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Revision: Atoms and Nuclei CUET (UG) Atoms and Nuclei

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Definitions [11]

Definition: Isotopes

The atoms of the same element, having same atomic number Z, but different mass number A, are called isotopes.

OR

Atoms having the same atomic number (Z) but different mass numbers (A).

Definition: Radioactivity

Radioactivity is a nuclear phenomenon. It is the process of spontaneous emission of α or β and γ radiations from the nucleus of atoms during their decay.

Define bound electrons.

As nucleus is positively charged it strongly attracts the negative charged electrons. The electron orbit close to the nucleus are tightly bound by strong attractive force of nucleus. These electrons are known as bound electrons.

Define the term radioactivity.

The phenomenon of spontaneous disintegration of an unstable nucleus of a naturally occurring isotope accompanied by emission of active radiations, α particles, β particles and γ radiations is called radioactivity.

Define free electrons.

Electrons in outer orbits are weakly bound with the nucleus. In solids these weakly bound electrons leave their individual atom and become a part of it. These electrons are known as free electrons.

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.

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.

Define unified atomic mass unit.

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

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`

Definition: Nuclear Energy

The energy released due to loss in mass during the processes of nuclear fission and fusion is called nuclear (or atomic) energy.

OR

The energy released when nuclei undergo a nuclear reaction (change in structure, forming new nuclei) is called nuclear energy.

Definition: Nuclear Fission

Nuclear fission is the process in which a heavy nucleus splits into two lighter nuclei of nearly the same size, when bombarded with slow neutrons. In each fission reaction, a tremendous amount of energy (≈ 190 MeV) is released.

Key Points

Key Points: Nuclear Fission
  • In nuclear fission of U‑235, a slow neutron is absorbed to form unstable U‑236, which splits into two nuclei with the release of three neutrons and energy.
  • Energy released in fission is due to loss of mass, and is given by Einstein’s mass‑energy relation, E = (Δm)c2.
  • In each fission reaction, atomic number (Z) and mass number (A) remain conserved, though mass is converted into energy.
  • Fission of one U‑235 nucleus releases nearly 190 MeV energy, mainly as kinetic energy of fragments, neutrons, γ‑rays, heat, and light.
 
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