Animated Solution for Physics - Work, Energy, and Power: A particle of mass 10−2 kg is moving along the positive X-axis under the influence of a force F(x)=−2x2k where k=10−2 Nm2. At time t=0, it is at x=1.0 m and its velocity v=0.
(a) Find its velocity when it reaches x=0.5 m.
(b) Find the time at which it reaches x=0.25 m.
Visualized Solution
Analyzing the Setup
Particle of mass m=10−2 kg starts from rest at x=1.0 m.
Force F(x)=−2x2k is always negative (since k>0 and x2>0).
The particle will accelerate towards the origin (negative X-direction).
Work-Energy Theorem
To find the velocity at x=0.5 m, we use the Work-Energy Theorem: W=ΔK.
W=∫xixfF(x)dx=21mvf2−21mvi2.
Since vi=0, the work done equals the final kinetic energy.
Setting up the Integral
Substitute the force expression into the work integral.
W=∫1.00.5(−2x2k)dx.
We can pull the constants out: W=−2k∫1.00.5x−2dx.
Evaluating the Work Done
The integral of x−2 is −x−1=−x1.
W=−2k[−x1]1.00.5=2k[x1]1.00.5.
W=2k(0.51−1.01)=2k(2−1)=2k.
Velocity at x=0.5 m
Equate work to kinetic energy: 21mv2=2k⟹v2=mk.
Given k=10−2 Nm2 and m=10−2 kg, we get mk=1.
v2=1⟹v=±1 m/s.
Since the particle moves in the negative X-direction, v=−1 m/s.
General Velocity Function v(x)
For part (b), we need the time to reach x=0.25 m. First, find velocity as a function of x.
Integrate from x=1.0 to an arbitrary position x.
W=2k[x1]1.0x=2k(x1−1).
Expression for v(x)
21mv2=2k(x1−x).
Since mk=1, we have v2=x1−x.
Taking the square root and choosing the negative sign (moving left): v=−x1−x.
Kinematic Relation
Velocity is the rate of change of position: v=dtdx.
Therefore, dtdx=−x1−x.
We need to separate variables to solve for time t.
Separating Variables
Rearrange to isolate dt: dt=−1−xxdx.
Integrate both sides from the initial state (t=0,x=1.0) to the final state (t=?,x=0.25).
∫0tdt=−∫1.00.251−xxdx.
Trigonometric Substitution
The integral ∫1−xxdx is a classic form solved by trigonometric substitution.
The integrand becomes: (cosθsinθ)(2sinθcosθdθ)=2sin2θdθ.
Using the double angle identity: 2sin2θ=1−cos(2θ).
Changing the Limits
Initial limit: x=1.0⟹sin2θ=1⟹θ=2π.
Final limit: x=0.25⟹sin2θ=41⟹sinθ=21⟹θ=6π.
The time integral is t=−∫π/2π/6(1−cos2θ)dθ.
Evaluating the Time Integral
Integrate: ∫(1−cos2θ)dθ=θ−2sin2θ.
Apply limits: t=−[θ−2sin2θ]π/2π/6.
t=−((6π−2sin(π/3))−(2π−2sin(π))).
Final Calculation
t=−(6π−43−2π+0).
t=3π+43.
Substituting π≈3.1416 and 3≈1.732: t≈1.047+0.433=1.48 s.
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The Sigma Insight: Work Done by Forces
Solution Diagram
The Journey to the Origin
A Tale of Work, Energy, and Calculus
Imagine a particle resting peacefully on the positive X-axis at x=1.0 m. Suddenly, it experiences a force pulling it towards the origin. But this isn't just any constant force; it's a force that grows stronger as the particle gets closer to the origin, given by the inverse-square law F(x)=−2x2k.
Because the force is variable, we cannot rely on our standard kinematic equations like v2=u2+2as. Those are strictly reserved for constant acceleration. Instead, we must summon the elegant power of the Work-Energy Theorem and Calculus.
Part A
The Work-Energy Theorem
To find the velocity of the particle when it reaches x=0.5 m, we need to calculate the work done by this variable force. The Work-Energy Theorem states that the net work done on an object equals its change in kinetic energy:
W=ΔK=21mvf2−21mvi2
Since the particle starts from rest, vi=0, meaning the work done will directly equal the final kinetic energy. Let's set up the integral for the work done as the particle moves from x=1.0 m to x=0.5 m:
W=∫1.00.5F(x)dx=∫1.00.5(−2x2k)dx
Pulling the constant −2k out of the integral, we are left with integrating x−2, which is simply −x1.
W=−2k[−x1]1.00.5=2k(0.51−1.01)
Evaluating the limits, we get W=2k(2−1)=2k.
Now, we equate this work to the kinetic energy:
21mv2=2k⟹v2=mk
Given that k=10−2 Nm2 and m=10−2 kg, the ratio mk is exactly 1. Therefore, v2=1, which gives v=±1 m/s. Since the force is pulling the particle in the negative X-direction, we must choose the negative root.
The velocity at x=0.5 m is −1 m/s.
Part B
The Kinematic Differential Equation
Now for the real challenge: finding the exact time it takes to reach x=0.25 m. To find time, we first need velocity as a general function of position, v(x). We repeat our Work-Energy integration, but this time, we integrate from x=1.0 to an arbitrary position x:
W=2k[x1]1.0x=2k(x1−1)
Equating this to kinetic energy and substituting mk=1, we get:
v2=x1−x
Taking the negative square root (because it's moving left), we find our velocity function:
v=−x1−x
Velocity is fundamentally the rate of change of position, v=dtdx. This gives us a beautiful, yet intimidating, differential equation:
dtdx=−x1−x
The Calculus Climax
To solve for time, we separate the variables, moving all x terms to one side and dt to the other:
dt=−1−xxdx
Integrating both sides from the initial state (t=0,x=1.0) to the final state (t=?,x=0.25):
∫0tdt=−∫1.00.251−xxdx
This integral is a classic candidate for trigonometric substitution. The term 1−x in the denominator screams for the Pythagorean identity. Let's substitute x=sin2θ. This means the differential dx becomes 2sinθcosθdθ.
The square root simplifies beautifully:
1−sin2θsin2θ=cosθsinθ
Multiplying this by our new dx, the integrand transforms into:
(cosθsinθ)(2sinθcosθdθ)=2sin2θdθ
Using the double-angle identity, 2sin2θ=1−cos(2θ).
We must also update our limits. When x=1.0, sin2θ=1, so θ=2π. When x=0.25, sin2θ=41, so sinθ=21, which means θ=6π.
Our time integral is now a straightforward trigonometric evaluation:
t=−∫π/2π/6(1−cos2θ)dθ
Integrating yields θ−2sin2θ. Applying the limits:
t=−[(6π−2sin(π/3))−(2π−2sin(π))]
t=−(6π−43−2π)=3π+43
Substituting the approximate values π≈3.1416 and 3≈1.732, we get:
t≈1.047+0.433=1.48 s
The particle reaches x=0.25 m at exactly 1.48 s. A perfect harmony of physics and calculus!