The binding energy per nucleon of deuterium and helium atom is 1.1 MeV and 7.0 MeV. If two deuterium nuclei fuse to form a helium atom, the energy released is:

1. 19.2 MeV

2. 23.6 MeV

3. 26.9 MeV 

4. 13.9 MeV

Subtopic:  Nuclear Binding Energy |
 76%
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PMT - 2001
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In a fission reaction,

\(^{236}_{92}U\rightarrow ~^{117}X~+~^{117}Y~+~^1_0n~+~^1_0n,\) the binding energy per nucleon of X and Y is 8.5 MeV whereas that of \(^{236}U\) is 7.6 MeV. The total energy liberated will be about:

1. 2000 MeV

2. 200 MeV

3. 2 MeV 

4. 1 keV

Subtopic:  Nuclear Binding Energy |
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A nuclear decay is expressed as 

C116B115+β++X

Then the unknown particle X is:

1. Neutron 

2. antineutrino

3. proton 

4. neutrino

Subtopic:  Types of Decay |
 60%
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When a deuterium is bombarded on O168 nucleus, an α-particle is emitted, then the product nucleus is:

1. N137 

2. B105

3. B4e9 

4. N147

Subtopic:  Types of Decay |
 76%
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A nuclear reaction given by \({ }_{Z}^{A} \mathrm{~X} \rightarrow{ }_{Z+1}^{A} \mathrm{Y}+e^{-}+\bar{v}\) represents:
1. fusion
2. fission
3. \(\beta^{-} \text-\)decay
4. \(\gamma \)-decay

Subtopic:  Types of Decay |
 88%
From NCERT
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The mass of N157 is 15.00011 amu, mass of O168 is 15.99492 amu and mp= 1.00783 amu. Determine the binding energy of the last proton of \({ }_8 O_{16}\).

1. 2.13 MeV

2. 0.13 MeV 

3. 10 MeV 

4. 12.13 MeV

Subtopic:  Nuclear Binding Energy |
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The rate of disintegration of a fixed quantity of a radioactive substance can be increased by:

1. increasing the temperature.

2. increasing the pressure.

3. chemical reaction.

4. it is not possible.

Subtopic:  Radioactivity (OLD NCERT) |
 54%
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The energy released by the fission of one  uranium atom is 200 MeV. The number of fission per second required to produce 3.2 W of power is (Take, 1 eV = 1.6×10-19 J) [WB JEE 2010]

1. 107 

2. 1010 

3. 1015

4. 1011

Subtopic:  Nuclear Binding Energy |
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The power obtained in a reactor using U235 disintegration is 1000 kW. The mass decay of \(U^{235}\) per hour is:

1. 1 microgram           

2. 10 microgram       

3. 20 microgram     

4. 40 microgram

Subtopic:  Nuclear Energy |
From NCERT
PMT - 2011
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Light energy emitted by stars is due to

1. Breaking of nuclei 

2.Joining of nuclei       

3. Burning of nuclei

4. Reflection of solar light

Subtopic:  Mass-Energy Equivalent |
 62%
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