1. Then for any h > 0, (Ph) has at least 8 geometrically distinct noncollision periodic solutions. Proof. Under the assumption of Corollary 1.4, we have m ≈ 5/4, c4 ≈ 13π , 2
c1 ≈ 1/20,
c2 ≈ π 2 /10,
c3 ≈ 1/16,
c5 ≈ (1/2)c3 × c4 ≈ (13/32)π 2 < 9c2 .
2. Functional setting and the proof of Theorem 1.3 Let us introduce the following notation: H = W 1,2 (S 1 , R2 ), 1 H# = u ∈ H|u t + = −u(t) , 2 E = {u = (u1 , . . . , uN )|ui ∈ H# , i = 1, . . . , N }, Λ0 = {u ∈ E|ui (t) 6= uj (t), ∀t, i 6= j}, Z 1 Z 1 hu, vi = u˙ v˙ dt, kuk2 = |u| ˙ 2 dt, ∀u, v ∈ H# . 0
0
It is well known that kui k is a norm which is equivalent to the usual one and we have kui k ≥ 4|ui |∞ . Hence for all u = (u1 , . . . , uN ) ∈ E, setting kuk2E =
N X
mi kuik2 ,
i=1
we obtain kuk2E ≥ 16m|u|2∞ , P 2 where m = min{mi |i = 1, . . . , N } and |u|2∞ = N i=1 |ui |∞ . On Λ0 define the following functional: Z 1 1 (2.2) f (u) = kuk2E (h − V (u)) dt. 2 0 (2.1)
Similar to the proof of [1] and [8], we have the following variational principle: Lemma 2.1. Let u ∈ Λ0 be the critical point of f and kukE > 0. Let R1 0 V (u) · u dt 2 (2.3) ω = 0 > 0. kuk2E Then x(t) = u(ωt) is a noncollision periodic solution of (Ph). Lemma 2.2 ([5]). Let X = (x1 , . . . , xN ) ∈ (Rk )N . Then 1 X mi mj 1 (2.4) ≥ c1 PN . 2 |xi − xj |α ( i=1 mi |xi |2 )α/2 1≤i6=j≤N
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3042
ZHANG SHIQING
Lemma 2.3. Suppose V satisfies (V 2) of Theorem 1.3. Then 1 (2.5) −V (x) ≥ c PN . ( i=1 |xi |2 )α/2 PN PN 2 2 Proof. By i=1 mi |xi | ≤ m i=1 |xi | and Lemma 2.2, the inequality (2.5) is proved. Lemma 2.4. Assume (V 1) and (V 2) hold. Then f ∈ C 1 (Λ0 , R) and f (un ) → +∞,
(2.6)
∀un * u ∈ ∂Λ.
Proof. (i) If u(t) ≡ 0, then by the embedding theorem, |un |∞ → 0,
(2.7)
n → ∞.
Hence by inequality (2.1), (V 2) and Lemma 2.3, we have Z 1 Z 1 1 1 f (un ) = kun k2E (h − V (un )) dt ≥ kun k2E (−V (un )) dt 2 2 0 0 Z 1 ≥ 8m|un |2∞ c |un |−α dt ≥ 8mc|un |2∞ |un |−α ∞ . 0
Hence f (un ) → +∞ as n → ∞. P (ii) If u(t) 6≡ 0, then kuk2E = N ˙ ik22 6= 0. In fact, if kukE = 0, then i=1 mi ku 1 ui (t) ≡ c = 0 by ui (t + 2 ) = −ui (t). By the weak lower semi-continuous property of g(u) = kukE , we have lim inf kun kE ≥ kukE > 0.
(2.8)
n→∞
By (V 2), Vij satisfies the strong force condition of Gordon ([7]), and so Z 1 (2.9) V (un ) dt → −∞, ∀un * u ∈ ∂Λ0 . 0
Hence by (2.8) and (2.9), we have Z 1 1 2 (h − V (un )) dt → +∞, f (un ) = kukE 2 0
n → ∞.
Lemma 2.5. f satisfies the Palais-Smale condition in Λ0 . Proof. Assume {un } ⊂ Λ0 and that it satisfies (2.10)
|f (un )| ≤ M,
(2.11)
f 0 (un ) → 0.
Then by (2.10) and V (un ) ≤ 0, we know Z 1 1 h 2 0 ≤ − kun kE V (un ) dt ≤ M − kun k2E ; 2 2 0 hence kun k is bounded, and there is a weakly convergent subsequence {unk } of {un }. Similar to the proof of [1], unk → u ∈ Λ0 , and hence f satisfies the Palais-Smale condition. Lemma 2.6. On Λ0 , f possesses a positive lower bound : inf f (u) ≥ c2 .
u∈Λ0
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GEOMETRICALLY DISTINCT NONCOLLISION ORBITS
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Proof. By Lemma 2.2, for any u ∈ Λ0 , we have that ! !−α/2 Z Z 1 X N N 1 1 X f (u) ≥ mi |u˙ i |2 dt h + bc1 mi |ui |2 dt . 2 0 0 i=1 i=1 By the H¨ older inequality, we have !1/2 Z Z T
Z
T
|q| dt ≤ T
|q| dt
1/2
0
2
0
!α/2
T
|q| dt
≥T
2
,
Z
−α/2
!α
T
|q| dt
0
.
0
By the Chebychev inequality, we have Z T Z T 1 dt · |q| dt ≥ T 2 , 0 |q| 0 so !−α/2 !α Z T Z T 1 3α/2 2 ≥T |q| dt . dt 0 |q| 0 Using the above results and the Jensen inequality, we have !−α/2 !α Z T Z Z T 1 T 1 1 1+α/2 2 dt ≥ T ≥T |q| dt , dt α T 0 |q| 0 |q| 0 !−α/2 "Z ! #−α/2 Z T X N N T X 2 1+α/2 2 mi |ui | dt ≥ T mi |ui | dt . 0
0
i=1
By the Wirtinger inequality, we have that ! "Z Z 1 X N 1 f (u) ≥ 2π2 mi |ui |2 dt h + bc1 0 0 i=1
i=1
N X
! mi |ui |2
i=1
#−α/2 . dt
R 1 PN Let r2 = 0 ( i=1 mi |ui |2 ) dt and g(r) = 2π2 r2 (h + bc1 r−α ). Then f (u) ≥ minr>0 g(r) since r = r0 = [(α − 2)bc1 /2h]1/α satisfies g 0 (r0 ) = 0 and g 00 (r0 ) > 0. Hence g(r) has minimum value g(r0 ) and 2/α 2π2 α α − 2 f (u) ≥ g(r0 ) = (bc1 )2/α · h(α−2)/α ≡ c2 h(α−2)/α . α−2 2 In the following, we define a S 1 × O(2) invariant set A and estimate the above bound of f on A. Let Zi = {ν(t) = Ri(ξ cos 2πt + η sin 2πt)|ξ, η ∈ R2 , |ξ| = |η| = 1, hξ, ηi = 0}, A = Z1 × · · · × ZN . Then for any u = (u1 , . . . , uN ) ∈ A, there are ξi , ηi ∈ R2 such that |ξi | = |ηi | = 1, ξi · ηi = 0 and ui (t) = Ri(ξi cos 2πt + ηi sin 2πt). Hence |ui (t)|2 = R2 i2 and |ui (t) − uj (t)|2 ≥ |ui (t)|2 + |uj (t)|2 − 2|ui (t)| · |uj (t)| = R2 (i2 + j 2 − 2ij) = [R(i − j)]2 .
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3044
ZHANG SHIQING
Hence by (V 2), we have
1 a X mi mj 1 = c3 · α . −V (u) ≤ α α R 2 |i − j| R i6=j
It is easily seen that u˙ i = 2πRi(−ξi sin 2πt + ηi cos 2πt), ! Z 1 N N X X kuk2E = mi |u˙ i |2 dt = R2 4π 2 i2 mi = c4 R2 . i=1
0
i=1
By the above estimates, we have Lemma 2.7. If we choose the R of the set A as R∗ = [(α − 2)c4 /2h]1/α , then max f (u) ≤ c5 . u∈A
Proof.
Z 1 Z 1 1 1 1 (h − V (u)) dt ≤ c4 R2 kuk2E · h + c3 α dt 2 2 R 0 0 1 1 = c4 hR2 + c3 c4 R2−α = g(R). 2 2
f (u) =
Then R = R∗ = [(α − 2)c4 /2h]1/α satisfies g 0 (R∗ ) = 0, g 00 (R∗ ) > 0. So g(R) has unique minimum value 2/α 1 2/α α − 2 2 g(R∗ ) = c4 h(α−2)/α c4 + c3 ≡ c5 h(α−2)/α . 2 2 α−2 In the following, we apply the equivariant Ljusternik-Schnirelmann theory to prove the existence of multiple geometrically distinct periodic solutions for (Ph). We note that A is S 1 × O(2) invariant, in fact, H(τ, R) · x(t) ≡ (Rx1 (t + τ ), . . . , RxN (t + τ )) ∈ A for any x(t) = (x1 (t), . . . , xN (t)), τ ∈ S 1 and R ∈ O(2). We also note that the functional f is S 1 × O(2) invariant. Hence in order to obtain multiple distinct S 1 × O(2) invariant orbits of the system (Ph), we need to estimate the S 1 × O(2) equivariant category of the special set A. We note that each Zi (i = 1, . . . , N ) is diffeomorphic to T1 S 1 , which is the unit tangent bundle of S 1 . Hence cat(Zi ) ≥ 3. Now A = Z1 × · · · × ZN is diffeomorphic to T1 S 1 ⊗ · · · ⊗ T1 S 1 (N factors), and A is diffeomorphic to the set Z(n1 ,...,nN ) of Coti Zelati ([4]), so by [4], we have Lemma 2.8. cat(A/S 1 × O(2)) ≥ 2(N − 1)2N −2 . Remark. Although the set A is diffeomorphic to the critical manifold Z(n1 ,...,nN ) of Coti Zelati ([4]), the above bound of f on A is more easily estimated than on Z(n1 ,...,nN ) . Lemma 2.9. Let X be a Banach space, Λ an open subset of X and f ∈ C 1 (Λ, R). Let G be a compact Lie group, T (G) a linear continuous representation with equivariant distance and M a C 2−0 submanifold of Λ. Assume M and f both are
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GEOMETRICALLY DISTINCT NONCOLLISION ORBITS
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invariant under T (G), f satisfies the Palais-Smale condition on some closed subset N of M and the following boundary condition holds: f (un ) → +∞,
(B.C.)
∀un * u ∈ ∂Λ.
Let i be a T (G)-invariant index. Let cm = inf i(A)≥m supx∈A f (x), m = 1, 2, . . . , where A ⊂ N, A ∈ Σ = {B ⊂ N |B is T (G)-invariant and closed in N }. Then: (1) When −∞ < cm < +∞, cm is a critical value of f . (2) If −∞ < c = cm+1 = · · · = cm+k < +∞, then i(Kc ) ≥ k, where Kc = {x ∈ N |f 0 (x) = 0, f (x) = c}. (3) cm ≤ cm+1 . We note that, from the boundary condition (B.C.) and the Palais-Smale condition, one can deduce the complete property of the open set Λ, that is, for any {xn } ⊂ Λ such that xn ∈ fc = {x ∈ Λ|f (x) ≤ c} and xn → x, we have x ∈ Λ. The rest of the proof is standard (see Rabinowitz [10]). Lemma 2.10. If u is a critical point of f in Λ0 which has minimal period 1l , l 6= 1, then (i) l ≥ 3, (ii) v(t) = u(t/l) is also a critical point of f in Λ0 and f (v) = l12 f (u) < 19 f (u). Proof. (i) If l = 2, then u(t + 12 ) = u(t). By u ∈ Λ0 , we have u(t + 12 ) = −u(t). Hence u(t) = (u1 (t), . . . , uN (t)) ≡ 0; this contradicts u ∈ Λ0 . (ii) Z Z 1 1 2 |v(t)| ˙ 2 dt = 2 |u(t)| ˙ dt, l 0 Z 1 Z 1 (h − V (v)) dt = (h − V (u)) dt, 0
0
1 1 f (v) = 2 f (u) ≤ f (u). l 9 Now Theorem 1.3 can be proved by Lemma 2.1 and Lemmas 2.4–2.10. Acknowledgement The author wishes to thank the referee for useful suggestions. References [1] [2] [3] [4] [5] [6] [7]
A. Ambrosetti and V. Coti Zelati, Closed orbits of fixed energy for a class of N-body problems, Ann. IHP Analyse Nonlineaire 9 (1992), 187–200. MR 93e:58156a A. Bari and P. H. Rabinowitz, Periodic solutions of Hamiltonian systems of 3-body type, Ann. IHP Analyse Nonlineaire 8 (1991), 561–649. MR 92k:58223 U. Bessi and V. Coti Zelati, Symmetries and non-collision closed orbits for planar N-body type problems, J. Nonlinear Anal. T.M.A. 16 (1991), 587–598. MR 92a:70006 V. Coti Zelati, A class of periodic solutions of the N-body problem, Celestial Mech. 46 (1989), 177–186. MR 91c:58116 , The periodic solutions of N-body type problems, Ann. IHP Analyse Nonlineaire 7 (1990), 477–492. MR 93a:70009 E. Fadell and S. Husseini, Infinite cuplength in free loop spaces with an application to a problem of the N-body type, Ann. IHP Analyse Nonlineaire 9 (1992), 305–319. MR 94a:58034 W. Gordon, Conservative dynamical systems involving strong forces, Trans. Amer. Math. Soc. 204 (1975), 113–135. MR 51:14152
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ZHANG SHIQING
E. W. C. Van Groesen, Analytical min-max methods for Hamiltonian break orbits of prescribed energy, J. Math. Anal. Appl. 132 (1988), 1–12. MR 89m:58062 P. Majer and S. Terracini, Periodic solutions to some N-body type problems, preprint, 1992. P. Rabinowitz, Minimax methods in critical point theory with applications to differential equations, C.B.M.S. Reg. Conf. Ser. in Math. 65 (1986). MR 87j:58024 E. Serra and S. Terracini, Noncollision solutions to some three-body problems, Arch. Rational Mech. Anal. 120 (1992), 305–325. MR 93i:70013 , Noncollision solutions to some singular minimization problems with Keplerian-like potentials, Nonlinear Analysis T.M.A. 22 (1994), 45–62. MR 94m:58091 C. L. Siegel and K. Moser, Lectures on celestial mechanics, Springer-Verlag, 1971. MR 58:19464 S. Q. Zhang, Multiple closed orbits of fixed energy for N-body-type problems with gravitational potentials, preprint.
Department of Applied Mathematics, Chongqing University, Chongqing 630044, People’s Republic of China E-mail address:
[email protected]
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