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Modern Physics with Modern Computational Methods for Scientists and Engineers – 3rd Edition by Morrison | Solution Manual Chapters 1–15

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This document provides the complete solution manual for Modern Physics with Modern Computational Methods for Scientists and Engineers (3rd Edition) by Morrison. It covers detailed, step-by-step solutions for all exercises and problems from chapters 1 through 15. A valuable resource for students aiming to understand problem-solving methods and computational applications in modern physics.

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SOLUTION MANUAL Modern Physics
with Modern Computational Methods:
for Scientists and Engineers 3rd Edition
by Morrison Chapters 1- 15

,Table of contents go go




1. The Wave-Particle Duality
go go go




2. The Schrödinger Wave Equation
go go go go




3. Operators and Waves
go go go




4. The Hydrogen Atom
go go go




5. Many-Electron Atoms
go go




6. The Emergence of Masers and Lasers
go go go go go go




7. Diatomic Molecules
go go




8. Statistical Physics
go go




9. Electronic Structure of Solids
go go go go




10. Charge Carriers in Semiconductors
go go go go




11. Semiconductor Lasers
go go




12. The Special Theory of Relativity
go go go go go




13. The Relativistic Wave Equations and General Relativity
go go go go go go go




14. Particle Physics
go go




15. Nuclear Physics
go go

,1

The Wave-Particle Duality - Solutions
g o g o g o g o




1. The energy of photons in terms of the wavelength of light is gi
go go go go go go go go go go go go




ven by Eq. (1.5). Following Example 1.1 and substituting λ = 2
go go go go go g o go go go go go




00 eV gives:
go go




hc 1240 eV · nm
= = 6.2 eV
go g o go




Ephoton = λ
go go



200 nm go go




2. The energy of the beam each second is:
g o g o g o g o g o g o g o




power 100 W
= = 100 J
go




Etotal = time
go go



1s go go




The number of photons comes from the total energy divided by t
go go go go go go go go go go go




he energy of each photon (see Problem 1). The photon’s energy
go go go go go go go go go go go




must be converted to Joules using the constant 1.602 × 10−19 J/e
go go go go go go go go go go go




V , see Example 1.5. The result is:
go go go go go go go




N =Etotal = 100 J = 1.01 × 1020 go g o go




photons E
go go go




pho
ton 9.93 × 10−19 go go




for the number of photons striking the surface each second.
g o g o g o g o g o g o g o g o g o




3.We are given the power of the laser in milliwatts, where 1 mW =
go go go go go go go go go go go go go go




10−3 W . The power may be expressed as: 1 W = 1 J/s. Followin
go go go go go go go go go go go go go go




g Example 1.1, the energy of a single photon is:
go go go go go go go go go




1240 eV · nm
hc = 1.960 eV
go g o go




Ephoton = 632.8 nm
go go go


g go
g o



=
λ
o


g o




We now convert to SI units (see Example 1.5):
go go go go go go go g o




1.960 eV × 1.602 × 10−19 J/eV = 3.14 × 10−19 J
go go go go go go go go go go go




Following the same procedure as Problem 2: go go go go go go




1 × 10−3 J/s 15 photons go go go
g o



Rate of emission = = 3.19 × 10
3.14 × 10−19 J/photon s
go g o go g o go go go
g o
go go g o

, 2

4.The maximum kinetic energy of photoelectrons is found usin
go go go go go go go go




g Eq. (1.6) and the work functions, W, of the metals are given in
go go go go go go go go go go go go go go




Table 1.1. Following Problem 1, Ephoton = hc/λ = 6.20 eV . For
go go go g o g o go go go go g o go g o g o




part (a), Na has W = 2.28 eV :
g o g o g o g o g o go g o go




(KE)max = 6.20 eV − 2.28 eV = 3.92 eV go go go go go go g o go go




Similarly, for Al metal in part (b), W = 4.08 eV giving (KE)max = 2.12 eV
go go go go go go go g o go go g o go go go go




and for Ag metal in part (c), W = 4.73 eV , giving (KE)max = 1.47 eV .
go go go go go go go go go go go go go go go go go




5.This problem again concerns the photoelectric effect. As in Prob
go go go go go go go go go




lem 4, we use Eq. (1.6):
go go go go go




hc − go



(KE)max = go





go




go




where W is the work function of the material and the term hc/
g o g o g o g o g o g o g o g o g o g o g o g o




λ describes the energy of the incoming photons. Solving for the latte
g o go go go go go go go go go go




r:
hc
= (KE)max + W = 2.3 eV + 0.9 eV = 3.2 eV
λ
go go go g o go go g o go go g o go go


g o




Solving Eq. (1.5) for the wavelength: go go go go go




1240 eV · nm
λ=
go g o go



= 387.5 nm go



3.2 e
go go


g o



V
6. A potential energy of 0.72 eV is needed to stop the flow of electrons.
go go go go go go go go go go go go go go




Hence, (KE)max of the photoelectrons can be no more than 0.72 eV.
go go go go go go go go go go go go




Solving Eq. (1.6) for the work function: go go go go go go




hc 1240 eV · n — 0.72 eV = 1.98 eV
W= —
go g o go




λ m
go go g o go go
go g o




(KE)max g



= o




460 nm go




7. Reversing the procedure from Problem 6, we start with Eq. (1.6): go go go go go go go go go go




hc 1240 eV · n
(KE)max = − W
g o




— 1.98 eV = 3.19 eV
go g o go
go g o




m
go go go g o go go




=
λ
240 nm go




Hence, a stopping potential of 3.19 eV prohibits the electrons from
go go go go go go go go go go go




reaching the anode. go go




8. Just at threshold, the kinetic energy of the electron is
g o g o g o g o g o g o g o g o g o g o




zero. Setting (KE)max = 0 in Eq. (1.6),
g o go go go g o g o g o




hc 1240 eV · n
W= = = 3.44 eV
go g o go




λ0
go



m
go go




360 nm go




9. A frequency of 1200 THz is equal to 1200 × 1012 Hz. Using Eq. (1.10),
go go go go go go go go go go go go go go

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Raymond A. Serway, Clement J. Moses, Curt A. Moyer Student Solutions Manual for Serway/Moses/Moyer S Modern Physics, 3rd
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Subido en
22 de septiembre de 2025
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