The Art of the Reduced Universe
Mastering Conditional Probability
Welcome, future engineer. Today, we are going to dismantle a classic problem that appears simple on the surface but holds the key to understanding one of the most powerful concepts in probability theory: the conditional sample space.
When you look at a biased die, you are not just looking at numbers; you are looking at a system where reality is skewed. In a fair die, every face has a probability of 61. But here, the universe is uneven, with probabilities ranging from 0.1 to 0.32. This is the reality of the problem, and we must respect it.
Phase 1
The Shrinking Universe
Imagine you are holding this die and you toss it. You do not see the result yet, but a voice tells you, "The result is either Face 1 or Face 2." In that single moment, your entire world changes.
Before that voice spoke, you were considering six possibilities. Now, you are only considering two. This is the essence of conditional probability. We are not dealing with the original sample space of {1,2,3,4,5,6} anymore; our new, restricted universe is just {1,2}.
In JEE Advanced, the trap is often not the calculation; it is the failure to redefine the sample space. When we are told that the outcome is restricted to a subset, we must treat that subset as our new "total" probability. We are effectively "zooming in" on the events that are actually possible.
Phase 2
The Mathematical Toolkit
To solve this, we rely on the fundamental definition of conditional probability. Let E1 be the event that "Face 1 turns up" and E2 be the event that "Face 1 or Face 2 turns up." We are looking for the probability of E1 given that E2 has occurred, denoted as P(E1∣E2).
The formula is our North Star:
P(E1∣E2)=P(E2)P(E1∩E2)
Let us pause and look at the numerator, P(E1∩E2). This represents the probability that both E1 and E2 happen. Since E1 is a subset of E2, the intersection is simply E1 itself, which is 0.1.
Phase 3
The Calculation
Now, let us look at the denominator, P(E2). This is the probability of our new, restricted universe. Since the events "Face 1" and "Face 2" are mutually exclusive, we simply sum their individual probabilities:
P(E2)=P(Face 1)+P(Face 2)
Substituting the values from our data table:
This 0.42 is the total weight of our new universe. We are now ready to perform the final calculation by taking our numerator and dividing it by our new total:
Phase 4
The Final Polish
In an exam setting, you want to be clean and precise. To clear the decimals, multiply both the numerator and the denominator by 100:
Now, we simplify by dividing both terms by 2:
The probability that the face is 1, given the condition, is 215.
The Takeaway
Why did we go through the formal definition? Because in harder problems, the intuition of "just dividing" might fail you if the events are not mutually exclusive or if the intersection is not a simple subset.
By mastering the formula P(A∣B)=P(B)P(A∩B), you are building a robust mental framework. You have learned to shrink the universe, identify the intersection, and normalize the probability. Keep this mindset, and you will find that even the most "biased" problems become fair game for your intellect.