Difference between revisions of "Kinetic Energy"

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== Kinetic Energy in Relativity ==
 
== Kinetic Energy in Relativity ==
  
The energy of a particle in [[relativity]] is:
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In [[relativity]], kinetic energy can be expressed as:
  
<math> E = \gamma m_0 c^2 </math>
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<math> K = (\gamma - 1) m_0 c^2 </math>
  
where <math>\gamma</math> is the Lorentz factor, <math>m_0</math> is the [[rest mass]] and c is the [[speed of light]].
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where
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:<math>\gamma</math> is the [[Lorentz factor]]
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:<math>m_0</math> is the [[rest mass]]
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:<math>c</math> is the [[speed of light]]
  
Since this includes the mass energy of the particle, we must subtract a factor of <math> m_0 c^2 </math> to get the energy due to the particle's motion, the kinetic energy, as:
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===Derivation===
  
<math> K = (\gamma - 1) m_0 c^2 </math>
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The kinetic energy is the [[work|work done]] accelerating a particle from rest to some speed <math>v</math>. Suppose the particle is at rest at <math>x_1</math> and speed <math>v</math> at position <math>x_2</math>. Hence:
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 +
<math>K = \int^{x_2}_{x_1} \vec{F} \dot d \vec{x}</math>
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Since <math>\vec{F} = \vec{F}_{\perp} + \vec{F}_{\parallel}</math>, and a perpendicular force does no work, we can ignore the perpendicular component and write:
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<math>K = \int^{x_2}_{x_1} F_{\parallel} dx = \int^{x_2}_{x_1}  \gamma^3 m_0 a dx</math>
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Since <math>a \, dx = \frac{dv_{\parallel}}{dt} dx = \frac{dx}{dt} dv</math>, we find the integral can be rewritten as:
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<math>K = \int^{v_2}_{v_1} \frac{mv}{(1- \frac{v^2}{c^2})} dv</math>
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where <math>v_1</math> is the initial speed and hence 0 by definition and <math>v_2</math> is the final speed.
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Performing the integration reveals the kinetic energy as:
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 +
<math>K=(\gamma -1)m_0 c^2</math>
  
 
==References==
 
==References==

Revision as of 16:16, September 23, 2016

Kinetic energy represents the energy associated with the motion of an object.[1] It is defined as the work done by a force to accelerate that object from rest to some speed , in the absence of any other forces acting upon the object. Kinetic energy is a scalar and has the same units as work (i.e. Joule).

Classical mechanics

Translational kinetic energy

In classical mechanics, the translational kinetic energy of a ridid object, , can be found as:

Where

is the mass of the object
is the velocity of the object

Rotational kinetic energy

The rotational kinetic energy of a rigid object is:

Where

is the moment of inertia of the object
is the angular velocity of the object

Work-Energy theorem

The change of kinetic energy is equal to the total work done on it by the resultant of all forces acting on it. For a point mass this can be expressed as:

Where

is the initial speed
is the final speed

Note that if the mass of an object is increased, the increase in kinetic energy increases linearly; if the velocity of an object is increased, the increase in kinetic energy increases quadratically. For example, doubling the mass of an object doubles its kinetic energy; doubling its velocity quadruples its kinetic energy.

Derivation of translational kinetic energy

The work done by a force accelerating an object from rest, which is the kinetic energy is:

From Newton's second law, the force, , is . Hence we can make the substitution and use the chain rule

This is the same as

In classical mechanics, momentum is given by . Differentiating and substituting into the above equation results in

We want to integrate between 0 and the speed of the object, as this defines kinetic energy. Performing the integration reveals that the kinetic energy is, as expected, the following:

A similar method may be used to derive the formula for rotational kinetic energy.

Kinetic Energy in Relativity

In relativity, kinetic energy can be expressed as:

where

is the Lorentz factor
is the rest mass
is the speed of light

Derivation

The kinetic energy is the work done accelerating a particle from rest to some speed . Suppose the particle is at rest at and speed at position . Hence:

Since , and a perpendicular force does no work, we can ignore the perpendicular component and write:

Since , we find the integral can be rewritten as:

where is the initial speed and hence 0 by definition and is the final speed.

Performing the integration reveals the kinetic energy as:

References

  1. Serway and Beichner, Physics for Scientists and Engineers, Fifth Edition