Atomic Physics Problems Set Solutions

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SPH3U1 - Energy Problems Set 2
Problems
1. Write the nuclear reaction equation for
the following nuclei undergoing the
indicated type of decay:
a)
210
84π‘ƒπ‘œ
b)
45
20πΆπ‘Ž
→
45
21𝑆𝑐
c)
46
24πΆπ‘Ÿ
→
46
23𝑉
d)
152
∗
66𝐷𝑦
e)
240
94𝑃𝑒
→
236
92π‘ˆ
+ 42𝐻𝑒
g) 214
83𝐡𝑖 →
214
84𝐡𝑖
f)
58
∗
29𝐢𝑒
→
58
29𝐢𝑒
+ 00𝛾
h) 22
11π‘π‘Ž →
22
10𝑁𝑒
→
206
82𝑃𝑏
→
+ 42𝐻𝑒
a.
b.
c.
d.
e.
f.
g.
h.
Nucleus
Polonium-210
Calcium-45
Chromium-46
Dysprosium-152
Plutonium-240
Copper-58
Bismuth-214
Sodium-22
+ −10𝛽
+ 01𝛽
152
66𝐷𝑦
+ 00𝛾
Decay type
alpha decay
beta-negative decay
beta-positive decay
γ decay
α decay
gamma decay
β- decay
β+decay
+ −10𝛽
+ 01𝛽
2. The following shows the products of part of a decay series known as the Thorium Series. Write a nuclear
reaction equation for each decay stage of the series and identify its type.
232
228
228
228
224
220
90π‘‡β„Ž → 88π‘…π‘Ž → 89𝐴𝑐 → 90π‘‡β„Ž → 88π‘…π‘Ž → 86𝑅𝑛
232
228
4
90π‘‡β„Ž → 88π‘…π‘Ž + 2𝐻𝑒
228
88π‘…π‘Ž
→
228
89𝐴𝑐
+ −10𝛽
228
89𝐴𝑐
→
228
90π‘‡β„Ž
+ −10𝛽
228
90π‘‡β„Ž
→
224
88π‘…π‘Ž
+ −10𝛽
224
88π‘…π‘Ž
→
220
86𝑅𝑛
+ 42𝐻𝑒
Half-life
3. The half-life of carbon-14 is 5730 a. An ancient piece of bark is estimated to have originally contained
2.00 µg of carbon-14. If its age has been determined to be 1.7x104 a, how much carbon-14 does it now
have?
1
𝑑⁄
𝑇1/2
𝑁 = 𝑁0 (2)
𝑁=
1.7×104 π‘Ž⁄
1 (
5730 π‘Ž)
(2.00 πœ‡π‘”) ( )
2
𝑁 = 0.2558 πœ‡π‘”
𝑁 = 0.26 πœ‡π‘”
4. A specimen of peat from an ancient bog contains 800.0 µg of carbon-14. What will be the amount of
carbon-14 remaining after 1.0 x104 a?
1
𝑑⁄
𝑇1/2
𝑁 = 𝑁0 (2)
1.0×104 π‘Ž⁄
1 (
5730 π‘Ž)
2
𝑁 = (800.0 πœ‡π‘”) ( )
𝑁 = 238.6 πœ‡π‘”
𝑁 = 240 πœ‡π‘”
SPH3U1 - Energy Problems Set
5. Uranium-238 has a half-life of 4.468x109 a. A sample of uranium ore currently has 722 mg of uranium238. If the sample is 5.9x108 a, how much uranium-238 was there when it formed?
1
𝑑⁄
𝑇1/2
𝑁 = 𝑁0 (2)
𝑁0 =
𝑁0 =
𝑁0 = 791.20 π‘šπ‘”
𝑁
𝑁0 = 790 π‘šπ‘”
𝑑
1 ⁄𝑇
( ) 1/2
2
722 π‘šπ‘”
5.9×108 π‘Ž⁄
)
1 (
4.468×109 π‘Ž
( )
2
6. Iodine 131
53𝐼 is used in diagnostic and therapeutic techniques in the treatment of thyroid disorders. This
isotope has a half-life of 8.04 days. What percentage of an initial sample of 131
53𝐼 remains after 30.0 days?
1
𝑑⁄
𝑇1/2
𝑁
𝑁0
𝑁 = 𝑁0 (2)
𝑁
𝑁0
𝑁
𝑁0
1
𝑑⁄
𝑇1/2
= (2)
=
1 (
(2)
= 0.07529
% π‘Ÿπ‘’π‘šπ‘Žπ‘–π‘›π‘–π‘›π‘” = 7.529 % = 7.53 %
30.0 π‘‘π‘Žπ‘¦π‘ 
⁄8.04 π‘‘π‘Žπ‘¦π‘ )
7. To make the dial of a watch glow in the dark, 1.000 ×10-9 kg of radium 226
88π‘…π‘Ž is used. The half-life of this
isotope has a value of 1.60 ×103 yr. How many kilograms of radium disappear while the watch is in use
for fifty years?
1
2
𝑑⁄
𝑇1/2
𝑁 = 𝑁0 ( )
50 π‘Ž⁄
)
1 (
1.60×103 π‘Ž
𝑁 = (1.000 × 10−9 π‘˜π‘”) (2)
𝑁 = 9.7857 × 10−10 π‘˜π‘”
π‘…π‘Žπ‘‘π‘–π‘ π‘Žπ‘π‘π‘’π‘Žπ‘Ÿπ‘’π‘‘ = 1.000 × 10−9 π‘˜π‘” − 9.7857 × 10−10 π‘˜π‘”
π‘…π‘Žπ‘‘π‘–π‘ π‘Žπ‘π‘π‘’π‘Žπ‘Ÿπ‘’π‘‘ = 2.14 × 10−11 π‘˜π‘”
8. The shroud of Turin is a religious artefact known since the Middle Ages. In 1988 its age was measured
using the radiocarbon dating technique, which revealed that the shroud could not have been made
before 1200 AD. Of the 146𝐢 nuclei that were present in the living matter from which the shroud was
made, what percentage remained in 1988?
1
𝑑⁄
𝑇1/2
𝑁 = 𝑁0 (2)
1
𝑑⁄
𝑇1/2
𝑁
𝑁0
= (2)
𝑁
𝑁0
= (2)
𝑁
𝑁0
= 0.9080
1988 π‘Ž−1200 π‘Ž⁄
1 (
5730 π‘Ž)
% π‘Ÿπ‘’π‘šπ‘Žπ‘–π‘›π‘–π‘›π‘” = 90.80 % = 91 %
SPH3U1 - Energy Problems Set
Nuclear Fission
9. During a nuclear reaction, an unknown particle is absorbed by a copper 63
29𝐢𝑒 nucleus, and the reaction
products are 62
𝐢𝑒
,
a
neutron,
and
a
proton.
Determine
the
unknown
particle
and the nucleus
29
63
temporarily formed when the copper 29𝐢𝑒 nucleus absorbs the unknown particle.
63
29𝐢𝑒
??
+ ??
??? ? → ??? ? →
62
29𝐢𝑒
63
29𝐢𝑒
+ 11𝑝+ →
→
64
30𝑍𝑛
+ 10𝑛 + 11𝑝+
62
29𝐢𝑒
+ 10𝑛 + 11𝑝+
10. A neutron causes 232
90π‘‡β„Ž to fission according to the reaction
232
1
𝐴
0
90π‘‡β„Ž + 0𝑛 → 𝑍𝑋 + 0𝛾
a. Identify the unknown nucleus , giving its atomic mass number A, its atomic
number Z, and the symbol X for the element.
232
1
233
0
90π‘‡β„Ž + 0𝑛 → 90π‘‡β„Ž + 0𝛾
b. Nucleus X then undergoes β- decay, and its daughter does too. Identify the final nucleus, giving
its atomic mass number, atomic number, and name.
233
233
0
90π‘‡β„Ž → 91π‘ƒπ‘Ž + −1𝛽
233
91π‘ƒπ‘Ž
→
233
92π‘ˆ
+ −10𝛽
11. A small sample of coal, when completely converted to energy, releases 4.5 × 1014 J of energy. Determine
the original mass of coal, assuming the final mass is zero.
𝐸 = βˆ†π‘šπ‘ 2
π‘š = 5.0068 × 10−3 π‘˜π‘”
𝐸
π‘š2 − π‘š1 = 𝑐 2
π‘š = 5.0 𝑔
4.5×1014
π‘š = (2.998×108
𝐽
π‘š/𝑠)2
12. Calculate the mass defect, in kilograms, and the energy released, in joules, of the following nuclear
reaction:
140
235
1
93
1
92π‘ˆ + 0𝑛 → 55𝐢𝑠 + 37𝑅𝑏 + 3 0𝑛
93
= 235.044 𝑒, 10𝑛 = 1.009 𝑒, 140
55𝐢𝑠 = 139.909 𝑒, 37𝑅𝑏 = 92.922 𝑒
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = π‘šπΆπ‘  + π‘šπ‘…π‘ + 3π‘šπ‘› − (π‘šπ‘ˆ + π‘šπ‘› )
βˆ†π‘š = 139.909 𝑒 + 92.922 𝑒 + 3(1.009 𝑒) − (235.044 𝑒 + 1.009 𝑒)
βˆ†π‘š = −0.195 𝑒
βˆ†π‘š = 0.195 𝑒 𝑙𝑒𝑠𝑠
235
92π‘ˆ
𝐸
𝐸
𝐸
𝐸
= βˆ†π‘šπ‘ 2
= (0.195 𝑒)(1.660538782 × 10−27 π‘˜π‘”/𝑒)(2.998 × 108 π‘š/𝑠)2
= 2.91036 × 10−11 𝐽
= 2.91 × 10−11 𝐽
SPH3U1 - Energy Problems Set
13. How much energy, in MeV, is released by the following fission reaction?
235
92π‘ˆ
235
92π‘ˆ
= 235.044 𝑒, 10𝑛 = 1.009 𝑒,
96
38π‘†π‘Ÿ
+ 10𝑛 →
94
38π‘†π‘Ÿ
1
+ 140
54𝑋𝑒 + 2 0𝑛
= 93.915 𝑒,
140
54𝑋𝑒
= 139.922 𝑒
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = π‘šπ‘†π‘Ÿ + π‘šπ‘‹π‘’ + 2π‘šπ‘› − (π‘šπ‘ˆ + π‘šπ‘› )
βˆ†π‘š = 93.915 𝑒 + 139.922 𝑒 + 2(1.009 𝑒) − (235.044 𝑒 + 1.009 𝑒)
βˆ†π‘š = −0.198 𝑒
βˆ†π‘š = 0.198 𝑒 𝑙𝑒𝑠𝑠
𝐸
𝐸
𝐸
𝐸
= βˆ†π‘šπ‘ 2
= (0.198 𝑒)(930 𝑀𝑒𝑉/𝑒)
= 184.14 𝑀𝑒𝑉
= 184 𝑀𝑒𝑉
2
14. The energy released during each 235
92π‘ˆ fission is 2.0 × 10 MeV. How many kilograms of coal must be
7
burned to produce the same energy as 1.0 kg of 235
92π‘ˆ if 3.0 × 10 J of energy is released when 1.0 kg of
24
coal is burned?
(n.b. 2.6 x10 U nuclei are found in a 1 kg sample of uranium)
π‘›π‘ˆ 𝑛𝑒𝑐𝑙𝑒𝑖
π‘›π‘ˆ 𝑛𝑒𝑐𝑙𝑒𝑖
π‘›π‘ˆ 𝑛𝑒𝑐𝑙𝑒𝑖
π‘›π‘ˆ 𝑛𝑒𝑐𝑙𝑒𝑖
= (π‘šπ‘Žπ‘ π‘  π‘œπ‘“ π‘ˆ235 ) ÷ (π‘šπ‘œπ‘™π‘Žπ‘Ÿ π‘šπ‘Žπ‘ π‘  π‘œπ‘“ π‘ˆ235 ) × (6.02 × 1023 π‘Žπ‘‘π‘œπ‘šπ‘ /π‘šπ‘œπ‘™)
= (1.0 π‘˜π‘”) ÷ (0.235 π‘˜π‘”/π‘šπ‘œπ‘™) × (6.02 × 1023 π‘Žπ‘‘π‘œπ‘šπ‘ /π‘šπ‘œπ‘™)
= 2.56170 × 1024
= 2.6 × 1024
𝐸 = (π‘›π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘  )(πΈπ‘›π‘’π‘Ÿπ‘”π‘¦/π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›)
𝐸 = (2.6 × 1024 )(2.0 × 102 𝑀𝑒𝑉)(1.602 × 10−13 𝐽/𝑀𝑒𝑉)
𝐸 = 8.3304 × 1013 𝐽
πΈπ‘›π‘’π‘Ÿπ‘”π‘¦ π‘Ÿπ‘’π‘žπ‘’π‘–π‘Ÿπ‘’π‘‘
π‘’π‘›π‘˜π‘›π‘œπ‘€π‘› π‘šπ‘Žπ‘ π‘ π‘π‘œπ‘Žπ‘™
πΈπ‘›π‘’π‘Ÿπ‘”π‘¦
= 1.0 π‘˜π‘”
π‘’π‘›π‘˜π‘›π‘œπ‘€π‘› π‘šπ‘Žπ‘ π‘ π‘π‘œπ‘Žπ‘™
π‘’π‘›π‘˜π‘›π‘œπ‘€π‘› π‘šπ‘Žπ‘ π‘ π‘π‘œπ‘Žπ‘™
π‘’π‘›π‘˜π‘›π‘œπ‘€π‘› π‘šπ‘Žπ‘ π‘ π‘π‘œπ‘Žπ‘™
π‘’π‘›π‘˜π‘›π‘œπ‘€π‘› π‘šπ‘Žπ‘ π‘ π‘π‘œπ‘Žπ‘™
π‘π‘œπ‘Žπ‘™
= (πΈπ‘›π‘’π‘Ÿπ‘”π‘¦ π‘Ÿπ‘’π‘žπ‘’π‘–π‘Ÿπ‘’π‘‘)/(πΈπ‘›π‘’π‘Ÿπ‘”π‘¦/π‘˜π‘”)
= (8.3304 × 1013 𝐽)/(3.0 × 107 𝐽/π‘˜π‘”)
= 2776800 π‘˜π‘”
= 2.8 × 106 π‘˜π‘”
SPH3U1 - Energy Problems Set
Nuclear Fusion
15. One reaction to produce carbon in stars is as follows:
4
4
4
12
2𝐻𝑒 + 2𝐻𝑒 + 2𝐻𝑒 → 6𝐢
Calculate the mass defect, in atomic mass units, and energy released, in electronvolts, of this reaction.
12
( 42𝐻𝑒 m=4.002603 u,
6𝐢 m = 12.00000 u)
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = π‘šπΆ − 3(π‘šπ»π‘’ )
βˆ†π‘š = 12.00000 𝑒 − 3(4.002603 𝑒)
βˆ†π‘š = −7.809 × 10−3 𝑒
βˆ†π‘š = 7.8 × 10−3 𝑒 𝑙𝑒𝑠𝑠
𝐸
𝐸
𝐸
𝐸
= βˆ†π‘šπ‘ 2
= (7.8 × 10−3 𝑒 )(930 𝑀𝑒𝑉/𝑒)
= 7.254 × 106 𝑒𝑉
= 7.3 × 106 𝑒𝑉
16. Consider the induced nuclear reaction 21𝐻 + 147𝑁 → 126𝐢 + 42𝐻𝑒 . The atomic masses are 21𝐻 (2.014 102
u), 147𝑁 (14.003 074 u), 126𝐢 (12.000 000 u), and 42𝐻𝑒 (4.002 603 u). Determine the energy released, in
joules, when the 126𝐢 and 42𝐻𝑒 nuclei are formed in this way.
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = π‘šπΆ + π‘šπ»π‘’ − (π‘šπ‘ + π‘šπ» )
βˆ†π‘š = 12.00000 𝑒 + 4.002 603 𝑒 − (14.003 074 𝑒 + 2.014 102 𝑒)
βˆ†π‘š = −0.014573 𝑒
𝐸
𝐸
𝐸
𝐸
= βˆ†π‘šπ‘ 2
= (0.014573 𝑒 )(930 𝑀𝑒𝑉/𝑒)(1.602 × 10−13 𝐽/𝑀𝑒𝑉)
= 2.17117 × 10−12 𝐽
= 2.2 × 10−12 𝐽
17. Two deuterium atoms ( 21𝐻= 2.014102 u) react to produce tritium
( 31𝐻= 3.016050 u) and hydrogen ( 11𝐻= 1.007825 u) according to the reaction:
2
2
3
1
1𝐻 + 1𝐻 → 1 𝐻 + 1𝐻
What is the energy released by this deuterium-deuterium reaction?
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = π‘šπ»−3 + π‘šπ» − 2(π‘šπ»−2 )
βˆ†π‘š = 3.016050 𝑒 + 1.007825 𝑒 − 2(2.014102 𝑒)
βˆ†π‘š = −4.329 × 10−3 𝑒
𝐸
𝐸
𝐸
𝐸
𝐸
= βˆ†π‘šπ‘ 2
= (4.329 × 10−3 𝑒 )(930 𝑀𝑒𝑉/𝑒)
= 4.02597 𝑀𝑒𝑉
= 4.0 𝑀𝑒𝑉
= 6.4 × 10−3 𝐽
SPH3U1 - Energy Problems Set
18. One proposed fusion reaction combines lithium 63𝐿𝑖 (6.015 u) with deuterium 21𝐻 (2.014 u) to give helium
4
2𝐻𝑒 (4.003 u):
2
1𝐻
+ 63𝐿𝑖 → 2 42𝐻𝑒
a) How many of the above reactions would need to occur to supply the energy needs of one household
for a year (estimated to be 3.8 × 1010 J)?
βˆ†π‘š = π‘šπ‘π‘Ÿπ‘œπ‘‘π‘’π‘π‘‘π‘  − π‘šπ‘Ÿπ‘’π‘Žπ‘π‘‘π‘Žπ‘›π‘‘π‘ 
βˆ†π‘š = 2π‘šπ»π‘’ − (π‘šπΏπ‘– + π‘šπ»−2 )
βˆ†π‘š = 2(4.003 𝑒) − (6.015 𝑒 + 2.014 𝑒)
βˆ†π‘š = −0.023 𝑒
𝐸 = βˆ†π‘šπ‘ 2
𝐸 = (0.023 𝑒)(930 𝑀𝑒𝑉/𝑒)(1.602 × 10−13 𝐽/𝑀𝑒𝑉)
𝐸 = 3.426678 × 10−12 𝐽
π‘›π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘  =
π‘›π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘  =
π‘‘π‘œπ‘‘π‘Žπ‘™ π‘’π‘›π‘’π‘Ÿπ‘”π‘¦
π‘’π‘›π‘’π‘Ÿπ‘”π‘¦ π‘π‘’π‘Ÿ π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›
3.8×1010 𝐽
3.426678×10−12 𝐽/π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›
22
π‘›π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘  = 1.10895 × 10 π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘ 
π‘›π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘  = 1.1 × 1022 π‘Ÿπ‘’π‘Žπ‘π‘‘π‘–π‘œπ‘›π‘ 
b) How many grams of lithium would be needed if there are 8.673x1025 Li nuclei in 1 kg of a lithium
sample?
π‘₯ π‘˜π‘”
1 π‘˜π‘”
=
1.1×1022 𝑛𝑒𝑐𝑙𝑒𝑖
8.673×1025 𝑛𝑒𝑐𝑙𝑒𝑖
(1 π‘˜π‘”)(1.1×1022 𝑛𝑒𝑐𝑙𝑒𝑖)
π‘₯=
8.673×1025 𝑛𝑒𝑐𝑙𝑒𝑖
−4
π‘₯ = 1.268304 × 10
π‘šπ‘Žπ‘ π‘ πΏπ‘– = 0.13 𝑔
π‘˜π‘”
19. The following shows the carbon-nitrogen-oxygen (CNO) cycle that occurs inside stars. Write a nuclear
reaction equation for each stage in the cycle and identify its type.
12
13
13
14
15
15
12
4
6𝐢 → 7𝑁 → 6𝐢 → 7𝑁 → 8𝑂 → 7𝑁 → 6𝐢 + 2𝐻𝑒
12
1
13
nuclear fusion ( + gamma particle released)
6𝐢 + 1𝐻 → 7𝑁
13
7𝑁
→
13
6𝐢
13
6𝐢
+ 11𝐻 →
14
7𝑁
nuclear fusion ( + gamma particle released)
14
7𝑁
+ 11𝐻 →
15
8𝑂
nuclear fusion ( + gamma particle released)
15
8𝑂
→
15
7𝑁
+ 11𝐻 →
15
7𝑁
+ 01𝛽
beta+ decay
+ + 01𝛽
12
6𝐢
+ 42𝐻𝑒
beta+ decay
nuclear fusion ( + alpha particle released)
SPH3U1 - Energy Problems Set
Conceptual Questions
1. To which of the following objects, each about 1000 yr old, can the radiocarbon dating technique not be
applied: a wooden box, a gold statue, and some plant seeds? Explain.
Wooden box and plant seeds. Both of these objects contain carbon, so can be used for radiocarbon
dating, whereas a gold statue does not.
2. Some preserved seed were found and their age, through the technique of carbon dating, was determined
to be 5000 years old. However, new evidence suggests that the amount of carbon in the air at that time
is higher than previously thought. Are the seeds older or younger than 5000 years? Explain.
Older. If there were more C-14 in the beginning but that same amount currently, this would mean that
the seeds have lost more C-14 than previously thought. In order to do so, they must have existed for a
longer amount of time, so are older than 5000 years.
3. Compare and contrast nuclear fission and fusion. How are they alike? How are they different?
Fission and fusion are similar because both processes result in more stable nuclei. They both achieve
this by releasing energy which can be used as a power source. They differ in that a large nucleus
breaks into smaller fragments when undergoing fission and smaller nuclei combine to make a larger
one when undergoing fusion. Fusion also, in general, releases more energy per reaction than fission.
4. Why are neutrons such good projectiles for producing nuclear reactions?
Neutrons are good projectiles for producing nuclear reactions because they are neutral and they are
massive. If you want a particle to hit the nucleus with a lot of energy, a more massive particle is the
better choice. A light electron would not be as effective. Using a positively charged projectile like an
alpha or a proton means that the projectile will have to overcome the large electrical repulsion from
the positively charged nucleus. Neutrons can penetrate directly to the nucleus and cause nuclear
reactions.
5. Explain why nuclear fusion is much more difficult to obtain than nuclear fission
To fuse two nuclei together they must have enough energy (travelling fast enough) to overcome their
mutual repulsion. To break apart a large nucleus, a neutron with relatively low energy can be used to
strike and destabilize it as the neutron has no charge and is not repelled.
6. Why is nuclear fusion more desirable than nuclear fission for power generation? Explain.
Fusion releases more energy per reaction than does fission, and so it is more efficient. Also, the
products of fusion are stable nuclei, and have minimal environmental impact, whereas fission
products are radioactive (and can be for thousands of years) and so storing them pose serious
environmental (and technological) challenges.
7. The energy from nuclear fission appears in the form of thermal energy – but the thermal energy of what?
Explain.
The thermal energy from nuclear fission appears in the kinetic energy of the fission products (daughter
nuclei and neutrons). In other words, the fission products are moving very fast (especially the
neutrons).
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