Animated Solution for Physics - Kinematics: Two vectors A and B have equal magnitudes. The magnitude of (A+B) is 'n' times the magnitude of (A−B). The angle between A and B is
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Visualized Solution
Visualizing the Vectors
Let the two vectors be A and B.
Given: ∣A∣=∣B∣=A
Let the angle between them be θ.
Vector Addition and Subtraction
Using the parallelogram law:
∣A+B∣=A2+B2+2ABcosθ
∣A−B∣=A2+B2−2ABcosθ
Substituting Equal Magnitudes
Since ∣A∣=∣B∣=A:
∣A+B∣2=A2+A2+2A2cosθ
∣A+B∣2=2A2(1+cosθ)
Magnitude of Difference
Similarly, for the difference:
∣A−B∣2=A2+A2−2A2cosθ
∣A−B∣2=2A2(1−cosθ)
Applying the Given Condition
Given condition:
∣A+B∣=n∣A−B∣
Squaring both sides:
∣A+B∣2=n2∣A−B∣2
Substituting the Expressions
Substitute the squared magnitudes:
2A2(1+cosθ)=n2⋅2A2(1−cosθ)
Canceling 2A2 from both sides:
1+cosθ=n2(1−cosθ)
Solving for cosθ
Rearranging the terms:
1n2=1−cosθ1+cosθ
Applying Componendo and Dividendo:
n2+1n2−1=(1+cosθ)+(1−cosθ)(1+cosθ)−(1−cosθ)
n2+1n2−1=22cosθ=cosθ
Final Angle
cosθ=n2+1n2−1
θ=cos−1(n2+1n2−1)
Physical Interpretation
If n=1, then ∣A+B∣=∣A−B∣.
This implies cosθ=0, so θ=90∘.
The vectors are perpendicular.
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The Sigma Insight: Vector Addition, Subtraction, and Resolution
Solution Diagram
Visualizing the Vectors
Imagine you are standing at the origin of a coordinate system. You have two vectors, A and B, pointing outwards.
The problem gives us a beautiful symmetry: both vectors have the exact same length. Let's call this common magnitude A.
So, we can write ∣A∣=∣B∣=A. Let the angle between them be θ. This angle θ is exactly what we need to find!
The Power of the Parallelogram Law
To relate the sum and difference of these vectors, we need to use the parallelogram law of vector addition.
The magnitude of the sum of two vectors is given by the formula ∣A+B∣=A2+B2+2ABcosθ.
Since A=B, we can substitute this into our formula. This gives us ∣A+B∣2=A2+A2+2A2cosθ.
Factoring out 2A2, we get a neat expression: ∣A+B∣2=2A2(1+cosθ).
Similarly, the magnitude of the difference is ∣A−B∣=A2+B2−2ABcosθ.
Following the exact same logic, we find that ∣A−B∣2=2A2(1−cosθ).
Setting Up the Master Equation
Now, let's look at the core condition given in the problem. We are told that the magnitude of the sum is n times the magnitude of the difference.
Mathematically, this translates to ∣A+B∣=n∣A−B∣.
Square roots can be messy to deal with, so let's square both sides of this equation. This gives us ∣A+B∣2=n2∣A−B∣2.
The Elegance of Componendo and Dividendo
Now, we substitute the expressions we derived earlier into our squared condition.
This yields 2A2(1+cosθ)=n2⋅2A2(1−cosθ).
Notice how the 2A2 terms are present on both sides? They beautifully cancel each other out! We are left with 1+cosθ=n2(1−cosθ).
We can rearrange this into a ratio: 1n2=1−cosθ1+cosθ.
To isolate cosθ quickly, we can use a brilliant algebraic trick called Componendo and Dividendo.
Applying this rule, we get n2+1n2−1=(1+cosθ)+(1−cosθ)(1+cosθ)−(1−cosθ).
The right side simplifies perfectly to 22cosθ, which is just cosθ.
The Final Revelation
We have successfully isolated our trigonometric term!
We found that cosθ=n2+1n2−1.
To find the angle θ itself, we simply take the inverse cosine of both sides.
This gives us our final, elegant answer: θ=cos−1(n2+1n2−1).
As a fun thought experiment, imagine if n=1. This would mean cosθ=0, which implies θ=90∘. This perfectly aligns with the geometric fact that the diagonals of a rhombus are equal only when it is a square!