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Solution Manual for Game Theory Basics 1st Edition By Bernhard von Stengel, ISBN: 9781108843300, All 12 Chapters Covered

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Solution Manual for Game Theory Basics 1st Edition By Bernhard von Stengel, ISBN: 9781108843300, All 12 Chapters Covered

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Game Theory Basics By Bernhard Von Stengel
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Institution
Game Theory Basics By Bernhard Von Stengel
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Game Theory Basics By Bernhard Von Stengel

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Uploaded on
February 8, 2025
Number of pages
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Written in
2024/2025
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SOLUTION MANUAL Modern Physics with Modern
f f f f f




f Computational Methods: for Scientists and Engineers
f f f f f




f 3rd Edition by Morrison Chapters 1- 15
f f f f f f

,Table of contents f f




1. The Wave-Particle Duality
f f f




2. The Schrödinger Wave Equation
f f f f




3. Operators and Waves
f f f




4. The Hydrogen Atom
f f f




5. Many-Electron Atoms
f f




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




7. Diatomic Molecules
f f




8. Statistical Physics
f f




9. Electronic Structure of Solids
f f f f




10. Charge Carriers in Semiconductors
f f f f




11. Semiconductor Lasers
f f




12. The Special Theory of Relativity
f f f f f




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




14. Particle Physics
f f




15. Nuclear Physics
f f

,1

The Wave-Particle Duality - Solutions
f f f f




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



given by Eq. (1.5). Following Example 1.1 and substituting λ =
f f f f f f f f f f f



200 eV gives:
f f f




hc 1240 eV · nm
= = 6.2 eV
f f f



Ephoton = λ
f f


200 nm f f




2. The energy of the beam each second is:
f f f f f f f




power 100 W
= = 100 J
f



Etotal = time
f f


1s f f




The number of photons comes from the total energy divided by
f f f f f f f f f f



the energy of each photon (see Problem 1). The photon’s energy
f f f f f f f f f f f



must be converted to Joules using the constant 1.602 × 10−19
f f f f f f f f f f f



J/eV , see Example 1.5. The result is:
f f f f f f f f




N =Etotal = 100 J = 1.01 × 1020 f f f


photons E
f f f



pho
ton 9.93 × 10−19 f f




for the number of photons striking the surface each second.
f f f f f f f f f




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



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



Example 1.1, the energy of a single photon is:
f f f f f f f f f




1240 eV · nm
hc = 1.960 eV
f f f

f f

Ephoton = 632.8 nm f f f


=
λ
f

f



We now convert to SI units (see Example 1.5):
f f f f f f f f




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




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




1 × 10−3 J/s 15 photons f f f
f


Rate of emission = = 3.19 × 10
3.14 × 10−19 J/photon s
f f f f f f f
f
f f f

, 2

4. The maximum kinetic energy of photoelectrons is found
f f f f f f f



f using Eq. (1.6) and the work functions, W, of the metals are
f f f f f f f f f f f



f given in Table 1.1. Following Problem 1, Ephoton = hc/λ = 6.20
f f f f f f f f f f f



f eV . For part (a), Na has W = 2.28 eV :
f f f f f f f f f f f




(KE)max= 6.20 eV − 2.28 eV = 3.92 eV f f f f f f f f f




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



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




5.This problem again concerns the photoelectric effect. As in
f f f f f f f f



Problem 4, we use Eq. (1.6):
f f f f f f




hc − f

(KE)max =

f



f f




where W is the work function of the material and the term hc/λ
f f f f f f f f f f f f



describes the energy of the incoming photons. Solving for the latter:
f f f f f f f f f f f




hc
= (KE)max + W = 2.3 eV + 0.9 eV = 3.2 eV
λ
f f f f f f f f f f f f

f




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




1240 eV · nm
λ=
f f f


= 387.5 nm f


3.2
f f




eV f




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



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



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




hc 1240 eV · — 0.72 eV = 1.98 eV
W= (KE)max
f f



λ
f f f f f

nm
f f



=
f

f




460 nm f




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




hc 1240 eV ·
(KE)max = − W
f


— 1.98 eV = 3.19 eV
f f
f


nm
f f f f f f


= f
f



λ
240 nm f




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



reaching the anode.
f f f




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



f zero. Setting (KE)max = 0 in Eq. (1.6),
f f f f f f f




hc
W= f = 1240 eV · = 3.44 eV f f



λ0 nm f
f f




360 nm f




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

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