PHY3702
ASSIGNMENT 1
Quantum Physics
FULL SOLUTIONS
COMPLETE SOLUTIONS
MEMORANDUM
UNISA 2026
Page 1 of 21
,SOLUTIONS:
Question 1
(a) Using the Stefan–Boltzmann law for a blackbody,
𝐼 = 𝜎𝑇 4
where 𝜎 = 5.67 × 10−8 W m−2 K −4 and 𝐼 = 575 × 106 W m−2,
1/4
𝐼 1/4 575 × 106
𝑇=( ) =( ) = (1.014 × 1016 )1/4 ≈ 1.00 × 104 K.
𝜎 5.67 × 10−8
The surface temperature is approximately 1.0 × 104 K.
Using the Stefan–Boltzmann law 𝐼 = 𝜎𝑇 4 , with 𝐼 = 575 × 106 W m−2 and 𝜎 =
5.67 × 10−8 W m−2 K−4 ,
1/4
575 × 106
𝑇=( ) ≈ 1.78 × 104 K
5.67 × 10−8
2.898×10−3
Using Wien’s law 𝜆max = ,
𝑇
2.898 × 10−3
𝜆max ≈ ≈ 1.63 × 10−7 m = 163 nm
1.78 × 104
Page 2 of 21
, SOLUTIONS:
Question 2
(a) The photoelectric equation:
ℎ𝑐
𝑒𝑉0 = −𝜙
𝜆
With 𝑉0 = 1.2 V and 𝜆 = 480 nm:
ℎ𝑐 1240 eV nm
= ≈ 2.583 eV.
𝜆 480 nm
𝜙 = 2.583 eV − 1.2 eV = 1.383 eV.
The work function is 1.38 eV.
Photon energy:
ℎ𝑐 1240
𝐸= = ≈ 2.58 eV
𝜆 480
Work function:
𝜙 = 𝐸 − 𝑒𝑉𝑠 = 2.58 − 1.2 = 1.38 eV
Page 3 of 21
ASSIGNMENT 1
Quantum Physics
FULL SOLUTIONS
COMPLETE SOLUTIONS
MEMORANDUM
UNISA 2026
Page 1 of 21
,SOLUTIONS:
Question 1
(a) Using the Stefan–Boltzmann law for a blackbody,
𝐼 = 𝜎𝑇 4
where 𝜎 = 5.67 × 10−8 W m−2 K −4 and 𝐼 = 575 × 106 W m−2,
1/4
𝐼 1/4 575 × 106
𝑇=( ) =( ) = (1.014 × 1016 )1/4 ≈ 1.00 × 104 K.
𝜎 5.67 × 10−8
The surface temperature is approximately 1.0 × 104 K.
Using the Stefan–Boltzmann law 𝐼 = 𝜎𝑇 4 , with 𝐼 = 575 × 106 W m−2 and 𝜎 =
5.67 × 10−8 W m−2 K−4 ,
1/4
575 × 106
𝑇=( ) ≈ 1.78 × 104 K
5.67 × 10−8
2.898×10−3
Using Wien’s law 𝜆max = ,
𝑇
2.898 × 10−3
𝜆max ≈ ≈ 1.63 × 10−7 m = 163 nm
1.78 × 104
Page 2 of 21
, SOLUTIONS:
Question 2
(a) The photoelectric equation:
ℎ𝑐
𝑒𝑉0 = −𝜙
𝜆
With 𝑉0 = 1.2 V and 𝜆 = 480 nm:
ℎ𝑐 1240 eV nm
= ≈ 2.583 eV.
𝜆 480 nm
𝜙 = 2.583 eV − 1.2 eV = 1.383 eV.
The work function is 1.38 eV.
Photon energy:
ℎ𝑐 1240
𝐸= = ≈ 2.58 eV
𝜆 480
Work function:
𝜙 = 𝐸 − 𝑒𝑉𝑠 = 2.58 − 1.2 = 1.38 eV
Page 3 of 21