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Revision: Atoms and Nuclei >> Nuclei Physics Science (English Medium) Class 12 CBSE

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Definitions [21]

Define binding energy per nucleon.

Binding energy per nucleon is the least amount of energy required to liberate all of the nucleons from the nucleus.

As a result, the binding energy per nucleon is
`E_B/A`

Define unified atomic mass unit.

`1/12`th of the mass of an atom of 6C12 isotope.

With reference to Nuclear Physics, answer the following question.

Define lu (where u stands for unified atomic mass unit).

1 AMU is the average of proton rest mass and the neutron rest mass. Thus can be expressed as

1 AMU = 1.67377 × 10-27 kg

= 1.67377 × 10-24 gram

and C-12 is considered a reference for all atomic mass calculations.

Definition: Nuclear Force

Nuclear force is the strong attractive force of a totally different kind which binds protons and neutrons in the nucleus and overcomes the Coulomb repulsion between protons.

Definition: Nuclear Fusion

Nuclear fusion is the process in which two or more light nuclei combine to form a heavier nucleus, accompanied by the release of a large amount of energy.

Definition: Radioactivity

 Radioactivity is the phenomenon in which nuclei of a given species transform by giving out α, β, or γ rays.

α-rays are helium nuclei; β-rays are electrons. γ-rays are electromagnetic radiation of wavelengths shorter than X-rays.

Definition: Radioactive Decay

The process by which an unstable nucleus transforms into another nucleus by emitting radiation is called radioactive decay.

Definition: Nuclear Fission

Nuclear fission is the process in which a heavy nucleus splits into two or more lighter nuclei of nearly equal mass, accompanied by the release of a large amount of energy and neutrons.

Definition: Mass Defect (ΔM)

The difference between the sum of masses of individual nucleons and the actual mass of the nucleus.

\[\Delta M=[Zm_p+(A-Z)m_n]-M\]

Definition: Binding Energy per Nucleon

The average energy required to remove one nucleon from the nucleus.

\[E_{bn}=\frac{E_b}{A}\]

Definition: Controlled Thermonuclear Fusion

Controlled thermonuclear fusion is the process in which steady power is generated by heating nuclear fuel to very high temperatures so that fusion reactions occur in a controlled manner.

Definition: Atomic Mass Unit

Atomic mass unit (u), defined as `1/12`th of the mass of the carbon (12C) atom. According to this definition, 

\[1\mathrm{u}=\frac{\text{mass of one }^{12}\mathrm{C~atom}}{12}\]

\[=\frac{1.992647\times10^{-26}\mathrm{kg}}{12}\]

\[=1.660539\times10^{-27}\mathrm{kg}\]

Definition: Atomic Number (Z)

Atomic number (Z) is defined as the number of protons present in the nucleus of an atom.

Definition: Neutron Number (N)

Neutron number (N) is defined as the number of neutrons present in the nucleus of an atom.

N = number of neutrons

Definition: Mass Number (A)

Mass number (A) is defined as the total number of nucleons (protons and neutrons) present in the nucleus of an atom.

A = Z + N

Definition: Isotopes

Isotopes are atoms of the same element having the same atomic number (Z) but different mass numbers (A) or different neutron numbers (N).

Definition: Isobars

Isobars are atoms of different elements having the same mass number (A) but different atomic numbers (Z).

Definition: Isotones

Isotones are atoms of different elements having the same neutron number (N) but different atomic numbers (Z).

Definition: Nuclear Radius

The nuclear radius is the distance from the centre of the nucleus to its surface.

Definition: Binding Energy (Eb)

The energy required to separate a nucleus completely into its individual nucleons.

\[E_b=\Delta Mc^2\]

Define one Becquerel.

One Becquerel (Bq) is defined as the activity of a quantity of radioactive samples in which one nucleus decays per second. It is the SI unit of the activity.

Formulae [3]

Formula: Nuclear Radius

\[R=R_0A^{1/3}\]

Where:

R0 = 1.2 × 10−15 m = 1.2 

Formula: Mass–Energy Equivalence (Einstein)

\[E=mc^2\]

Where:

  • E = energy

  • m = mass

  • c = 3 × 108 m/s

Formula: Q-Value

 The Q-value of a nuclear process is

Q = final kinetic energy – initial kinetic energy.

Due to conservation of mass-energy, this is also,

Q = (sum of initial masses – sum of final masses)c2

Key Points

Key Points: Properties of Nuclear Force
Property Key Point
Very Strong Stronger than Coulomb & gravitational forces
Short Range Effective only up to a few femtometres (fm)
Saturation Acts only on nearby nucleons
Charge Independent Same for p–p, n–n, p–n
Nature Attractive (>0.8 fm), repulsive (<0.8 fm)

Important Questions [61]

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