RIEMANN SUM APPROXIMATOR
Left, Right, Midpoint & Trapezoidal Area ApproximationsRiemann Sum & Area Approximations ($\Delta x = \text{0.5000}$)
Riemann Sum Approximator: Left, Right, Midpoint & Trapezoidal Rules
A Riemann Sum is a fundamental technique in real analysis and numerical calculus for approximating the definite integral (area under a curve) of a function $f(x)$ over a bounded interval $[a, b]$. By partitioning the domain into $n$ equal subintervals of width $\Delta x = \frac{b - a}{n}$, the region is divided into rectangular or trapezoidal slices whose areas are summed.
1. Summary of Riemann Sum Approximations
| Method | Sampling Point ($x_i^*$) | Summation Formula | Behavior on Monotonic Functions |
|---|---|---|---|
| Left Riemann Sum ($L_n$) | Left endpoint: $x_i^* = x_{i-1}$ | $$L_n = \Delta x \sum_{i=0}^{n-1} f(x_i)$$ | Underestimates increasing functions; overestimates decreasing functions. |
| Right Riemann Sum ($R_n$) | Right endpoint: $x_i^* = x_i$ | $$R_n = \Delta x \sum_{i=1}^{n} f(x_i)$$ | Overestimates increasing functions; underestimates decreasing functions. |
| Midpoint Rule ($M_n$) | Subinterval midpoint: $x_i^* = \frac{x_{i-1} + x_i}{2}$ | $$M_n = \Delta x \sum_{i=1}^{n} f\left(\frac{x_{i-1} + x_i}{2}\right)$$ | Higher precision; cancellation of errors occurs across subintervals. |
| Trapezoidal Rule ($T_n$) | Average of endpoints | $$T_n = \frac{\Delta x}{2} \left[ f(x_0) + 2\sum_{i=1}^{n-1} f(x_i) + f(x_n) \right]$$ | Connects points linearly; overestimates concave up curves, underestimates concave down curves. |
2. Error Bounds & Convergence
As the number of subintervals $n \to \infty$ (and $\Delta x \to 0$), all valid Riemann sums converge to the exact value of the definite integral under Riemann integrability:
$$\lim_{n \to \infty} \sum_{i=1}^{n} f(x_i^*) \Delta x = \int_{a}^{b} f(x) \, dx$$- Trapezoidal Error Bound: $$|E_T| \le \frac{K_2 (b - a)^3}{12 n^2} \quad \text{where } K_2 \ge |f''(x)|$$
- Midpoint Error Bound: $$|E_M| \le \frac{K_2 (b - a)^3}{24 n^2}$$
Frequently Asked Questions
Why is the Midpoint Rule usually more accurate than the Trapezoidal Rule?
Although the Trapezoidal Rule uses two endpoints per slice, its error depends directly on linear secant lines. The Midpoint Rule uses tangent slopes at subinterval centers, leading to error cancellation where overestimation on one side of the midpoint balances underestimation on the other.
How does $n$ affect approximation accuracy?
Doubling $n$ halves $\Delta x$. For Left and Right sums, the error decreases linearly $\mathcal{O}(1/n)$. For Midpoint and Trapezoidal rules, doubling $n$ reduces error by a factor of 4 ($\mathcal{O}(1/n^2)$).
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