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84
Relative equilibria of Hamiltonian systems with symmetry: linearization, smoothness
, 1995
"... We show that, given a certain transversality condition, the set of relative equilibria E near pe ∈ E of a Hamiltonian system with symmetry is locally Whitneystratified by the conjugacy classes of the isotropy subgroups (under the product of the coadjoint and adjoint actions) of the momentumgenerat ..."
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Cited by 42 (9 self)
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We show that, given a certain transversality condition, the set of relative equilibria E near pe ∈ E of a Hamiltonian system with symmetry is locally Whitneystratified by the conjugacy classes of the isotropy subgroups (under the product of the coadjoint and adjoint actions) of the momentumgenerator pairs (µ, ξ) of the relative equilibria. The dimension of the stratum of the conjugacy class (K) is dimG+2dim Z(K) −dim K, where Z(K) is the center of K, and transverse to this stratum E is locally diffeomorphic to the commuting pairs of the Lie algebra of K/Z(K). The stratum E(K) is a symplectic submanifold of P near pe ∈ E if and only if pe is nondegenerate and K is a maximal torus of G. We also show that there is a dense subset of Ginvariant Hamiltonians on P for which all the relative equilibria are transversal. Thus, generically, the types of singularities that can be found in the set of relative equilibria of a Hamiltonian system with symmetry are those types found amongst the singularities at zero of the sets of commuting pairs of certain Lie subalgebras of the symmetry group.
A Proof of the Gutzwiller Semiclassical Trace Formula using Coherent Sates Decomposition
 Commun. in Math. Phys
, 1999
"... The Gutzwiller trace formula links the eigenvalues of the Schrödinger operator H as Planck’s constant goes to zero (the semiclassical régime) with the closed orbits of the corresponding classical mechanical system. Gutzwiller gave a heuristic proof of this trace formula, using the Feynman integral ..."
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Cited by 35 (5 self)
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The Gutzwiller trace formula links the eigenvalues of the Schrödinger operator H as Planck’s constant goes to zero (the semiclassical régime) with the closed orbits of the corresponding classical mechanical system. Gutzwiller gave a heuristic proof of this trace formula, using the Feynman integral representation for the propagator of H. Later, using the theory of Fourier integral operators, mathematicians gave rigorous proofs of the formula in various settings. Here we show how the use of coherent states allows us to give a simple and direct proof. 1
On the vertical families of twodimensional tori near the triangular points of the Bicircular problem
, 1999
"... This paper focuses on some aspects of the motion of a small particle moving near the Lagrangian points of the EarthMoon system. The model for the motion of the particle is the socalled Bicircular problem (BCP), that includes the eect of Earth and Moon as in the spatial Restricted Three Body Proble ..."
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Cited by 25 (6 self)
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This paper focuses on some aspects of the motion of a small particle moving near the Lagrangian points of the EarthMoon system. The model for the motion of the particle is the socalled Bicircular problem (BCP), that includes the eect of Earth and Moon as in the spatial Restricted Three Body Problem (RTBP), plus the eect of the Sun as a periodic timedependent perturbation of the RTBP. Due to this periodic forcing coming from the Sun, the Lagrangian points are no longer equilibrium solutions for the BCP. On the other hand, the BCP has three periodic orbits (with the same period as the forcing) that can be seen as the dynamical equivalent of the Lagrangian points. In this work, we rst discuss some numerical methods for the accurate computation of quasiperiodic solutions, and then we apply them to the BCP to obtain families of 2D tori in an extended neighbourhood of the Lagrangian points. These families start on the three periodic orbits mentioned above and they are continued in th...
A methodology for the numerical computation of normal forms, centre manifolds and first integrals of Hamiltonian systems
 Experiment. Math
, 1999
"... This paper deals with the e ective computation of normal forms, centre manifolds and rst integrals in Hamiltonian mechanics. These kind of calculations are very useful since they allow, for instance, to give explicit estimates on the di usion time or to compute invariant tori. The approach presente ..."
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Cited by 24 (6 self)
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This paper deals with the e ective computation of normal forms, centre manifolds and rst integrals in Hamiltonian mechanics. These kind of calculations are very useful since they allow, for instance, to give explicit estimates on the di usion time or to compute invariant tori. The approach presented here is based on using algebraic manipulation for the formal series but taking numerical coe cients for them. This, jointly with a very e cient implementation of the software, allows big savings in both memory and execution time of the algorithms if we compare with the use of commercial algebraic manipulators. The algorithms are presented jointly with their C/C++ implementations, and they are applied to some concrete examples coming from celestial mechanics. rst integrals, algebraic manipulators, in
A Restricted FourBody Model For The Dynamics Near The Lagrangian Points Of The SunJupiter System
 Discrete Contin. Dynam. Systems  Series B
, 2001
"... We focus on the dynamics of a small particle near the Lagrangian points of the SunJupiter system. To try to account for the eect of Saturn, we develop a specic model based on the computation of a true solution of the planar threebody problem for Sun, Jupiter and Saturn, close to the real motion of ..."
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Cited by 23 (12 self)
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We focus on the dynamics of a small particle near the Lagrangian points of the SunJupiter system. To try to account for the eect of Saturn, we develop a specic model based on the computation of a true solution of the planar threebody problem for Sun, Jupiter and Saturn, close to the real motion of these three bodies. Then, we can write the equations of motion of a fourth innitesimal particle moving under the attraction of these three masses. Using suitable coordinates, the model is written as a timedependent perturbation of the wellknown spatial Restricted ThreeBody Problem. Then, we study the dynamics of this model near the triangular points. The tools are based on computing, up to high order, suitable normal forms and rst integrals. From these expansions, it is not dicult to derive approximations to invariant tori (of dimensions 2, 3 and 4) as well as bounds on the speed of diusion on suitable domains. We have also included some comparisons with the motion of a few Trojan asteroids in the real Solar system.
Hamiltonian Square Roots of SkewHamiltonian Matrices
, 1997
"... We present a constructive existence proof that every real skewHamiltonian matrix W has a real Hamiltonian square root. The key step in this construction shows how one may bring any such W into a real quasiJordan canonical form via symplectic similarity. We show further that every W has infinitely ..."
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Cited by 21 (7 self)
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We present a constructive existence proof that every real skewHamiltonian matrix W has a real Hamiltonian square root. The key step in this construction shows how one may bring any such W into a real quasiJordan canonical form via symplectic similarity. We show further that every W has infinitely many real Hamiltonian square roots, and give a lower bound on the dimension of the set of all such square roots. AMS subject classification. 65F15 1 Introduction Any matrix X such that X 2 = A is said to be a square root of the matrix A. For general complex matrices A 2 C n\Thetan there exists a welldeveloped although somewhat complicated theory of matrix square roots [7, 14], and a number of algorithms for their effective computation [2, 11]. Similarly for the theory and computation of real square roots for real matrices [10, 14]. By contrast structured square root problems, where both the matrix A and its square root X are required to have some extra (not necessarily the same) spe...
Hamiltonian Systems Near Relative Equilibria
 J. Dierential Equations
, 1999
"... We give explicit differential equations for the dynamics near relative equilibria of Hamiltonian systems. These split the dynamics into motion along the group orbit and motion inside a slice transversal to the group orbit. The form of the differential equations that is inherited from the symplectic ..."
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Cited by 16 (6 self)
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We give explicit differential equations for the dynamics near relative equilibria of Hamiltonian systems. These split the dynamics into motion along the group orbit and motion inside a slice transversal to the group orbit. The form of the differential equations that is inherited from the symplectic structure and symmetry properties of the Hamiltonian system is analysed and the effects of time reversing symmetries are included. The results will be applicable to the stability and bifurcation theories of relative equilibria of Hamiltonian systems.
NormalInternal Resonances in QuasiPeriodically Forced Oscillators: A Conservative Approach
, 2002
"... We perform a bifurcation analysis of normalinternal resonances in parametrised families of quasiperiodically forced Hamiltonian oscillators, for small forcing. The unforced system is a one degree of freedom oscillator, called the `backbone' system; forced, the system is a skewproduct flow with a ..."
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Cited by 14 (13 self)
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We perform a bifurcation analysis of normalinternal resonances in parametrised families of quasiperiodically forced Hamiltonian oscillators, for small forcing. The unforced system is a one degree of freedom oscillator, called the `backbone' system; forced, the system is a skewproduct flow with a quasiperiodic driving with n basic frequencies. The dynamics of the forced system are simplified by averaging over the orbits of a linearisation of the unforced system. The averaged system turns out to have the same structure as in the wellknown case of periodic forcing (n = 1); for a real analytic system, the nonintegrable part can even be made exponentially small in the forcing strength. We investigate the persistence and the bifurcations of quasiperiodic ndimensional tori in the averaged system, filling normalinternal resonance `gaps' that had been excluded in previous analyses. However, these gaps cannot completely be filled up: secondary resonance gaps appear, to which the averaging analysis can be applied again. This phenomenon of `gaps within gaps' makes the quasiperiodic case more complicated than the periodic case.
Structured factorizations in scalar product spaces
 SIAM J. Matrix Anal. Appl
, 2004
"... Abstract. Let A belong to an automorphism group, Lie algebra or Jordan algebra of a scalar product. When A is factored, to what extent do the factors inherit structure from A? We answer this question for the principal matrix square root, the matrix sign decomposition, and the polar decomposition. Fo ..."
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Cited by 12 (7 self)
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Abstract. Let A belong to an automorphism group, Lie algebra or Jordan algebra of a scalar product. When A is factored, to what extent do the factors inherit structure from A? We answer this question for the principal matrix square root, the matrix sign decomposition, and the polar decomposition. For general A, we give a simple derivation and characterization of a particular generalized polar decomposition, and we relate it to other such decompositions in the literature. Finally, we study eigendecompositions and structured singular value decompositions, considering in particular the structure in eigenvalues, eigenvectors and singular values that persists across a wide range of scalar products. A key feature of our analysis is the identification of two particular classes of scalar products, termed unitary and orthosymmetric, which serve to unify assumptions for the existence of structured factorizations. A variety of different characterizations of these scalar product classes is given.
Effective Computations in Celestial Mechanics and Astrodynamics
, 1997
"... Problems in Celestial Mechanics and Astrodynamics are considered under the point of view of ..."
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Cited by 11 (0 self)
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Problems in Celestial Mechanics and Astrodynamics are considered under the point of view of