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Ejection-collision orbits in some models of two degrees
of freedom in Celestial Mechanics
M.´Alvarez-Ram´ırez,2
E. Barrab´es,1
M. Medina,2
M. Oll´e3
1
Universitat de Girona
2
Universidad Aut´onoma de M´exico-Iztapalapa
3
Universitat Polit`ecnica de Catalunya
CRM- HamSys 2018
ABMO (September 3, 2018) Ejection-Collision orbits 1 / 29
Outline
1 The symmetric collinear 4 body problem
2 Generalization
3 Existence of ECO in the SC4BP
4 Computation of ECO
ABMO (September 3, 2018) Ejection-Collision orbits 2 / 29
The symmetric collinear 4 body problem
Symmetric Collinear 4 Body Problem (SC4BP)
O
m1 = 1m2 = 1m4 = α m3 = α
x
y/
√
α
H =
p2
x
4
+
p2
y
4
− U(x, y)
U(x, y) =
1
2x
+
α5/2
2y
+
4α3/2
y
y2 − αx2
, {(x, y) ∈ R2
; 0 <
√
αx < y}
ABMO (September 3, 2018) Ejection-Collision orbits 3 / 29
The symmetric collinear 4 body problem
Collisions
Single binary collision (SBC): central masses m1 and m2 collide
x = 0, y = 0
O
Double binary collision (DBC): simultaneous binary collisions between
m1 − m3 and m2 − m4.
y =
√
α x = 0
O
Quadruple collision (QC): collisions between the four bodies
x = y = 0
O
ABMO (September 3, 2018) Ejection-Collision orbits 4 / 29
The symmetric collinear 4 body problem
Energy and Hill’s region
First integral:
h = ˙x2
+ ˙y2
− U(x, y)
In a N-body problem, bounded motion can occur only if h < 0.
Configuration space
0
2
4
6
8
10
0 2 4 6 8 10
SBC
DBC
y
x
Polar coordinates:



x =
r
√
2
cos θ,
y =
r
√
2
sin θ,
{(r, θ); r ≥ 0, θα ≤ θ ≤ π/2}
ABMO (September 3, 2018) Ejection-Collision orbits 5 / 29
The symmetric collinear 4 body problem
Ejection-Collision Orbits (ECO)
Definition
An ejection-collision orbit (ECO) is a solution Γ = {γ(s)}s∈R such that
lim
s→±∞
r(s) = 0.
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
x
ABMO (September 3, 2018) Ejection-Collision orbits 6 / 29
Generalization
General setup
Consider a 2-d.o.f. Hamiltonian system with singularities (“collisions”):
H(q, p) =
1
2
pT
· A−1
· p − U(q), (q, p) ∈ D ⊂ R4
Introducing “polar” coordinates (r, θ), the hypothesis on the model are:
Configuration space D = {(r, θ); r > 0, θa < θ < θb}
The potential U(q) = V (θ)/r where
V (θ) =
c1
sin(θb − θ)
+
c2
sin(θ − θa)
+ V (θ)
0 < θb − θa < π, V (θ) > 0 is smooth and bounded.
R. Mart´ınez, (2012)
V (θ) has one non-degenerate critical point, θc, which is a minimum
“Total collision”: r = 0 “Partial collisions”: θ = θa, θb
ABMO (September 3, 2018) Ejection-Collision orbits 7 / 29
Generalization
Regularization
Change to polar-McGehee’s coordinates with a scaling of time:
(t, r, θ, v, u)
r = rv, θ = u,
v = u2
+ 1
2 v2
− V (θ), u = −1
2 uv +
dV
dθ
The flow has been extended to r = 0. The total collision manifold
C = {r = 0} is a 2-dimensional invariant manifold and the flow on C is
gradient-like with respect v.
Regularization of the singularities θ = θa, θb (Sundman, Devaney):
(s, r, θ, v, w)
w = F(θ)u,
dt
ds
= F(θ) F(θ) =
f(θ)
W(θ)
where f(θ) = sin(θ − θa) sin(θb − θ) and W(θ) = f(θ)V (θ) is positive and
bounded analytic function in [θa, θb].
ABMO (September 3, 2018) Ejection-Collision orbits 8 / 29
Generalization
Main features
For a fixed energy level h < 0:
w2
+ F(θ)2
v2
= 2f(θ) + 2rhF(θ)2
Two hyperbolic equilibrium points E+
and E−
in the collision manifold:
r = 0, θ = θc, v = ±v0, w = 0
where θc is the non-degenerate critical point of V (θ).
Ws
(E−
), Wu
(E+
) are 2-dimensional manifolds
Wu
(E−
), Ws
(E+
) are 1-dimensional manifolds restricted to C,
ECO belong to Wu
(E+
) ∩ Ws
(E−
)
At each energy level, there exists a homothetic solution
γ(s) = (r(s), θ = θc, v(s), w = 0)
and r(s) −→
t→±∞
0 (ECO)
ABMO (September 3, 2018) Ejection-Collision orbits 9 / 29
Generalization
Total collision manifold
For a fixed energy level h < 0:
w2
+ F(θ)2
v2
= 2f(θ) + 2rhF(θ)2
ABMO (September 3, 2018) Ejection-Collision orbits 10 / 29
Generalization
Some body problems
Symmetric collinear four body problem (SC4BP)
Collinear three body problem (C3BP)
Rectangular four body Problem (R4BP)
Rhomboidal four body problem
Planar 2N equal masses on a circle with some symmetries
ABMO (September 3, 2018) Ejection-Collision orbits 11 / 29
Generalization
References
Lacomba-Sim´o
Analysis of some degenerate quadruple collisions, Celest. Mech. (1982)
Behavior of the invariant manifolds on the total collision in the CS4BP,
R4BP
Lacomba-Medina
Symbolic dynamics in the symmetric collinear four-body problem, Qual.
Theory Dyn. Syst. (2004)
Existence of ECO for specific values of the mass parameter in the SC4BP
Mart´ınez
Families of double symmetric ”Schubart-like” periodic orbits, Celest. Mech.
117 (2012, 2013)
Study of the total collision manifold in a general framework and
application to several n-body problems
Sekiguchi-Tanikawa, Sweatman, Ouyang et al. (2002-2015)
SC4BP: periodic orbits, scattering orbits, Schubart orbits, escape orbits,
....(equal masses)
ABMO (September 3, 2018) Ejection-Collision orbits 12 / 29
Generalization
Aims
To understand the mechanisms that explain the existence of ECO
(generalize the ideas of Lacomba-Medina). Main tools:
Total collision manifold
Hyperbolic equilibrium points and their invariant manifolds
To give a numerical procedure to compute ECO
ABMO (September 3, 2018) Ejection-Collision orbits 13 / 29
Existence of ECO in the SC4BP
Symmetric Collinear 4 Body Problem (SC4BP)
O
m1 = 1m2 = 1m4 = α m3 = α
x
y/
√
α
V (θ) =
1
√
2 cos θ
+
1
√
2 sin θ
+
2
√
2 α3/2
sin θ −
√
α cos θ
+
2
√
2 α3/2
sin θ +
√
α cos θ
{(r, θ) ∈ R2
; 0 ≤ r, θα ≤ θ ≤ π/2}
ABMO (September 3, 2018) Ejection-Collision orbits 14 / 29
Existence of ECO in the SC4BP
Key ingredients
Collision manifold: C = {r = 0}
Two equilibrium points E+
and E−
in the collision manifold:
r = 0, θ = θc v = ±v0, w = 0
Inv. Manif. Ws
(E+
) Wu
(E+
) Ws
(E−
) Wu
(E−
)
Dimension 1 2 2 1
θc the non-degenerate critical point (minimum) of the potential V
ECO belong to Wu
(E+
) ∩ Ws
(E−
)
Ws
C (E+
) and Wu
C (E−
) live inside C (total collision manifold)
The flow on C is gradient-like with respect v
ABMO (September 3, 2018) Ejection-Collision orbits 15 / 29
Existence of ECO in the SC4BP
The quadruple collision manifold
C = {r = 0} is an invariant manifold
W
C is at the boundary of the constant energy surface Mh on (θ, v, w).
ABMO (September 3, 2018) Ejection-Collision orbits 16 / 29
Existence of ECO in the SC4BP
Invariant manifolds on the quadruple collision manifold
The invariant manifolds Wu
C (E−
) and Ws
C (E+
) (dim 1) live in C
α = α1 = 0.09187... α1 < α = 0.25 < α2 α = α2 = 0.36142...
-4
-2
0
2
4
0.4 0.6 0.8 1 1.2 1.4
v
θ
-4
-2
0
2
4
0.6 0.8 1 1.2 1.4
v
θ
-4
-2
0
2
4
0.6 0.8 1 1.2 1.4
v
θ
Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or
both branches of Wu
C (E−
) and Ws
C (E+
) coincide (single or double
heteroclinic).
ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
Existence of ECO in the SC4BP
Invariant manifolds on the quadruple collision manifold
The invariant manifolds Wu
C (E−
) and Ws
C (E+
) (dim 1) live in C
α2 < α = 0.75 < α3 α = α3 = 0.90764... α3 < α = 1.25 < α4
-6
-4
-2
0
2
4
6
0.8 0.9 1 1.1 1.2 1.3 1.4 1.5
v
θ
-6
-4
-2
0
2
4
6
0.8 0.9 1 1.1 1.2 1.3 1.4 1.5
v
θ
-8
-4
0
4
8
0.9 1 1.1 1.2 1.3 1.4 1.5
v
θ
Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or
both branches of Wu
C (E−
) and Ws
C (E+
) coincide (single or double
heteroclinic).
ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
Existence of ECO in the SC4BP
Invariant manifolds on the quadruple collision manifold
The invariant manifolds Wu
C (E−
) and Ws
C (E+
) (dim 1) live in C
α = α4 = 1.34496... α4 < α = 2 < α5 α = α5 = 2.21775...
-8
-4
0
4
8
0.9 1 1.1 1.2 1.3 1.4 1.5
v
θ
-12
-8
-4
0
4
8
12
1 1.1 1.2 1.3 1.4 1.5
v
θ
-12
-8
-4
0
4
8
12
1 1.1 1.2 1.3 1.4 1.5
v
θ
Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or
both branches of Wu
C (E−
) and Ws
C (E+
) coincide (single or double
heteroclinic).
ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
Existence of ECO in the SC4BP
Invariant manifolds on the quadruple collision manifold
-8
-4
0
4
8
0.9 1 1.1 1.2 1.3 1.4 1.5
v
θ
α ∈ (αk, αk+1) such that there are no heteroclinic connection on C and the two
branches of Wu
C (E−
) escape preforming different binary collisions
ABMO (September 3, 2018) Ejection-Collision orbits 18 / 29
Existence of ECO in the SC4BP
Existence of ECO (1)
The intersection of Wu
C (E−
) and Ws
C (E+
) with the section Σc give 4
sequences of points {u±
j }, {s±
j }
ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
Existence of ECO in the SC4BP
Existence of ECO (1)
The sequences follow a specific order (the branches do not intersect)
ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
Existence of ECO in the SC4BP
Existence of ECO (1)
The intersection of Wu
(E+
) and Ws
(E−
) (2-dim i.m.) with C give four orbits
which intersections with the section Σc give 4 sequences of points {p±
j }, {q±
j }
ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
Existence of ECO in the SC4BP
Existence of ECO (2)
We look for Wu
(E+
) ∩ Ws
(E−
)
Consider 1st intersection with Σc = {θ = θα, θ = π/2}: J, I
E
-
E
+
J
u1
+
p1
+
s1
s2
s*
s s1
-
q1
-
I
J =< u+
1 , p+
1 > I =< q−
1 , s−
1 , >
ECO of first order
ABMO (September 3, 2018) Ejection-Collision orbits 20 / 29
Existence of ECO in the SC4BP
Existence of ECO (2)
u2
+
u4
+
u1
-
u3
-
u5
-
s1
+
s3
+
s5
+
s4
-
s2
-
q1
+
u1
+
u3
+
u5
+
u2
-
u4
-
s2
+
s4
+
s1
-
s3
-
s5
-
p1
+
q1
-
p1
-
P (I )
-1
1
P (I )
-3
1
P(J )1
P (I )-2
1
P (I )-4
1
q2
-
I1
I2
J1
q= aq
q=p/2
ECO(1)
P (I )
-1
2
ECO(1)
ECO(1,1)
ECO(1,2,1,2,1)
W (E )
u +
W (E )
s -
Following the endpoints of the arches and the flow on C, ECO of higher order exists
ABMO (September 3, 2018) Ejection-Collision orbits 20 / 29
Computation of ECO
Parametrization of invariant manifolds (I)
Parametrizations of the invariant manifolds up to a certain order:
Ψ−
1 (ξ, ϕ) = E−
+ ξ (cos(2πϕ) σ1 + sin(2πϕ) σ4) ,
Ψ+
1 (ξ, ϕ) = E+
+ ξ (cos(2πϕ) σ1 + sin(2πϕ) σ3)
σ1 and σ3,4 give the slow and fast directions
The parameter ϕ ∈ (1/4, 3/4) (r > 0):
ϕ ∈ (1/4, 1/2): θ > θc, SBC
region
ϕ ∈ (1/2, 3/4): θ < θc, DBC
region
ϕ = 1/2: homothetic orbit,
slow direction
ϕ = 1/4, 3/4 fast direction
on C 0
1
2
3
4
5
6
7
0 1 2 3 4 5 6 7
y
x
ABMO (September 3, 2018) Ejection-Collision orbits 21 / 29
Computation of ECO
Parametrization of invariant manifolds (II)
Time to satisfy the escape condition for each initial condition Ψ+
1 (ξ, ϕ)
0.01
0.1
1
10
100
1000
-14 -12 -10 -8 -6 -4 -2 0
se
(ϕ-0.5)10
3
0.01
0.1
1
10
100
1000
0 2 4 6 8 10 12 14
se
(ϕ-0.5)10
3
1
4
< ϕ <
1
2
1
2
< ϕ <
3
4
ECOs live in a narrow interval of values of ϕ close to ϕ = 1/2 (slow direction)
−→ a parametrization of the inv. manif. of higher order is needed.
ABMO (September 3, 2018) Ejection-Collision orbits 22 / 29
Computation of ECO
Characterization of ECO
Let B be the set of all possible sequences of the elements 1 and 2.
P : Wu
(E+
) −→ B
Γ −→ (p1, p2, . . . , pn, . . . )
pj =
1 the j-th intersection is a SBC,
2 the j-th intersection is a DBC,
for j = 1, . . . , n.
Theorem
Let Γ ∈ Wu
(E+
). Then
1 P(Γ) is finite if and only if it corresponds to an ECO.
2 If Γ is an ECO such that P(Γ) = (p1, p2, . . . , pn), then Γ is an ECO with
P(Γ) = (pn, pn−1, . . . , p1).
3 Γ is a symmetric ECO if and only if P(Γ) is a symmetric sequence.
ABMO (September 3, 2018) Ejection-Collision orbits 23 / 29
Computation of ECO
Computation of ECO (I)
Section
Σc = {(r, v, θ, w); w = 0, θ = θα or θ = π/2},
Let Γ an orbit with initial condition given by the parametrization Ψ+
k (ξ, ϕ).
The map Pn(ϕ) = (p1, . . . , pn) codes the first n intersections with Σc.
Proposition
Let ϕ1 and ϕ2 be such that
Pn+1(ϕ1) = (p1, p2, . . . , pn, p1
n+1),
Pn+1(ϕ2) = (p1, p2, . . . , pn, p2
n+1),
with p1
n+1 = p2
n+1. Then, there exists a value ϕ ∈ (ϕ1, ϕ2) such that
P(ϕ) = (p1, p2, . . . , pn).
ABMO (September 3, 2018) Ejection-Collision orbits 24 / 29
Computation of ECO
Computation of ECO (II)
Section
Σc = {(r, v, θ, w); w = 0, θ = θα or θ = π/2},
To detect a change in pn we look for the zeros of
Fn(ϕ) = r(θ − θc)
-4
-2
0
2
4
-0.015 -0.01 -0.005 0
θ5
F5
Fn
(ϕ-0.5)10
3
-4
-2
0
2
4
-0.015 -0.01 -0.005 0
θ6
F6
Fn
(ϕ-0.5)10
3
1
4
< ϕ <
1
2
1
2
< ϕ <
3
4
ABMO (September 3, 2018) Ejection-Collision orbits 25 / 29
Computation of ECO
ECO of order 1 and 2 for SC4BP
(1) (2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
x
(1,1) (2,2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
xABMO (September 3, 2018) Ejection-Collision orbits 26 / 29
Computation of ECO
ECO of order 3 and 4 for SC4BP
(1,1,1) (2,2,2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
x
(1,1,1,1) (2,2,2,2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
xABMO (September 3, 2018) Ejection-Collision orbits 27 / 29
Computation of ECO
ECO of order 6: symmetric and non-symmetric
(1, 6)
. . .,1) (2, 6)
. . .,2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
10
0 2 4 6 8 10
y
x
(1,2,1,2,1,2) (1,1,2,1,2,1) (2,2,1,2,1,2)
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
x
0
2
4
6
8
0 2 4 6 8
y
xABMO (September 3, 2018) Ejection-Collision orbits 28 / 29
Computation of ECO
...
Thank you!
ABMO (September 3, 2018) Ejection-Collision orbits 29 / 29

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Ejection-collision orbits

  • 1. Ejection-collision orbits in some models of two degrees of freedom in Celestial Mechanics M.´Alvarez-Ram´ırez,2 E. Barrab´es,1 M. Medina,2 M. Oll´e3 1 Universitat de Girona 2 Universidad Aut´onoma de M´exico-Iztapalapa 3 Universitat Polit`ecnica de Catalunya CRM- HamSys 2018 ABMO (September 3, 2018) Ejection-Collision orbits 1 / 29
  • 2. Outline 1 The symmetric collinear 4 body problem 2 Generalization 3 Existence of ECO in the SC4BP 4 Computation of ECO ABMO (September 3, 2018) Ejection-Collision orbits 2 / 29
  • 3. The symmetric collinear 4 body problem Symmetric Collinear 4 Body Problem (SC4BP) O m1 = 1m2 = 1m4 = α m3 = α x y/ √ α H = p2 x 4 + p2 y 4 − U(x, y) U(x, y) = 1 2x + α5/2 2y + 4α3/2 y y2 − αx2 , {(x, y) ∈ R2 ; 0 < √ αx < y} ABMO (September 3, 2018) Ejection-Collision orbits 3 / 29
  • 4. The symmetric collinear 4 body problem Collisions Single binary collision (SBC): central masses m1 and m2 collide x = 0, y = 0 O Double binary collision (DBC): simultaneous binary collisions between m1 − m3 and m2 − m4. y = √ α x = 0 O Quadruple collision (QC): collisions between the four bodies x = y = 0 O ABMO (September 3, 2018) Ejection-Collision orbits 4 / 29
  • 5. The symmetric collinear 4 body problem Energy and Hill’s region First integral: h = ˙x2 + ˙y2 − U(x, y) In a N-body problem, bounded motion can occur only if h < 0. Configuration space 0 2 4 6 8 10 0 2 4 6 8 10 SBC DBC y x Polar coordinates:    x = r √ 2 cos θ, y = r √ 2 sin θ, {(r, θ); r ≥ 0, θα ≤ θ ≤ π/2} ABMO (September 3, 2018) Ejection-Collision orbits 5 / 29
  • 6. The symmetric collinear 4 body problem Ejection-Collision Orbits (ECO) Definition An ejection-collision orbit (ECO) is a solution Γ = {γ(s)}s∈R such that lim s→±∞ r(s) = 0. 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y x ABMO (September 3, 2018) Ejection-Collision orbits 6 / 29
  • 7. Generalization General setup Consider a 2-d.o.f. Hamiltonian system with singularities (“collisions”): H(q, p) = 1 2 pT · A−1 · p − U(q), (q, p) ∈ D ⊂ R4 Introducing “polar” coordinates (r, θ), the hypothesis on the model are: Configuration space D = {(r, θ); r > 0, θa < θ < θb} The potential U(q) = V (θ)/r where V (θ) = c1 sin(θb − θ) + c2 sin(θ − θa) + V (θ) 0 < θb − θa < π, V (θ) > 0 is smooth and bounded. R. Mart´ınez, (2012) V (θ) has one non-degenerate critical point, θc, which is a minimum “Total collision”: r = 0 “Partial collisions”: θ = θa, θb ABMO (September 3, 2018) Ejection-Collision orbits 7 / 29
  • 8. Generalization Regularization Change to polar-McGehee’s coordinates with a scaling of time: (t, r, θ, v, u) r = rv, θ = u, v = u2 + 1 2 v2 − V (θ), u = −1 2 uv + dV dθ The flow has been extended to r = 0. The total collision manifold C = {r = 0} is a 2-dimensional invariant manifold and the flow on C is gradient-like with respect v. Regularization of the singularities θ = θa, θb (Sundman, Devaney): (s, r, θ, v, w) w = F(θ)u, dt ds = F(θ) F(θ) = f(θ) W(θ) where f(θ) = sin(θ − θa) sin(θb − θ) and W(θ) = f(θ)V (θ) is positive and bounded analytic function in [θa, θb]. ABMO (September 3, 2018) Ejection-Collision orbits 8 / 29
  • 9. Generalization Main features For a fixed energy level h < 0: w2 + F(θ)2 v2 = 2f(θ) + 2rhF(θ)2 Two hyperbolic equilibrium points E+ and E− in the collision manifold: r = 0, θ = θc, v = ±v0, w = 0 where θc is the non-degenerate critical point of V (θ). Ws (E− ), Wu (E+ ) are 2-dimensional manifolds Wu (E− ), Ws (E+ ) are 1-dimensional manifolds restricted to C, ECO belong to Wu (E+ ) ∩ Ws (E− ) At each energy level, there exists a homothetic solution γ(s) = (r(s), θ = θc, v(s), w = 0) and r(s) −→ t→±∞ 0 (ECO) ABMO (September 3, 2018) Ejection-Collision orbits 9 / 29
  • 10. Generalization Total collision manifold For a fixed energy level h < 0: w2 + F(θ)2 v2 = 2f(θ) + 2rhF(θ)2 ABMO (September 3, 2018) Ejection-Collision orbits 10 / 29
  • 11. Generalization Some body problems Symmetric collinear four body problem (SC4BP) Collinear three body problem (C3BP) Rectangular four body Problem (R4BP) Rhomboidal four body problem Planar 2N equal masses on a circle with some symmetries ABMO (September 3, 2018) Ejection-Collision orbits 11 / 29
  • 12. Generalization References Lacomba-Sim´o Analysis of some degenerate quadruple collisions, Celest. Mech. (1982) Behavior of the invariant manifolds on the total collision in the CS4BP, R4BP Lacomba-Medina Symbolic dynamics in the symmetric collinear four-body problem, Qual. Theory Dyn. Syst. (2004) Existence of ECO for specific values of the mass parameter in the SC4BP Mart´ınez Families of double symmetric ”Schubart-like” periodic orbits, Celest. Mech. 117 (2012, 2013) Study of the total collision manifold in a general framework and application to several n-body problems Sekiguchi-Tanikawa, Sweatman, Ouyang et al. (2002-2015) SC4BP: periodic orbits, scattering orbits, Schubart orbits, escape orbits, ....(equal masses) ABMO (September 3, 2018) Ejection-Collision orbits 12 / 29
  • 13. Generalization Aims To understand the mechanisms that explain the existence of ECO (generalize the ideas of Lacomba-Medina). Main tools: Total collision manifold Hyperbolic equilibrium points and their invariant manifolds To give a numerical procedure to compute ECO ABMO (September 3, 2018) Ejection-Collision orbits 13 / 29
  • 14. Existence of ECO in the SC4BP Symmetric Collinear 4 Body Problem (SC4BP) O m1 = 1m2 = 1m4 = α m3 = α x y/ √ α V (θ) = 1 √ 2 cos θ + 1 √ 2 sin θ + 2 √ 2 α3/2 sin θ − √ α cos θ + 2 √ 2 α3/2 sin θ + √ α cos θ {(r, θ) ∈ R2 ; 0 ≤ r, θα ≤ θ ≤ π/2} ABMO (September 3, 2018) Ejection-Collision orbits 14 / 29
  • 15. Existence of ECO in the SC4BP Key ingredients Collision manifold: C = {r = 0} Two equilibrium points E+ and E− in the collision manifold: r = 0, θ = θc v = ±v0, w = 0 Inv. Manif. Ws (E+ ) Wu (E+ ) Ws (E− ) Wu (E− ) Dimension 1 2 2 1 θc the non-degenerate critical point (minimum) of the potential V ECO belong to Wu (E+ ) ∩ Ws (E− ) Ws C (E+ ) and Wu C (E− ) live inside C (total collision manifold) The flow on C is gradient-like with respect v ABMO (September 3, 2018) Ejection-Collision orbits 15 / 29
  • 16. Existence of ECO in the SC4BP The quadruple collision manifold C = {r = 0} is an invariant manifold W C is at the boundary of the constant energy surface Mh on (θ, v, w). ABMO (September 3, 2018) Ejection-Collision orbits 16 / 29
  • 17. Existence of ECO in the SC4BP Invariant manifolds on the quadruple collision manifold The invariant manifolds Wu C (E− ) and Ws C (E+ ) (dim 1) live in C α = α1 = 0.09187... α1 < α = 0.25 < α2 α = α2 = 0.36142... -4 -2 0 2 4 0.4 0.6 0.8 1 1.2 1.4 v θ -4 -2 0 2 4 0.6 0.8 1 1.2 1.4 v θ -4 -2 0 2 4 0.6 0.8 1 1.2 1.4 v θ Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or both branches of Wu C (E− ) and Ws C (E+ ) coincide (single or double heteroclinic). ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
  • 18. Existence of ECO in the SC4BP Invariant manifolds on the quadruple collision manifold The invariant manifolds Wu C (E− ) and Ws C (E+ ) (dim 1) live in C α2 < α = 0.75 < α3 α = α3 = 0.90764... α3 < α = 1.25 < α4 -6 -4 -2 0 2 4 6 0.8 0.9 1 1.1 1.2 1.3 1.4 1.5 v θ -6 -4 -2 0 2 4 6 0.8 0.9 1 1.1 1.2 1.3 1.4 1.5 v θ -8 -4 0 4 8 0.9 1 1.1 1.2 1.3 1.4 1.5 v θ Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or both branches of Wu C (E− ) and Ws C (E+ ) coincide (single or double heteroclinic). ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
  • 19. Existence of ECO in the SC4BP Invariant manifolds on the quadruple collision manifold The invariant manifolds Wu C (E− ) and Ws C (E+ ) (dim 1) live in C α = α4 = 1.34496... α4 < α = 2 < α5 α = α5 = 2.21775... -8 -4 0 4 8 0.9 1 1.1 1.2 1.3 1.4 1.5 v θ -12 -8 -4 0 4 8 12 1 1.1 1.2 1.3 1.4 1.5 v θ -12 -8 -4 0 4 8 12 1 1.1 1.2 1.3 1.4 1.5 v θ Sim´o and Lacomba (1982) give a sequence of values {αk}k≥1 for which one or both branches of Wu C (E− ) and Ws C (E+ ) coincide (single or double heteroclinic). ABMO (September 3, 2018) Ejection-Collision orbits 17 / 29
  • 20. Existence of ECO in the SC4BP Invariant manifolds on the quadruple collision manifold -8 -4 0 4 8 0.9 1 1.1 1.2 1.3 1.4 1.5 v θ α ∈ (αk, αk+1) such that there are no heteroclinic connection on C and the two branches of Wu C (E− ) escape preforming different binary collisions ABMO (September 3, 2018) Ejection-Collision orbits 18 / 29
  • 21. Existence of ECO in the SC4BP Existence of ECO (1) The intersection of Wu C (E− ) and Ws C (E+ ) with the section Σc give 4 sequences of points {u± j }, {s± j } ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
  • 22. Existence of ECO in the SC4BP Existence of ECO (1) The sequences follow a specific order (the branches do not intersect) ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
  • 23. Existence of ECO in the SC4BP Existence of ECO (1) The intersection of Wu (E+ ) and Ws (E− ) (2-dim i.m.) with C give four orbits which intersections with the section Σc give 4 sequences of points {p± j }, {q± j } ABMO (September 3, 2018) Ejection-Collision orbits 19 / 29
  • 24. Existence of ECO in the SC4BP Existence of ECO (2) We look for Wu (E+ ) ∩ Ws (E− ) Consider 1st intersection with Σc = {θ = θα, θ = π/2}: J, I E - E + J u1 + p1 + s1 s2 s* s s1 - q1 - I J =< u+ 1 , p+ 1 > I =< q− 1 , s− 1 , > ECO of first order ABMO (September 3, 2018) Ejection-Collision orbits 20 / 29
  • 25. Existence of ECO in the SC4BP Existence of ECO (2) u2 + u4 + u1 - u3 - u5 - s1 + s3 + s5 + s4 - s2 - q1 + u1 + u3 + u5 + u2 - u4 - s2 + s4 + s1 - s3 - s5 - p1 + q1 - p1 - P (I ) -1 1 P (I ) -3 1 P(J )1 P (I )-2 1 P (I )-4 1 q2 - I1 I2 J1 q= aq q=p/2 ECO(1) P (I ) -1 2 ECO(1) ECO(1,1) ECO(1,2,1,2,1) W (E ) u + W (E ) s - Following the endpoints of the arches and the flow on C, ECO of higher order exists ABMO (September 3, 2018) Ejection-Collision orbits 20 / 29
  • 26. Computation of ECO Parametrization of invariant manifolds (I) Parametrizations of the invariant manifolds up to a certain order: Ψ− 1 (ξ, ϕ) = E− + ξ (cos(2πϕ) σ1 + sin(2πϕ) σ4) , Ψ+ 1 (ξ, ϕ) = E+ + ξ (cos(2πϕ) σ1 + sin(2πϕ) σ3) σ1 and σ3,4 give the slow and fast directions The parameter ϕ ∈ (1/4, 3/4) (r > 0): ϕ ∈ (1/4, 1/2): θ > θc, SBC region ϕ ∈ (1/2, 3/4): θ < θc, DBC region ϕ = 1/2: homothetic orbit, slow direction ϕ = 1/4, 3/4 fast direction on C 0 1 2 3 4 5 6 7 0 1 2 3 4 5 6 7 y x ABMO (September 3, 2018) Ejection-Collision orbits 21 / 29
  • 27. Computation of ECO Parametrization of invariant manifolds (II) Time to satisfy the escape condition for each initial condition Ψ+ 1 (ξ, ϕ) 0.01 0.1 1 10 100 1000 -14 -12 -10 -8 -6 -4 -2 0 se (ϕ-0.5)10 3 0.01 0.1 1 10 100 1000 0 2 4 6 8 10 12 14 se (ϕ-0.5)10 3 1 4 < ϕ < 1 2 1 2 < ϕ < 3 4 ECOs live in a narrow interval of values of ϕ close to ϕ = 1/2 (slow direction) −→ a parametrization of the inv. manif. of higher order is needed. ABMO (September 3, 2018) Ejection-Collision orbits 22 / 29
  • 28. Computation of ECO Characterization of ECO Let B be the set of all possible sequences of the elements 1 and 2. P : Wu (E+ ) −→ B Γ −→ (p1, p2, . . . , pn, . . . ) pj = 1 the j-th intersection is a SBC, 2 the j-th intersection is a DBC, for j = 1, . . . , n. Theorem Let Γ ∈ Wu (E+ ). Then 1 P(Γ) is finite if and only if it corresponds to an ECO. 2 If Γ is an ECO such that P(Γ) = (p1, p2, . . . , pn), then Γ is an ECO with P(Γ) = (pn, pn−1, . . . , p1). 3 Γ is a symmetric ECO if and only if P(Γ) is a symmetric sequence. ABMO (September 3, 2018) Ejection-Collision orbits 23 / 29
  • 29. Computation of ECO Computation of ECO (I) Section Σc = {(r, v, θ, w); w = 0, θ = θα or θ = π/2}, Let Γ an orbit with initial condition given by the parametrization Ψ+ k (ξ, ϕ). The map Pn(ϕ) = (p1, . . . , pn) codes the first n intersections with Σc. Proposition Let ϕ1 and ϕ2 be such that Pn+1(ϕ1) = (p1, p2, . . . , pn, p1 n+1), Pn+1(ϕ2) = (p1, p2, . . . , pn, p2 n+1), with p1 n+1 = p2 n+1. Then, there exists a value ϕ ∈ (ϕ1, ϕ2) such that P(ϕ) = (p1, p2, . . . , pn). ABMO (September 3, 2018) Ejection-Collision orbits 24 / 29
  • 30. Computation of ECO Computation of ECO (II) Section Σc = {(r, v, θ, w); w = 0, θ = θα or θ = π/2}, To detect a change in pn we look for the zeros of Fn(ϕ) = r(θ − θc) -4 -2 0 2 4 -0.015 -0.01 -0.005 0 θ5 F5 Fn (ϕ-0.5)10 3 -4 -2 0 2 4 -0.015 -0.01 -0.005 0 θ6 F6 Fn (ϕ-0.5)10 3 1 4 < ϕ < 1 2 1 2 < ϕ < 3 4 ABMO (September 3, 2018) Ejection-Collision orbits 25 / 29
  • 31. Computation of ECO ECO of order 1 and 2 for SC4BP (1) (2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y x (1,1) (2,2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y xABMO (September 3, 2018) Ejection-Collision orbits 26 / 29
  • 32. Computation of ECO ECO of order 3 and 4 for SC4BP (1,1,1) (2,2,2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y x (1,1,1,1) (2,2,2,2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y xABMO (September 3, 2018) Ejection-Collision orbits 27 / 29
  • 33. Computation of ECO ECO of order 6: symmetric and non-symmetric (1, 6) . . .,1) (2, 6) . . .,2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 10 0 2 4 6 8 10 y x (1,2,1,2,1,2) (1,1,2,1,2,1) (2,2,1,2,1,2) 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y x 0 2 4 6 8 0 2 4 6 8 y xABMO (September 3, 2018) Ejection-Collision orbits 28 / 29
  • 34. Computation of ECO ... Thank you! ABMO (September 3, 2018) Ejection-Collision orbits 29 / 29