Linearity of time evolution in classical mechanics

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SUMMARY

Time evolution in classical mechanics is predominantly non-linear, with linearity achieved in specific cases such as harmonic oscillators. The equation of motion for a damped harmonic oscillator is given by m \ddot{x} + 2 m \gamma \dot{x} + m \omega^2 x = F(t), where F(t) represents an external force, \gamma is the damping coefficient, and \omega is the eigenfrequency. This linear approximation is valid for small oscillations around a stable equilibrium point, where the potential can be expressed as a quadratic function. The harmonic oscillator serves as a foundational concept in both classical and quantum mechanics.

PREREQUISITES
  • Understanding of classical mechanics principles
  • Familiarity with differential equations
  • Knowledge of harmonic oscillators and their properties
  • Basic concepts of potential energy and stability
NEXT STEPS
  • Study the solutions of the harmonic oscillator equation of motion
  • Explore the Taylor series expansion for potential functions
  • Learn about the implications of damping in oscillatory systems
  • Investigate the role of harmonic oscillators in quantum mechanics
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This discussion is beneficial for physics students, educators, and researchers interested in classical mechanics, particularly those focusing on oscillatory systems and their applications in both classical and quantum contexts.

Anupama
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I came to know that time evolution in classical mechanics is highly non linear. Is there any case that it become linear?
 
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You get linear equations of motion for the important case of harmonic oscillators. The EoM reads
$$m \ddot{x}+2 m \gamma \dot{x}+m\omega^2 x=F,$$
where ##F=F(t)## is an external force, ##\gamma## the damping, and ##\omega## the eigenfrequency of the (undamped) oscillator.

It's among the most simple equations of state, and you should carefully study its solutions. It's often a good approximation for the bound motion around the minimum of a more complicated potential, if the deviation from this stable fix point doesn't become too large (small amplitudes of oscillations).
 
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Well, linearity is ensured if you can define a potential ##V## such that ##L=T-V## and this potential is at most quadratic in ##x##.
As stated in the post above, the (possibly driven and damped) harmonic oscillator is the standard (and probably the most important) example, since every potential can be written locally around its minimum as a quadratic potential (Taylor series). Hence, the harmonic oscillator is a good approximation for any (conservative) system around its stable equilibrium.
If you later on study quantum mechanics, you will also come across the harmonic oscillator several times.
 
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