The potential energy function for a particle executing linear simple harmonic motion is given by V(x) = kx2/2, where k is the force constant of the oscillator. For k = 0.5 N m-1, the graph of V(x) versus x is shown in Fig. 5.12. Show that a particle of total energy 1 J moving under this potential must ‘turn back’ when it reaches x = ± 2 m.
Total energy of the particle, E = 1 J
Force constant, k = 0.5 N m–1
Kinetic energy of the particle, K =\( \frac{1 }{ 2}\) mv2
According to the conservation law: E = V + K
1 =\(\frac{ 1 }{ 2} \) kx2 + \(\frac{ 1 }{ 2} \) mv2
At the moment of ‘turn back’, velocity (and hence K) becomes zero.
∴ 1 = \(\frac{1 }{2 }\) kx2
\(\frac{1 }{2 }\) × 0.5 x2 = 1
x2 = 4
x = ± 2
Hence, the particle turns back when it reaches x = ± 2m.
The energy retained by an object as a result of its stationery position is known as potential energy. The intrinsic energy of the body to its static position is known as potential energy.
The joule, abbreviated J, is the SI unit of potential energy. William Rankine, a Scottish engineer, and physicist coined the word "potential energy" in the nineteenth century. Elastic potential energy and gravitational potential energy are the two types of potential energy.
The formula for gravitational potential energy is
PE = mgh
Where,
Potential energy is one of the two main forms of energy, along with kinetic energy. There are two main types of potential energy and they are: