Physics (5th Edition)
5th Edition
ISBN: 9780134051802
Author: Walker
Publisher: PEARSON
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Chapter 31.4, Problem 4EYU
To determine
The value of
n
for the Bohr orbit shows in Figure 31-14.
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Check out a sample textbook solutionStudents have asked these similar questions
The second member of Balmer series
of hydrogen atom has wavelength 4860 A.U.
Calculate Rydberg's constant. Hence calculate
the energy in eV when electron is orbiting in
the third Bohr orbit. [Planck's constant = 6.63 ×
10-34 Js; Speed of light in vaccum = 3 × 10³ m/s;
1 eV = 1.6 × 10-¹⁹ Jl
19
Energy changes of -1.8167 x 10-19 is recorded when an electron jump from n=6 in an unknown series of hydrogen line spectra.
a) calculate the value of nf- [ RH = 2.18 x 10-19]b) identify the line spectra for this radiation
How does the distance between adjacent orbits in a hydrogen atom vary with increasing
values of the orbital number n?
What should take place for a hydrogen atom to emit longest possible wavelength in
Balmer series? Explain.
Chapter 31 Solutions
Physics (5th Edition)
Ch. 31.1 - Prob. 1EYUCh. 31.2 - Prob. 2EYUCh. 31.3 - Prob. 3EYUCh. 31.4 - Prob. 4EYUCh. 31.5 - Prob. 5EYUCh. 31.6 - Prob. 6EYUCh. 31.7 - Prob. 7EYUCh. 31 - Prob. 1CQCh. 31 - Prob. 2CQCh. 31 - Prob. 3CQ
Ch. 31 - Prob. 4CQCh. 31 - Prob. 5CQCh. 31 - Prob. 6CQCh. 31 - Prob. 7CQCh. 31 - Prob. 8CQCh. 31 - Prob. 9CQCh. 31 - Prob. 1PCECh. 31 - Prob. 2PCECh. 31 - Prob. 3PCECh. 31 - Prob. 4PCECh. 31 - Prob. 5PCECh. 31 - Prob. 6PCECh. 31 - Prob. 7PCECh. 31 - Prob. 8PCECh. 31 - Prob. 9PCECh. 31 - Prob. 10PCECh. 31 - Prob. 11PCECh. 31 - Prob. 12PCECh. 31 - Prob. 13PCECh. 31 - Prob. 14PCECh. 31 - Prob. 15PCECh. 31 - Prob. 16PCECh. 31 - Prob. 17PCECh. 31 - Prob. 18PCECh. 31 - Prob. 19PCECh. 31 - Prob. 20PCECh. 31 - Prob. 21PCECh. 31 - Prob. 22PCECh. 31 - Prob. 23PCECh. 31 - Prob. 24PCECh. 31 - Prob. 25PCECh. 31 - Prob. 26PCECh. 31 - Prob. 27PCECh. 31 - Prob. 28PCECh. 31 - Prob. 29PCECh. 31 - Prob. 30PCECh. 31 - Prob. 31PCECh. 31 - Prob. 32PCECh. 31 - Prob. 33PCECh. 31 - Prob. 34PCECh. 31 - Prob. 35PCECh. 31 - Prob. 36PCECh. 31 - Prob. 37PCECh. 31 - Prob. 38PCECh. 31 - Prob. 39PCECh. 31 - Prob. 40PCECh. 31 - Prob. 41PCECh. 31 - Prob. 42PCECh. 31 - Prob. 43PCECh. 31 - Prob. 44PCECh. 31 - Prob. 45PCECh. 31 - Prob. 46PCECh. 31 - Prob. 47PCECh. 31 - Prob. 48PCECh. 31 - Prob. 49PCECh. 31 - Prob. 50PCECh. 31 - Prob. 51PCECh. 31 - Prob. 52PCECh. 31 - Give the electronic configuration for the ground...Ch. 31 - Prob. 54PCECh. 31 - Prob. 55PCECh. 31 - Prob. 56PCECh. 31 - The configuration of the outer electrons in Ni is...Ch. 31 - Prob. 58PCECh. 31 - Prob. 59PCECh. 31 - Prob. 60PCECh. 31 - Prob. 61PCECh. 31 - Prob. 62PCECh. 31 - Prob. 63PCECh. 31 - Prob. 64PCECh. 31 - Prob. 65PCECh. 31 - Prob. 66PCECh. 31 - Prob. 67PCECh. 31 - Prob. 68GPCh. 31 - Prob. 69GPCh. 31 - Prob. 70GPCh. 31 - Prob. 71GPCh. 31 - Prob. 72GPCh. 31 - Prob. 73GPCh. 31 - Prob. 74GPCh. 31 - Prob. 75GPCh. 31 - Prob. 76GPCh. 31 - Prob. 77GPCh. 31 - Prob. 78GPCh. 31 - Prob. 79GPCh. 31 - Prob. 80GPCh. 31 - Prob. 81GPCh. 31 - Prob. 82GPCh. 31 - Prob. 83GPCh. 31 - Prob. 84PPCh. 31 - Prob. 85PPCh. 31 - Prob. 86PPCh. 31 - Prob. 87PPCh. 31 - Prob. 88PPCh. 31 - Prob. 89PP
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- (a) What is the momentum of a 0.0100-nm-wavelength photon that could detect details of an atom? (b) What is its energy in MeV?arrow_forward(a) If one subshell of an atom has 9 electrons in it, what is the minimum value of l ? (b) What is the spectroscopic notation for this atom, if this subshell is part of the n=3 shell?arrow_forwardShow that Stefan’s law results from Planck’s radiation law. Hin: To compute the total power of blackbody radiation emitted across the entire spectrum of wavelengths at a given temperature, integrate Planck’s law over the entire spectrum P(T)=0I(,T)d. Use the substitution x=hckT and the tabulated value of the integral 0dx x 3( e x 1)=415arrow_forward
- How do the allowed orbits for electrons in atoms differ from the allowed orbits for planets around the sun? Explain how the correspondence principle applies here.arrow_forwardWhen the absorption spectrum of hydrogen at room temperature is analyzed, absorption lines for the Lyman series are found, but none are found for the Balmer series. What does this tell us about the energy state of most hydrogen atoms at room temperature?arrow_forward85 In about 1916, R. A. Millikan found the following stopping- potential data for lithium in his photoelectric experiments: Wavelength (nm) 433.9 404.7 Stopping potential (V) 365.0 312.5 253.5 0.55 0.73 1.09 1.67 2.57 Use these data to make a plot like Fig. 38-2 (which is for sodium) and then use the plot to find (a) the Planck constant and (b) the work function for lithium.arrow_forward
- The de Broglie wavelength of an electron is 0.75 A°. What is its velocity? What is the P.D. required to accelerate the electron from rest to this velocity? m = 9 x 10-31 kg; h = 6.63 x 10-34 Js; e = 1.6 x 10-19 C. %3Darrow_forward5.) In the textbook and workbook we saw that an electron in the n = 3 energy level yielded three wavelengths, 2 in the UV (3->1 and 2->1) and one in the visible region (3->2). In lecture we looked at an electron in the n = 4 energy level and determined that it yielded six wavelengths, 3 in the UV (4-> 1, 3->1 and 2->1), 2 in the visible region (4->2 and 3->2) and 1 in the IR region (4->3). Now consider an electron in the n = 5 energy level. How many wavelengths would you expect in the UV region? Just a number like 6.arrow_forwardThe photoelectric work function for a metal is 4.2 eV. If the stopping potential is 3V. Find the threshold wavelength and maximum kinetic energy of emitted electrons. (velocity of light in air = 3 x 10° m's, Planck's constant = 6.63 x 10 J-s, charge on electron = 1.6 x 10 C). %3Darrow_forward
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