SUMMARY
The integral of the function f(x) = x^3/(e^x-1) from 0 to infinity results in pi^4/15, a key aspect of deriving the Boltzmann law. This integral is identified as the Debye-Einstein integral, denoted as \mathcal{D}_3. The solution involves the use of the gamma function and the Riemann zeta function, specifically \Gamma(4) and \zeta(4). The discussion emphasizes the relationship between the integral and the formula \int_0^{\infty}\frac{x^n}{e^x-1}dx = \Gamma(n+1)\zeta(n+1>.
PREREQUISITES
- Understanding of integral calculus, particularly improper integrals.
- Familiarity with the gamma function and its properties.
- Knowledge of the Riemann zeta function and its applications.
- Basic concepts of statistical mechanics related to the Boltzmann law.
NEXT STEPS
- Study the properties and applications of the gamma function in integration.
- Learn about the Riemann zeta function and its significance in number theory and physics.
- Explore the derivation and applications of the Debye-Einstein integral.
- Investigate the relationship between statistical mechanics and thermodynamic integrals.
USEFUL FOR
Scientists, mathematicians, and engineers interested in statistical mechanics, particularly those working on problems related to the Boltzmann law and integrals in theoretical physics.