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In hy drogen spectrum, a hydrogen atom ...

In hy drogen spectrum, a hydrogen
atom emits a photon of wavelength
1027 `Å` its angular momentum
changes by

A

`(h)/(pi)`

B

`(h)/(2 pi)`

C

`(3 h)/(2 pi)`

D

`(2 h)/(pi)`

Text Solution

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The correct Answer is:
To solve the problem of how much the angular momentum of a hydrogen atom changes when it emits a photon of wavelength 1027 Å, we can follow these steps: ### Step 1: Calculate the energy of the emitted photon The energy of the emitted photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( h \) is Planck's constant (\( 6.626 \times 10^{-34} \, \text{Js} \)), - \( c \) is the speed of light (\( 3 \times 10^8 \, \text{m/s} \)), - \( \lambda \) is the wavelength in meters. First, convert the wavelength from angstroms to meters: \[ 1027 \, \text{Å} = 1027 \times 10^{-10} \, \text{m} \] Now, substitute the values into the energy formula: \[ E = \frac{(6.626 \times 10^{-34} \, \text{Js})(3 \times 10^8 \, \text{m/s})}{1027 \times 10^{-10} \, \text{m}} \] Calculating this gives: \[ E \approx 1.24 \times 10^{-6} \, \text{J} \] To convert this energy into electron volts (1 eV = \( 1.6 \times 10^{-19} \, \text{J} \)): \[ E \approx \frac{1.24 \times 10^{-6}}{1.6 \times 10^{-19}} \approx 12.1 \, \text{eV} \] ### Step 2: Determine the initial and final energy states For a hydrogen atom, the energy levels are given by: \[ E_n = -\frac{13.6 \, \text{eV}}{n^2} \] Assuming the electron transitions from the third energy level (\( n = 3 \)) to the ground state (\( n = 1 \)): - Initial energy (\( E_3 \)): \[ E_3 = -\frac{13.6}{3^2} = -\frac{13.6}{9} \approx -1.51 \, \text{eV} \] - Final energy (\( E_1 \)): \[ E_1 = -\frac{13.6}{1^2} = -13.6 \, \text{eV} \] ### Step 3: Calculate the change in energy The change in energy (\( \Delta E \)) when the electron transitions from \( n = 3 \) to \( n = 1 \) is: \[ \Delta E = E_1 - E_3 = (-13.6) - (-1.51) = -12.1 \, \text{eV} \] ### Step 4: Calculate the angular momentum The angular momentum for an electron in a given orbit is given by: \[ L_n = \frac{nh}{2\pi} \] - For \( n = 3 \): \[ L_3 = \frac{3h}{2\pi} \] - For \( n = 1 \): \[ L_1 = \frac{1h}{2\pi} \] ### Step 5: Calculate the change in angular momentum The change in angular momentum (\( \Delta L \)) is: \[ \Delta L = L_3 - L_1 = \frac{3h}{2\pi} - \frac{1h}{2\pi} = \frac{(3 - 1)h}{2\pi} = \frac{2h}{2\pi} = \frac{h}{\pi} \] ### Final Answer The change in angular momentum when the hydrogen atom emits a photon of wavelength 1027 Å is: \[ \Delta L = \frac{h}{\pi} \] ---

To solve the problem of how much the angular momentum of a hydrogen atom changes when it emits a photon of wavelength 1027 Å, we can follow these steps: ### Step 1: Calculate the energy of the emitted photon The energy of the emitted photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( h \) is Planck's constant (\( 6.626 \times 10^{-34} \, \text{Js} \)), - \( c \) is the speed of light (\( 3 \times 10^8 \, \text{m/s} \)), ...
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Knowledge Check

  • When a hydrogen atoms emits a photon of energy 12.1 eV , its orbital angular momentum changes by (where h os Planck's constant)

    A
    `3h/pi`
    B
    `2h/pi`
    C
    `h/pi`
    D
    `4h/pi`
  • If a hydrogen atom emit a photon of energy 12.1 eV , its orbital angular momentum changes by Delta L. then Delta L equals

    A
    `1.05 xx 10^(-34) J s`
    B
    `2.11 xx 10^(-34) J s`
    C
    `3.16 xx 10^(-34) J s`
    D
    `4.22 xx 10^(-34)`
  • Whenever a hydrogen atom emits a photon in the Balmer series ,

    A
    it must emit another photon in the Balmer series
    B
    it must emit another photon in the Lyman series
    C
    the second photon, if emitted will have a wavelenth of about 122 nm
    D
    it may emit a second photon, but the wavelength of this photon cannot be predicted
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