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Nuclear fusion – Energy Generation in Stars
Nuclear fusion – Energy Generation in Stars
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Nuclear Fusion (Phy)
Example
Definitions
Formulaes
Controlled Thermonuclear Fusion
Example
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Nuclear Holocaust
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Thermonuclear Fusion
13 mins
Nuclear Reactions taking place in Sun and Nuclear Fusion
5 mins
Nuclear fusion reactions and its examples
6 mins
Quick Summary With Stories
Nuclear fission reaction
2 mins read
Nuclear fusion reactions and its examples
2 mins read
Thermonuclear Fusion
3 mins read
Controlled Thermonuclear Fusion
3 mins read
Nuclear Holocaust
3 mins read
Important Questions
The fission properties of
9
4
2
3
9
P
u
are very similar to those of
9
2
2
3
5
U
. The average energy released per fission is 180 MeV. How much energy, in MeV, is released if all the atoms in 1 kg of pure
9
4
2
3
9
P
u
undergo fission?
Medium
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>
The necessary condition for nuclear fusion is
Medium
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>
Why high temperature is required for Nuclear fusion ?
Easy
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>
Fusion reaction takes place at very high temperature because
Easy
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>
For a nuclear fusion process, suitable nuclei are
Medium
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>
What were ghettos?
Medium
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Which of the following statement best describe Nuclear fusion reaction ?
Easy
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>
Fusion processes, like combining two deuterons to form a
H
e
nucleus are impossible at ordinary temperatures and pressure. The reasons for this can be traced to the fact:
This question has multiple correct options
Medium
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>
The equation,
4
1
H
1
→
[
2
H
e
4
]
2
+
+
2
e
−
;
+
2
6
M
e
V
represents :
Medium
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>
What is the source of energy in sun and stars ?
Easy
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>