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The wavelengths of photons emitted by el...

The wavelengths of photons emitted by electron transition between two similar leveis in H and `He^(+)` are `lambda_(1)` and `lambda_(2)` respectively. Then :-

A

`lambda_(2)=lambda_(1)`

B

`lambda_(2)=2lambda_(1)`

C

`lambda_(2)=lambda_(1)//2`

D

`lambda_(2)=lambda_(1)//4`

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To solve the problem regarding the wavelengths of photons emitted by electron transitions in hydrogen (H) and helium ion (He⁺), we need to analyze the energy levels and the relationship between energy and wavelength. ### Step-by-Step Solution: 1. **Understanding Energy Levels**: The energy of an electron in a hydrogen-like atom is given by the formula: \[ E_n = -\frac{E_1 \cdot Z^2}{n^2} \] where \(E_1\) is the energy of the ground state, \(Z\) is the atomic number, and \(n\) is the principal quantum number. 2. **Energy of Photons**: The energy of a photon emitted during a transition is also related to its wavelength (\(\lambda\)) by the equation: \[ E = \frac{hc}{\lambda} \] where \(h\) is Planck's constant and \(c\) is the speed of light. 3. **Relating the Two Atoms**: For hydrogen (H), \(Z = 1\) and for helium ion (He⁺), \(Z = 2\). Therefore, the energy levels for both can be expressed as: - For hydrogen: \[ E_n^{H} = -\frac{E_1 \cdot 1^2}{n^2} = -\frac{E_1}{n^2} \] - For helium ion: \[ E_n^{He^+} = -\frac{E_1 \cdot 2^2}{n^2} = -\frac{4E_1}{n^2} \] 4. **Setting Up the Relationship**: The energy of the emitted photon during a transition can be expressed as: \[ E = E_{\text{initial}} - E_{\text{final}} \] Therefore, for transitions in hydrogen and helium ion, we can write: \[ E_{\text{photon}}^{H} = E_n^{H} \quad \text{and} \quad E_{\text{photon}}^{He^+} = E_n^{He^+} \] 5. **Finding the Wavelengths**: From the energy-wavelength relationship, we can derive: \[ \lambda_1 \propto \frac{1}{E_n^{H}} \quad \text{and} \quad \lambda_2 \propto \frac{1}{E_n^{He^+}} \] 6. **Calculating the Ratio of Wavelengths**: The ratio of the wavelengths can be expressed as: \[ \frac{\lambda_2}{\lambda_1} = \frac{E_n^{H}}{E_n^{He^+}} = \frac{1^2}{2^2} = \frac{1}{4} \] Thus, we can conclude: \[ \lambda_2 = 4 \lambda_1 \] ### Final Result: The relationship between the wavelengths of photons emitted by electron transitions in hydrogen and helium ion is: \[ \lambda_2 = 4 \lambda_1 \]

To solve the problem regarding the wavelengths of photons emitted by electron transitions in hydrogen (H) and helium ion (He⁺), we need to analyze the energy levels and the relationship between energy and wavelength. ### Step-by-Step Solution: 1. **Understanding Energy Levels**: The energy of an electron in a hydrogen-like atom is given by the formula: \[ E_n = -\frac{E_1 \cdot Z^2}{n^2} ...
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ALLEN-ATOMIC STRUCTURE-Exercise - 02
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  2. According to Schrodinger model nature of electron in an atom is as :-

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  3. Which describes orbital :-

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  4. In order to have the same wavelength for the electron (mass m(e)) and ...

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  5. The quantum number + 1//2 and -1//2 for the electron spin represent

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  6. Which is true about Psi :-

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  7. The circumference of n^(th) orbit in H-atom can be expressed in terms ...

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  8. A particle X moving with a certain velocity has a debroglie wave lengt...

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  9. What are the values of the orbital angular momentum of an electron in ...

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  10. If m = magnetic quantum number and l = azimuthal quantum number then :...

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  11. The number of unpaired electron in Mn^(4+) (Z = 25) is :-

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  12. After np orbitals are filled, the next orbital filled will be :-

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  13. The value of the magnetic moment of a particular ion is 2.83 Bohr magn...

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  14. In Bohr's model of the hydrogen atom, the ratio between the period of ...

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  15. If v1 is the frequency of the series limit of lyman seies, v2 is the f...

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  16. The energies of energy levels A, B and C for a given atom are in the s...

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  17. The wavelengths of photons emitted by electron transition between two ...

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  18. If first ionisation potential of a hypothetical atom is 16 V, then the...

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  19. In which transition minimum energy is emitted :-

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  20. No. of visible lines when an electron returns from 5^(th) orbit up to ...

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