SUMMARY
The trapezoidal rule for approximating definite integrals is derived from the formula $$h[(1/2)y_{0} + y_{1} + y_{2} + ... +y_{n-1} + (1/2)y_{n}]$$, where the term $$h$$ represents the width of each subinterval. The first and last y-values are multiplied by $$1/2$$ to account for the fact that they only contribute half of their respective heights to the area of the trapezoids formed. This ensures an accurate approximation of the area under the curve by effectively averaging the heights at the endpoints.
PREREQUISITES
- Understanding of definite integrals in calculus
- Familiarity with the concept of Riemann sums
- Basic knowledge of trapezoidal geometry
- Ability to manipulate mathematical equations
NEXT STEPS
- Study the derivation of the trapezoidal rule in detail
- Explore the error analysis of the trapezoidal rule
- Learn about Simpson's rule for comparison with the trapezoidal rule
- Practice solving definite integrals using the trapezoidal rule with various functions
USEFUL FOR
Students studying calculus, educators teaching integral approximation methods, and anyone looking to deepen their understanding of numerical integration techniques.