^Critical mass
^Critical mass
The minimum of Uranium needed to sustain chain reaction is called critical mass. It is 10 kg.
^Critical mass
The minimum of Uranium needed to sustain chain reaction is called critical mass. It is 10 kg.
^Nuclear fuel
Fissionable material is called nuclear fuel. The isotopes like U-235, Th -232 and Pu 239 can be used as the reactor fuel. A certain mass of the fuel is taken in the form of rods, tightly sealed in Aluminium containers. The rods, separated by moderator are placed in the core of the reactor.
^Uranium enrichment
The 0.69% U235 is not sufficient to produce a self-sustaining critical chain reaction. To ensure high probability of chain reaction concentration of 235U has to be increased called enrichment. For reactors, the fuel must be enriched to 2.5-3.5%, U-235.
^Natural Uranium
Found as uranium oxide (U2 O3) which when purified has a rich yellow color and is called “yellowcake”. Uranium has three isotopes namely:
92U238 (99.3%), 92U235 (0.69%) & 92U234 (0.01%).
As the relative of abundance is highest for 92U238, it is called FERTILE. However fission is possible only with 92U235, thus is called FISSILE.
Chemical isotopes that can sustain a fission chain reaction are called nuclear fuels, and are said to be fissile.

Here IP = Ionizing power & PP = Penetrating power
Also All the three type of rays namely α, β & ϒ affect photographic plate produce flourescence & artificial radioactivity.
^γ-decay
Most radioisotopes, after an alpha decay or a beta decay, leave the daughter nucleus in an excited state, these excited nuclei make a transition to a state of lower energy by emitting a photon. These photons are charge less, mass less & high energy electromagnetic waves (of the order of million electron volt) & are called the gamma rays.
ZXA (unstable nuclei) → ZXA (stable nuclei) + γ
^β-decay
In the beta-minus decay, a neutron inside the nucleus transforms into a proton with the emission of an electron and anti-neutrino are emitted.
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Note, the spins of the neutron, proton and electron are all 1/2. In the beta-plus decay, a proton inside the nucleus transforms into a neutron with the emission of a positron and neutrino are emitted.
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^α-decay
Consider the following decay
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As a nucleus decays due to internal force of repulsion, there is no net external force on it, hence in any nuclear reaction linear momentum must be conserved.
Before disintegration, the nucleus can be assumed to be at rest, so the total momentum was zero. After disintegration let it be mava & mD vD for alpha particle & daughter nuclei respectively. To conserve linear momentum the total vector momentum must still be zero i.e. mava + mDvD = 0 or mava = -mDvD
i.e. momentum of a particle must be equal & opposite to that of daughter’s nucleus.
In magnitude, mava = mDvD


As mass of alpha particle is much lighter than thorium, thus the lighter α particle carries off most of the energy in the form its KE (about 98% of the total KE).
1. A heavy unstable nucleus (e.g. Uranium, polonium, radium, thorium, actinium, etc.) disintegrates itself naturally, spontaneously & randomly without being forced by any external agent to do so until it acquires stability.
2. The disintegration is independent of all physical and chemical conditions and so it can neither be accelerated nor retarded.
3. The disintegration is random. It is purely a matter of chance for any atom to disintegrate first. It is not possible to predict whether a particular nucleus will decay in a given time interval.
4. The activity (or rate of disintegration, A or R) of a radioactive sample at any instant is directly proportional to the number of undecayed nuclei present in the sample at that instant.

Here λ = disintegration constant or decay constant. & N0 = no. of the atoms present initially i.e. at t = 0.
From above result we can say
5. Half life (T): ![]()
6. Fraction ‘f’ of substance left undecayed after ‘n’ half lives is given by: ![]()
7. Mean life (τ): ![]()
8. Decay constant (λ) is the reciprocal of time for which ![]()
9. λ = 0 for a stable element (e.g. Pb).
10. (a) 1 Bacqueral (Bq) = 1 d.p.s.
(b) 1 Curie (rd) = 3.7 x 1010 d.p.s.
(c) 1 Rutherford (Rd) = 106 d.p.s.
Here d.p.s. = disintegrations per second.
^Binding energy per nucleon
1. is low for both heavy & light nuclei.
2. increases rapidly up to A = 20 & have peaks for 2He4, 6C12 & 8 O16 .
3. increases gradually after A = 20.
4. becomes less or more flat between A = 40 to 120.
Also it has average value in this region is 8.5 MeV.
5. has maximum value 8.8 MeV for the 26Fe56.
6. decrease after A =120 & drops to 7.6Mev for 92U238.

In order to increases the values of binding energies light nuclei undergo fusion while heavy nuclei undergo fission reactions i.e. heavy nuclei become more stable after fission & light nuclei become more stable after fusion.