Nuclear Reaction:
Nuclear reaction is the procedure whereby mass number or atomic number of target nuclei changes due to bombardment with projectile particles resulting in release of energy. Essential things for nuclear reaction are:
i) Target nucleus
ii) Projectile example 10n, 11H, 42He, 21H
X + x → Y + y + Q or X(x,y)Y
e.g. 147N(α, p) 177O
147N + 42He → 178O + 11H + Q
Kinds of Nuclear Reaction
1) F - Fission - X + x → y1 + y2
2) I - Inelastic nuclear reaction - X + x → Xk +x
3) T - Transmutation - X + x → Y + y
4) E - Elastic nuclear reaction - X + x → X + x
5) C - Capture - X + x → Yk
Physical qualities that are conserved in any nuclear reaction comprise:
1) Total electric change EZ = K
2) Total number of nuclei EA = K
3) Linear momentum EP = K
4) Sum of mass and energy E(mass + Ke)
5) Parity K
Q - Value Equation:
This is nuclear change or amount of energy released in the nuclear reaction. For nuclear reaction, the total rest mass and kinetic energy are conserved.
Example X + x → Y + y + Q
i.e [EX + mXC2] + [Ex + mxC2]
= [EY + mYC2] + [Ey + myC2] + Q
As target nucleus X is at rest, then equation turns to
[MxC2] + [Ex + mxC2] = [Ey + MyC2] + [Ey + MyC2] + Q
But Q = change in energy
Hence Q = Ex - (EY + Ey)
Q = [(MX + mx) - (MY + My)]C2
Q = Δmc2
Conventional Q-value Equation:
Applying principle of conservation of momentum
MxVx = MYVYcosΦ + MyVycosθ(x-direction)
O = MYVYsinΦ + MyVysinθ(y-direction)
Form E = P2/2m, p2 = 2mE
Thus, momentum mv = √2ME
Equation turns into:
(MxEx)1/2 = (MYEY)1/2cosΦ + (MyEy)1/2cosθ
O = (MYEY)1/2 sinΦ + (MyEy)1/2sinθ
Square equations and add:
MxEx = MyEYcos2Φ + MyEycos2θ
MxEx = MYEY + MyEy
Minimum energy projectile should have before it can induce nuclear reaction is known as threshold energy
Conservation of linear momentum:
MxVx = McVc
Vc = MxVx/Mc
But -Q = 1/2MxVx2 - 1/2McVc2
-Q = 1/2MxVx2 - 1/2Mc(Mx2Vx2/Mc2)
-Q = 1/2MxVx2[1 - Mx/Mc]
But Mc = MX + Mx
-Q = 1/2MxVx2[1 - Mx/(MX + Mx)]
-Q = 1/2MxVx2[(MX + Mx - Mx)/(MX + Mx)]
-Q = 1/2MxVx2[MX/(MX + Mx)]
Take 1/2MxVx2 = Ethr
-Q = Ethr[MX/(MX + Mx)]
Ethr = -Q x [MX + Mx/MX]
Ethr = -Q x [1 + Mx/MX]
Nuclear Fission Reaction:
This is the reaction that involves splitting of heavy nuclei in two or more lighter nuclei by bombarding heavy nuclei with thermal neutrons and it is generally accompanied with high energy released. Nuclides which can be fissioned by thermal neutrons as follow: 235U, 237U and 239Pu.
Only 235U takes place as expected while others are gotten from fertile materials. Procedure of conversion of fertile materials to fissionable material is referred to as breeder reaction. Energy released in the fission reaction is Q = Δmc2 = [(Σmi - Σmf)c2]
Nuclear Fusion Reaction:
This is a combination of two or more light nuclei to form heavier one and this involves supply of high energy. In which this energy will be able to beat coulombs force between them.
11H + 21H → 31H + γ + Q
And in doing so they should overcome potential barrier that is equal to
V = Z1Z2e2/4πε0r
V = 0.15Z1Z2Mev, for r = 10-14m
This type of energy (109k) can only be attained during nuclear explosions that are not practicable. Generally at this temperature, atoms exist as ions and are collected as plasma. Due to high temperature, it is also referred to as thermonuclear reaction.
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