Math Problem Statement

Change into polar coordinates and evaluate double integral of 0 to infinity e*-x2+y2dxdy and also evaluate integral of 0 to infinity e-t*2dt

Solution

First Integral: Double Integral of e(x2+y2)e^{-(x^2 + y^2)}

We are asked to evaluate the double integral of the function e(x2+y2)e^{-(x^2 + y^2)} from 0 to infinity in both the xx- and yy-directions:

I=00e(x2+y2)dxdyI = \int_0^\infty \int_0^\infty e^{-(x^2 + y^2)} \, dx \, dy

To convert this double integral into polar coordinates, we follow these steps:

  1. Convert to Polar Coordinates:

    In polar coordinates, the relationships are:

    • x=rcosθx = r \cos \theta
    • y=rsinθy = r \sin \theta
    • The differential area element becomes dxdy=rdrdθdx \, dy = r \, dr \, d\theta.

    The function e(x2+y2)e^{-(x^2 + y^2)} becomes: e(x2+y2)=er2e^{-(x^2 + y^2)} = e^{-r^2} where r2=x2+y2r^2 = x^2 + y^2.

  2. Adjust the Limits:

    Since the limits of integration are from 0 to infinity for both xx and yy, the corresponding polar coordinate limits for rr go from 0 to infinity, and θ\theta ranges from 0 to π2\frac{\pi}{2} (as we are working within the first quadrant).

  3. Rewrite the Integral in Polar Coordinates:

    The integral becomes: I=0π20er2rdrdθI = \int_0^{\frac{\pi}{2}} \int_0^\infty e^{-r^2} r \, dr \, d\theta

  4. Evaluate the Inner Integral:

    We can first evaluate the rr-integral: 0er2rdr\int_0^\infty e^{-r^2} r \, dr This is a standard Gaussian integral, which is known to evaluate to: 12\frac{1}{2}

  5. Evaluate the Outer Integral:

    The outer integral with respect to θ\theta is straightforward: 0π2dθ=π2\int_0^{\frac{\pi}{2}} d\theta = \frac{\pi}{2}

  6. Combine Results:

    The final result of the double integral is: I=12×π2=π4I = \frac{1}{2} \times \frac{\pi}{2} = \frac{\pi}{4}

Second Integral: Single Integral of et2e^{-t^2}

We are asked to evaluate the following integral: 0et2dt\int_0^\infty e^{-t^2} \, dt

This is also a standard Gaussian integral. The value of the Gaussian integral is well-known: et2dt=π\int_{-\infty}^{\infty} e^{-t^2} \, dt = \sqrt{\pi}

However, since the limits are from 0 to infinity (half of the total range), we divide the result by 2: 0et2dt=π2\int_0^\infty e^{-t^2} \, dt = \frac{\sqrt{\pi}}{2}

Summary:

  • The value of the double integral is π4\frac{\pi}{4}.
  • The value of the single integral is π2\frac{\sqrt{\pi}}{2}.

Would you like further details on any of these steps or have additional questions?


Further Questions:

  1. How can you convert more complex integrals into polar coordinates?
  2. What is the relationship between Gaussian integrals and their applications in probability theory?
  3. How does the result of the single integral relate to the error function (erf)?
  4. Can you extend these integrals to higher dimensions?
  5. How does the factor rr arise in polar coordinate transformations of integrals?

Tip: When working with Gaussian integrals, recognize that they often appear in problems involving heat diffusion, probability distributions (normal distribution), and quantum mechanics.

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Math Problem Analysis

Mathematical Concepts

Polar Coordinates
Double Integrals
Gaussian Integrals

Formulas

x = r * cos(θ)
y = r * sin(θ)
dx dy = r dr dθ
∫_0^∞ e^(-r^2) r dr = 1/2
∫_0^∞ e^(-t^2) dt = √π / 2

Theorems

Gaussian Integral
Polar Coordinate Transformation

Suitable Grade Level

Grades 11-12 (Advanced Calculus or College Level)