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1.4 Calculus
Achievable FE Civil
1. Mathematics
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Calculus

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This chapter covers the following topics:

  • The Derivative
  • L’Hospital’s Rule (L’Hôpital’s Rule)
  • Test for a Maximum and Minimum
  • Point of Inflection
  • Curvature and Radius of Curvature
  • Partial Derivative
  • Derivatives
  • Integral Calculus
  • Indefinite Integrals
  • Differential Equations
  • Fourier Transform
  • Laplace Transforms

The derivative

The derivative of a function describes how the function’s output changes as its input changes. In other words, it measures the function’s instantaneous rate of change.

For a function f(x), the derivative is defined by the limit:

f′(x)=h→0lim​hf(x+h)−f(x)​

L’Hospital’s rule (L’Hôpital’s rule)

L’Hospital’s Rule helps you evaluate limits that produce indeterminate forms such as 00​ or ∞∞​. The idea is to differentiate the numerator and denominator separately.

If

x→alim​g(x)f(x)​

is indeterminate, then:

x→alim​g(x)f(x)​=x→alim​g′(x)f′(x)​

provided the right-hand limit exists.

Test for a maximum and minimum

To decide whether a function f(x) has a local maximum or local minimum at a critical point x=c, you can use the second derivative test.

  • If f′′(c)>0, then f(c) is a local minimum.
  • If f′′(c)<0, then f(c) is a local maximum.

Point of inflection

A point of inflection is a point where the curve changes concavity (the curvature changes direction). In terms of derivatives, this happens when the second derivative changes sign.

A common condition to check is:

dx2d2y​=0

and there is a sign change in dx2d2y​ around that point.

Curvature and radius of curvature

Curvature (κ) measures how sharply a curve bends at a point. One way to define curvature is:

κ=dsdθ​=[1+(y′)2]3/2∣y′′∣​

where θ is the angle of the tangent and s is the arc length.

The radius of curvature (R) is the reciprocal of curvature:

R=∣κ∣1​

It represents the radius of the circular arc that best approximates the curve at that point.

Partial derivative

A partial derivative is the derivative of a multivariable function with respect to one variable, treating the other variables as constants.

For a function f(x,y), the partial derivative with respect to x is:

∂x∂f​=dxd​f(x,y)

Derivatives

In these formulas, u,v,w represent functions of x. Also, a,c and n represent constants.

All arguments of the trigonometric functions are in radians. A constant of integration should be added to the integrals.

The following definitions are used:

arcsinu=sin−1u,(sinu)−1=sinu1​

Basic differentiation rules

dxd​c=0

dxd​x=1

dxd​(cu)=cdxdu​

dxd​(u+v−w)=dxdu​+dxdv​−dxdw​

dxd​(uv)=udxdv​+vdxdu​

dxd​(uvw)=uvdxdw​+uwdxdv​+vwdxdu​

dxd​(vu​)=v2vdxdu​−udxdv​​

Power and logarithmic differentiation

dxd​(un)=nun−1dxdu​

dxd​(f(u))=f′(u)dxdu​

dxdu​=dx/du1​

dxd​(loga​u)=(loga​e)u1​dxdu​

dxd​(lnu)=u1​dxdu​

dxd​(au)=(lna)audxdu​

Exponential and trigonometric differentiation

dxd​(eu)=eudxdu​

dxd​(uu)=uu[u1​dxdu​+(lnu)uu−1dxdu​]

dxd​(sinu)=cosudxdu​

dxd​(cosu)=−sinudxdu​

dxd​(tanu)=sec2udxdu​

dxd​(cotu)=−csc2udxdu​

dxd​(secu)=secutanudxdu​

dxd​(cscu)=−cscucotudxdu​

Inverse trigonometric differentiation

dxd​(sin−1u)=1−u2​1​dxdu​,(−π/2≤sin−1u≤π/2)

dxd​(cos−1u)=1−u2​−1​dxdu​,(0≤cos−1u≤π)

dxd​(tan−1u)=1+u21​dxdu​,(−π/2<tan−1u<π/2)

dxd​(cot−1u)=1+u2−1​dxdu​,(0<cot−1u<π)

dxd​(sec−1u)=∣u∣u2−1​1​dxdu​,(0<sec−1u<π/2)∪(−π<sec−1u<−π/2)

dxd​(csc−1u)=∣u∣u2−1​−1​dxdu​,(0<csc−1u≤π/2)∪(−π<csc−1u≤−π/2)

Integral calculus

Integral calculus focuses on accumulation. It’s used to compute quantities like area under a curve, volume, and total change.

An indefinite integral represents a family of antiderivatives. For a function f(x):

∫f(x)dx=F(x)+C

where F(x) is an antiderivative of f(x), and C is the constant of integration.

Indefinite integrals

Basic integration rules

∫f′(x)dx=f(x)

∫dx=x

∫af(x)dx=a∫f(x)dx

∫[u(x)+v(x)]dx=∫u(x)dx+∫v(x)dx

∫xmdx=m+1xm+1​,(m=−1)

∫u(x)dv(x)=u(x)v(x)−∫v(x)du(x)

Logarithmic and exponential integrals

∫ax+bdx​=a1​ln∣ax+b∣

∫x​dx​=2x​

∫axdx=lnaax​

Trigonometric integrals

∫sinxdx=−cosx

∫cosxdx=sinx

∫sin2xdx=2x​−4sin2x​

∫cos2xdx=2x​+4sin2x​

∫xsinxdx=−xcosx+sinx

∫xcosxdx=cosx+xsinx

∫sinxcosxdx=(sin2x)/2

∫sinaxcosbxdx=2(a−b)cos(a−b)x​−2(a+b)cos(a+b)x​,(a2=b2)

Logarithmic and hyperbolic integrals

∫tanxdx=ln∣cosx∣=ln∣secx∣

∫cotxdx=ln∣sinx∣

∫tan2xdx=tanx−x

∫cot2xdx=−cotx−x

∫exdx=(1/a)ex

∫eaxdx=a1​eax

∫lnxdx=x(lnx−1)

∫x2+a2dx​=a1​tan−1ax​,(a>0)

Rational integrals

∫ax2+cdx​=ac​1​tan−1(ca​​x),(a>0,c>0)

∫ax2+bx+cdx​=4ac−b2​2​tan−14ac−b2​2ax+b​,(4ac−b2>0)

∫ax2+bx+cdx​=b2−4ac​1​ln​2ax+b+b2−4ac​2ax+b−b2−4ac​​​,(b2−4ac>0)

∫ax2+bx+cdx​=2ax+b2​,(b2−4ac=0)

Differential equations

Ordinary linear differential equations

A common class of ordinary linear differential equations has the form:

bn​dxndny​+bn−1​dxn−1dn−1y​+⋯+b1​dxdy​+b0​y=f(t)

where

b0​,b1​,…,bn​

are constants.

Homogeneous solution

When the equation is homogeneous (i.e., f(x)=0), the solution is:

y(x)=C1​er1​x+C2​er2​x+⋯+Cn​ern​x

where ri​ is a distinct root of the characteristic polynomial P(r) with:

P(r)=bn​rn+bn−1​rn−1+⋯+b1​r+b0​

Higher orders of multiplicity imply higher powers of x. The complete solution for the differential equation is:

y(x)=yh​(x)+yp​(x),

where yh​(x) is the general solution for the homogeneous equation, and yp​(x) is any particular solution for f(x). If f(x) has eλx terms, then resonance is involved.

Furthermore, specific f(x) forms result in specific yp​(x) forms, some of which are:

  • If f(x)=A then yp​(x)=B
  • If f(x)=Aeλx then yp​(x)=Beλx
  • If f(x)=Axmeλx then yp​(x)=Pm​(x)eλx, where Pm​(x) is a polynomial of degree $m.

If the independent variable is time, t, then transient dynamic solutions are implied.

First-order linear homogeneous differential equations with constant coefficients

dtdy​+ay=0

where a is a real constant.

Solution:

y=Ce−at

where C is a constant that satisfies the initial conditions.

First-order linear nonhomogeneous differential equations

dtdy​+ay=Kebt,(a=b)

with initial condition:

y(0)=Kt

where, τ = time constant, and K = gain

Solution:

y(t)=Kt+(KB−KC)[1−e−τt​]

where:

τ=a1​,B=aKB−KC​

Second-order linear homogeneous differential equations with constant coefficients

An equation of the form:

y′′+ay′+by=0

can be solved by the method of undetermined coefficients, where a solution of the form:

y=Cert

is sought.

By substitution, the characteristic equation is:

r2+ar+b=0

The roots of the characteristic equation are:

r1,2​=2−a±a2−4b​​

The nature of the solution depends on the discriminant Δ=a2−4b:

  • If Δ>0, the solution is in the form of real distinct roots:

    y=C1​er1​t+C2​er2​t

  • If Δ=0, the solution is in the form of repeated roots:

    y=(C1​+C2​t)ert

  • If Δ<0, the solution is in the form of complex conjugate roots:

    Given:

    r=α±iβ

    The solution is:

    y=eαt(C1​cosβt+C2​sinβt)

where:

α=−2a​,β=24b−a2​​

Fourier transform

The Fourier transform converts a signal from the time domain to the frequency domain. This is useful because many signals can be viewed as a sum of sinusoids (sines and cosines) at different frequencies. The transform tells you which frequencies are present and how strong they are.

For a continuous-time signal x(t), the Fourier transform is:

X(f)=∫−∞∞​x(t)⋅e−j2πftdt

Where:

  • X(f): Fourier transform of x(t)
  • f: frequency in Hz
  • t: time in seconds
  • j: imaginary unit (−1​)

To retrieve the original time-domain signal x(t) from its frequency-domain representation X(f), use the inverse transform:

x(t)=∫−∞∞​X(f)⋅ej2πftdf

Key properties

Please refer to the FE Handbook for detailed properties of the Fourier Transform.

Laplace transform

The Laplace transform converts a time-domain function (often written as f(t)) into a function of a complex variable s. It’s widely used in engineering, physics, and control systems, especially for solving differential equations.

The Laplace transform of f(t) is defined as:

F(s)=∫0∞​f(t)e−stdt

and the inverse Laplace transform is:

f(t)=2πj1​∫σ−j∞σ+j∞​F(s)estds

Where:

  • f(t): a real- or complex-valued function defined for t≥0
  • s: a complex number, s=σ+jω
  • F(s): the Laplace transform of f(t)

The inverse Laplace transform is used to retrieve the time-domain function f(t) from its Laplace domain F(s).

Often, inverse transforms are found using partial fractions or standard transform tables.

Key properties

Please refer to the FE Handbook for detailed properties of the Laplace transform.

The derivative

  • Measures instantaneous rate of change of a function
  • Defined as f′(x)=limh→0​hf(x+h)−f(x)​

L’Hospital’s Rule (L’Hôpital’s Rule)

  • Used for limits with indeterminate forms (0/0, ∞/∞)
  • Differentiate numerator and denominator: limx→a​g(x)f(x)​=limx→a​g′(x)f′(x)​

Test for a Maximum and Minimum

  • Use second derivative test at critical point x=c
    • f′′(c)>0: local minimum
    • f′′(c)<0: local maximum

Point of Inflection

  • Where curve changes concavity (second derivative changes sign)
  • Condition: dx2d2y​=0 with sign change around the point

Curvature and Radius of Curvature

  • Curvature: κ=[1+(y′)2]3/2∣y′′∣​
  • Radius of curvature: R=∣κ∣1​

Partial Derivative

  • Derivative of multivariable function with respect to one variable
  • Example: ∂x∂f​ for f(x,y)

Derivatives

  • Basic rules: sum, product, quotient, chain rule
  • Power, exponential, logarithmic, and trigonometric differentiation formulas
  • Inverse trigonometric differentiation formulas
    • E.g., dxd​(sin−1u)=1−u2​1​dxdu​

Integral Calculus

  • Concerned with accumulation (area, volume, total change)
  • Indefinite integral: ∫f(x)dx=F(x)+C

Indefinite Integrals

  • Basic integration rules: linearity, power rule, integration by parts
  • Common integrals for exponential, logarithmic, trigonometric, and rational functions
  • Special forms for integrals involving quadratics and trigonometric functions

Differential Equations

  • Ordinary linear differential equations: bn​y(n)+⋯+b0​y=f(t)
  • Homogeneous solution: sum of exponentials with roots of characteristic polynomial
  • Nonhomogeneous solution: y(x)=yh​(x)+yp​(x)
  • First-order linear (homogeneous): y=Ce−at
  • Second-order linear: solution form depends on discriminant (Δ)
    • Real, repeated, or complex roots yield different solution structures

Fourier Transform

  • Converts time-domain signal to frequency domain
  • Forward: X(f)=∫−∞∞​x(t)e−j2πftdt
  • Inverse: x(t)=∫−∞∞​X(f)ej2πftdf

Laplace Transforms

  • Converts time-domain function f(t) to F(s) in complex s-domain
  • Forward: F(s)=∫0∞​f(t)e−stdt
  • Inverse: f(t)=2πj1​∫σ−j∞σ+j∞​F(s)estds
  • Used for solving differential equations and system analysis

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Calculus

This chapter covers the following topics:

  • The Derivative
  • L’Hospital’s Rule (L’Hôpital’s Rule)
  • Test for a Maximum and Minimum
  • Point of Inflection
  • Curvature and Radius of Curvature
  • Partial Derivative
  • Derivatives
  • Integral Calculus
  • Indefinite Integrals
  • Differential Equations
  • Fourier Transform
  • Laplace Transforms

The derivative

The derivative of a function describes how the function’s output changes as its input changes. In other words, it measures the function’s instantaneous rate of change.

For a function f(x), the derivative is defined by the limit:

f′(x)=h→0lim​hf(x+h)−f(x)​

L’Hospital’s rule (L’Hôpital’s rule)

L’Hospital’s Rule helps you evaluate limits that produce indeterminate forms such as 00​ or ∞∞​. The idea is to differentiate the numerator and denominator separately.

If

x→alim​g(x)f(x)​

is indeterminate, then:

x→alim​g(x)f(x)​=x→alim​g′(x)f′(x)​

provided the right-hand limit exists.

Test for a maximum and minimum

To decide whether a function f(x) has a local maximum or local minimum at a critical point x=c, you can use the second derivative test.

  • If f′′(c)>0, then f(c) is a local minimum.
  • If f′′(c)<0, then f(c) is a local maximum.

Point of inflection

A point of inflection is a point where the curve changes concavity (the curvature changes direction). In terms of derivatives, this happens when the second derivative changes sign.

A common condition to check is:

dx2d2y​=0

and there is a sign change in dx2d2y​ around that point.

Curvature and radius of curvature

Curvature (κ) measures how sharply a curve bends at a point. One way to define curvature is:

κ=dsdθ​=[1+(y′)2]3/2∣y′′∣​

where θ is the angle of the tangent and s is the arc length.

The radius of curvature (R) is the reciprocal of curvature:

R=∣κ∣1​

It represents the radius of the circular arc that best approximates the curve at that point.

Partial derivative

A partial derivative is the derivative of a multivariable function with respect to one variable, treating the other variables as constants.

For a function f(x,y), the partial derivative with respect to x is:

∂x∂f​=dxd​f(x,y)

Derivatives

In these formulas, u,v,w represent functions of x. Also, a,c and n represent constants.

All arguments of the trigonometric functions are in radians. A constant of integration should be added to the integrals.

The following definitions are used:

arcsinu=sin−1u,(sinu)−1=sinu1​

Basic differentiation rules

dxd​c=0

dxd​x=1

dxd​(cu)=cdxdu​

dxd​(u+v−w)=dxdu​+dxdv​−dxdw​

dxd​(uv)=udxdv​+vdxdu​

dxd​(uvw)=uvdxdw​+uwdxdv​+vwdxdu​

dxd​(vu​)=v2vdxdu​−udxdv​​

Power and logarithmic differentiation

dxd​(un)=nun−1dxdu​

dxd​(f(u))=f′(u)dxdu​

dxdu​=dx/du1​

dxd​(loga​u)=(loga​e)u1​dxdu​

dxd​(lnu)=u1​dxdu​

dxd​(au)=(lna)audxdu​

Exponential and trigonometric differentiation

dxd​(eu)=eudxdu​

dxd​(uu)=uu[u1​dxdu​+(lnu)uu−1dxdu​]

dxd​(sinu)=cosudxdu​

dxd​(cosu)=−sinudxdu​

dxd​(tanu)=sec2udxdu​

dxd​(cotu)=−csc2udxdu​

dxd​(secu)=secutanudxdu​

dxd​(cscu)=−cscucotudxdu​

Inverse trigonometric differentiation

dxd​(sin−1u)=1−u2​1​dxdu​,(−π/2≤sin−1u≤π/2)

dxd​(cos−1u)=1−u2​−1​dxdu​,(0≤cos−1u≤π)

dxd​(tan−1u)=1+u21​dxdu​,(−π/2<tan−1u<π/2)

dxd​(cot−1u)=1+u2−1​dxdu​,(0<cot−1u<π)

dxd​(sec−1u)=∣u∣u2−1​1​dxdu​,(0<sec−1u<π/2)∪(−π<sec−1u<−π/2)

dxd​(csc−1u)=∣u∣u2−1​−1​dxdu​,(0<csc−1u≤π/2)∪(−π<csc−1u≤−π/2)

Integral calculus

Integral calculus focuses on accumulation. It’s used to compute quantities like area under a curve, volume, and total change.

An indefinite integral represents a family of antiderivatives. For a function f(x):

∫f(x)dx=F(x)+C

where F(x) is an antiderivative of f(x), and C is the constant of integration.

Indefinite integrals

Basic integration rules

∫f′(x)dx=f(x)

∫dx=x

∫af(x)dx=a∫f(x)dx

∫[u(x)+v(x)]dx=∫u(x)dx+∫v(x)dx

∫xmdx=m+1xm+1​,(m=−1)

∫u(x)dv(x)=u(x)v(x)−∫v(x)du(x)

Logarithmic and exponential integrals

∫ax+bdx​=a1​ln∣ax+b∣

∫x​dx​=2x​

∫axdx=lnaax​

Trigonometric integrals

∫sinxdx=−cosx

∫cosxdx=sinx

∫sin2xdx=2x​−4sin2x​

∫cos2xdx=2x​+4sin2x​

∫xsinxdx=−xcosx+sinx

∫xcosxdx=cosx+xsinx

∫sinxcosxdx=(sin2x)/2

∫sinaxcosbxdx=2(a−b)cos(a−b)x​−2(a+b)cos(a+b)x​,(a2=b2)

Logarithmic and hyperbolic integrals

∫tanxdx=ln∣cosx∣=ln∣secx∣

∫cotxdx=ln∣sinx∣

∫tan2xdx=tanx−x

∫cot2xdx=−cotx−x

∫exdx=(1/a)ex

∫eaxdx=a1​eax

∫lnxdx=x(lnx−1)

∫x2+a2dx​=a1​tan−1ax​,(a>0)

Rational integrals

∫ax2+cdx​=ac​1​tan−1(ca​​x),(a>0,c>0)

∫ax2+bx+cdx​=4ac−b2​2​tan−14ac−b2​2ax+b​,(4ac−b2>0)

∫ax2+bx+cdx​=b2−4ac​1​ln​2ax+b+b2−4ac​2ax+b−b2−4ac​​​,(b2−4ac>0)

∫ax2+bx+cdx​=2ax+b2​,(b2−4ac=0)

Differential equations

Ordinary linear differential equations

A common class of ordinary linear differential equations has the form:

bn​dxndny​+bn−1​dxn−1dn−1y​+⋯+b1​dxdy​+b0​y=f(t)

where

b0​,b1​,…,bn​

are constants.

Homogeneous solution

When the equation is homogeneous (i.e., f(x)=0), the solution is:

y(x)=C1​er1​x+C2​er2​x+⋯+Cn​ern​x

where ri​ is a distinct root of the characteristic polynomial P(r) with:

P(r)=bn​rn+bn−1​rn−1+⋯+b1​r+b0​

Higher orders of multiplicity imply higher powers of x. The complete solution for the differential equation is:

y(x)=yh​(x)+yp​(x),

where yh​(x) is the general solution for the homogeneous equation, and yp​(x) is any particular solution for f(x). If f(x) has eλx terms, then resonance is involved.

Furthermore, specific f(x) forms result in specific yp​(x) forms, some of which are:

  • If f(x)=A then yp​(x)=B
  • If f(x)=Aeλx then yp​(x)=Beλx
  • If f(x)=Axmeλx then yp​(x)=Pm​(x)eλx, where Pm​(x) is a polynomial of degree $m.

If the independent variable is time, t, then transient dynamic solutions are implied.

First-order linear homogeneous differential equations with constant coefficients

dtdy​+ay=0

where a is a real constant.

Solution:

y=Ce−at

where C is a constant that satisfies the initial conditions.

First-order linear nonhomogeneous differential equations

dtdy​+ay=Kebt,(a=b)

with initial condition:

y(0)=Kt

where, τ = time constant, and K = gain

Solution:

y(t)=Kt+(KB−KC)[1−e−τt​]

where:

τ=a1​,B=aKB−KC​

Second-order linear homogeneous differential equations with constant coefficients

An equation of the form:

y′′+ay′+by=0

can be solved by the method of undetermined coefficients, where a solution of the form:

y=Cert

is sought.

By substitution, the characteristic equation is:

r2+ar+b=0

The roots of the characteristic equation are:

r1,2​=2−a±a2−4b​​

The nature of the solution depends on the discriminant Δ=a2−4b:

  • If Δ>0, the solution is in the form of real distinct roots:

    y=C1​er1​t+C2​er2​t

  • If Δ=0, the solution is in the form of repeated roots:

    y=(C1​+C2​t)ert

  • If Δ<0, the solution is in the form of complex conjugate roots:

    Given:

    r=α±iβ

    The solution is:

    y=eαt(C1​cosβt+C2​sinβt)

where:

α=−2a​,β=24b−a2​​

Fourier transform

The Fourier transform converts a signal from the time domain to the frequency domain. This is useful because many signals can be viewed as a sum of sinusoids (sines and cosines) at different frequencies. The transform tells you which frequencies are present and how strong they are.

For a continuous-time signal x(t), the Fourier transform is:

X(f)=∫−∞∞​x(t)⋅e−j2πftdt

Where:

  • X(f): Fourier transform of x(t)
  • f: frequency in Hz
  • t: time in seconds
  • j: imaginary unit (−1​)

To retrieve the original time-domain signal x(t) from its frequency-domain representation X(f), use the inverse transform:

x(t)=∫−∞∞​X(f)⋅ej2πftdf

Key properties

Please refer to the FE Handbook for detailed properties of the Fourier Transform.

Laplace transform

The Laplace transform converts a time-domain function (often written as f(t)) into a function of a complex variable s. It’s widely used in engineering, physics, and control systems, especially for solving differential equations.

The Laplace transform of f(t) is defined as:

F(s)=∫0∞​f(t)e−stdt

and the inverse Laplace transform is:

f(t)=2πj1​∫σ−j∞σ+j∞​F(s)estds

Where:

  • f(t): a real- or complex-valued function defined for t≥0
  • s: a complex number, s=σ+jω
  • F(s): the Laplace transform of f(t)

The inverse Laplace transform is used to retrieve the time-domain function f(t) from its Laplace domain F(s).

Often, inverse transforms are found using partial fractions or standard transform tables.

Key properties

Please refer to the FE Handbook for detailed properties of the Laplace transform.

Key points

The derivative

  • Measures instantaneous rate of change of a function
  • Defined as f′(x)=limh→0​hf(x+h)−f(x)​

L’Hospital’s Rule (L’Hôpital’s Rule)

  • Used for limits with indeterminate forms (0/0, ∞/∞)
  • Differentiate numerator and denominator: limx→a​g(x)f(x)​=limx→a​g′(x)f′(x)​

Test for a Maximum and Minimum

  • Use second derivative test at critical point x=c
    • f′′(c)>0: local minimum
    • f′′(c)<0: local maximum

Point of Inflection

  • Where curve changes concavity (second derivative changes sign)
  • Condition: dx2d2y​=0 with sign change around the point

Curvature and Radius of Curvature

  • Curvature: κ=[1+(y′)2]3/2∣y′′∣​
  • Radius of curvature: R=∣κ∣1​

Partial Derivative

  • Derivative of multivariable function with respect to one variable
  • Example: ∂x∂f​ for f(x,y)

Derivatives

  • Basic rules: sum, product, quotient, chain rule
  • Power, exponential, logarithmic, and trigonometric differentiation formulas
  • Inverse trigonometric differentiation formulas
    • E.g., dxd​(sin−1u)=1−u2​1​dxdu​

Integral Calculus

  • Concerned with accumulation (area, volume, total change)
  • Indefinite integral: ∫f(x)dx=F(x)+C

Indefinite Integrals

  • Basic integration rules: linearity, power rule, integration by parts
  • Common integrals for exponential, logarithmic, trigonometric, and rational functions
  • Special forms for integrals involving quadratics and trigonometric functions

Differential Equations

  • Ordinary linear differential equations: bn​y(n)+⋯+b0​y=f(t)
  • Homogeneous solution: sum of exponentials with roots of characteristic polynomial
  • Nonhomogeneous solution: y(x)=yh​(x)+yp​(x)
  • First-order linear (homogeneous): y=Ce−at
  • Second-order linear: solution form depends on discriminant (Δ)
    • Real, repeated, or complex roots yield different solution structures

Fourier Transform

  • Converts time-domain signal to frequency domain
  • Forward: X(f)=∫−∞∞​x(t)e−j2πftdt
  • Inverse: x(t)=∫−∞∞​X(f)ej2πftdf

Laplace Transforms

  • Converts time-domain function f(t) to F(s) in complex s-domain
  • Forward: F(s)=∫0∞​f(t)e−stdt
  • Inverse: f(t)=2πj1​∫σ−j∞σ+j∞​F(s)estds
  • Used for solving differential equations and system analysis

More from Mathematics

  • Coordinate geometry
  • Geometric feature and trigonometry
  • Algebra
  • Matrices and Vectors