The Alchemy of the Nucleus
Welcome to the fascinating world of radioactive decay, where elements literally transform into entirely different elements! This isn't medieval alchemy; it's the rigorous, mathematically beautiful reality of nuclear physics. In this problem, we are presented with four distinct nuclear reactions. Our mission is to act as nuclear detectives and deduce exactly which particles were emitted during these transformations.
To solve this, we don't need complex quantum mechanics. We just need to rely on two unbreakable laws of the universe: the conservation of mass number and the conservation of atomic number (charge).
The Unbreakable Laws of Conservation
Every nuclear reaction can be written in a general form:
ZAX→Z′A′Y+nα24He+nβe
1. Conservation of Mass Number (A):
The total mass number before the decay must equal the total mass number after the decay. Since β particles (electrons or positrons) have a mass number of zero, any change in the mass number is entirely due to the emission of α particles (Helium nuclei). Each α particle carries away a mass number of 4. Therefore, the number of α particles emitted is simply:
2. Conservation of Atomic Number (Z):
The total charge must also be conserved. The original atomic number Z must equal the new atomic number Z′, plus 2 times the number of α particles, plus the net charge carried away by the β particles.
Zinitial=Zfinal+2nα+ΔZβ
If ΔZβ is negative, it means β− particles (electrons, charge −1) were emitted. If ΔZβ is positive, it means β+ particles (positrons, charge +1) were emitted.
Decoding the Matrix
Step-by-Step
Let's apply our detective tools to each reaction.
Reaction P: 92238U→91234Pa
First, we check the mass number. It drops from 238 to 234, a difference of 4. This immediately tells us exactly 1 α particle is emitted.
Now for the charge: 92=91+2(1)+ΔZβ. Solving this gives ΔZβ=−1.
Conclusion: 1α and 1β− are emitted. This matches option (4).
Reaction Q: 82214Pb→82210Pb
The mass number decreases from 214 to 210, a difference of 4, so we have 1 α particle.
For the atomic number: 82=82+2(1)+ΔZβ. This means ΔZβ=−2 to balance the equation.
Conclusion: 1α and 2β− are emitted. This matches option (3).
Reaction R: 81210Tl→82206Pb
The mass number difference is 210−206=4, yielding 1 α particle.
The atomic number equation is 81=82+2(1)+ΔZβ. Solving this gives ΔZβ=−3.
Conclusion: 1α and 3β− are emitted. This matches option (2).
Reaction S: 91228Pa→88224Ra
The mass number drops by 4, so 1 α particle is emitted.
The atomic number equation is 91=88+2(1)+ΔZβ. This time, ΔZβ=+1! This is a crucial difference. It means a positive charge was emitted.
Conclusion: 1α and 1β+ (positron) are emitted. This matches option (1).
The Final Verdict
By systematically applying the conservation laws, we have successfully decoded the entire matrix. The beauty of physics lies in its consistency; no matter how complex the nucleus, the fundamental rules of arithmetic always hold true.