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Give step-by-step solution with explanation and final answer: generate the answer in englishKon 2 fo ESE Epa Avere v elves 20 OTN ’ Ky REC suites, 7 ‘TOAOYIOTE T0 © oxhipopa de so 2m on po [Yim (6, 9)? sin 6 db dg wry o Jo Na El ws 1 ORES TIS ETTPENTES THES TOL m. : Poon To svpmEpaod cag amodeilte Ott pmopovue vo yoTotponoticovue Tv eiowon 7.26 2] Rn PE TPOKEIHEVOL va vToAoY{coVpE TV aKTIVIKT) ZVKVETNTE mbavémTa. Bpeite T 0 n=’ = XOL GYESUOTE TN.

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Give step-by-step solution with explanation and final answer: generate the answer in englishUploaded ImageKon 2 fo ESE Epa Avere v elves 20 OTN ’ Ky REC suites, 7 ‘TOAOYIOTE T0 © oxhipopa de so 2m on po [Yim (6, 9)? sin 6 db dg wry o Jo Na El ws 1 ORES TIS ETTPENTES THES TOL m. : Poon To svpmEpaod cag amodeilte Ott pmopovue vo yoTotponoticovue Tv eiowon 7.26 2] Rn PE TPOKEIHEVOL va vToAoY{coVpE TV aKTIVIKT) ZVKVETNTE mbavémTa. Bpeite T 0 n=’ = XOL GYESUOTE TN.

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Asked by: pr
Created at: 2025-05-26 18:15:13

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Let's break down the problem step by step: --- **Step 1: Understand the Integral** You are asked to compute: \[ \int_{0}^{2\pi} \int_0^{\pi} |Y_{lm}(\theta, \phi)|^2 \sin\theta \, d\theta \, d\phi \] for \( l = 1 \) and all allowed values of \( m \). --- **Step 2: Properties of Spherical Harmonics** Spherical harmonics \( Y_{lm}(\theta, \phi) \) are normalized such that: \[ \int_{0}^{2\pi} \int_0^{\pi} |Y_{lm}(\theta, \phi)|^2 \sin\theta \, d\theta \, d\phi = 1 \] for any allowed \( l \) and \( m \). --- **Step 3: Allowed Values of \( m \) for \( l = 1 \)** For \( l = 1 \), \( m = -1, 0, 1 \). --- **Step 4: Calculation** For each \( m \) (i.e., \( m = -1, 0, 1 \)): \[ \int_{0}^{2\pi} \int_0^{\pi} |Y_{1m}(\theta, \phi)|^2 \sin\theta \, d\theta \, d\phi = 1 \] This is **true for all normalized spherical harmonics**. --- **Step 5: Second Part of the Question** > Show that we can use \( P_r(r) = r^2 |R_{nl}(r)|^2 \) to compute the radial probability density. Find it for \( n = 2 \), \( l = 1 \) and plot it. - The total probability density is given by the modulus squared of the wavefunction: \[ |\Psi_{nlm}(r, \theta, \phi)|^2 = |R_{nl}(r)|^2 |Y_{lm}(\theta, \phi)|^2 \] - Integrating over all angles (as above) leaves: \[ P_r(r) = r^2 |R_{nl}(r)|^2 \] **For \( n = 2, l = 1 \):** - Use the known hydrogen atom radial function for \( n = 2, l = 1 \): \[ R_{21}(r) = \frac{1}{\sqrt{24 a_0^3}} \left(\frac{r}{a_0}\right) e^{-r/2a_0} \] - The radial probability density is: \[ P_r(r) = r^2 |R_{21}(r)|^2 = r^2 \left[ \frac{1}{\sqrt{24 a_0^3}} \left(\frac{r}{a_0}\right) e^{-r/2a_0} \right]^2 \] \[ = \frac{1}{24 a_0^3} \left(\frac{r}{a_0}\right)^2 r^2 e^{-r/a_0} \] \[ = \frac{1}{24 a_0^5} r^4 e^{-r/a_0} \] --- ### **Summary / Final Answers** 1. **Integral value:** \[ \int_{0}^{2\pi} \int_0^{\pi} |Y_{1m}(\theta, \phi)|^2 \sin\theta \, d\theta \, d\phi = 1 \] for each \( m = -1, 0, 1 \). 2. **Radial probability density for \( n=2 \), \( l=1 \):** \[ P_r(r) = \frac{1}{24 a_0^5} r^4 e^{-r/a_0} \] --- **Plot:** To plot \( P_r(r) \), use the above formula for various values of \( r \) (in units of \( a_0 \)). The curve starts at 0, peaks at some \( r \), and then decays to 0 as \( r \to \infty \). If you want the explicit plot, let me know!

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