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183_notes:point_particle [2014/10/03 21:08] – caballero | 183_notes:point_particle [2021/05/06 20:42] (current) – [The Total Energy of a Single Particle] stumptyl | ||
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+ | Section 6.2 in Matter and Interactions (4th edition) | ||
+ | |||
===== The Simplest System: A Single Particle ===== | ===== The Simplest System: A Single Particle ===== | ||
- | The [[183_notes: | + | The [[183_notes: |
+ | ==== Lecture Video ==== | ||
+ | |||
+ | {{youtube> | ||
==== The Total Energy of a Single Particle ==== | ==== The Total Energy of a Single Particle ==== | ||
- | [{{183_notes: | + | [{{ 183_notes:week7_cartopoint.png?500|A real car crushed down to a point particle for the purpose of modeling the translation of the car. }}] |
- | The systems that you will consider will be approximated by a single object, | + | The systems that you will consider will be approximated by a single object, |
Thanks to Einstein, we know the total energy of a single particle system is given by, | Thanks to Einstein, we know the total energy of a single particle system is given by, | ||
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Etot=γmc2 | Etot=γmc2 | ||
- | where m is the mass of the particle, c is the speed of light in vacuum (3$\times$10^8 m/s), and γ is the [[183_notes: | + | where m is the mass of the particle, c is the speed of light in vacuum (3$\times10^8$ m/s), and γ is the [[183_notes: |
- | Etot=γmc2=1√1−v2/c2mc2=1√1−02/c2mc2=mc2 | + | $$E_{tot} = \gamma m c^2 = \dfrac{1}{\sqrt{1-(v^2/c^2)}}mc^2 = \dfrac{1}{\sqrt{1-(0^2/c^2)}} mc^2 = mc^2$$ |
Evidently, a particle at rest has a total energy that is simply associated with its mass. This is called the // | Evidently, a particle at rest has a total energy that is simply associated with its mass. This is called the // | ||
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Erest=mc2 | Erest=mc2 | ||
- | It appears that the rest of the energy is associated with the motion of the particle. As such, it is refereed to as the //kinetic energy// of the particle. | + | It appears that the rest of the energy is associated with the motion of the particle. As such, it is refereed to as the __**kinetic energy |
K=Etot−Erest=γmc2−mc2=(γ−1)mc2 | K=Etot−Erest=γmc2−mc2=(γ−1)mc2 | ||
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This is probably not the form of the kinetic energy that you are used to seeing. This is because for most purposes, objects are moving slowly enough where the relativistic correction doesn' | This is probably not the form of the kinetic energy that you are used to seeing. This is because for most purposes, objects are moving slowly enough where the relativistic correction doesn' | ||
- | K=(γ−1)mc2=(1√1−v2/c2−1)mc2≈((1+12v2c2)−1)mc2=12v2c2mc2=12mv2 | + | $$K = (\gamma - 1)mc^2 = \left(\dfrac{1}{\sqrt{1-v^2/ |
This definition of kinetic energy is due to Newton, but was confirmed by Coriolis and others. The total energy of a particle is thus the sum of its rest mass energy and its kinetic energy, which at low speeds is given by, | This definition of kinetic energy is due to Newton, but was confirmed by Coriolis and others. The total energy of a particle is thus the sum of its rest mass energy and its kinetic energy, which at low speeds is given by, | ||
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Etot=Erest+K=mc2+12mv2 | Etot=Erest+K=mc2+12mv2 | ||
- | For the time being you will neglect heat exchanges (although you will later relax that assumption), | + | For the time being you will neglect heat exchanges (although you will [[183_notes: |
ΔEtot=ΔErest+ΔK=Wsurr | ΔEtot=ΔErest+ΔK=Wsurr | ||
- | If the particle does not change | + | If the particle does not change |
ΔK=Kf−Ki=Wsurr | ΔK=Kf−Ki=Wsurr | ||
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Kf=Ki+W | Kf=Ki+W | ||
- | This is the update form of the [[183_notes: | + | This is the update form of the [[183_notes: |