MTH166Semester 2 • 4 CreditsCore Subjects

Differential Equations And Vector Calculus

This course focuses on the definitions, distinctions, and solution methods for various differential equations, including first-order and higher-order ordinary differential equations, linear differential equations, partial differential equations (heat, wave, and Laplace equations), and vector calculus encompassing gradient, divergence, curl, line, surface, and volume integrals, along with Green's, Stokes's, and Gauss divergence theorems.

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Unit 1:Unit 1: Ordinary differential equations
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Unit 1: Ordinary differential equations

Unit 1 Exam Focus & Core Takeaways

Review the core definitions, standard architectures, and syntax patterns below. Pay special attention to sections highlighted with bullet points for your mid-term and end-term subjective questions.

Unit 1: Ordinary Differential Equations of First Order

1. Mathematical Foundations and Definitions

An Ordinary Differential Equation (ODE) is a mathematical equation establishing an algebraic relationship between an independent variable, a single dependent variable, and one or more ordinary derivatives of the dependent variable with respect to the independent variable.

Φ(x,y,dydx,d2ydx2,…,dnydxn)=0\Phi\left(x, y, \frac{dy}{dx}, \frac{d^2y}{dx^2}, \dots, \frac{d^ny}{dx^n}\right) = 0

Where:

  • x∈Rx \in \mathbb{R} is the independent variable.
  • y=y(x)y = y(x) is the unknown dependent function.
  • dkydxk\frac{d^ky}{dx^k} denotes the kk-th order ordinary derivative of yy with respect to xx.
CODE
                              Differential Equations
                                        |
                   +--------------------+--------------------+
                   |                                         |
       Ordinary Differential Equations            Partial Differential Equations
                   (ODEs)                                    (PDEs)
         (Single independent variable)            (Two or more independent variables)

1.1 Order and Degree of a Differential Equation

  • Order: The order of a differential equation is the order of the highest derivative appearing in the equation.
  • Degree: The degree of a differential equation is the power (positive integer exponent) of the highest derivative, after the equation has been expressed in a form free of fractional exponents and radicals involving derivatives.

Illustrative Examples:

  1. (d2ydx2)3+(dydx)5+y=sin⁡x\left(\frac{d^2y}{dx^2}\right)^3 + \left(\frac{dy}{dx}\right)^5 + y = \sin x
    • Highest derivative is d2ydx2  ⟹  Order=2\frac{d^2y}{dx^2} \implies \text{Order} = 2.
    • Power of highest derivative is 3  ⟹  Degree=33 \implies \text{Degree} = 3.
  2. [1+(dydx)2]3/2=kd2ydx2\left[1 + \left(\frac{dy}{dx}\right)^2\right]^{3/2} = k \frac{d^2y}{dx^2}
    • Squaring both sides to eliminate the fractional exponent:
      [1+(dydx)2]3=k2(d2ydx2)2\left[1 + \left(\frac{dy}{dx}\right)^2\right]^3 = k^2 \left(\frac{d^2y}{dx^2}\right)^2
    • Highest derivative is d2ydx2  ⟹  Order=2\frac{d^2y}{dx^2} \implies \text{Order} = 2.
    • Power of highest derivative is 2  ⟹  Degree=22 \implies \text{Degree} = 2.
  3. dydx=edy/dx\frac{dy}{dx} = e^{dy/dx} or sin⁡(dydx)+y=0\sin\left(\frac{dy}{dx}\right) + y = 0
    • Order=1\text{Order} = 1; however, the equation cannot be expanded as a polynomial in dydx  ⟹  Degree is undefined\frac{dy}{dx} \implies \text{Degree is undefined}.

1.2 Linearity of Differential Equations

A differential equation is defined as linear if it satisfies two strict criteria:

  1. The dependent variable yy and all its derivatives dydx,…,dnydxn\frac{dy}{dx}, \dots, \frac{d^ny}{dx^n} occur strictly to the first power (11).
  2. There are no product terms involving the dependent variable and any of its derivatives (e.g., no ydydxy \frac{dy}{dx} or (dydx)2\left(\frac{dy}{dx}\right)^2) and no transcendental functions of yy (e.g., sin⁡y,ey,ln⁡y\sin y, e^y, \ln y).

A first-order linear differential equation always conforms to the standard canonical structure:

dydx+P(x)y=Q(x)\frac{dy}{dx} + P(x)y = Q(x)


1.3 Nature of Solutions: General, Particular, and Singular

  • General Solution (Complete Integral): A solution containing a number of arbitrary, independent constants equal to the order of the differential equation. For a first-order ODE, the general solution contains exactly one arbitrary constant CC:
    F(x,y,C)=0F(x, y, C) = 0
  • Particular Solution: A solution obtained from the general solution by assigning specific numerical values to the arbitrary constants, typically dictated by initial conditions (e.g., y(x0)=y0y(x_0) = y_0) or boundary conditions.
  • Singular Solution: A solution that satisfies the differential equation but cannot be obtained from the general solution for any choice of the arbitrary constant. Geometrically, a singular solution represents the envelope of the one-parameter family of curves described by the general solution.

1.4 Existence and Uniqueness: The Picard–Lindelöf Theorem

Consider the first-order Initial Value Problem (IVP):

dydx=f(x,y),y(x0)=y0\frac{dy}{dx} = f(x, y), \quad y(x_0) = y_0

Let R={(x,y)∈R2:∣x−x0∣≤a,∣y−y0∣≤b}R = \{(x, y) \in \mathbb{R}^2 : |x - x_0| \le a, |y - y_0| \le b\} be a closed rectangle centered at (x0,y0)(x_0, y_0).

  • Existence Condition: If f(x,y)f(x, y) is continuous on RR, then there exists at least one solution y(x)y(x) in an interval ∣x−x0∣≤h|x - x_0| \le h.
  • Uniqueness Condition: If, in addition, the partial derivative ∂f∂y\frac{\partial f}{\partial y} is continuous on RR (satisfying the Lipschitz condition ∣f(x,y1)−f(x,y2)∣≤L∣y1−y2∣|f(x, y_1) - f(x, y_2)| \le L|y_1 - y_2|), then the solution y(x)y(x) is unique.

2. Classical First-Order ODE Solution Techniques

2.1 Separation of Variables

An equation of the form:

M(x)dx+N(y)dy=0ordydx=g(x)h(y)M(x)dx + N(y)dy = 0 \quad \text{or} \quad \frac{dy}{dx} = g(x)h(y)

is solved by isolating terms containing xx with dxdx and terms containing yy with dydy:

1h(y)dy=g(x)dx  ⟹  ∫1h(y)dy=∫g(x)dx+C\frac{1}{h(y)}dy = g(x)dx \implies \int \frac{1}{h(y)}dy = \int g(x)dx + C

Equations Reducible to Separable Form:

Equations of the form dydx=f(ax+by+c)\frac{dy}{dx} = f(ax + by + c) are made separable by the linear transformation:

u=ax+by+c  ⟹  dudx=a+bdydx  ⟹  dydx=1b(dudx−a)u = ax + by + c \implies \frac{du}{dx} = a + b\frac{dy}{dx} \implies \frac{dy}{dx} = \frac{1}{b}\left(\frac{du}{dx} - a\right)

Substituting into the ODE yields:

dudx=a+bf(u)  ⟹  dua+bf(u)=dx\frac{du}{dx} = a + bf(u) \implies \frac{du}{a + bf(u)} = dx


2.2 Homogeneous Differential Equations

A function f(x,y)f(x, y) is homogeneous of degree nn if f(λx,λy)=λnf(x,y)f(\lambda x, \lambda y) = \lambda^n f(x, y). A first-order ODE:

dydx=f1(x,y)f2(x,y)\frac{dy}{dx} = \frac{f_1(x, y)}{f_2(x, y)}

is homogeneous if f1f_1 and f2f_2 are homogeneous functions of the exact same degree. In this case, the equation can be expressed as:

dydx=ϕ(yx)\frac{dy}{dx} = \phi\left(\frac{y}{x}\right)

Solution Strategy:

  1. Substitute y=vxy = vx, which implies dydx=v+xdvdx\frac{dy}{dx} = v + x\frac{dv}{dx}.
  2. Substitute into the differential equation:
    v+xdvdx=ϕ(v)  ⟹  xdvdx=ϕ(v)−vv + x\frac{dv}{dx} = \phi(v) \implies x\frac{dv}{dx} = \phi(v) - v
  3. Separate variables:
    dvϕ(v)−v=dxx\frac{dv}{\phi(v) - v} = \frac{dx}{x}
  4. Integrate both sides and substitute back v=yxv = \frac{y}{x}.

2.3 Non-Homogeneous Equations Reducible to Homogeneous Form

Equations having linear fractional arguments:

dydx=a1x+b1y+c1a2x+b2y+c2\frac{dy}{dx} = \frac{a_1x + b_1y + c_1}{a_2x + b_2y + c_2}

  • Case 1: a1a2≠b1b2\frac{a_1}{a_2} \neq \frac{b_1}{b_2} (Intersecting Lines):
    Shift the origin to the intersection point (h,k)(h, k) by setting x=X+hx = X + h and y=Y+ky = Y + k, where (h,k)(h, k) satisfies:
    a1h+b1k+c1=0anda2h+b2k+c2=0a_1h + b_1k + c_1 = 0 \quad \text{and} \quad a_2h + b_2k + c_2 = 0
    Since dx=dXdx = dX and dy=dYdy = dY, the equation transforms into the homogeneous form:
    dYdX=a1X+b1Ya2X+b2Y\frac{dY}{dX} = \frac{a_1X + b_1Y}{a_2X + b_2Y}
    Now solve by setting Y=vXY = vX.

  • Case 2: a1a2=b1b2=m\frac{a_1}{a_2} = \frac{b_1}{b_2} = m (Parallel Lines):
    Here a2x+b2y=m(a1x+b1y)a_2x + b_2y = m(a_1x + b_1y). Substitute u=a1x+b1yu = a_1x + b_1y, reducing the equation directly to variable separable form.


3. Exact Differential Equations

A first-order differential equation expressed in Pfaffian differential form:

M(x,y)dx+N(x,y)dy=0M(x, y)dx + N(x, y)dy = 0

is called Exact if there exists a scalar potential function u(x,y)u(x, y) such that its total differential equals the left-hand side:

du=∂u∂xdx+∂u∂ydy=M(x,y)dx+N(x,y)dy=0du = \frac{\partial u}{\partial x}dx + \frac{\partial u}{\partial y}dy = M(x, y)dx + N(x, y)dy = 0

Since du=0du = 0, the general solution is simply:

u(x,y)=Cu(x, y) = C

3.1 Euler's Condition for Exactness

The necessary and sufficient condition for M(x,y)dx+N(x,y)dy=0M(x, y)dx + N(x, y)dy = 0 to be an exact differential equation (assuming M,NM, N and their first partials are continuous on a simply connected domain) is:

∂M∂y=∂N∂x\frac{\partial M}{\partial y} = \frac{\partial N}{\partial x}

Proof Outline: Since M=∂u∂xM = \frac{\partial u}{\partial x} and N=∂u∂yN = \frac{\partial u}{\partial y}, Clairaut's theorem on the equality of mixed second partial derivatives guarantees:
∂M∂y=∂2u∂y∂x=∂2u∂x∂y=∂N∂x\frac{\partial M}{\partial y} = \frac{\partial^2 u}{\partial y \partial x} = \frac{\partial^2 u}{\partial x \partial y} = \frac{\partial N}{\partial x}


3.2 Standard Integration Formula for Exact Equations

Once exactness is verified (∂M∂y=∂N∂x\frac{\partial M}{\partial y} = \frac{\partial N}{\partial x}), the general solution is evaluated directly using the standard formula:

∫y=constantM(x,y) dx+∫(terms of N free from x) dy=C\int_{y = \text{constant}} M(x, y)\,dx + \int (\text{terms of } N \text{ free from } x)\,dy = C


4. Integrating Factors (Non-Exact Differential Equations)

If M(x,y)dx+N(x,y)dy=0M(x, y)dx + N(x, y)dy = 0 is not exact (∂M∂y≠∂N∂x\frac{\partial M}{\partial y} \neq \frac{\partial N}{\partial x}), it can often be made exact by multiplying the entire equation by a non-zero integrating factor μ(x,y)\mu(x, y):

μ(x,y)M(x,y)dx+μ(x,y)N(x,y)dy=0\mu(x, y)M(x, y)dx + \mu(x, y)N(x, y)dy = 0

The condition for exactness of the new equation requires:

∂∂y(μM)=∂∂x(μN)  ⟹  μ∂M∂y+M∂μ∂y=μ∂N∂x+N∂μ∂x\frac{\partial}{\partial y}(\mu M) = \frac{\partial}{\partial x}(\mu N) \implies \mu \frac{\partial M}{\partial y} + M \frac{\partial \mu}{\partial y} = \mu \frac{\partial N}{\partial x} + N \frac{\partial \mu}{\partial x}

From this governing PDE, five standardized rules for finding Integrating Factors (IF) are derived:

CODE
                       Rules for Integrating Factors (IF)
                                       |
     +-------------+-------------+-----+-------------+-------------+
     |             |             |                   |             |
  Rule 1        Rule 2        Rule 3              Rule 4        Rule 5
Inspection   Homogeneous   f₁(xy)y dx +        Function of   Function of
               Equations   f₂(xy)x dy = 0       x alone       y alone

4.1 Rule 1: Method of Grouping (Inspection)

Recognize standard exact total differential pairs:

  • x dy+y dx=d(xy)x\,dy + y\,dx = d(xy)
  • x dy−y dxx2=d(yx)\frac{x\,dy - y\,dx}{x^2} = d\left(\frac{y}{x}\right)
  • y dx−x dyy2=d(xy)\frac{y\,dx - x\,dy}{y^2} = d\left(\frac{x}{y}\right)
  • x dy−y dxxy=d(ln⁡yx)\frac{x\,dy - y\,dx}{xy} = d\left(\ln\frac{y}{x}\right)
  • x dy−y dxx2+y2=d(arctan⁡yx)\frac{x\,dy - y\,dx}{x^2 + y^2} = d\left(\arctan\frac{y}{x}\right)
  • x dx+y dyx2+y2=d(12ln⁡(x2+y2))\frac{x\,dx + y\,dy}{x^2 + y^2} = d\left(\frac{1}{2}\ln(x^2 + y^2)\right)

4.2 Rule 2: Homogeneous Non-Exact Equations

If M(x,y)dx+N(x,y)dy=0M(x, y)dx + N(x, y)dy = 0 is a homogeneous equation of degree nn and Mx+Ny≠0Mx + Ny \neq 0:

IF=1Mx+Ny\text{IF} = \frac{1}{Mx + Ny}


4.3 Rule 3: Equations of the Form f1(xy)y dx+f2(xy)x dy=0f_1(xy)y\,dx + f_2(xy)x\,dy = 0

If the equation can be written as f1(xy)y dx+f2(xy)x dy=0f_1(xy)y\,dx + f_2(xy)x\,dy = 0 and Mx−Ny≠0Mx - Ny \neq 0:

IF=1Mx−Ny\text{IF} = \frac{1}{Mx - Ny}


4.4 Rule 4: Function of xx Alone

If the quantity:

1N(∂M∂y−∂N∂x)=f(x)\frac{1}{N}\left(\frac{\partial M}{\partial y} - \frac{\partial N}{\partial x}\right) = f(x)

is a function of xx only (or constant), then:

IF=e∫f(x) dx\text{IF} = e^{\int f(x)\,dx}


4.5 Rule 5: Function of yy Alone

If the quantity:

1M(∂N∂x−∂M∂y)=g(y)\frac{1}{M}\left(\frac{\partial N}{\partial x} - \frac{\partial M}{\partial y}\right) = g(y)

is a function of yy only (or constant), then:

IF=e∫g(y) dy\text{IF} = e^{\int g(y)\,dy}


5. Linear First-Order Equations (Leibniz's Equation)

5.1 Standard Form and Solution

The canonical form of a first-order linear differential equation is:

dydx+P(x)y=Q(x)\frac{dy}{dx} + P(x)y = Q(x)

Where P(x)P(x) and Q(x)Q(x) are continuous functions of xx alone.

Derivation of the Integrating Factor:

Multiplying by an integrating factor μ(x)\mu(x):

μ(x)dydx+μ(x)P(x)y=μ(x)Q(x)\mu(x)\frac{dy}{dx} + \mu(x)P(x)y = \mu(x)Q(x)

The left-hand side is identical to the product rule expansion ddx(μy)=μdydx+dμdxy\frac{d}{dx}(\mu y) = \mu \frac{dy}{dx} + \frac{d\mu}{dx}y if:

dμdx=μP(x)  ⟹  dμμ=P(x)dx  ⟹  ln⁡μ=∫P(x)dx  ⟹  μ(x)=e∫P(x) dx\frac{d\mu}{dx} = \mu P(x) \implies \frac{d\mu}{\mu} = P(x)dx \implies \ln \mu = \int P(x)dx \implies \mu(x) = e^{\int P(x)\,dx}

Hence, the Integrating Factor is:

IF=e∫P(x) dx\text{IF} = e^{\int P(x)\,dx}

Integrating both sides yields the general solution:

y⋅e∫P(x) dx=∫Q(x)e∫P(x) dx dx+C  ⟹  y⋅(IF)=∫Q(x)⋅(IF) dx+Cy \cdot e^{\int P(x)\,dx} = \int Q(x) e^{\int P(x)\,dx}\,dx + C \quad \implies \quad y \cdot (\text{IF}) = \int Q(x) \cdot (\text{IF})\,dx + C


5.2 Equations Linear in xx

When an equation cannot be expressed linearly in yy, it may be linear when viewed with xx as the dependent variable:

dxdy+P(y)x=Q(y)\frac{dx}{dy} + P(y)x = Q(y)

  • IF=e∫P(y) dy\text{IF} = e^{\int P(y)\,dy}
  • General solution: x⋅(IF)=∫Q(y)⋅(IF) dy+Cx \cdot (\text{IF}) = \int Q(y) \cdot (\text{IF})\,dy + C

6. Non-Linear Equations Reducible to Linear Form

6.1 Bernoulli's Differential Equation

A first-order non-linear differential equation of the form:

dydx+P(x)y=Q(x)yn(n≠0,n≠1)\frac{dy}{dx} + P(x)y = Q(x)y^n \quad (n \neq 0, n \neq 1)

is known as Bernoulli's Equation.

Transformation to Linear Form:

  1. Divide both sides by yny^n:
    y−ndydx+P(x)y1−n=Q(x)y^{-n}\frac{dy}{dx} + P(x)y^{1-n} = Q(x)
  2. Introduce the substitution:
    v=y1−n  ⟹  dvdx=(1−n)y−ndydx  ⟹  y−ndydx=11−ndvdxv = y^{1-n} \implies \frac{dv}{dx} = (1 - n)y^{-n}\frac{dy}{dx} \implies y^{-n}\frac{dy}{dx} = \frac{1}{1-n}\frac{dv}{dx}
  3. Substitute into the equation:
    11−ndvdx+P(x)v=Q(x)  ⟹  dvdx+(1−n)P(x)v=(1−n)Q(x)\frac{1}{1-n}\frac{dv}{dx} + P(x)v = Q(x) \implies \frac{dv}{dx} + (1-n)P(x)v = (1-n)Q(x)
    This is a standard first-order linear ODE in vv, solvable via integrating factor:
    IF=e(1−n)∫P(x) dx\text{IF} = e^{(1-n)\int P(x)\,dx}

6.2 Clairaut's Equation

An equation of the form:

y=px+f(p)where p=dydxy = px + f(p) \quad \text{where } p = \frac{dy}{dx}

Differentiating both sides with respect to xx:

dydx=p=p+xdpdx+f′(p)dpdx  ⟹  dpdx[x+f′(p)]=0\frac{dy}{dx} = p = p + x\frac{dp}{dx} + f'(p)\frac{dp}{dx} \implies \frac{dp}{dx}\left[x + f'(p)\right] = 0

This yields two distinct branches of solutions:

  1. General Solution: dpdx=0  ⟹  p=C\frac{dp}{dx} = 0 \implies p = C. Substituting into the original equation gives:
    y=Cx+f(C)y = Cx + f(C)
    (A one-parameter family of straight lines)
  2. Singular Solution: x+f′(p)=0x + f'(p) = 0. Eliminating pp between y=px+f(p)y = px + f(p) and x+f′(p)=0x + f'(p) = 0 yields the singular solution, which forms the envelope of the general solution lines.

7. Engineering and Physical Applications

First-order ordinary differential equations serve as mathematical models for a wide variety of dynamic engineering phenomena.

CODE
                         First-Order ODE Applications
                                      |
         +--------------------+-------+--------------------+
         |                    |                            |
  Thermal Modeling       RL / RC Circuits         Kinematics & Geometry
(Newton's Law of        (Kirchhoff's Laws:        (Orthogonal Trajectories,
    Cooling)            L di/dt + Ri = E(t))        Pursuit curves, Decay)

7.1 Orthogonal Trajectories

Given a one-parameter family of plane curves F(x,y,C)=0F(x, y, C) = 0, an Orthogonal Trajectory is a curve that intersects every member of the family at right angles (90∘90^\circ).

Algorithm for Cartesian Coordinates F(x,y,C)=0F(x, y, C) = 0:

  1. Differentiate F(x,y,C)=0F(x, y, C) = 0 with respect to xx to obtain an expression involving dydx\frac{dy}{dx}.
  2. Eliminate the parameter CC between the original equation and the derivative to find the governing ODE:
    f(x,y,dydx)=0f\left(x, y, \frac{dy}{dx}\right) = 0
  3. Replace dydx\frac{dy}{dx} with −dxdy-\frac{dx}{dy} (since the product of orthogonal slopes m1m2=−1m_1 m_2 = -1).
  4. Solve the resulting differential equation:
    f(x,y,−dxdy)=0f\left(x, y, -\frac{dx}{dy}\right) = 0

Algorithm for Polar Coordinates F(r,θ,C)=0F(r, \theta, C) = 0:

  1. Form the differential equation by eliminating CC, yielding f(r,θ,drdθ)=0f\left(r, \theta, \frac{dr}{d\theta}\right) = 0.
  2. Replace drdθ\frac{dr}{d\theta} with −r2dθdr-r^2 \frac{d\theta}{dr}.
  3. Solve the resulting orthogonal trajectory ODE.

7.2 Newton's Law of Cooling

The rate of change of temperature T(t)T(t) of a body is directly proportional to the difference between its temperature and the ambient medium temperature TmT_m:

dTdt=−k(T−Tm),k>0\frac{dT}{dt} = -k(T - T_m), \quad k > 0

Separating variables:

dTT−Tm=−k dt  ⟹  ln⁡∣T−Tm∣=−kt+C1  ⟹  T(t)=Tm+(T0−Tm)e−kt\frac{dT}{T - T_m} = -k\,dt \implies \ln|T - T_m| = -kt + C_1 \implies T(t) = T_m + (T_0 - T_m)e^{-kt}

Where T0=T(0)T_0 = T(0) is the initial temperature at t=0t = 0.


7.3 Transient Electrical Circuits

Series RL Circuit:

Applying Kirchhoff's Voltage Law (KVL) to a resistor RR and inductor LL connected to voltage source E(t)E(t):

Ldidt+Ri=E(t)  ⟹  didt+RLi=E(t)LL\frac{di}{dt} + Ri = E(t) \implies \frac{di}{dt} + \frac{R}{L}i = \frac{E(t)}{L}

  • This is a linear first-order ODE with IF=e(R/L)t\text{IF} = e^{(R/L)t}.
  • If E(t)=E0E(t) = E_0 (constant DC voltage) and i(0)=0i(0) = 0:
    i(t)=E0R(1−e−(R/L)t)i(t) = \frac{E_0}{R}\left(1 - e^{-(R/L)t}\right)
  • The time constant of the circuit is τ=LR\tau = \frac{L}{R}.

Series RC Circuit:

Applying KVL to a resistor RR and capacitor CC with charge q(t)q(t) (where current i=dqdti = \frac{dq}{dt}):

Rdqdt+qC=E(t)  ⟹  dqdt+1RCq=E(t)RR\frac{dq}{dt} + \frac{q}{C} = E(t) \implies \frac{dq}{dt} + \frac{1}{RC}q = \frac{E(t)}{R}

  • This is a linear first-order ODE with IF=et/(RC)\text{IF} = e^{t/(RC)}.
  • For constant voltage E0E_0 and uncharged capacitor q(0)=0q(0) = 0:
    q(t)=CE0(1−e−t/(RC))q(t) = CE_0\left(1 - e^{-t/(RC)}\right)
  • The capacitive time constant is τ=RC\tau = RC.

7.4 Radioactive Decay and Population Growth

  • Radioactive Decay: The rate of disintegration is proportional to the active mass present:
    dNdt=−λN  ⟹  N(t)=N0e−λt\frac{dN}{dt} = -\lambda N \implies N(t) = N_0 e^{-\lambda t}
    The half-life t1/2t_{1/2} is the time when N=N0/2N = N_0/2:
    t1/2=ln⁡2λ≈0.693λt_{1/2} = \frac{\ln 2}{\lambda} \approx \frac{0.693}{\lambda}
  • Malthusian Population Growth:
    dPdt=kP  ⟹  P(t)=P0ekt\frac{dP}{dt} = kP \implies P(t) = P_0 e^{kt}

8. Summary Checklist for Solving First-Order ODEs

Before selecting an integration strategy for a given first-order ODE, follow this diagnostic checklist:

  1. Can variables be separated directly? Check if dydx=g(x)h(y)\frac{dy}{dx} = g(x)h(y) or if it can be transformed via u=ax+by+cu = ax + by + c.
  2. Is it homogeneous? Check if replacing (x,y)(x, y) with (λx,λy)(\lambda x, \lambda y) leaves the equation invariant; if so, substitute y=vxy = vx.
  3. Is it exact? Test Euler's condition: ∂M∂y=∂N∂x\frac{\partial M}{\partial y} = \frac{\partial N}{\partial x}. If exact, integrate using ∫y=constM dx+∫(terms of N free from x) dy=C\int_{y=\text{const}} M\,dx + \int (\text{terms of } N \text{ free from } x)\,dy = C.
  4. If not exact, does it admit an Integrating Factor?
    • Check if 1N(∂M∂y−∂N∂x)=f(x)  ⟹  IF=e∫f(x) dx\frac{1}{N}(\frac{\partial M}{\partial y} - \frac{\partial N}{\partial x}) = f(x) \implies \text{IF} = e^{\int f(x)\,dx}.
    • Check if 1M(∂N∂x−∂M∂y)=g(y)  ⟹  IF=e∫g(y) dy\frac{1}{M}(\frac{\partial N}{\partial x} - \frac{\partial M}{\partial y}) = g(y) \implies \text{IF} = e^{\int g(y)\,dy}.
    • Check if homogeneous with Mx+Ny≠0  ⟹  IF=1Mx+NyMx + Ny \neq 0 \implies \text{IF} = \frac{1}{Mx + Ny}.
  5. Is it linear in yy? If dydx+P(x)y=Q(x)\frac{dy}{dx} + P(x)y = Q(x), use IF=e∫P dx\text{IF} = e^{\int P\,dx}.
  6. Is it linear in xx? If dxdy+P(y)x=Q(y)\frac{dx}{dy} + P(y)x = Q(y), use IF=e∫P dy\text{IF} = e^{\int P\,dy}.
  7. Is it a Bernoulli equation? If dydx+Py=Qyn\frac{dy}{dx} + Py = Qy^n, substitute v=y1−nv = y^{1-n}.
  8. Is it Clairaut's form? If y=px+f(p)y = px + f(p), the general solution is y=cx+f(c)y = cx + f(c).