Physics MCQs for NEET — Practice Questions with Answers

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When a deuterium is bombarded on O168 nucleus, an α-particle is emitted, then the product nucleus is [2002]

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Explanation

Let the unknown product nucleus be XAZ

The reaction can be writted as

    O168  +   H21      XAz  +  H2e4(oxygen)  (deuterium) (unknown   α-particle                                  nucleus)

Conservartion of mass number between product and reactant of above reaction gives.

16 + 2 = A + 4 A = 14

Conservation of atomic number between reactant and product of above reaction gives

8 + 1 = Z + 2 Z = 7

Thus, the unknown product nucleus is nitrogen N147

Note:- Fusion reaction can take place at very high temperature (108 K) and very high pressure which can be provided at sun or by fission of atom bomb.

A nuclear reaction given by  XAzYAz+1+e0-1+ν¯ represents  [2003]

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Explanation

Since in the given reaction e0-1 and antineutrino ν¯ are released, so it can be considered β-decay.

The mass of N157 is 15.00011 amu, mass of O168 is 15.99492 amu and mp= 1.00783 amu. Determine binding energy of the last proton of O168

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Explanation

MN157+1 mp  MO168

binding energy of last proton

=M(N15)+mp-MO161×931.5 MeV=15.00011+1.00783-15.99492 ×931.5 MeV=0.01302 ×931.5 MeV=12.13 MeV

The rate of disintegration of a fixed quantity of a radioactive substance can be increased by

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Explanation

Radioactivity is a nuclear property and cannot be controlled by external factors.

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]

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Explanation

We have the energy released by fission of one uranium atom is 200 MeV.

So, E=200×106×1.6×10-19

           = 3.2×10-11 J

The power required = 3.2 W

Thus the number of fission required is equal to 3.23.2×10-11=1011 fissions.

The power obtained in a reactor using U235 disintegration is 1000 kW. The mass decay of U235 per hour is

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Explanation

E=mc21000×103×3600=m×3 ×1082

Light energy emitted by stars is due to

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Explanation

Nuclear fusion takes place in stars which results in joining of nuclei accompanied by release of tremendous amount of energy.

The constituents of atomic nuclei are believed to be [1991]

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Explanation

According to proton-neutron hypothesis, a nucleus of mass number A and atomic number Z contains Z protons and (A-Z) neutrons. Constituents of atomic nucleus are Nucleons i.e neutron and proton.

The half-life of radium is about 1600 yr. of 100 g of radium existing now, 25 g will remain unchanged after [2004]

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Explanation

Amount of substance remained is 

M=M012n[M=substance remained][M0=initial amount]

Given, M0= 100 g, M = 25 g,

Half life of radioactive substance T1/2=1600 yr

So, 25=10012nor 25100=12nor 122=12nComparing the power, we haven=2or tT1/2=2or t=2T1/2=2×1600=3200 yr

The binding energy of deuteron is 2.2 MeV and that of H24e is 28 MeV. If two deuterons are fused to form one H24e, then the energy released is [2006]

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Explanation

The reaction can be written as

H21+H21H2e4+energy

The energy released in the reaction is the difference of binding energies of daughter and parent nuclei. Hence, energy released 

= binding energy of H2e4-2×binding energy of H21

28-2×2.2=23.6 MeV

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