Radioactivity and Nuclear Reaction
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Radioactivity
The process of emission of α, β, γ radiations when an unstable nucleus becomes stable is called radioactivity or radioactive disintegration.
Properties of α-Particles
- They are helium nuclei.
- They are positively charged.
- They are deflected in electric and magnetic field.
- They have less penetrating power.
- They can ionise the gas through which they pass.
Properties of β-Particles
- They are fast moving electrons.
- They are negatively charged.
- They are deflected in electric and magnetic field.
- The penetrating power is more than α-particles.
- They have less ionising power than α-particles.
Properties of γ-Rays
- They are electromagnetic waves.
- They are chargeless.
- They are not deflected in electric and magnetic field.
- They have high penetrating power.
- The ionising power is less than α and β-particles.
Laws of Radioactivity
- The radioactivity process is not affected by external factors like pressure, temperature, humidity etc.
- Either α-particle is emitted or β-particle is emitted but not both simultaneously.
When α-Particle is Emitted
When α-particle is emitted, atomic number decreases by 2 and mass number decreases by 4.
Example
When β-Particle is Emitted
When β-particle is emitted, atomic number increases by 1 and mass number remains unchanged / same.
Example
Radioactive Decay Law
The rate of decay of a radioactive sample at time is directly proportional to number of atoms present at that time.
If a sample contains N atoms at time t, then:
where λ is decay constant.
Let N0 be the initial number of atoms at time t = 0.
N = N0e−λt
A = A0e−λt
m = m0e−λt
Decay Curve
Fig: Decay curve
Half Life (T1/2)
The time taken to decay half the number of atoms is called half-life.
Relation Between Half-Life and Decay Constant
Since:
If t = T1/2 and N = N0/2, then:
Mean-Life
The ratio of total life of atoms to the total number of atoms is called mean-life.
Also,
Remaining Number of Atoms after nth Half-Life
Remaining atoms after nth half-life:
Remaining activity after nth half-life:
Discussion
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