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The smooth P-periodic pulsed oscillator: the normalized pulse, its Hamiltonian and its stroboscopic (period) map

Definition

The normalized pulse. By Test function cutoffs and euclidean localization, applied to K={1/2}⊂(0,1), choose χ∈Cc∞((0,1)) with 0≤χ≤1 and χ=1 on a neighborhood of 1/2. Thus there are 0<α<β<1 with χ=1 on [α,β]. Before taking any integral, extend χ by zero to R, retaining the notation χ. Its compact support inside (0,1) makes this extension identically zero near both endpoints, hence smooth on R. The continuous extended function χ is integrable on [0,1]; by additivity and monotonicity of the integral and the integral of a constant,

I:=∫01χ(s) ds≥∫αβχ(s) ds=β−α>0,

using integrability of continuous functions (A continuous function on [a,b] is Riemann integrable, by Heine-Cantor and Riemann's criterion), additivity and monotonicity (For a<c<b: f is integrable on [a,b] if and only if it is integrable on [a,c] and on [c,b], and then ∫abf=∫acf+∫cbf; with the oriented form for arbitrary a,b,c, If f≤g on [a,b] and both are integrable then ∫abf≤∫abg; and m(b−a)≤∫abf≤M(b−a)), and the integral of a constant (If m≤f≤M on [a,b] then m(b−a)≤L(f,P)≤∫ab‾f≤∫ab‾f≤U(f,P)≤M(b−a) for every partition P; in particular every constant function is integrable, with ∫abc=c(b−a)).

Define w0:=χ/I on (0,1) and let w:R→R be its extension by zero outside (0,1). Since χ has compact support in (0,1), this zero extension is smooth and compactly supported in (0,1). Linearity of the integral (Integrable functions on [a,b] form a set closed under sums and scalar multiples, and ∫ab(λf+μg)=λ∫abf+μ∫abg) gives

w∈Cc∞((0,1)),w≥0,∫01w(s) ds=1.

Fix such a pulse w for the constructions below. The resulting coefficient and endpoint maps may depend on this choice; the later estimates apply to every such w, with constants allowed to depend on it.

The periodic pulse. Fix a real parameter a≥100 and a smallness parameter δ>0, and put P:=π/2+δ. Define βδ:R→R to be the P-periodic function whose restriction to [0,P] is

βδ(t):=0(t∈[0,π2]),βδ(t):=1δ w(t−π/2δ)(t∈[π2,P]).

Both definitions use the same zero extension w:R→R, so the endpoint values w(0) and w(1) are defined and equal to 0. Since w vanishes on neighborhoods of 0 and 1, all its derivatives vanish there; the P-periodic extension of βδ is therefore of class C∞ on R (Ck Euclidean maps and diffeomorphisms). Also βδ≥0. To verify its normalization, put

Bδ(t):={0,0≤t≤π/2,∫0(t−π/2)/δw(s) ds,π/2≤t≤P.

The integral function of the continuous w has derivative w by The first fundamental theorem: if f is integrable on [a,b] and continuous at c, then F′(c)=f(c); in particular a continuous f has F as a primitive and A continuous function on [a,b] is Riemann integrable, by Heine-Cantor and Riemann's criterion, and the chain rule (The chain rule, in one line from Carathéodory: if g is differentiable at c and f is differentiable at g(c), then f∘g is differentiable at c with (f∘g)′(c)=f′(g(c)) g′(c)) gives Bδ′(t)=βδ(t) on the pulse interval. Since w vanishes near its endpoints, Bδ is differentiable across t=π/2 as well. Since βδ is continuous and therefore integrable on [0,P], the second part of the fundamental theorem (The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a)) gives

∫0Pβδ(t) dt=Bδ(P)−Bδ(0)=∫01w(s) ds=1.

The Hamiltonian and its equations. Use the phase domain U=R2 with coordinates (q,p) and standard symplectic form ω=dq∧dp and matrix J=(01−10), as in A phase domain, its canonical one-form and its standard symplectic two-form. For each fixed time t, define the smooth Hamiltonian function

Hδ:R×R2⟶R,Hδ(t,q,p):=p2+q22+βδ(t)(aq−q33).

The Hamiltonian-vector-field convention is ιXHω=dH, for which The Hamiltonian field of a C2 function on a phase domain is J∇H, and the Poisson bracket is ∑i(∂qif ∂pig−∂pif ∂qig) gives XH=J∇H=(∂pH,−∂qH). Here ∂pHδ=p and ∂qHδ=q+βδ(t)(a−q2), so the associated time-dependent first-order system is

q′=p,p′=−q+βδ(t) (q2−a),

equivalently the second-order equation q′′=−q+βδ(t)(q2−a); the right-hand side is C∞ in (t,q,p), hence continuous and locally Lipschitz in the state variable, so every initial condition has a unique maximal solution (First-order systems, initial value problems, and solutions on intervals, Extensions, maximal solutions, maximal intervals, and global solutions, Every Picard–Lindelöf initial value problem has one maximal solution on an open interval). The system is P-periodic in t.

Free rotation and pulse endpoint maps. Over the first subinterval [0,π/2] the pulse vanishes and the system is the free oscillator; define the free rotation

R0:R2→R2,R0(q,p):=(p,−q),

which is the time-π/2 solution operator of q′=p, p′=−q: the map t↦(q0cos⁡t+p0sin⁡t, −q0sin⁡t+p0cos⁡t) solves the free system by the derivative identities of sine and cosine (The derivatives of sine and cosine are cosine and minus sine) and has initial data (q0,p0). Moreover cos⁡(π/2)=0 by the zero-set statement (The zero sets of sine and cosine and the least positive common period 2 pi), sin⁡(π/2)>0 by positivity on (0,π) (Pi is the first positive zero of sine), and sin⁡2(π/2)+cos⁡2(π/2)=1 (Parity and the Pythagorean identity for sine and cosine), so sin⁡(π/2)=1. Uniqueness of solutions then identifies the endpoint map with R0.

For s∈[0,1] the rescaled pulse equation is

qs=δ p,ps=−δ q+w(s) (q2−a),

obtained from the second half of the period by the substitution s=(t−π/2)/δ. For each initial state z=(q,p)∈R2, let Jzδ be the open maximal interval containing 0 of its solution to the rescaled equation. Define

Dδ:={z∈R2:[0,1]⊆Jzδ},Kδ:Dδ→R2,Kδ(z):=(q(1),p(1)),

where (q(s),p(s)) is the unique maximal solution with (q,p)(0)=z (Every Picard–Lindelöf initial value problem has one maximal solution on an open interval). For the original P-periodic system, let Jz be the maximal existence interval of the solution through z at time 0, and set DP:={z∈R2:[0,P]⊆Jz}. Define the stroboscopic map by

Gδ:DGδ→R2,DGδ:={z∈R2:R0(z)∈Dδ},Gδ(z):=Kδ(R0(z)).

The change of time variable s=(t−π/2)/δ identifies solutions on [π/2,P] with solutions of the rescaled equation on [0,1]. Concatenating with the unique free solution on [0,π/2] shows DGδ=DP and Gδ=θP there, where θP:DP→R2 is the stroboscopic map of The stroboscopic (time-P) map of a P-periodic first-order system. Conversely, restricting any solution through time P to the pulse interval and applying the same change of variables gives a solution of the rescaled equation through s=1; uniqueness identifies both maps.

Remarks

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