ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Chapter 2 Laplace Transform A. Bazoune 2.1 INTRODUCTION Laplace Transform is one of the most important mathematical tools available for modeling and analyzing linear systems. 2.2 COMPLEX NUMBERS, COMPLEX VARIABLES, AND COMPLEX FUNCTIONS Complex Numbers Using the notation j = −1 , one can express all complex numbers in engineering calculations as z = x + jy where x is the real part and are real and that j jy is the imaginary part. Notice that both x and y is the only imaginary quantity in the expression above. z y θ x Fig. 2-1 Complex plane representation of a complex number z. The Magnitude, or absolute value, of z is defined as the length of the directed segment shown in Fig. 2-1. Magnitude of z = z = x 2 + y 2 The angle of z is the angle that the directed line segment makes with the positive real axis. A counterclockwise rotation is defined as the positive direction for the measurement of angles. 1/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform angle of z = θ = tan −1 (y x) A complex number can be written in rectangular form as: ⎫ ⎬ z ( cos θ + j sin θ ) ⎭ z = x + jy z= rectangular form and in polar form as z = z ∠θ z= ze ⎫ ⎬ ⎭ jθ polar form In converting complex numbers from rectangular to polar from , we use z= z = 2 ⎛y⎞ ⎟ ⎝x⎠ θ = tan ⎜ −1 x +y , 2 To convert complex numbers from polar to rectangular form, we employ x = z cos θ , y = z sin θ Complex Conjugate. defined as The complex conjugate of z = x + jy is z = x − jy The complex conjugate of z thus has the same real part as z and an imaginary part that is the negative of the imaginary part of z as shown in Fig. 2-2. Notice that z y θ x −y z Fig. 2-2 Complex number z and its complex conjugate 2/36 z. ME 413 Systems Dynamics & Control Chapter Two: Laplace transform z = x + jy = z ∠θ = z ( cos θ + j sin θ ) z = x − jy = z ∠ ( −θ ) = z ( cos θ − j sin θ ) The power series expansions of cos θ Euler’s Theorem. sin θ are, respectively, θ cos θ = 1 − 2 + θ 2! and sin θ = θ − θ θ 3 + 3! Thus cos θ + j sin θ = 1 + jθ + 4 − 4! 5 − Since e = 1+ x + x it follows that x +L ( jθ ) + 2! +L 7 7! 2 6 6! θ 5! ( jθ ) θ 3 + ( jθ ) 3! 2 + 2! x and 4! 4 +L 3 +L 3! cos θ + j sin θ = e jθ Using the above relation, one can express the sine and cosine in complex form. Noting that e − jθ is the complex conjugate of e jθ and that jθ e = cos θ + j sin θ e − jθ = cos θ − j sin θ By adding the above expressions together, we find that jθ cos θ = e +e − jθ 2 while by subtracting the second expression above from the first one, we obtain jθ sin θ = 3/36 e −e 2j − jθ ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Complex Algebra. Equality of complex numbers. Two complex numbers z1 and z2 are said to be equal if and only if their real parts are equal and their imaginary parts are equal. So if two complex numbers are written z1 = x1 + jy1 , Then z1 = z2 if and only if x1 = x2 and and z2 = x2 + jy 2 y1 = y 2 . Addition. Two complex numbers z1 and z2 in rectangular form can be added by adding the real parts and the imaginary parts separately: z1 + z2 = ( x1 + jy1 ) + ( x2 + jy 2 ) = ( x1 + x2 ) + j ( y1 + y 2 ) Subtraction. Subtracting one complex number from another can be considered as adding the negative of the former: z1 − z2 = ( x1 + jy1 ) − ( x2 + jy 2 ) = ( x1 − x2 ) + j ( y1 − y 2 ) Multiplication. If a complex number is multiplied by a real number, the result is a complex number whose real and imaginary parts are multiplied by that real number: az = a ( x + jy ) = ax + jay , ( a = real number) If two complex numbers appear in rectangular form and we want the product in rectangular form, multiplication is accomplished by using the fact that j = −1 . Thus, 2 if two complex numbers are written z1 = x1 + jy1 , z2 = x2 + jy 2 Then z1z2 = ( x1 + jy1 )( x2 + jy 2 ) = x1x2 + jx1y 2 + jy1x2 + j 2 y1y 2 = ( x1x2 − y1y 2 ) + j ( x1y 2 + y1x2 ) In polar form, multiplication of two complex numbers can be done easily. The magnitude of the product is the product of the two magnitudes, and the angle of the product is the sum of the two angles. So if two complex numbers are written 4/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform z1 = z1 ∠θ1 , then z2 = z2 ∠θ 2 z1z2 = z1 z2 ∠ (θ1 + θ 2 ) Multiplication by j. It is important to note that multiplication by equivalent to a counterclockwise rotation by 90o. j is For example, if z = x + jy then jz = j ( x + jy ) = jx + j 2 y = − y + jx or, noting that j = 1 ∠90 , if z = z ∠θ then jz = 1 ∠90 z ∠θ = z ∠ (θ + 90 ) Fig. 2-3 illustrates the multiplication of a complex number z by by j. j. z jz Fig. 2-3 Multiplication of a complex number Division. complex number If a complex number z2 = z2 ∠θ 2 z1 z2 = z1 = z1 ∠θ1 , then z1 ∠θ1 z2 ∠θ 2 = z1 z2 5/36 z ∠ (θ1 − θ 2 ) is divided by another ME 413 Systems Dynamics & Control Chapter Two: Laplace transform That is, the result consists of the quotient of the magnitudes and the difference of the angles. Division in rectangular form can be done by multiplying the denominator and numerator by the complex conjugate of the denominator. For instance, z1 z2 = ( x + jy ) ( x + jy ) 1 1 2 = 2 (x (x + jy1 )( x 2 − jy 2 ) 1 + jy 2 ) ( x 2 − jy 2 ) 1 424 3 2 complex Conjugate of z 2 = = (x x 1 (x x 1 2 (x Division by j. 90o. 2 2 2 + y1 y 2 ) + j ( x 2 y1 − x1 y 2 ) (x 2 z j = +j ) (x y j Division by For example, if then 2 + y1 y 2 ) + y2 ) + y2 2 2 2 (x − x1 y 2 ) 1 + y2 2 2 2 ) is equivalent to a clockwise rotation by z = x + jy ( x + jy ) ( x + jy ) j = j jj = jx − y −1 = y − jx or, z j = z ∠θ 1 ∠90 o ( = z ∠ θ − 90 Fig. 2-4 illustrates the division of a complex number o ) z by j. z by j. z/ j Fig. 2-4 Division of a complex number 6/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Powers and roots. z Multiplying by n times, we obtain z = ( z ∠θ ) = z ∠nθ n n Extracting the 1/ n th power. n n th root of a complex number is equivalent to raising the number to z1 n = ( z ∠θ ) 1n For instance, calculate (8.66 − j5) 3 =z 1n ∠ θ n =? Remember : The real part = x = 8.66 The imaginary part = y = −5 The magnitude = z = The angle = θ = tan Therefore, ( 8.66 − j 5 ) 3 ( −1 () y x = 10 ∠ − 30 x +y 2 = tan o ) 3 −1 2 = 8 .66 + 5 = 10 2 ( ) −5 8.66 = −30 2 o = 1000∠ − 90 = 0 − j1000 = − j1000 . o Remarks. It is important to note that zw = z w z+w ≠ z + w Complex Variable. A complex variable has a real part and an imaginary part, both of which are constant. If the real part or the imaginary part (or both) are variables, the complex number is called a complex variable. In the Laplace transformation, we use the notation s to denote a complex variable; that is, s = σ + jω where ω σ is the real part and jω is the imaginary part. (Notice that both σ and are real.) Complex Function. has a real part and an imaginary part, or 7/36 A complex function F ( s ) , a function of s ME 413 Systems Dynamics & Control Chapter Two: Laplace transform F ( s ) = Fx + jFy where Fx and Fy are real quantities. F ( s ) = F ( s ) = Fx2 + Fy2 Magnitude of Angle of ( F ( s ) = θ = tan −1 Fy Fx ) The angle is measured counterclockwise from the positive real axis. The complex conjugate of F (s) is F ( s ) = Fx − jFy . Complex functions commonly encountered in linear systems analysis are singlevalued functions of s and are uniquely determined for a given value of s . Typically, such functions have the form F (s) = F ( s ) = 0 are called zeros. That is, s = − z1 , s = − z2 ,L , s = − zm are zeros of F ( s ) . • Points at which • Points at which • K ( s + z1 )( s + z2 )L ( s + zm ) ( s + p1 )( s + p2 )L( s + pn ) F ( s ) = ∞ are called poles. That is, s = − p1 , s = − p2 ,L , s = − pn are poles of F ( s ) . k − multiple factors ( s + p ) , then s = − p is called a multiple pole of order k or repeated pole of multiplicity k . If k = 1 , the pole is called a simple pole. If the denominator of F (s) k involves Example █ G( s) = K ( s + 2 )( s + 10 ) s ( s + 1)( s + 5 )( s + 15 ) G ( s ) are values of s s = −2, s = −10 • Zeros of • Poles of G (s) are values of s 2 which make G ( s ) = 0 , that is which make G ( s ) = ∞ , that is s = −0 , s = − 1, s = − 5 ⇒ 8/36 Simple and distinct poles ME 413 Systems Dynamics & Control Chapter Two: Laplace transform s = − 1 5 , s = − 1 5 ⇒ double pole or (pole of multiplicity 2) Since for large values of s (when s → ∞) G (s) = G (s) possesses a triple zero at infinity are included, To summarize: and five poles, k s3 ( s = ∞ , ∞ , ∞ ) ( pole of multiplicity 3). If points at G ( s ) has the same number of poles as zeros. G ( s ) has five zeros, ( s = −2 , − 10 , ∞ , ∞ , ∞ ) ( s = 0, − 1, − 5, − 15, − 15) 9/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform 2.3 LAPLACE TRANSFORMATION What is the Laplace Transform? It is a solution technique that transforms differential equations in the time domain into algebraic equations in the s-domain. Why use Laplace Transform? The Laplace transform is a powerful tool formulated to solve a wide variety of Initial-Value Problems (IVP). The strategy is to transform the difficult differential equations into simple algebraic problems where solutions can be easily obtained. One then applies the Inverse Laplace transform to retrieve the solutions of the original problems. This can be illustrated as follows: L L −1 Definition The Laplace Transform F ( s) of f (t ) is defined as 10/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform f (t ) = a time function such that f (t ) = 0 for t < 0 s = a complex variable F ( s ) = Laplace transform of f (t ) where Exponential Function: Consider the exponential function shown in Fig. 2-5: f (t) for t < 0 ⎧0 f (t ) = ⎨ −αt ⎩Ae for t ≥ 0 where A and α are constants. The Laplace transform of f (t ) can be obtained as follows A Ae −α t t Fig. 2-5. Exponential function ∞ ∞ A − α +s t F ( s ) = L ⎡⎣ Ae −α t ⎤⎦ = ∫ Ae −α t e − st dt = A∫ e ( ) dt = s +α 0 0 Step Function: Consider a step function as shown in Fig. 2-6: ⎧0 f (t ) = ⎨ ⎩A where A for t < 0 f (t ) for t > 0 is a constant. Notice that this is a A −α t special case of the exponential function Ae where α = 0. The step function is undefined at t = 0 . Its Laplace Transform is given by: t Fig. 2-6. Step function ∞ A F (s ) = L ⎡⎣f (t ) ⎤⎦ = L [ A ] = ∫ Ae − st dt = s 0 The step function whose height is unity is called a unit-step function. The unit step t = t0 is frequently written as 1( t − t0 ) . The previous step function whose height is A can be written as A1( t ) . The Laplace Transform of function that occurs at time the unit-step function that is defined by 11/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform for t < 0 for t > 0 ⎧0 1(t ) = ⎨ ⎩1 is ∞ 1 F (s ) = L ⎡⎣1(t ) ⎦⎤ = ∫1e − st dt = s 0 t = t0 corresponds to a constant signal t equals t0 . Physically, a step function occurring at time suddenly applied to the system at time Ramp Function: Consider a ramp function as shown in Fig. 2-7 ⎧0 f (t ) = ⎨ ⎩ At for t < 0 for t ≥ 0 f (t ) f (t ) = At where A is a constant. The Laplace Transform of the ramp function is: α slope = tan α = A ∞ t F (s ) = L [ At ] = A ∫ te − st dt Fig. 2-7. Ramp function 0 To evaluate the above integral we use the formula for the integration by parts ∞ ∞ ∫ udv = uv | − ∫ vdu ∞ 0 0 0 where in this case u = At ⇒ du = A 1 ⇒ v = − e − st s dv = e − st dt Substituting these expressions into equation the above integral leads to the following expression: ∞ ∞ Ate − st ∞ Ae − st |0 + ∫ dt F (s ) = L [ At ] = ∫ Ate dt = − s s 0 0 − st ( −Ae ) | = (0 − 0) + − st s2 12/36 ∞ 0 =0− ( −A ) = A s2 s2 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Sinusoidal Function: The Laplace Transform of the sinusoidal function for t < 0 ⎧0 f (t ) = ⎨ ⎩ A sin (ω t ) for t ≥ 0 Fig. 2-8. Sinusoidal function where A and ω are constants, is obtained as follows. Noting that e jω t = cos ω t + j sin ω t sin ω t and and e − jω t = cos ω t − j sin ω t cos ω t can be written as sin ω t = 1 jω t e − e − jω t ) ( 2j and cos ω t = 1 jω t e + e − jω t ) ( 2 Hence ∞ A A 1 A 1 L [ A sin ω t ] = ∫ ( e jω t − e− jω t ) e− st dt = − 2j 0 2 j s − jω 2 j s + jω = A ⎛ s + jω − s + jω ⎞ A ⎛ 2 jω ⎞ Aω = 2 ⎜ ⎟= ⎜ 2 2 2 2 ⎟ 2 s +ω 2j⎝ ⎠ 2 j ⎝ s +ω ⎠ s +ω Similarly ∞ A A 1 A 1 L [ A cos ω t ] = ∫ ( e jω t + e − jω t ) e− st dt = + 20 2 s − jω 2 s + jω = A ⎛ s + jω + s − jω ⎞ A ⎛ 2 s ⎞ As = 2 ⎜ ⎟= ⎜ 2 2 2 2 ⎟ 2 2⎝ s +ω ⎠ 2 ⎝ s +ω ⎠ s +ω 13/36 ME 413 Systems Dynamics & Control f (t ) from Remark: Chapter Two: Laplace transform The Laplace Transform of any Laplace transformable function f (t ) can be obtained by multiplying 0 to ∞. by e − st and then integrating the product Once we now the method of obtaining the Laplace Transform, however, it is not necessary to derive the Laplace transform of f (t ) each time. Laplace Transform Tables can conveniently be used to find the transform of a given function f (t ) . Refer to Table 2.1 of the Textbook. Notice that the Laplace Transforms provided in Tables in general are valid for 0≤t <∞ . Translated Functions: Let us obtain the Laplace transform translated function f ( t − α )1( t − α ) where α ≥ 0. This function is zero for of the t < α. f (t − α )1(t − α ) f (t )1(t ) t 0 Fig. 2-9 Function f ( t )1( t ) 0 α and translated function By definition, the Laplace transform of f ( t − α )1( t − α ) t f ( t − α )1( t − α ) is ∞ L ⎡⎣f (t − α )1(t − α ) ⎤⎦ = ∫ f (t − α )1(t − α )e −st dt 0 Let τ = t − α , then t = 0 ⇒ τ = −α , t → ∞ ⇒ τ → ∞ and dt = dτ and ∞ ∫ f ( t − α )1( t − α )e − st ∞ dt = f (τ )1(τ ) = 0 for τ < 0, − s (τ +α ) dτ − 0 Noting that ∫α f (τ )1(τ )e we can change the lower limit from Thus 14/36 −α to 0. ME 413 Systems Dynamics & Control ∞ ∫α f (τ )1(τ )e Chapter Two: Laplace transform ∞ d τ = ∫ f (τ )1(τ ) e − s (τ +α ) − 0 =e ∞ ∫ f (τ )e −α s ∞ d τ = ∫ f (τ )e − sτ e −α s d τ − s (τ +α ) 0 − sτ d τ = e −α s F (s ) 0 where ∞ F ( s ) = L ⎡⎣f (t ) ⎤⎦ = ∫ f (t ) e − st dt 0 and also L ⎡⎣f (t − α )1(t − α ) ⎤⎦ = e −α s F (s ) α ≥0 Pulse Function: Consider the pulse function shown in Fig. 2-10 ⎧A ⎪ f (t ) = ⎨ t 0 ⎪0 ⎩ where A and t0 f (t ) for 0 < t < t0 for t < 0, t0 < t A t0 are constants. The pulse function may be considered as a step function of height A t0 by that begins at a negative beginning at t =0 step and that is superimposed function of height t = t0 ; that is , t A t0 0 t0 Fig. 2-10 A pulse function A f (t ) = t0 1( t ) − A t0 1( t − t 0 ) f (t ) A 1( t ) t0 A 1( t − t0 ) t0 A t0 t 0 t t0 0 Then the Laplace Transform of L ⎡A ⎤ ⎡⎣f (t ) ⎤⎦ = L ⎢ 1(t ) ⎥ − L ⎣t0 ⎦ t0 f (t ) 0 t t0 is obtained as ⎡A ⎤ A ⎛ 1 ⎞ A ⎛ 1 ⎞ − st 0 A − 1 t t 1 − e − st 0 ( ) 0 ⎥ = ⎢ ⎜ ⎟ − ⎜ ⎟e = t 0s ⎣t0 ⎦ t0 ⎝ s ⎠ t0 ⎝ s ⎠ ( 15/36 ) ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Impulse Function: The impulse function is a special limiting case of the pulse function. Consider the impulse function ⎧lim A ⎪ f ( t ) = ⎨ t →0 t0 ⎪0 ⎩ for 0 < t < t0 f (t ) 0 t0 → 0 for t < 0, t0 < t A →∞ t0 Fig. 2-11 depicts the impulse function shown in Fig. 2-10 as t0 approaches 0. t Fig. 2-11. Impulse function Since the height of the impulse function the impulse is equal to and the duration is t0 , the area under A / t0 As the duration A. t0 approaches 0, the height A / t0 approaches infinity, but the area under the impulse remains equal to A. Notice that the magnitude of the impulse is measured by its area. Referring to the transformed equation previously derived for the pulse function, i.e., L [ f ( t )] = A (1 − e ) ts − s t0 0 the Laplace Transform of the impulse function is shown to be L ⎡ A (1 − e [ f ( t )] = lim ⎢ ts ⎣ t0 →0 0 − s t0 ) ⎤ = lim ⎥ ⎦ t0 →0 d dt0 ⎡⎣ A (1 − e d dt 0 − s t0 )⎤⎦ = lim (t s ) t0 →0 ⎡⎣ A ( se − s t0 (s) )⎤⎦ = A 0 Thus the Laplace Transform of the impulse function is equal to the area under the impulse. The impulse function whose area is equal to unity is called the unit impulse function or the Dirac delta function. The unit impulse function occurring at t = t0 is usually denoted by ⎧ ⎪δ ( t − t ) = 0 0 ⎪⎪ ⎨δ ( t − t0 ) = ∞ ⎪∞ ⎪ ∫ δ ( t − t0 ) = 1 ⎪⎩ −∞ 16/36 for t ≠ t0 for t = t0 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Relationships among Singular Functions The ramp, step, and impulse functions represent a family of functions, which as shown in Fig. 2-12 are related by successive integrations. δ (t ) u s (t ) u r (t ) 1.0 1.0 0 0 t Time 0 t Time L ⎡⎣δ (t ) ⎤⎦ = 1 L ⎡⎣u s (t ) ⎤⎦ = 1 s 1.0 Time L ⎡⎣u r (t ) ⎤⎦ = t 1 s2 Fig. 2-12 The relationship between singularity functions. Time Shifting of Singularity Functions The singularity functions may be used to describe transient inputs that take place at t = 0 . The discontinuity associated with each function occurs when the function argument is zero; therefore, a step that occurs at time t 0 may be written as u s (t − t 0 ) since t − t 0 = 0 at t = t 0 . This property may be used to a time other than synthesize a transient function from a sum of singularity functions; for example, Fig. () () ( ) ( ) ( ) 2-13 shows the function u t = u s t − 2u s t − t 0 + ur t − 2 − ur t − 3 . u (t ) u (t ) 2 u t s ( ) 1 −1 −2 u r (t − 2 ) 1 2 3 4 2 1 t −u r (t − 3) −2u s (t − 1) Fig. 2-13 A transient function −1 −2 1 2 3 4 t u ( t ) = u s ( t ) − 2u s ( t − 1) + ur ( t − 2 ) − ur ( t − 3 ) synthesized from unit singularity functions 17/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Multiplication of f ( t ) by e If f (t ) is Laplace transformable, its Laplace transform being Laplace transform of L ⎡⎣e −α t e f (t ) −α t ∞ f (t ) ⎤⎦ = ∫ e −α t 0 █ Example F (s) , is ∞ f (t ) e dt = ∫ f (t )e − st −( s +α )t dt = F ( s + α ) 0 ω 2 + ω2 = F (s) Find Laplace transform of and e −α t sin ω t L [cos ω t ] = s and s = G (s) 2 + ω2 e −α t cos ω t Solution L ⎡⎣e −α t sin ω t ⎤⎦ = F ( s + α ) = ω 2 (s + α ) + ω2 L ⎡⎣e −α t cos ω t ⎤⎦ = G ( s + α ) = s +α and 2 (s + α ) + ω2 Laplace Transform Theorems Differentiation Theorem L L ⎡d ⎤ ⎢⎣ dt f ( t ) ⎥⎦ = sF ( s ) − f ( 0 ) ⎡ d2 ⎤ 2 & ⎢ dt 2 f ( t ) ⎥ = s F ( s ) − sf ( 0 ) − f ( 0 ) ⎣ ⎦ Similarly for the nth derivative of L then the Given Laplace transforms of L [sin ω t ] = s █ −α t f ( t ) , we obtain ( n −1) ⎡dn ⎤ n n −1 n −2 & ⎢ dt n f (t ) ⎥ = s F (s ) − s f (0) − s f (0) − L − f (0) ⎣ ⎦ 18/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform ( n −1) In the above, the following quantities of █ f ( t ) , df ( t ) / dt , L, d Example n −1 f ( t ) / dt f ( 0 ) , f& ( 0 ) , L, f ( 0 ) n −1 , represent the values respectively, evaluated at t = 0. Given Find the Laplace transform F(s) of f(t). █ Solution Using the Differentiation Theorem on the first two terms leads to: Using the definition of the Laplace transform on the remaining term gives: From these results, the Laplace transform F(s) of the given equation can be expressed as: Rearranging this expression by factoring leads to: Solving this expression for X(s) gives the following answer: 19/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Final Value Theorem (FVT) lim [ f (t ) ] = lim ⎡⎣s F ( s ) ⎤⎦ t →∞ █ Example s →0 Given: Find the final value of x(t). █ Solution To solve this problem, use the Final Value Theorem (FVT) lim [ f (t ) ] = lim ⎡⎣s F ( s ) ⎤⎦ t →∞ s →0 Substituting the given expression into this equation leads to the solution: Initial Value Theorem (IVT) f (0+ ) = lim ⎡⎣s F ( s ) ⎤⎦ s →∞ █ Example Given: Find the initial value of x(t), i.e. find x(0). █ Solution To solve this problem, use the Initial Value Theorem (IVT): Substituting the given expression into this equation leads to the solution: 20/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform For this example, as "s" goes to infinity, all terms involving "s" in the numerator and denominator cancel. (Note that if there was one extra "s" term in the denominator than there was in the numerator, this extra term would not be cancelled out and the entire expression would go to zero.) Integration Theorem L █ Example ⎡t ⎤ F (s ) ⎢ ∫ f (t )dt ⎥ = s ⎣0 ⎦ Given: Find Laplace transform of the given expression. (Hint: Let f(t) = At) █ Solution To solve this problem, use the integration theorem: Substituting the result for F(s) obtained in the previous example leads to the solution: Use of MATLAB █ Example Use MATLAB to find Laplace Transform of 21/36 f ( t ) = t cos(3t ) ME 413 Systems Dynamics & Control Chapter Two: Laplace transform █ Matlab Solution >> >> syms t s f = t*cos(3*t); Then the Laplace transform of f is given by >> >> F F F F = laplace(f) =1/(s^2+9)*cos(2*atan(3/s)) = simplify(expand(F)) =(s^2-9)/(s^2+9)^2 Thus we obtain the Laplace transform F (s) = █ Example █ Matlab Solution >> >> syms t s f=3*t-5*sin(2*t); s2 − 9 (s + 9) 2 2 Use MATLAB to find Laplace Transform of f ( t ) = 3t − 5cos(2t ) Then the Laplace transform of f is given by >> F = laplace(f) F=3/s^2-10/(s^2+4) >> F = simplify(expand(F)) F =-(7*s^2-12)/s^2/(s^2+4) Thus we obtain the Laplace transform −7 s 2 + 12 F (s) = 2 2 s ( s + 4) 2.4 INVERSE LAPLACE TRANSFORMATION The inverse Laplace transformation refers to the process of finding the time function f ( t ) from the corresponding Laplace transform F ( s ) ; i.e., f (t ) = L [ F (s ) ] −1 Several methods are available for finding the inverse Laplace transforms 22/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform 1. Use Tables of Laplace transforms 2. Use partial-fraction expansion method. Partial-Fraction Transforms Expansion for Finding Inverse Laplace If F ( s ) , the Laplace transform of f ( t ) , is broken up into components F ( s ) = F1 ( s ) + F2 ( s ) + F3 ( s ) + L +F n (s) and if the inverse Laplace transform of F1 ( s ) , F2 ( s ) , F3 ( s ) , L , F n ( s ) , are readily available then L −1 [ F (s )] = L −1 ⎡⎣ F1 ( s ) ⎤⎦ + L −1 ⎡⎣ F2 ( s ) ⎤⎦ + L = f 1 (t ) + f 2 (t ) + L + f n (t ) + L −1 ⎡⎣ F n ( s )⎤⎦ where f1 ( t ) , f 2 ( t ) , L , f n ( t ) are the inverse Laplace transform of F1 ( s ) , F2 ( s ) , L, F n ( s ) , respectively. F (s ) = F ( s ) frequently occurs in the form N (s ) , m = deg N ( s ) < deg D ( s ) = n D (s ) where N ( s ) and D ( s ) are polynomials in s and the degree of D ( s ) is not higher than the degree of N ( s ) . Notice that applying the partial-fraction expansion technique in the search for the inverse Laplace transform of F ( s ) = N ( s ) / D ( s ) requires that the poles of D ( s ) (roots of the denominator) must be known in advance. Consider F ( s ) written in the factored form F (s ) = N ( s ) K ( s + z 1 )( s + z 2 )L ( s + z n ) = D (s ) ( s + p1 )( s + p 2 )L ( s + p n ) p1 , p2 , K , pn and z1 , z2 , K , zn are either real or complex quantities, but for each pi or zi there will occur the complex conjugate of pi or zi , respectively. Here where the highest power of s in N ( s ) is assumed to be higher than that in D ( s ) . Notice that if the degree of the numerator is greater than (or equal to) that of the denominator, then polynomial division must be performed so that the remainder polynomial is of a lower degree than D ( s ) . For instance, 23/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform s3 +2 −s + 2 , =s + 2 2 s +1 s +1 Case I. deg ( −s + 2 ) < deg ( s + 1 ) 2 Distinct Real Poles In this case, F ( s ) can be expanded into a sum of partial fractions F (s ) = N (s ) r1 r2 rn = + +L+ D ( s ) ( s + p1 ) ( s + p 2 ) (s + pn ) where rk ( k = 1, 2,K , n ) are constants. The coefficient rk is called the residue at the s = − pk . The value of rk can be found by multiplying both sides of the above pole at equation ( s + pk ) and letting s = − pk , which gives ⎡ ⎡ r ( s + pk ) r2 ( s + pk ) N (s) ⎤ r ( s + pk ) r ( s + pk ) ⎤ =⎢ 1 + +L+ k +L+ n = rk ⎢( s + pk ) ⎥ ⎥ D ( s ) ⎦ s =− p ⎣ ( s + p1 ) s + p2 ) s + pk ) s + pn ) ⎦ s =− p ( ( ( ⎣ k k We see that all the expanded terms drop out with the exception of residue rk is found from ⎡ N (s ) ⎤ rk = ⎢( s + p k ) ⎥ D ( s ) ⎦ s =− p ⎣ k (2.6) Since ⎡ rk ⎤ −p t L−1 ⎢ ⎥ = rk e k ⎣ (s + pk ) ⎦ f ( t ) is obtained as f (t ) = L −1 [ F (s ) ] = r1e − p1t + r2e − p 2t + L + rk e − p k t █ Example Find the inverse Laplace transform of F (s) = █ rk .Thus the Solution s+3 ( s + 1)( s + 2 ) The partial fraction expansion of F ( s ) is F (s) = s+3 r r2 = 1 + ( s + 1)( s + 2 ) ( s + 1) ( s + 2 ) 24/36 t ≥0 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform where r1 and r2 are found by using Equation (2.6) ⎡ ( s + 3) ⎤⎥ = ⎡ ( s + 3) ⎤ = −1 + 3 = 2 r1 = ⎢ ( s + 1) ⎢ ⎥ ⎢ ( s + 1) ( s + 2 ) ⎦⎥ s =−1 ⎣ ( s + 2 ) ⎦ s =−1 −1 + 2 ⎣ ⎡ ( s + 3) ⎥⎤ = ⎡ ( s + 3) ⎤ = −2 + 3 = −1 r2 = ⎢ ( s + 2 ) ⎢ ⎥ ⎢ ( s + 1) ( s + 2 ) ⎥⎦ s =−2 ⎣ ( s + 1) ⎦ s =−2 −2 + 1 ⎣ Thus F (s) = s+3 2 −1 = + ( s + 1)( s + 2 ) ( s + 1) ( s + 2 ) ⎡ 2 ⎤ ⎡ −1 ⎤ −1 −t −2t f (t ) = L −1 [ F (s ) ] = L −1 ⎢ ⎥ +L ⎢ ⎥ = 2e − e ⎣ ( s + 1) ⎦ ⎣ (s + 2) ⎦ t ≥0 Use of MATLAB: Use MATLAB to find the inverse Laplace Transform of the above example F (s) = s+3 ( s + 1)( s + 2 ) >> syms t s >> F = (s+3)/((s+1)*(s+2)) Then the inverse Laplace transform of f (t ) is given by >> F = ilaplace(f) f =2*exp(-t)-exp(-2*t) >> pretty(f) 2 exp(-t) - exp(-2 t) Thus we obtain the Laplace transform f ( t ) = L−1 [ F ( s ) ] = 2e −t − e −2t █ Example t≥0 Obtain the inverse Laplace transform of F (s) = s 3 + 5s 2 + 9 s + 7 ( s + 1)( s + 2 ) 25/36 ME 413 Systems Dynamics & Control █ Chapter Two: Laplace transform Solution Since the degree of the numerator is higher than that of the denominator polynomial, we must divide the numerator by the denominator F (s ) = s + 2 + s +3 2 −1 = s + 2+ + 1) ( s + 2 ) ( s + 1)( s + 2 ) ( s +4 144 2444 3 previous example Notice that F (s) L ⎡⎣δ (t ) ⎤⎦ = 1 and ⎡ d δ (t ) ⎤ ⎥ = s , so the inverse Laplace transform of ⎣ dt ⎦ L ⎢ is given by f (t ) = Case II. d δ ( t ) + 2δ ( t ) + 2e − t − e−2t dt t≥0 Complex Conjugate Poles Consider a function F ( s ) that involves a quadratic factor s 2 + as + b in the denominator. If this quadratic factor has a pair of complex conjugate poles, then it is better not to factor this term in order to avoid complex numbers. For example, if F ( s ) is given as F ( s) = where a ≥ 0 and b ≥ 0 , and p(s) s ( s 2 + as + b ) s 2 + as + b = 0 has a pair of complex conjugate poles, then expand F ( s ) into the following partial-fraction expansion form: F ( s) = █ Example c ds + e + 2 s s + as + b Obtain: the inverse Laplace transform of F ( s) = █ 2 s + 12 s + 2s + 5 2 Solution 1: Use of Complex Numbers 26/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Notice that the poles of the denominator are s1,2 = Therefore F (s ) F (s ) = −b ± b 2 − 4ac −2 ± 4 − 4 × 1× 5 −2 ± −16 = = = −1 ± j 2 . 2a 2 2 can be written as 2s + 12 2s + 12 α β = = + s 2 + 2s + 5 ( s + 1 + j 2 )( s + 1 − j 2 ) s + 1 + j 2 s + 1 − j 2 where the constants α and β that can be found as before α= ( s + 1 + j 2 ) ( 2s + 12 ) ( 2 ( −1 − j 2 ) + 12 ) = 10 − j 4 = 1 − j 5 = 2 ( s + 1 + j 2 ) ( s + 1 − j 2 ) s =−1− j 2 ( −1 − j 2 + 1 − j 2 ) − j 4 β= ( s + 1 − j 2 ) ( 2s + 12 ) (s + 1 + j 2) (s + 1 − j 2) Notice that β = s = −1+ j 2 ( 2 ( −1 + j 2 ) + 12 ) = 10 + j 4 = 1 + j 5 ( −1 + j 2 + 1 + j 2 ) is the complex conjugate of into the expression of α. +j4 Substitute the values of 2 α F (s ) 5 5 j 1 + 2s + 12 2 + 2 F (s ) = 2 = s + 2s + 5 s + 1 + j 2 s + 1 − j 2 1− j and 5 ⎞ − 1+ j 2 t ⎛ 5 ⎞ − 1− j 2 t ⎛ f (t ) = L −1 [ F (s ) ] = ⎜1 − j ⎟e ( ) + ⎜1 + j ⎟e ( ) 2⎠ 2⎠ ⎝ ⎝ 5 5 = e −t e − j 2t − j e −t e − j 2t + e −t e j 2t + j e −t e j 2t 2 2 j 2t − j 2t j 2t ⎞ − e − j 2t ⎞ +e −t ⎛ e −t ⎛ e = 2e ⎜ ⎟ ⎟ + j 5e ⎜ 2 2 ⎝ ⎠ ⎝ ⎠ j 2t ⎛ e j 2t + e − j 2t ⎞ − e − j 2t ⎞ −t ⎛ e 5 e = 2e −t ⎜ − ⎜ ⎟ ⎟ 2j 2 ⎝ ⎝144244 ⎠ 3 144244 3⎠ cos( 2t ) = 2e −t cos ( 2t ) − 5e −t sin ( 2t ) 27/36 sin ( 2t ) and β ME 413 Systems Dynamics & Control Chapter Two: Laplace transform Solution 2: Completing The square █ The expression of can be written in general as F (s) F (s) = cs + d s + 2as + a 2 + ω 2 2 where a and ω are positive real. It is clear that the denominator in the above expression is a complete square, i.e., it can be written as s 2 + 2as + a 2 + ω 2 = ( s 2 + a 2 ) + ω 2 F ( s ) into the following form c ( s + a ) + d − ca cs + d cs + d = = F (s) = 2 2 s + 2as + a 2 + ω 2 ( s + a )2 + ω 2 (s + a) + ω2 Let’s us write the expression of = c(s + a) d − ca + c(s + a) = (s + a) + ω2 (s + a) + ω2 (s + a) + ω2 2 2 2 + d − ca ω ω 2 (s + a) + ω2 The inverse Laplace transform is then ⎡ ( s + a ) ⎤ ⎛ d − ca ⎞ -1⎡ ⎤ ω + L ⎢ ⎥ ⎢ ⎥ ⎜ ⎟ 2 2 2 2 ω ⎝ ⎠ ω ω s a s a + + + + ( ) ( ) ⎢⎣ ⎣⎢ ⎦⎥ ⎦⎥ ⎛ d − ca ⎞ − at = ce− at cos ωt + ⎜ ⎟ e sin ωt ⎝ ω ⎠ f (t ) = L [ F ( s)] = c L -1 -1 In our example we have F (s) = 2 s + 12 2 s + 12 2 s + 12 = 2 = 2 2 s + 2s + 5 1 s4 +24 2s + 31 + 4{ ( s + 1) + 2 2 =( s +1) Thus we have f (t ) 2 22 a = 1, ω = 2, c = 2, d = 12. Therefore, substitute into the expression of 28/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform ⎛ d − ca ⎞ − a t f ( t ) = L −1 [ F ( s ) ] = ce − a t cos ω t + ⎜ ⎟ e sin ω t ⎝ ω ⎠ ⎛ 12 − 2 × 1 ⎞ − t = 2e− t cos 2t + ⎜ ⎟ e sin 2t 2 3⎠ ⎝1424 =5 = 2e cos 2t + 5e sin 2t = e − t ( 2cos 2t + 5sin 2t ) −t −t Method 2: Use of Complex numbers This method is a lengthy process we will see it in a separate problem in the help session. Case III. Multiple Poles Consider the following expression of As can be seen F (s) has poles of multiplicity 3 . Hence F (s) = where ( s + 1) ( s + 1) 3 3 3 , s = −1, − 1, − 1. Thus we say F ( s ) has a pole s = −1 = B(s) b3 b2 b1 = + + 3 2 A ( s ) ( s + 1) ( s + 1) ( s + 1) are determined as follows. By multiplying both sides of the last , we obtain ( s + 1) Then, letting ( s + 1) can be written in the following form s 2 + 2s + 3 b1 , b2 , and b3 equation by F (s) F (s) = s 2 + 2s + 3 s = −1, 3 B(s) 2 = b3 + b2 ( s + 1) + b1 ( s + 1) A( s ) (2.7) Equation (2.7) gives ⎡ 3 B(s) ⎤ = b3 ⎢( s + 1) ⎥ A s ( ) ⎣ ⎦ s =−1 Also differentiation of both sides of Equation (2.7) gives If we let d ⎡ 3 B(s) ⎤ s + 1 ( ) ⎢ ⎥ = b2 + 2b1 ( s + 1) ds ⎣ A( s ) ⎦ s = −1, in Equation (2.8), then 29/36 (2.8) ME 413 Systems Dynamics & Control Chapter Two: Laplace transform d ⎡ 3 B(s) ⎤ s + 1 = b2 ( ) ⎢ ⎥ ds ⎣ A ( s ) ⎦ s =−1 By differentiating both sides of Equation (2.8) with respect to s , we obtain d2 ⎡ 1 d2 ⎡ 3 B(s) ⎤ 3 B(s) ⎤ s + = b ⇒ b = s + 1 2 1 ( ) ( ) ⎢ ⎥ ⎢ ⎥ 1 1 ds 2 ⎣ A( s ) ⎦ A( s ) ⎦ 2! ds 2 ⎣ Therefore ⎡ ⎤ 2 ⎡ 3 B(s) ⎤ 3 s + 2s + 3 ⎢ ⎥ b3 = ⎢( s + 1) = ( s + 1) ⎥ 3 ⎥ ⎢ A ( s ) ⎦ s =−1 ⎣ ( s + 1) ⎦ ⎣ = ( −1) + 2 ( −1) + 3 = 2 2 s =−1 ⎡ ⎤ 2 d ⎡ d ⎢ 3 B(s)⎤ 3 s + 2s + 3 ⎥ b2 = ⎢( s + 1) = ( s + 1) ⎥ 3 ⎥ ds ⎣ A ( s ) ⎦ s =−1 ds ⎢ ( s + 1) ⎦ s=−1 ⎣ d = ⎡⎣ s 2 + 2 s + 3⎤⎦ = [ 2 s + 2]s =−1 = ⎡⎣ 2 ( −1) + 2 ⎤⎦ = 0 s =−1 ds ⎡ ⎤ 2 1 d2 ⎡ 1 d2 ⎢ 3 B(s) ⎤ 3 s + 2s + 3 ⎥ b1 = s + 1) s + 1) = ⎥ 2 ⎢( 2 ( 3 ⎥ ⎢ A ( s ) ⎦ s =−1 2! ds 2! ds ⎣ ( s + 1) ⎦ s=−1 ⎣ 1 d 1 = [ 2s + 2]s=−1 = [ 2]s=−1 = 1 2! ds 2! Therefore F (s) = and 2 ( s + 1) 3 + 0 ( s + 1) 2 + 1 ( s + 1) f (t ) = L −1 [ F (s ) ] = t 2e −t + 0 + e −t t ≥0 2.5 SOLVING LINEAR, TIME INVARIANT DIFFERENTIAL EQUATIONS The Laplace transform method yields the complete solution (complementary solution and particular solution) of linear, time invariant, differential equations. Classical methods for finding the complete solution of a differential equation require the evaluation of integration constants from the initial conditions. In the case of Laplace transform method, however, this requirement is unnecessary because the initial 30/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform conditions are automatically included in the Laplace transform of the differential equation. █ Example y "+ y = t , Solve: █ Initial Value Problem (IVP) y ( 0 ) = 1, y '( 0) = 1 Solution By writing the Laplace transform of y (t ) as L ⎡⎣ y (t ) ⎤⎦ =Y ( s ) , we obtain L ⎡⎣ y& (t ) ⎤⎦ = sY ( s ) − y ( 0 ) L ⎡⎣ y&& (t ) ⎤⎦ = s 2Y ( s ) − s y ( 0 ) − y& ( 0 ) y ( 0 ) = y& ( 0 ) = 0 , the above transforms become For zero initial conditions, i.e., L ⎡⎣ y& (t ) ⎤⎦ = sY ( s ) L ⎡⎣ y&& (t ) ⎤⎦ = s 2Y ( s ) Step 1: Take Laplace Transform (LT) of both sides of the above equation: s 2 Y (s ) − sy (0) − y '(0) + Y{ (s ) = 1/ s2 { 1444 424444 3 L ⎡⎣⎢ y ⎤⎦⎥ L ⎡⎢⎣t ⎤⎥⎦ L ⎡⎢ y "⎤⎥ ⎣ ⎦ or (s Step 2: Let Solving for Y (s ) 2 + 1) Y (s ) = 1 + s +1 s2 gives Y (s ) = 1 s 1 + 2 + 2 2 s ( s + 1) ( s + 1) ( s + 1) Q (s ) = 1 1 1 = 2− 2 2 s s ( s + 1) ( s + 1) 2 2 Therefore 31/36 ME 413 Systems Dynamics & Control Y (s ) = Step 3: Chapter Two: Laplace transform 1 1 s 1 1 s − 2 + 2 + 2 = 2+ 2 2 s ( s + 1) ( s + 1) ( s + 1) s ( s + 1) Solving y (t ) = L −1 ⎡1⎤ ⎢⎣ s 2 ⎥⎦ + L −1 ⎡ s ⎤ ⎢ 2 ⎥ = t + cos(t ) ⎢⎣ ( s + 1) ⎦⎥ The diagram below summarizes the approach L y "+ y =t , y ( 0) =1, y '( 0) =1 y (t ) = L −1 ⎡1⎤ ⎢⎣ s 2 ⎥⎦ + L −1 s 2 Y (s ) − sy (0) − y '(0) + Y{ (s ) = 1/ s2 { 1444 424444 3 L ⎡⎣⎢ y ⎤⎦⎥ L ⎡⎢⎣t ⎤⎥⎦ L ⎡⎢ y "⎤⎥ ⎣ L −1 ⎡ s ⎤ ⎢ 2 ⎥ ⎢⎣ ( s + 1) ⎥⎦ ⎦ Y (s ) = y (t ) = t + cos(t ) █ Example Find the solution x (t ) 1 s + 2 2 s ( s + 1) of the following Initial Value Problem (IVP) && x + 3 x& + 2 x = 0, x ( 0 ) = a, x& ( 0 ) = b where a and b are constants. █ Solution Step 1: Take LT of both sides of the given equation to obtain an algebraic equation X(s) By writing the Laplace transform of x (t ) 32/36 as L ⎡⎣ x (t ) ⎤⎦ = X ( s ) , we obtain ME 413 Systems Dynamics & Control Chapter Two: Laplace transform L ⎡⎣ x& (t ) ⎤⎦ = sX ( s ) − x ( 0 ) L ⎡⎣ x&& (t ) ⎤⎦ = s 2 X ( s ) − s x ( 0 ) − x& ( 0 ) Take Laplace transform of both sides of the given equation ⎡⎣s 2 X ( s ) − s x ( 0 ) − x& ( 0 ) ⎤⎦ + 3 ⎡⎣sX ( s ) − x ( 0 ) ⎤⎦ + 2 ⎡⎣ X ( s ) ⎤⎦ = 0 1442443 1 424 3 14444244443 L ⎣⎡ x& (t )⎦⎤ L ⎡⎣ x&&(t )⎤⎦ By substituting the initial conditions x ( 0 ) = a, L ⎣⎡ x (t )⎦⎤ x& ( 0 ) = b into the last equations, one obtains ⎡⎣ s 2 X ( s ) − a s − b ⎤⎦ + 3 ⎡⎣ sX ( s ) − a ⎤⎦ + 2 ⎡⎣ X ( s ) ⎤⎦ = 0 or ⎡⎣ s 2 + 3s + 2 ⎤⎦ X ( s ) = as + b + 3a Step 2: Solving for X ( s ) , we obtain X (s) = as + b + 3a K K = 1 + 2 2 s14 3s +32 s + 1 s + 2 +24 =( s +1)( s + 2 ) since X (s) has distinct poles, K1 and K2 can be found easily K1 = ( s + 1) ( as + b + 3a ) ( a ( −1) + b + 3a ) = ( −1 + 2 ) ( s + 1) ( s + 2 ) s=−1 K2 = ( s + 2 ) ( as + b + 3a ) ( a ( −2 ) + b + 3a ) = ( −2 + 1) ( s + 2 ) ( s + 1) s=−2 Thus X (s) = Step 3: Take = 2a + b = −( a + b) 2a + b a + b − s +1 s + 2 L −1 ⎡⎣ X ( s ) ⎤⎦ to obtain the time domain solution x (t ) 33/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform ⎡ 2a + b ⎤ −1 ⎡ a + b ⎤ x (t ) = L −1 ⎡⎣ X ( s ) ⎤⎦ = L −1 ⎢ − L ⎢⎣ s + 2 ⎥⎦ ⎣ s + 1 ⎥⎦ t ≥0 = ( 2a + b )e −t − ( a + b )e −2t █ Example Find the solution x (t ) of the following Initial Value Problem (IVP) && x + 2 x& + 5 x = f (t ), where x ( 0 ) = 0, x& ( 0 ) = 0 f (t ) f (t ) is a function given by its graph. 3 █ Solution t Step 1: Find the explicit expression of The function f (t ) f (t ) given on the RHS of the IVP is a step function u (t ) with height equals to 3. and L [u (t )] = L [3] = 3 s Step 2: Take LT of both sides of the given equation to obtain an algebraic equation X (s ) Remember that we have zero initial conditions. For zero initial conditions, i.e., x ( 0 ) = x& ( 0 ) = 0 , the above transforms become L ⎡⎣ x& (t ) ⎤⎦ = sX ( s ) L ⎡⎣ x&& (t ) ⎤⎦ = s 2 X ( s ) Take Laplace transform of both sides of the given equation s 2 X ( s ) + 2 sX ( s ) + 5 X ( s ) = Solving for X ( s ) , we obtain X (s) = where K1 , K 2 and K3 3 s 3 K1 cs + d = + 2 s ( s 2 + 2s + 5) s s + 2s + 5 are found as follows 34/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform 3 = K1 ( s 2 + 2 s + 5 ) + ( cs + d ) s or 3 = ( K1 + c ) s 2 + ( 2 K1 + d ) s + 5 K1 By comparing coefficients of the equation respectively, we obtain s2 , s s 0 terms: 5K1 = 3 ⇒ and s0 , terms on both sides of this last K1 = 3/ 5 s1 terms: 2 K1 + d = 0 ⇒ d = −2 K1 = −2(3/ 5) = −6 / 5 s 2 terms: K1 + c = 0 ⇒ c = − K1 = −3/ 5 Thus X (s) = ( 3/ 5) + ( −3/ 5) s + ( −6 / 5) = ( 3/ 5) + ( −3/ 5) s + ( −6 / 5) 3 = 2 2 s s1 +24 2 s +35 s s ( s 2 + 2s + 5) ( s + 1) + 22 4 = s 2 + 2 s +1+ 4 ⎡ ⎤ − + − 3/ 5 3/ 5 s 6 / 5 ⎡ ⎤ ⎢ ⎥ ( ) ( ) ( ) −1 x (t ) = L −1 ⎣⎡ X ( s ) ⎦⎤ = L −1 ⎢ ⎥ +L ⎢ ⎥ 2 + + s 2 s 5 ⎣ s ⎦ 14 24 3 ⎢ ⎥ =s 2 + 2 s +1+ 4 ⎣ ⎦ ⎡ ⎤ ⎢ ⎥ −1 ⎡ ( 3/ 5 ) ⎤ −1 ( −3/ 5 ) s + ( −6 / 5 ) ⎢ ⎥ =L ⎢ ⎥ +L 2 2 s ⎢ ( s + 1) + 2 ⎥ ⎣ ⎦ 42444 3⎥ ⎢ 144 G (s ) ⎣ ⎦ The second term of the last equation can be written according to the completing the square rule. Thus we have a = 1, ω = 2, c = −3 / 5, d = −6 / 5. Therefore substitute into the expression of f (t ) 35/36 ME 413 Systems Dynamics & Control Chapter Two: Laplace transform ⎛ d − ca ⎞ −at G (t ) = L −1 [G (s ) ] = ce −at cos ωt + ⎜ ⎟e sin ωt ⎝ ω ⎠ ⎛ 3 ⎛ 6⎞⎞ ⎜ −5 −⎜− 5 ⎟ ⎟ 3 −t ⎝ ⎠ ⎟e −t sin 2t = − 3 e −t cos 2t − 3 e −t sin 2t = − e cos 2t + ⎜ 5 2 5 10 ⎜ ⎟ ⎜ ⎟ ⎝144244 3⎠ = 3 5 Hence ⎡ ⎤ − + − 3/ 5 s 6 / 5 ⎢ ⎥ ( ) ( ) −1 ⎢ ⎥ 2 s 2 s 5 + + 14 24 3 ⎢ ⎥ =s 2 + 2 s +1+ 4 ⎣ ⎦ 3 3 3 = − e −t cos 2t − e −t sin 2t 5 5 10 ⎡ ( 3/ 5 ) ⎤ x (t ) = L −1 ⎡⎣ X ( s ) ⎤⎦ = L −1 ⎢ ⎥ +L s ⎣ ⎦ 36/36