Nuclear Energy
PHXII13:NUCLEI

363768 The explosive in a Hydrogen bomb is a mixture of \(_1{H^2},\,{\,_1}{H^3}\) and \({ }_{3} L i^{6}\) in some condensed form.
The chain reaction is given by
\({ }_{3} L i^{6}+{ }_{0} n^{1} \rightarrow{ }_{2} H e^{4}+{ }_{1} H^{3}\)
\({ }_{1} H^{2}+{ }_{1} H^{3} \rightarrow{ }_{2} H e^{4}+{ }_{0} n^{1}\). During the explosion the energy released is approximately
[Given : \(M\left( {Li} \right) = 6.01690\,amu,\)
\(M\left( {_1{H^2}} \right) = 2.01471\,amu,\)
\(M\left( {_2H{e^4}} \right) = 4.00388\,amu,\)
\({\rm{and}}\,\,\,\,1\,amu = 931.5\,MeV\)

1 \(28.12\,MeV\)
2 \(22.22\,MeV\)
3 \(12.64\,MeV\)
4 \(16.48\,MeV\)
PHXII13:NUCLEI

363769 The thermonuclear reaction of hydrogen inside the stars is taking place by a cycle of operations. The particular element which acts as a catalyst is

1 Nitrogen
2 Oxygen
3 Helium
4 Carbon
PHXII13:NUCLEI

363770 The equation \(4_1^1H \to _2^4He + 2e_{ - 1}^0 + 26MeV\) represents

1 \(\beta \)-decay
2 \(\gamma \)-decay
3 Fusion
4 Fission
PHXII13:NUCLEI

363771 As the age of star increases

1 Helium quantity increases
2 Helium quantity decreases
3 Helium quantity does not change
4 Helium, Hydrogen both quantities increase
PHXII13:NUCLEI

363768 The explosive in a Hydrogen bomb is a mixture of \(_1{H^2},\,{\,_1}{H^3}\) and \({ }_{3} L i^{6}\) in some condensed form.
The chain reaction is given by
\({ }_{3} L i^{6}+{ }_{0} n^{1} \rightarrow{ }_{2} H e^{4}+{ }_{1} H^{3}\)
\({ }_{1} H^{2}+{ }_{1} H^{3} \rightarrow{ }_{2} H e^{4}+{ }_{0} n^{1}\). During the explosion the energy released is approximately
[Given : \(M\left( {Li} \right) = 6.01690\,amu,\)
\(M\left( {_1{H^2}} \right) = 2.01471\,amu,\)
\(M\left( {_2H{e^4}} \right) = 4.00388\,amu,\)
\({\rm{and}}\,\,\,\,1\,amu = 931.5\,MeV\)

1 \(28.12\,MeV\)
2 \(22.22\,MeV\)
3 \(12.64\,MeV\)
4 \(16.48\,MeV\)
PHXII13:NUCLEI

363769 The thermonuclear reaction of hydrogen inside the stars is taking place by a cycle of operations. The particular element which acts as a catalyst is

1 Nitrogen
2 Oxygen
3 Helium
4 Carbon
PHXII13:NUCLEI

363770 The equation \(4_1^1H \to _2^4He + 2e_{ - 1}^0 + 26MeV\) represents

1 \(\beta \)-decay
2 \(\gamma \)-decay
3 Fusion
4 Fission
PHXII13:NUCLEI

363771 As the age of star increases

1 Helium quantity increases
2 Helium quantity decreases
3 Helium quantity does not change
4 Helium, Hydrogen both quantities increase
PHXII13:NUCLEI

363768 The explosive in a Hydrogen bomb is a mixture of \(_1{H^2},\,{\,_1}{H^3}\) and \({ }_{3} L i^{6}\) in some condensed form.
The chain reaction is given by
\({ }_{3} L i^{6}+{ }_{0} n^{1} \rightarrow{ }_{2} H e^{4}+{ }_{1} H^{3}\)
\({ }_{1} H^{2}+{ }_{1} H^{3} \rightarrow{ }_{2} H e^{4}+{ }_{0} n^{1}\). During the explosion the energy released is approximately
[Given : \(M\left( {Li} \right) = 6.01690\,amu,\)
\(M\left( {_1{H^2}} \right) = 2.01471\,amu,\)
\(M\left( {_2H{e^4}} \right) = 4.00388\,amu,\)
\({\rm{and}}\,\,\,\,1\,amu = 931.5\,MeV\)

1 \(28.12\,MeV\)
2 \(22.22\,MeV\)
3 \(12.64\,MeV\)
4 \(16.48\,MeV\)
PHXII13:NUCLEI

363769 The thermonuclear reaction of hydrogen inside the stars is taking place by a cycle of operations. The particular element which acts as a catalyst is

1 Nitrogen
2 Oxygen
3 Helium
4 Carbon
PHXII13:NUCLEI

363770 The equation \(4_1^1H \to _2^4He + 2e_{ - 1}^0 + 26MeV\) represents

1 \(\beta \)-decay
2 \(\gamma \)-decay
3 Fusion
4 Fission
PHXII13:NUCLEI

363771 As the age of star increases

1 Helium quantity increases
2 Helium quantity decreases
3 Helium quantity does not change
4 Helium, Hydrogen both quantities increase
PHXII13:NUCLEI

363768 The explosive in a Hydrogen bomb is a mixture of \(_1{H^2},\,{\,_1}{H^3}\) and \({ }_{3} L i^{6}\) in some condensed form.
The chain reaction is given by
\({ }_{3} L i^{6}+{ }_{0} n^{1} \rightarrow{ }_{2} H e^{4}+{ }_{1} H^{3}\)
\({ }_{1} H^{2}+{ }_{1} H^{3} \rightarrow{ }_{2} H e^{4}+{ }_{0} n^{1}\). During the explosion the energy released is approximately
[Given : \(M\left( {Li} \right) = 6.01690\,amu,\)
\(M\left( {_1{H^2}} \right) = 2.01471\,amu,\)
\(M\left( {_2H{e^4}} \right) = 4.00388\,amu,\)
\({\rm{and}}\,\,\,\,1\,amu = 931.5\,MeV\)

1 \(28.12\,MeV\)
2 \(22.22\,MeV\)
3 \(12.64\,MeV\)
4 \(16.48\,MeV\)
PHXII13:NUCLEI

363769 The thermonuclear reaction of hydrogen inside the stars is taking place by a cycle of operations. The particular element which acts as a catalyst is

1 Nitrogen
2 Oxygen
3 Helium
4 Carbon
PHXII13:NUCLEI

363770 The equation \(4_1^1H \to _2^4He + 2e_{ - 1}^0 + 26MeV\) represents

1 \(\beta \)-decay
2 \(\gamma \)-decay
3 Fusion
4 Fission
PHXII13:NUCLEI

363771 As the age of star increases

1 Helium quantity increases
2 Helium quantity decreases
3 Helium quantity does not change
4 Helium, Hydrogen both quantities increase
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