Physics, asked by Anonymous, 3 months ago

Deduce the expressions for the kinetic energy and potential energy of a particle
executing S.H.M. Hence obtain the expression for total energy of a particle performing S.H.M and show that the total energy is conserved. State the factors on which total energy depends.​

Answers

Answered by StylusMrVirus
8

\begin{gathered} \\ \Large{\bf{\pink{\underline{Answer \::}}}} \\ \end{gathered}

We know that kinetic energy is given by,

K.E = 1/2 × m × v²

where m is the mass and v is the velocity of the body.

But we know,

,

\tt v=\pm \omega\sqrt{A^2-x^2}v

Hence,

\tt K.E=\dfrac{1}{2} \times m\times \omega^{2}\times (A^2-x^2)K.E=

Also,

ω² = k/m

k = ω²m

Substituting this we get,

\boxed{ \red{\tt K.E=\dfrac{1}{2} \times k\times (A^2-x^2)} }

Now deducing the equation for potential energy. Here work done by the particle is stored as potential energy.

dW = -f dx

dW = -(-kx) dx

dW = kx dx

Integrating this we from position 0 to x get,

get,

\displaystyle \sf \int\limits {dW}=\int\limits^x_0 k{x} \,

W = k x²/2

\boxed{ \red{\tt P.E=\dfrac{1}{2}\times k\times x^2 } }</p><p>

Now total energy of the particle is given by,

T.E = K.E + P.E

\tt { \red{T.E=\dfrac{1}{2}\:k\times (A^2-x^2)+ \dfrac{1}{2}\: k\times x^2 }}

\tt{ \red{T.E=\dfrac{1}{2}\:k(A^2-x^2+x^2)}}

\boxed{ \red{\tt T.E=\dfrac{1}{2}\:k\:A^2} }

Here k and A are constants for a given SHM motion, therefore the total energy is conserved.

Factors on which total energy depends:

From the above expression,

\tt  \red{T.E=\dfrac{1}{2}\:k\:A^2 }

\tt  \red{T.E=\dfrac{1}{2}\: m\: \omega^{2} \:A^2}

Hence total energy depends upon the mass, angular velocity and amplitude of the particle.


StylusMrVirus: Hope this helps you dear :)
Anonymous: well done
Answered by GraceS
18

\sf\huge\bold{Answer:}

Consider a particle of mass M performing linear SHM with amplitude A.

The restoring force acting on the particle is f = - kx

where, k = force constant

and x = the displacement of the particle from its mean position

Kinetic energy :

At distance x from the mean position the velocity is

\sf\bold\purple{:⟶v =  \omega \:  \sqrt{A {}^{2} - x {}^{2}    } } \\

where,\sf\bold\purple {:⟶\omega =  \sqrt{ \frac{k}{m} }}  \\ .The Kinetic Energy (KE) of the particle is

\sf\bold\purple{:⟶ KE =  \frac{1}{2} mv {}^{2}  =  \frac{1}{2}m \omega {}^{2}  \:  ({A}^{2}  - x {}^{2})}   \\

\sf\bold\purple{ :⟶KE =   \frac{1}{2} k  \:  ({A}^{2}  - x {}^{2})...(i)} \\

If the phase of particle at an in.stant is t is \sf \theta \:  =  \omega \: t + x , where a is initial phase , its velocity at that inst.ant is

\sf:⟶ v =  \omega \:A cos( \omega \: t + x)

and,its KE at that in.stant is

\sf\bold\purple {:⟶KE =  \frac{1}{2} mv {}^{2}  =  \frac{1}{2}  \omega{}^{2} A {}^{2} \cos {}^{2} ( \omega \: t + x) }  \\

\sf\bold\purple{:⟶ KE =  \frac{1}{2} k A {}^{2} \cos {}^{2} ( \omega \: t + x) ...(ii) } \\

Hence,KE varies with time as \sf \cos 2\theta

Potential energy :

Consider a particle of mass m , performing a linear SHM along the path MN about the mean position O. Let the particle be at P, at a distance x from O.

The corresponding work done by the external agent will be dW = (-F)dx = kxdx. This work done is stored in the form of potential energy .The potential energy of the particle when its displacement from the mean position is x can be found by integrating the above expression from 0 to x.

\sf\bold:⟶ PE = ∫ \: dW= \int\limits^x_0 {x} \: kx \\  =  \frac{1}{2}kx {}^{2} ...(iii)

The displacement of particle at an inst.ant t being

\sf :⟶x = A \sin( \omega \: t + x )

and PE at that in.stant is

\sf\bold\purple{ :⟶PE =  \frac{1}{2} kx {A}^{2}  =  \frac{1}{2} k { \: }^{2}  \sin( \omega \: t + x) ...(iv)} \\

Thus,PE varies with time as  \sf \sin {}^{2}  \theta

Total energy :

The total energy of the particle is equal to the sum of its potential energy and kinetic energy.

From equations (i) and (ii)

Total energy

E = PE + KE

\sf\bold\blue{ =  \frac{1}{2}kx {}^{2}  +  \frac{1}{2} k( {A}^{2} -  x {}^{2} ) }\\

\sf \bold\blue{=  \frac{1}{2}k {x}^{2}  +  \frac{1}{2} k {A}^{2}  -  \frac{1}{2} k {x}^{2} } \\

\bold\blue{ \therefore \: E =  \frac{1}{2} k {A}^{2}  =  \frac{1}{2} m \omega {}^{2}  {A}^{2} ...(v)} \\

Total energy is conserved :

As m is constant , and \sf \omega and a are constants of the motion, the total energy of the particle remains constant (or is conserved)

Factors on which total energy depends :

The total energy depends upon

  • the mass (m)
  • angular velocity \sf \omega
  • amplitude of the particle ( A )
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