Oscillations: Particle On A Spring Under Force

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Oscillations: Particle on a Spring Under Force

Hey physics fanatics! Ever wondered what happens when you mess with a classic setup, like a particle on a spring? Well, today we're diving deep into a super interesting scenario: a particle of mass m chilling at rest at the end of a spring with a force constant k, hanging from a fixed support. You know, the usual setup. But then, things get exciting! At t = 0, we throw a wrench in the works by applying a constant downward force F. This force isn't just a fleeting guest; it sticks around for a specific duration, tβ‚€. After this time, the force is removed. Our mission, should we choose to accept it (and we totally do!), is to show that, after the force is removed, the displacement of the particle can be described by a particular equation. This isn't just about crunching numbers, guys; it's about understanding the dynamics of systems, how they respond to external influences, and how they settle back into their natural rhythm. We'll break down the physics step-by-step, making sure we grasp every concept along the way. Get ready to explore simple harmonic motion, damped oscillations, and forced oscillations – all bundled into one awesome problem!

Setting the Stage: The Undisturbed System

Before we even think about applying that external force F, let's get a handle on our system in its natural state. We have a particle of mass m attached to a spring with a force constant k. This spring is hanging vertically from a fixed support. When the system is just hanging there, at rest, the spring is stretched by some amount. Let's call this equilibrium position y=0y=0. At this equilibrium, the upward force exerted by the spring is exactly balancing the downward force of gravity on the mass. So, kyeq=mgky_{eq} = mg, where yeqy_{eq} is the equilibrium stretch. This is crucial because whenever we talk about displacement from this point onwards, we're measuring it from this equilibrium position. It simplifies our equations immensely. Now, if we were to pull this mass down a bit and let it go, it would oscillate up and down with a specific frequency, Ο‰=k/m\omega = \sqrt{k/m}. This natural frequency dictates how fast the system wants to oscillate when left to its own devices. It's the inherent rhythm of our mass-spring system. Understanding this baseline behavior is like learning the alphabet before you can write a novel; it's fundamental to grasping how the system will react when we introduce external forces. So, before t=0t=0, our particle is just hanging out, perfectly still, at its equilibrium position. No motion, no drama, just gravity and spring force in perfect harmony. This initial condition is our starting point, our blank canvas upon which we'll paint the complex dance of motion caused by the applied force.

The Perturbation: Applying the Force F

Alright, so things are calm, but not for long! At t=0t=0, we introduce our external agent: a constant downward force F. This force is applied to the particle of mass m and, crucially, it acts for a finite time tβ‚€. This means our system, which was happily at rest, is now being forced to move. The equation of motion for the particle, while this force is active (i.e., for 0≀t≀t00 \le t \le tβ‚€), is modified. Remember Newton's second law: Fnet=maF_{net} = ma. In our case, the net force is the sum of the gravitational force (mgmg), the spring force (βˆ’ky-ky, where yy is the displacement from the unstretched position, or more conveniently, βˆ’k(yinitial+ynew)-k(y_{initial} + y_{new}) if yy is from equilibrium and yinitialy_{initial} is the equilibrium stretch), and the applied force (FF). If we define yy as the displacement from the equilibrium position (where kyeq=mgky_{eq} = mg), then the gravitational force and the spring force at equilibrium cancel out. The equation of motion becomes: myΒ¨=Fβˆ’kym\ddot{y} = F - ky. Rearranging this, we get myΒ¨+ky=Fm\ddot{y} + ky = F. This is the differential equation governing the motion of the particle while the force F is applied. Notice how the applied force F acts as a constant driving term. This term shifts the equilibrium position and introduces a new type of motion. The system will not only oscillate but also exhibit a steady-state displacement due to this constant force. We need to solve this second-order non-homogeneous differential equation. The general solution will consist of a complementary solution (which describes the natural oscillations) and a particular solution (which describes the steady-state response to the constant force F). Solving this requires us to consider initial conditions at t=0t=0. Since the particle starts at rest at the equilibrium position, our initial conditions are y(0)=0y(0) = 0 and yΛ™(0)=0\dot{y}(0) = 0. These initial conditions will allow us to determine the constants of integration that arise from solving the differential equation. The duration for which this force acts, t0tβ‚€, is also a critical parameter. The state of the system (its position and velocity) at time t0tβ‚€ will become the initial conditions for the next phase of motion, where the applied force is no longer present.

The Transition: Force Removed at tβ‚€

Now, the exciting part! At time t=t0t = tβ‚€, the constant downward force F is removed. This is a critical juncture in our problem. What happens to the particle's motion after this point? The differential equation governing the motion changes. For t>t0t > tβ‚€, the applied force F is no longer acting on the mass. So, the equation of motion reverts back to the standard form for a simple harmonic oscillator, but with a crucial difference: the initial conditions for this new phase of motion are not the ones we started with at t=0t=0. Instead, the initial conditions for t>t0t > tβ‚€ are the position and velocity of the particle at the exact moment the force was removed, i.e., at t=t0t = tβ‚€. Let y(t0)y(tβ‚€) and yΛ™(t0)\dot{y}(tβ‚€) be the displacement and velocity of the particle at time t0tβ‚€. These values are determined by the solution of the equation of motion during the interval 0≀t≀t00 \le t \le tβ‚€. So, the first step is to solve myΒ¨+ky=Fm\ddot{y} + ky = F with initial conditions y(0)=0y(0) = 0 and yΛ™(0)=0\dot{y}(0) = 0. Once we have the solution y(t)y(t) for 0≀t≀t00 \le t \le tβ‚€, we can evaluate y(t0)y(tβ‚€) and yΛ™(t0)\dot{y}(tβ‚€). These values then become the initial conditions for the subsequent motion described by the equation myΒ¨+ky=0m\ddot{y} + ky = 0 for t>t0t > tβ‚€. This equation represents free oscillations. The general solution for this homogeneous equation is of the form y(t)=Acos⁑(Ο‰t)+Bsin⁑(Ο‰t)y(t) = A \cos(\omega t) + B \sin(\omega t), where Ο‰=k/m\omega = \sqrt{k/m}. The constants A and B are determined by the initial conditions y(t0)y(tβ‚€) and yΛ™(t0)\dot{y}(tβ‚€). This transition is key. The motion after t0tβ‚€ is a superposition of the system's natural tendency to oscillate at its own frequency Ο‰\omega and the imprint of the previous forced motion. The amplitude and phase of these free oscillations are directly dictated by the state of the system when the external force vanished. It's like giving a swing a push for a few seconds; the swing will continue to move with its own natural period, but the height it reaches and its subsequent motion depend entirely on how hard and for how long you pushed it. The removal of the force doesn't instantly reset the system; it carries the memory of the applied force in its momentum and position.

Deriving the Displacement After Force Removal

Alright, guys, let's get down to the nitty-gritty and actually show the displacement after the force is removed. We need to solve the problem in two stages.

Stage 1: 0≀t≀t00 \le t \le tβ‚€ (Force F is applied)

The equation of motion is myΒ¨+ky=Fm\ddot{y} + ky = F. The general solution is the sum of the complementary solution yc(t)=C1cos⁑(Ο‰t)+C2sin⁑(Ο‰t)y_c(t) = C_1 \cos(\omega t) + C_2 \sin(\omega t) (where Ο‰=k/m\omega = \sqrt{k/m}) and a particular solution yp(t)y_p(t). For a constant force F, a good guess for the particular solution is a constant, say yp=Ay_p = A. Substituting into the equation: m(0)+kA=Fm(0) + kA = F, so A=F/kA = F/k. This is the new equilibrium position under the influence of force F.

The total solution is y(t)=C1cos⁑(Ο‰t)+C2sin⁑(Ο‰t)+F/ky(t) = C_1 \cos(\omega t) + C_2 \sin(\omega t) + F/k.

Now, we apply the initial conditions at t=0t=0: y(0)=0y(0) = 0 and yΛ™(0)=0\dot{y}(0) = 0.

From y(0)=0y(0)=0: $C_1 \cos(0) + C_2 \sin(0) + F/k = 0 implies C_1 + F/k = 0

So, C1=βˆ’F/kC_1 = -F/k.

To find C2C_2, we need the velocity yΛ™(t)\dot{y}(t): yΛ™(t)=βˆ’C1Ο‰sin⁑(Ο‰t)+C2Ο‰cos⁑(Ο‰t)\dot{y}(t) = -C_1 \omega \sin(\omega t) + C_2 \omega \cos(\omega t).

From yΛ™(0)=0\dot{y}(0)=0: $-C_1 \omega \sin(0) + C_2 \omega \cos(0) = 0

This gives C2Ο‰=0C_2 \omega = 0. Since Ο‰β‰ 0\omega \ne 0, we must have C2=0C_2 = 0.

So, the displacement during the time the force is applied is: y(t)=Fk(1βˆ’cos⁑(Ο‰t))y(t) = \frac{F}{k} (1 - \cos(\omega t)) for 0≀t≀t00 \le t \le tβ‚€.

This equation tells us how the particle moves until time t0tβ‚€. It starts from rest and moves to a maximum displacement.

Now, we need the position and velocity at t=t0t = tβ‚€ to serve as initial conditions for the next stage.

y(t0)=Fk(1βˆ’cos⁑(Ο‰t0))y(tβ‚€) = \frac{F}{k} (1 - \cos(\omega tβ‚€))

yΛ™(t)=Fk(Ο‰sin⁑(Ο‰t))\dot{y}(t) = \frac{F}{k} (\omega \sin(\omega t))

yΛ™(t0)=FkΟ‰sin⁑(Ο‰t0)\dot{y}(tβ‚€) = \frac{F}{k} \omega \sin(\omega tβ‚€)

Stage 2: t>t0t > tβ‚€ (Force F is removed)

The equation of motion is now myΒ¨+ky=0m\ddot{y} + ky = 0. The general solution is y(t)=D1cos⁑(Ο‰t)+D2sin⁑(Ο‰t)y(t) = D_1 \cos(\omega t) + D_2 \sin(\omega t).

We use the values from Stage 1 at t=t0t = tβ‚€ as our initial conditions for this equation.

Let's shift our time variable for convenience. Let tβ€²=tβˆ’t0t' = t - tβ‚€. So, when t=t0t=tβ‚€, tβ€²=0t'=0. The equation becomes y(tβ€²)=D1cos⁑(Ο‰(tβ€²+t0))+D2sin⁑(Ο‰(tβ€²+t0))y(t') = D_1 \cos(\omega (t'+tβ‚€)) + D_2 \sin(\omega (t'+tβ‚€)).

Using the standard form y(tβ€²)=Aβ€²cos⁑(Ο‰tβ€²)+Bβ€²sin⁑(Ο‰tβ€²)y(t') = A' \cos(\omega t') + B' \sin(\omega t') and applying initial conditions at tβ€²=0t'=0 (which corresponds to t=t0t=tβ‚€):

$y(0) = y(tβ‚€) = \frac{F}{k} (1 - \cos(\omega tβ‚€)) = A' \cos(0) + B' \sin(0)

So, Aβ€²=Fk(1βˆ’cos⁑(Ο‰t0))A' = \frac{F}{k} (1 - \cos(\omega tβ‚€)).

Now for the velocity. The velocity in terms of tβ€²t' is yΛ™(tβ€²)=βˆ’Aβ€²Ο‰sin⁑(Ο‰tβ€²)+Bβ€²Ο‰cos⁑(Ο‰tβ€²)\dot{y}(t') = -A' \omega \sin(\omega t') + B' \omega \cos(\omega t').

At tβ€²=0t'=0 (which is t=t0t=tβ‚€):

$\dot{y}(0) = \dot{y}(tβ‚€) = \frac{F\omega}{k} \sin(\omega tβ‚€) = -A' \omega \sin(0) + B' \omega \cos(0)

So, yΛ™(t0)=Bβ€²Ο‰\dot{y}(tβ‚€) = B' \omega.

Bβ€²=yΛ™(t0)Ο‰=1Ο‰FΟ‰ksin⁑(Ο‰t0)=Fksin⁑(Ο‰t0)B' = \frac{\dot{y}(tβ‚€)}{\omega} = \frac{1}{\omega} \frac{F\omega}{k} \sin(\omega tβ‚€) = \frac{F}{k} \sin(\omega tβ‚€).

Substituting Aβ€²A' and Bβ€²B' back into y(tβ€²)y(t'):

y(tβ€²)=Fk(1βˆ’cos⁑(Ο‰t0))cos⁑(Ο‰tβ€²)+Fksin⁑(Ο‰t0)sin⁑(Ο‰tβ€²)y(t') = \frac{F}{k} (1 - \cos(\omega tβ‚€)) \cos(\omega t') + \frac{F}{k} \sin(\omega tβ‚€) \sin(\omega t')

y(tβ€²)=Fk[cos⁑(Ο‰tβ€²)βˆ’cos⁑(Ο‰t0)cos⁑(Ο‰tβ€²)+sin⁑(Ο‰t0)sin⁑(Ο‰tβ€²)]y(t') = \frac{F}{k} [\cos(\omega t') - \cos(\omega tβ‚€) \cos(\omega t') + \sin(\omega tβ‚€) \sin(\omega t')]

Using the trigonometric identity cos⁑(Aβˆ’B)=cos⁑Acos⁑B+sin⁑Asin⁑B\cos(A-B) = \cos A \cos B + \sin A \sin B, we can rearrange the terms inside the bracket. Let A=Ο‰tβ€²A = \omega t' and B=Ο‰t0B = \omega tβ‚€. Then cos⁑(Ο‰tβ€²)cos⁑(Ο‰t0)βˆ’sin⁑(Ο‰tβ€²)sin⁑(Ο‰t0)=cos⁑(Ο‰tβ€²+Ο‰t0)\cos(\omega t') \cos(\omega tβ‚€) - \sin(\omega t') \sin(\omega tβ‚€) = \cos(\omega t' + \omega tβ‚€).

Wait, that's not quite right. Let's re-examine the identity. We have βˆ’cos⁑(Ο‰t0)cos⁑(Ο‰tβ€²)+sin⁑(Ο‰t0)sin⁑(Ο‰tβ€²)- \cos(\omega tβ‚€) \cos(\omega t') + \sin(\omega tβ‚€) \sin(\omega t').

Let's use cos⁑(A+B)=cos⁑Acos⁑Bβˆ’sin⁑Asin⁑B\cos(A+B) = \cos A \cos B - \sin A \sin B. Not quite.

Let's use cos⁑(Aβˆ’B)=cos⁑Acos⁑B+sin⁑Asin⁑B\cos(A-B) = \cos A \cos B + \sin A \sin B. Not quite.

Consider the identity cos⁑(Xβˆ’Y)=cos⁑Xcos⁑Y+sin⁑Xsin⁑Y\cos(X - Y) = \cos X \cos Y + \sin X \sin Y. Let X=Ο‰tβ€²X = \omega t' and Y=Ο‰t0Y = \omega tβ‚€. Then cos⁑(Ο‰tβ€²βˆ’Ο‰t0)=cos⁑(Ο‰tβ€²)cos⁑(Ο‰t0)+sin⁑(Ο‰tβ€²)sin⁑(Ο‰t0)\cos(\omega t' - \omega tβ‚€) = \cos(\omega t') \cos(\omega tβ‚€) + \sin(\omega t') \sin(\omega tβ‚€).

We have: y(tβ€²)=Fk[cos⁑(Ο‰tβ€²)βˆ’(cos⁑(Ο‰t0)cos⁑(Ο‰tβ€²)βˆ’sin⁑(Ο‰t0)sin⁑(Ο‰tβ€²))]y(t') = \frac{F}{k} [\cos(\omega t') - (\cos(\omega tβ‚€) \cos(\omega t') - \sin(\omega tβ‚€) \sin(\omega t'))]

y(tβ€²)=Fk[cos⁑(Ο‰tβ€²)βˆ’cos⁑(Ο‰tβ€²+Ο‰t0)]y(t') = \frac{F}{k} [\cos(\omega t') - \cos(\omega t' + \omega tβ‚€)]

Substituting back tβ€²=tβˆ’t0t' = t - tβ‚€:

y(tβˆ’t0)=Fk[cos⁑(Ο‰(tβˆ’t0))βˆ’cos⁑(Ο‰t)]y(t - tβ‚€) = \frac{F}{k} [\cos(\omega (t - tβ‚€)) - \cos(\omega t)]

This is the displacement of the particle after the force is removed, expressed in terms of the time elapsed since the force was removed (tβˆ’t0t-tβ‚€) and the total time elapsed since the beginning (tt). This equation is valid for t>t0t > tβ‚€.

Let's check this. At t=t0t=tβ‚€ (so tβ€²=0t'=0), y(0)=Fk[cos⁑(0)βˆ’cos⁑(Ο‰t0)]=Fk(1βˆ’cos⁑(Ο‰t0))y(0) = \frac{F}{k} [\cos(0) - \cos(\omega tβ‚€)] = \frac{F}{k} (1 - \cos(\omega tβ‚€)), which matches y(t0)y(tβ‚€) from Stage 1. Good!

What about velocity at t=t0t=tβ‚€? Differentiating y(tβˆ’t0)y(t - tβ‚€) with respect to tt:

dydt=Fk[βˆ’Ο‰sin⁑(Ο‰(tβˆ’t0))βˆ’(βˆ’Ο‰sin⁑(Ο‰t))]=FΟ‰k[sin⁑(Ο‰t)βˆ’sin⁑(Ο‰(tβˆ’t0))]\frac{dy}{dt} = \frac{F}{k} [-\omega \sin(\omega (t - tβ‚€)) - (-\omega \sin(\omega t))] = \frac{F\omega}{k} [\sin(\omega t) - \sin(\omega (t - tβ‚€))]

At t=t0t=tβ‚€: dydt∣t=t0=FΟ‰k[sin⁑(Ο‰t0)βˆ’sin⁑(0)]=FΟ‰ksin⁑(Ο‰t0)\frac{dy}{dt}|_{t=tβ‚€} = \frac{F\omega}{k} [\sin(\omega tβ‚€) - \sin(0)] = \frac{F\omega}{k} \sin(\omega tβ‚€), which matches yΛ™(t0)\dot{y}(tβ‚€) from Stage 1. Excellent!

So, the final expression for the displacement after the force is removed is:

y(t)=Fk[cos⁑(Ο‰(tβˆ’t0))βˆ’cos⁑(Ο‰t)]forΒ t>t0 y(t) = \frac{F}{k} \left[ \cos(\omega (t - tβ‚€)) - \cos(\omega t) \right] \quad \text{for } t > tβ‚€

where Ο‰=k/m\omega = \sqrt{k/m}. This formula beautifully encapsulates the subsequent oscillatory motion of the particle, driven by its initial conditions set during the force application period.

Understanding the Result

So, what does this final equation, y(t)=Fk[cos⁑(Ο‰(tβˆ’t0))βˆ’cos⁑(Ο‰t)]y(t) = \frac{F}{k} [\cos(\omega (t - tβ‚€)) - \cos(\omega t)] for t>t0t > tβ‚€, actually tell us? It's a bit of a mind-bender at first, with those two cosine terms, but it elegantly describes the free oscillation of the particle after the external force F has been removed. Remember, this equation is valid after time t0tβ‚€. The term Ο‰=k/m\omega = \sqrt{k/m} is our familiar angular frequency, the natural 'beat' of the spring-mass system. The equation essentially shows that the motion for t>t0t > tβ‚€ is a superposition of two oscillations. One oscillation seems to be phase-shifted by t0tβ‚€, represented by cos⁑(Ο‰(tβˆ’t0))\cos(\omega (t - tβ‚€)), and the other is a standard cosine wave cos⁑(Ο‰t)\cos(\omega t).

Let's think about the amplitude. The term F/kF/k is the static displacement if the force F were applied permanently. So, the amplitude of the oscillations is somehow related to this static deflection. We can use a trigonometric identity to rewrite this expression, which might give us more physical insight. Recall the identity cos⁑Aβˆ’cos⁑B=βˆ’2sin⁑(A+B2)sin⁑(Aβˆ’B2)\cos A - \cos B = -2 \sin\left(\frac{A+B}{2}\right) \sin\left(\frac{A-B}{2}\right).

Let A=Ο‰tA = \omega t and B=Ο‰(tβˆ’t0)B = \omega (t - tβ‚€). Then A+B2=Ο‰t+Ο‰tβˆ’Ο‰t02=2Ο‰tβˆ’Ο‰t02=Ο‰tβˆ’Ο‰t02\frac{A+B}{2} = \frac{\omega t + \omega t - \omega tβ‚€}{2} = \frac{2\omega t - \omega tβ‚€}{2} = \omega t - \frac{\omega tβ‚€}{2}. And Aβˆ’B2=Ο‰tβˆ’(Ο‰tβˆ’Ο‰t0)2=Ο‰t02\frac{A-B}{2} = \frac{\omega t - (\omega t - \omega tβ‚€)}{2} = \frac{\omega tβ‚€}{2}.

So, cos⁑(Ο‰t)βˆ’cos⁑(Ο‰(tβˆ’t0))=βˆ’2sin⁑(Ο‰tβˆ’Ο‰t02)sin⁑(Ο‰t02)\cos(\omega t) - \cos(\omega (t - tβ‚€)) = -2 \sin\left(\omega t - \frac{\omega tβ‚€}{2}\right) \sin\left(\frac{\omega tβ‚€}{2}\right).

Therefore, our displacement equation becomes:

y(t)=Fk[βˆ’2sin⁑(Ο‰t02)sin⁑(Ο‰tβˆ’Ο‰t02)]y(t) = \frac{F}{k} \left[ -2 \sin\left(\frac{\omega tβ‚€}{2}\right) \sin\left(\omega t - \frac{\omega tβ‚€}{2}\right) \right]

y(t)=βˆ’2Fksin⁑(Ο‰t02)sin⁑(Ο‰tβˆ’Ο‰t02)y(t) = -2 \frac{F}{k} \sin\left(\frac{\omega tβ‚€}{2}\right) \sin\left(\omega t - \frac{\omega tβ‚€}{2}\right)

This form is much more revealing! It shows that the displacement is a sinusoidal wave sin⁑(Ο‰tβˆ’Ο‰t02)\sin(\omega t - \frac{\omega tβ‚€}{2}) whose amplitude is 2Fk∣sin⁑(Ο‰t02)∣2 \frac{F}{k} \left| \sin(\frac{\omega tβ‚€}{2}) \right|.

This amplitude depends on the duration t0tβ‚€ for which the force was applied. It also depends on F and k, as expected.

  • If sin⁑(Ο‰t02)=0\sin(\frac{\omega tβ‚€}{2}) = 0: This happens when Ο‰t02=nΟ€\frac{\omega tβ‚€}{2} = n\pi for integer nn. This means Ο‰t0=2nΟ€\omega tβ‚€ = 2n\pi. In this case, the amplitude is zero, and the particle returns to its equilibrium position and stays there after t0tβ‚€. This is a very specific scenario where the force was applied for exactly a half-integer multiple of the period T=2Ο€/Ο‰T = 2\pi/\omega. For example, if t0=T/2tβ‚€ = T/2, then Ο‰t0=(2Ο€/T)(T/2)=Ο€\omega tβ‚€ = (2\pi/T)(T/2) = \pi. Then sin⁑(Ο€/2)=1\sin(\pi/2) = 1. This doesn't result in zero amplitude. Let's recheck. If Ο‰t0=2nΟ€\omega tβ‚€ = 2n\pi, then t0=nTtβ‚€ = nT. This means the force was applied for an integer number of full periods. In this case, the system returns to its exact starting state (zero displacement and zero velocity) if the force was harmonic. However, here the force is constant. If Ο‰t0=2nΟ€\omega tβ‚€ = 2n\pi, then sin⁑(Ο‰t02)=sin⁑(nΟ€)=0\sin(\frac{\omega tβ‚€}{2}) = \sin(n\pi) = 0. So, the amplitude is indeed zero. This means the net effect of the force over these periods results in the particle being at rest at y=0y=0.
  • If sin⁑(Ο‰t02)\sin(\frac{\omega tβ‚€}{2}) is maximum (i.e., Β±1\pm 1): This happens when Ο‰t02=(n+1/2)Ο€\frac{\omega tβ‚€}{2} = (n + 1/2)\pi. This means Ο‰t0=(2n+1)Ο€\omega tβ‚€ = (2n+1)\pi. The force is applied for a half-integer number of periods. In this case, the amplitude of oscillation is maximal, equal to 2F/k2F/k. The particle is set into motion with the largest possible amplitude.

This derived equation shows that the motion after the force removal is a pure harmonic oscillation. The amplitude is determined by the duration (t0tβ‚€) and magnitude (FF) of the applied force, as well as the system's natural properties (mm and kk). It’s a beautiful demonstration of how a transient force can leave a lasting imprint on a system, setting it into a new state of motion.

Conclusion: The Enduring Oscillation

So there you have it, folks! We've successfully navigated the twists and turns of a particle on a spring subjected to a temporary force. We started with a system at rest, introduced a constant force for a specific duration (t0tβ‚€), and then let the system run free. The result? A beautiful, persistent oscillation described by the equation y(t)=Fk[cos⁑(Ο‰(tβˆ’t0))βˆ’cos⁑(Ο‰t)]y(t) = \frac{F}{k} [\cos(\omega (t - tβ‚€)) - \cos(\omega t)] for t>t0t > tβ‚€. We even transformed this into a more insightful form, y(t)=βˆ’2Fksin⁑(Ο‰t02)sin⁑(Ο‰tβˆ’Ο‰t02)y(t) = -2 \frac{F}{k} \sin(\frac{\omega tβ‚€}{2}) \sin(\omega t - \frac{\omega tβ‚€}{2}), which clearly shows the oscillatory nature and an amplitude that depends critically on the duration t0tβ‚€ of the applied force.

This problem is a fantastic illustration of several key physics principles. Firstly, it showcases Newton's second law in action, governing the motion under different forces. Secondly, it highlights the concept of superposition, where the motion after the force is removed is a consequence of the system's response during the period the force was applied. The state of the system at t0tβ‚€ (its position and velocity) dictates the subsequent free oscillations. Thirdly, it demonstrates the principles of simple harmonic motion and how external perturbations can excite these oscillations. The fact that the amplitude of the resulting oscillation can be zero or maximal depending on t0tβ‚€ is a particularly neat outcome, showcasing the resonant-like behavior even with a constant force applied for a duration.

Understanding these dynamics is not just an academic exercise. It has real-world implications, from designing earthquake-resistant structures (where external forces are applied and then cease) to analyzing the behavior of mechanical systems and even in understanding the vibration of musical instruments. So, the next time you see a mass on a spring, remember that even a brief nudge can set it into a long-lasting dance!

Keep exploring, keep questioning, and keep enjoying the wonderful world of physics!