Simpson's Rule Formula:
where \( h = \frac{b - a}{n} \) and \( n \) is even
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Simpson's Rule is a numerical method for approximating definite integrals. It works by approximating the area under a curve using quadratic polynomials (parabolic arcs) rather than straight lines (as in the Trapezoidal Rule), resulting in more accurate approximations.
The calculator uses Simpson's Rule formula:
where \( h = \frac{b - a}{n} \) and \( n \) is even
Where:
Explanation: The method weights the function values in a specific pattern (1, 4, 2, 4, ..., 4, 1) to achieve higher accuracy than simpler methods.
Details: Numerical integration is essential when an integral cannot be solved analytically or when working with empirical data. Simpson's Rule provides a good balance between accuracy and computational complexity.
Tips: Enter the lower and upper limits, an even number of subintervals (more intervals = better accuracy), and the function to integrate. Use standard mathematical notation (e.g., x^2 for x², sin(x) for sine function).
Q1: Why must n be even?
A: Simpson's Rule works by fitting parabolas to groups of three points, so we need an even number of intervals (odd number of points).
Q2: How accurate is Simpson's Rule?
A: The error is proportional to (b-a)h⁴, making it much more accurate than the Trapezoidal Rule for smooth functions.
Q3: What functions work best with Simpson's Rule?
A: It works best for smooth functions. For functions with discontinuities or sharp corners, other methods may be better.
Q4: Can I use this for improper integrals?
A: Not directly. Improper integrals require special treatment or transformation before numerical integration.
Q5: What's the difference between 1/3 and 3/8 rules?
A: The 1/3 rule uses quadratic polynomials (2nd order), while the 3/8 rule uses cubic polynomials (3rd order) and requires n divisible by 3.