Solutions_C20

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MR. SURRETTE
VAN NUYS HIGH SCHOOL
CHAPTER 20: MODERN PHYSICS
WORKSHEET SOLUTIONS
1. According to Einstein, what is true of the stopping potential for a photoelectric current as the
wavelength of incident light becomes shorter?
1A.
(E) increases
(1) The maximum kinetic energy of photoelectrons increases as the frequency of incident photons
increases: hf = Kmax + .
(2) The speed of light is constant
(c = 3.00 x 108 m/s). Therefore, frequency increases as wavelength decreases: c = f .
2. What is the de Broglie wavelength for a proton moving at a speed of 6.15 x 107 m/s?
2A.
(1) p = mv
(2) p = (1.67 x 10-27 kg)(6.15 x 107 m/s)
(3) p = 1.03 x 10-19 kg.m/s
(4) p = h / 
(5)  = h / p
(6)  = (6.63 x 10-34 J.s) / (1.03 x 10-19 kg.m/s)
(7)  = 6.46 x 10-15 m
3. A nearby star’s surface temperature is 6200 K and the peak wavelength in its radiation is 475 nm.
What is the surface temperature of a distant star where the peak wavelength is 585 nm?
3A.
(1) T11 = T22
(2) T2 = (T11 / 2)
(3) T2 = [(6200 K)(475 x 10-9 m) / (585 x 10-9 m)]
(4) T2 = 5034 K
4. According to Einstein, increasing the brightness of a beam of light without changing its color will
increase:
4A. (C) number of photons
5. How much energy (in eV) does a photon of light ( = 700 nm) have?
5A.
(1) v = f 
(2) f = v / 
(3) f = (3.00 x 108 m/s) / (700 x 10-9 m)
(4) f = 4.29 x 1014 Hz
(5) E = hf
(6) E = (4.14 x 10-15 eV.s)(4.29 x 1014 Hz)
(7) E = 1.77 eV
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CHEMISTRY
MR. SURRETTE
VAN NUYS HIGH SCHOOL
6. Light of wavelength 415 nm is incident onto the surface of a metal whose work function is 1.85 eV.
6a. What is the frequency of the light wave in petahertz?
A.
(1) v = f 
f = v / 
(3) f = (3.00 x 108 m/s) / 415 x 10-9 m
(4) f = 7.23 x 1014 Hz
(5) f = 0.723 PHz
6b.
A.
(1)
(2)
(3)
Compute the photon energy in eV.
E = hf
E = (4.14 x 10-15 eV.s)(7.23 x 1014 Hz)
E = 2.99 eV
6c. Will these photons eject electrons from the metal’s surface?
A.
Yes, the photon energy (2.99 eV) is greater than the minimum energy needed (1.85 eV), the work
function().
6d.
A.
(1)
(2)
(3)
(4)
What is the predicted value of the maximum kinetic energy of the photoelectrons?
E = Kmax + 
Kmax = E – 
Kmax = 2.99 eV – 1.85 eV
Kmax = 1.22 eV
6e. Would photons of wavelength 830 nm produce photoelectrons?
A.
No. Doubling the wavelength halves the photon energy:
(1) v = f 
(2) f = v / 
(3) f = (3.00 x 108 m/s) / (830 x 10-9 m)
(4) f = 3.61 x 1014 Hz
(5) E = hf
(6) E = (4.14 x 10-15 eV.s)(3.61 x 1014 Hz)
(7) E = 1.50 eV
Since the work function ( is 1.85 eV, photons of 1.50 eV will not release photoelectrons.
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CHEMISTRY
MR. SURRETTE
VAN NUYS HIGH SCHOOL
7. If a hydrogen atom in the state n = 4 makes a transition to the state n = 2, what is the energy of the
photon that is emitted?
7A.
(1) E = (13.6 eV / (n2)2) – (13.6 eV / (n4)2)
(2) E = (13.6 eV / 22) – (13.6 eV / 42)
(3) E = 3.4 eV – 0.85 eV
(4) E = 2.55 eV
8. The observed relativistic length of a super rocket moving by the observer at 0.875 c will be what
factor times that of the measured rocket length at rest?
8A.
(1) L = L’ [1 – v2/c2]1/2
(2) L = L’ [1 – (0.875 c)2/(1.0 c)2]1/2
(3) L = L’ (0.125)1/2
(4) L = (0.35) L’
(5) factor = 0.35
9. How fast would a rocket have to move past a ground observer if he observed a 12% length
contraction in the rocket length?
9A.
(1) L = L’ [1 – v2/c2]1/2
(2) (0.88 L’) = L’ [1 – v2/c2]1/2
(3) (0.88 L’) = L’ [1 – v2/c2]1/2
(4) 0.88 = (1 – v2/c2)1/2
(5) (0.88)2 = 1 – v2/c2
(6) - v2/c2 = (0.88)2 -1
(7) v2/c2 = 1 - (0.88)2
(8) v2/c2 = 0.0226
(9) v2 = (0.0226)(c2)
(10) v2 = (0.0226)(3.00 x 108 m/s)2
(11) v = [(0.0226)(3.00 x 108 m/s)2]1/2
(12) v = 1.42 x 108 m/s
10. An unknown particle in an accelerator moving at a speed of 2.85 x 108 m/s has a measured
relativistic mass of 3.2 x 10-26 kg. What is its rest mass?
10A.
(1) m = mo / [1 – (v2/c2)]1/2
(2) mo = (m)[1 – (v2/c2)]1/2
(3) mo = (3.2 x 10-26 kg)[1 – (2.85 x 108 m/s)2 / (3.00 x 108 m/s)2]1/2
(4) mo = 1.6 x 10-27 kg
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CHEMISTRY
MR. SURRETTE
VAN NUYS HIGH SCHOOL
11. An astronaut whose heart rate on Earth is 70 per minute increases his velocity to v = 0.980 c. What
is his heart rate now as measured by an Earth observer?
11A.
(1) t = (t)’ / [1 – (v2/c2)]1/2
(2) t =(t)’ / [1 - (0.980 c)2/(1.00 c)2]1/2
(3) t = (t)’ / 0.0199
(4) t’ = (0.0199) t
(5) t’ = (0.0199)(70 per minute)
(6) t’ = 13.9 per minute
12. The short lifetime of muons created in the upper atmosphere of the Earth would not allow them to
reach the surface of the Earth unless their lifetime increased by time dilation. From the reference system
of the muons, the muons can reach the surface of the Earth because:
12A. (D) length contraction decreases the distance to the Earth
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CHEMISTRY
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