- Solve real-world problems involving exponential and logarithmic equations.
- Create models for exponential growth and decay, including how to use Newton’s Law of Cooling and logistic growth.
- Evaluate data to determine the most suitable model, with an emphasis on exponential contexts.
Exponential Growth and Decay
In real-world applications, we need to model the behavior of a function. In mathematical modeling, we choose a familiar general function with properties that suggest that it will model the real-world phenomenon we wish to analyze.
In the case of rapid growth, we may choose the exponential growth function, [latex]A={A}_{0}{e}^{rt}[/latex], where [latex]{A}_{0}[/latex] (used to be labeled as [latex]P[/latex]) is equal to the value at time zero, [latex]e[/latex] is Euler’s constant, and [latex]r[/latex] is a positive constant that determines the rate (percentage) of growth.
We may use the exponential growth function in applications involving doubling time, the time it takes for a quantity to double. Such phenomena as wildlife populations, financial investments, biological samples, and natural resources may exhibit growth based on a doubling time. In some applications, however, as we will see when we discuss the logistic equation, the logistic model sometimes fits the data better than the exponential model.
On the other hand, if a quantity is falling rapidly toward zero, without ever reaching zero, then we should probably choose the exponential decay model. Again, we have the form [latex]y={A}_{0}{e}^{-kt}[/latex] where [latex]{A}_{0}[/latex] is the starting value, and [latex]e[/latex] is Euler’s constant. Now [latex]k[/latex] is a negative constant that determines the rate of decay. We may use the exponential decay model when we are calculating half-life, or the time it takes for a substance to exponentially decay to half of its original quantity. We use half-life in applications involving radioactive isotopes.
- one-to-one function
- horizontal asymptote: [latex]y = 0[/latex]
- domain: [latex]\left(-\infty , \infty \right)[/latex]
- range: [latex]\left(0,\infty \right)[/latex]
- [latex]x[/latex] intercept: none
- [latex]y[/latex]-intercept: [latex]\left(0,{A}_{0}\right)[/latex]
- increasing if [latex]k > 0[/latex]
- decreasing if [latex]k < 0[/latex]
An exponential function models exponential growth when [latex]k > 0[/latex] and exponential decay when [latex]k < 0[/latex].
[latex]\\[/latex]
For example, the distance to the nearest star, Proxima Centauri, measured in kilometers, is [latex]40,113,497,200,000[/latex] kilometers. Expressed in scientific notation, this is [latex]4.01134972\times {10}^{13}[/latex]. We could describe this number as having order of magnitude [latex]{10}^{13}[/latex].
Calculating Doubling Time
For growing quantities, we might want to find out how long it takes for a quantity to double. As we mentioned above, the time it takes for a quantity to double is called the doubling time.
Given the basic exponential growth equation [latex]A={A}_{0}{e}^{kt}[/latex], doubling time can be found by solving for when the original quantity has doubled, that is, by solving [latex]2{A}_{0}={A}_{0}{e}^{kt}[/latex].
The formula is derived as follows:
[latex]\begin{array}{l}2{A}_{0}={A}_{0}{e}^{kt}\hfill & \hfill \\ 2={e}^{kt}\hfill & \text{Divide both sides by }{A}_{0}.\hfill \\ \mathrm{ln}2=kt\hfill & \text{Take the natural logarithm of both sides}.\hfill \\ t=\frac{\mathrm{ln}2}{k}\hfill & \text{Divide by the coefficient of }t.\hfill \end{array}[/latex]
Thus the doubling time is
[latex]t=\frac{\mathrm{ln}2}{k}[/latex]