Physics Laboratory Manual
4th Edition
ISBN: 9781133950639
Author: David Loyd
Publisher: Cengage Learning
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Question
Chapter 43, Problem 1PLA
To determine
The Balmer formula for the wavelengths of the visible light spectrum of hydrogen.
Expert Solution & Answer
Answer to Problem 1PLA
The Balmer formula for the wavelengths of the visible light spectrum of hydrogen is
Explanation of Solution
Write the empirical equation for the wavelengths of the visible light spectrum of hydrogen by Johann Balmer
Here,
Conclusion:
Thus, the Balmer formula for the wavelengths of the visible light spectrum of hydrogen is
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=
Find the energy of the photon released in the transition from n₁
for a hydrogen atom. (Note: Use Rydberg Formula)
3 to n₂ = 2
An infrared photon is absorbed by a hydrogen atom.
A transition in which spectra series could account for this emission?
Question 14 options:
Lyman series
Balmer series
Paschen series
World series
None of the other responses are correct.
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- Derive an expression for the ratio of X-ray photon frequency for two elements with atomic numbers Z1 and Z2.arrow_forwardAnswer of the question immediately pleasearrow_forwardShow that different lines of the hydrogen spectrum in terms of angstroms are obtained from the following equation :arrow_forward
- The energy levels for a Bohr atom are shown below. Use this diagram to solve problems 7 and 8. 0 eV -2.5 eV -4.0 eV -7.0 eV -12.5 eV 7. What amount of energy is needed for an electron to jump from n = 1 to n = 4? 8. What is the wavelength of the photon needed to make this happen? Is it emission or absorption?arrow_forwardFind the wavelength of the photon that is emitted when a hydrogen atom undergoes a transition from n; = 6 to nf = 2. (RH = 1.097 x 10-3Å-1) Answerarrow_forwardFind the ratio between the wavelengths of the ‘most energetic’ spectral lines in the Balmer and Paschen series of the hydrogen spectrum.arrow_forward
- In the equation below, the Balmer series involves the emission lines (wavelengths) obtained when electrons go from higher energy (excited) level to 1 1 R n' 1 where, R = 1.097 x 107 m-1 %3D -- A. The ground level (n = 1) B. The first atomic level (n = 2) C. The third atomic level (n = 3) D. The fourth atomic level (n = 4) E. The fifth atomic level (n = 4) %3D %3Darrow_forwardالسؤال 12 Find the values of S for the representation of electron state H,arrow_forwardQuestion 2. Let us consider a hypothetical Atom with the following list of energy levels: E1 = 1.5 eV E2 = 3.5 eV E3 = 4.8 eV E4 = 5.6 eV a) Compute the energy of ALL the spectral lines in the ABSORPTION SPECTRUM and list the corresponding "colors" b) Compute the energy of ALL the spectral lines in the EMISSION SPECTRUM and list the corresponding "colors" Wavelength Frequency Photon energy (nm) (THz) 380-450 670-790 450-485 620-670 cyan 485-500 600-620 green 500-565 530-600 yellow 565-590 510-530 orange 590-625 480-510 red 625-750 400-480 Color violet blue (eV) 2.75-3.26 2.56-2.75 2.48-2.56 2.19-2.48 2.10-2.19 1.98-2.10 1.65-1.98arrow_forward
- A hydrogen atom emits light and ends in a state characterized by n₂ = 2. If the wavelength of the light emitted is 434 nm, use the Rydberg formula below to find the value of n₁ that characterizes the initial state of the atom. (RH= 1.09737316 × 107 m-1) (3) H 2 2 n n 2 1 -=R 2arrow_forwardUsing the Rydberg formula, calculate the wavelengths of the first four spectral lines in the Lyman series of the hydrogen spectrum.arrow_forwardA photoelectron is emitted from K shell (n = 1) of a carbon atom, and an election in L shell (n = 2) moves down to the vacancy in K shell. What is the wavelength, in the unit of nm, of the photon emitted during this transition? Use for the energy difference between two states in an atom. E0 = 13.6 eV and atomic number of carbon is Z = 12. Use σ = 1 for the transition to K shell and σ = 7.4 for the transition to L shellarrow_forward
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