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Revision: Modern Physics >> Radioactivity Physics (English Medium) ICSE Class 10 CISCE

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Definitions [17]

Definition: Atomic Number

The atomic number of an atom is equal to the number of protons in its nucleus (which is same as the number of electrons in a neutral atom).

Definition: Mass Number

The mass number of an atom is equal to the total number of nucleons (i.e., the sum of the number of protons and the number of neutrons) in its nucleus.

Define the term mass number.

The total number of neutrons and protons in the nucleus is called the mass number of the element and is denoted by A.

Define the term atomic number.

The number of protons in the nucleus is known as the atomic number of the element and is denoted by Z.

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: Isobars

The atoms of different elements which have the same mass number A, but different atomic number Z, are called isobars.

Definition: Isotones

The atoms having different number of protons but same number of neutrons i.e., different Z and A, but same (A-Z), are called isotones. They have different number of electrons.

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 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.

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.

Definition: Gamma (γ) Radiations

Gamma (γ) radiations are the radiations which are uncharged (neutral) and pass undeviated in both magnetic and electric fields, and are electromagnetic waves similar to light waves.

Definition: Beta (β) Radiations

Beta (β) radiations are the radiations which are negatively charged and turn to the right in a magnetic field or towards the positive plate in an electric field, and are deviated more than alpha particles.

Definition: Alpha (α) Radiations

Alpha (α) radiations are the radiations which are positively charged and turn to the left in a magnetic field or towards the negative plate in an electric field.

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.

Definition: Nuclear Fusion

Nuclear fusion is the process in which two light nuclei combine to form a heavy nucleus. In this process also, huge amount of energy is released.

Key Points

Key Points: Structure of the Atom and Nucleus
  • The structure of an atom and its nucleus was developed from the discovery of electrons by J.J. Thomson and alpha particle scattering experiments by Rutherford.
  • An atom consists of electrons, protons, and neutrons, with protons and neutrons in the nucleus and electrons revolving in stationary orbits.
  • The maximum number of electrons in a shell is given by 2n², and the shells are named K, L, M, N, O, P, and Q.
Key Points: Properties of Alpha Particles
  • Alpha particles strongly ionise the gas through which they pass, and their ionising power is about 100 times that of beta particles.
  • Alpha particles have very small penetrating power, as they can penetrate only 3 to 8 cm in air and are stopped by a thin card sheet or thick paper.
  • Alpha particles are deflected by electric and magnetic fields, but their deflection is less than that of beta particles due to their larger mass.
  • Alpha particles affect a photographic plate and cause fluorescence on striking a fluorescent material.
 
Key Points: Properties of Beta Particles
  • The speed of beta particles is of the order of 10⁸ m s⁻¹, but always less than 3 × 10⁸ m s⁻¹.
  • The penetrating power of beta particles is more than that of alpha particles but less than that of gamma radiation.
  • Beta particles are negatively charged and get deflected in electric and magnetic fields more than alpha particles.
  • Beta particles produce X-rays when stopped by metals of high atomic number and high melting point.
  • Beta particles cause more biological damage than alpha particles as they can easily pass through the skin.
Key Points: Properties of Gamma Radiations
  • The speed of γ‑radiations is the same as the speed of light, i.e., 3 × 10⁸ m s⁻¹ in vacuum or air.
  • The ionising power of γ‑radiations is very low, being 1/10,000 times that of α‑particles.
  • The penetrating power of γ‑radiations is very high, and they can pass through thick sheets of lead or iron.
  • Gamma radiations are not deflected by electric and magnetic fields, as it is not a charged particle.
  • Gamma radiation can easily pass through the human body; therefore, it causes immense biological damage.
 
Key Points: Changes Within the Nucleus in Alpha, Beta and Gamma Emission
  • In alpha emission, the atomic number (Z) decreases by 2, and the mass number (A) decreases by 4.
  • In beta emission, the atomic number (Z) increases by 1 and the mass number (A) remains unchanged.
  • In gamma emission, there is no change in atomic number (Z) and mass number (A); only the energy of the nucleus changes.
  • Beta emission is often followed by the emission of an antineutrino (ν̅) to conserve energy and momentum.
  • The daughter nucleus may still be radioactive and can undergo further α or β emission until a stable nucleus is formed.
Key Points: Sources of Harmful Radiations
  • Radioactive fallout from nuclear power plants can release harmful radiation into the atmosphere during accidents, affecting distant areas.
  • Nuclear waste from rejected fuel rods remains highly radioactive and can contaminate water and soil if not properly managed.
  • Cosmic radiation and X-rays are other sources of harmful radiation, as some uncharged radiation, such as γ-rays, reaches Earth's atmosphere.
Key Points: Background Radiations
  • The internal source - the radioactive substances such as potassium (K-40), carbon (C-14), and radium present inside
    our body.
  • External source - cosmic rays, naturally occurring radioactive elements such as radon-222, and solar radiation.
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.
 

Important Questions [38]

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