5. Initial Value Problems Flashcards

1
Q

First Order IVPs

General Form

A

x’ = f(x(t),t)

-with x(0)=xo

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2
Q

Second Order IVPs

General Form

A

x’’ = f(x’(t),x(t),t)

-with x(0)=xo and x’(0)=xo’

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3
Q

First Order IVPs - Standard Expansion

Steps

A
1) suppose that:
x ~ xo(t) + ε*x1(t) + ε²x2(t)+...
as ε->0
2) sub into equation
3) consider O(1) terms, then O(ε), then O(ε²) etc.
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4
Q

Second Order IVPs

Most Fundamental Form

A

x’’ + ωo²x = 0

-with initial conditions

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5
Q

Second Order IVPs

Fundamental Form - General Solution

A
x = a cos(ωot) + b sin(ωot)
OR
x = Ae^(iωot) + Be^(-iωot)
= Ae^(iωot) + A* e^(-iωot)
-since x(t) needs to be real
-to fit the initial conditions, use a and b i the first equation or Re(A) and Im(A) in the second
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6
Q

Second Order IVPs

Fundamental Form - Period and Frequency

A
  • solution is oscillatory and periodic in time, once cycle corresponds to ωot increasing by 2π
  • so the period is, T=2π/ωo
  • and ωo is the frequency
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7
Q

Second Order IVPs

Forced Systems

A

x’’ + ωo²x = α cosωt + β sinωt

-where ωo is the natural frequency and ω is the forcing frequency

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8
Q

Second Order IVPs

Forced Systems - Complimentary Function

A

xcf = a cosωot + b sinωot

-determine a and b with initial conditions

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9
Q

Second Order IVPs

Forced Systems - Particular Integral

A
xpi = C cosωot + D sinωot
-where:
C = α / (ωo²-ω²)
-and
D = β / (ωo² - ω²)
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10
Q

Second Order IVPs

Forced Systems - Resonant Response

A

-there is a resonant response when ω->ωo

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11
Q

Second Order IVPs

Forced Systems - Forcing at Resonant Frequency

A

-governing equation:
x’’ + ωo²x = α cosωot + β sinωot
=>
x(t) = a cosωot + b sinωot - β/2ωo t cos(ωot) + α/2ωo t sin(ωot)

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12
Q

Motion of a Non-Linear Pendulum

Equation

A
d²θ/dq² + g/L sinθ = 0
-with:
θ(0)=θo
dθ(0)/dq = 0
-where θo>0
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13
Q

Motion of a Non-Linear Pendulum

Non-Dimensionalising

A

-introduce a non-dimensional time, t, with t∝q where q has dimensions of seconds:
t = √[g/L] q

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14
Q

Motion of a Non-Linear Pendulum

Conservation of Energy

A
  • the non-linear pendulum system conserves energy

- prove this by multiplying by dθ/dt

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15
Q

Motion of a Non-Linear Pendulum

Solution

A

-make the substitution x(t) = θ/θo
-apply a Taylor expansion to sine
=>
x’’ + x = εx³/6 - ε²x^5/120 + O(ε³)
-gather terms of like order and apply the boundary conditions

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16
Q

Motion of a Non-Linear Pendulum

Time Period at Leading Order

A

-at leading order:
x(t) ~ cost
=>
T = 2π

17
Q

Motion of a Non-Linear Pendulum

Time Period at O(ε)

A

-we anticipate:
T = 2π + 4α1ε + O(ε²)
-we know that x=0 when t=T/4=π/2 + α1ε + O(ε²)
-sub in to the O(ε) expression for x(t)

18
Q

Motion of a Non-Linear Pendulum

Secular Term

A
  • the order ε expansion for x(t) contains a secular term ∝ tsint which grown in time
  • the expansion is valid when t=O(1) but the secular term makes it invalid when εt=Os(1)
  • to improve this, alternative techniques are needed
19
Q

Method of Multiple Scales

Aim

A

-to develop an asymptotic expansion that works for both t=O(1) and t=Os(1/ε), as ε->0

20
Q

Method of Multiple Scales

Time

A

-define fast and slow timescales:
τ = t and T = εt
-so if t=O(1) then τ=O(1) but T is small
-if t=Os(1/ε) then τ is large but T is O(1)
-as the name suggests, multiple of these timescales can be defined

21
Q

Method of Multiple Scales

Steps

A

1) define time scales e.g. τ=t and T=εt
2) we then seek solutions x(τ ,T) rather than x(t), so rewrite the governing equation in terms of τ and T
3) assume that x ~ xo + εx1 + ε²x2 +…
4) consider O(1) terms from the governing equation, then O(ε) terms etc.
5) make choices about the unknown constants which will eliminate the secular terms
6) convert back to original timescale, t

22
Q

Linstedt-Poincare Technique

Aim

A

-we use LPT when the initial value problem with ε≠0 (the perturbed problem) has a frequency shift from the unperturbed problem

23
Q

Linstedt-Poincare Technique

Strained Coordinate

A

-replace t by a strained coordinate:
τ = (1 + εω1 + ε²ω2 + …)t
-where we choose ω1,ω2,… to remove secularities

24
Q

Linstedt-Poincare Technique

Steps

A

1) introduce strained coordinate τ = (1 + εω1 + ε²ω2 + …)t
2) rewrite governing equation and boundary conditions in terms of τ instead of t
3) let x ~ xo + ε x1 + ε² x2 + ….
4) consider O(1) terms, choose ω’s to remove forcing at resonant frequency (i.e. to avoid secularities)
5) then do the same for O(ε) terms and so on

25
Q

Renormalisation

Aim

A

-similar technique to LPT
-starts from the results of a completely standard asymptotic expansion using:
x(t) ~ xo(t) + εx1(t) + ε²x2(t) + …
-the results of which is known to be secular

26
Q

Renormalisation

Straining Functions

A

-introduce:
t = τ + ε f1(τ) + ε² f2(τ) + …
-where the straining functions fj(τ) will be chosen to eliminate secularities

27
Q

Renormalisation

Steps

A

1) introduce strained functions, t = τ + ε f1(τ) + ε² f2(τ) + …
2) take the standard expansion with secularities that need removing and rewrite in terms of τ
3) choose fj(τ) to eliminate the secularities
4) truncate series at desired order