Special Relativity Force and Linearization

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SUMMARY

The discussion focuses on linearizing the equation of motion for a particle moving at relativistic speeds under the influence of a small oscillatory force F(t). The equation of motion is given by \(\vec{F}(t) = \dfrac{d}{dt}(\gamma m \vec{v})\), where \(\gamma\) is the Lorentz factor. Participants explore the correct method to linearize the terms involving \(\gamma\) and its derivatives, emphasizing the need to expand \(\gamma\) in powers of velocity. The goal is to determine the acceleration of the particle when the force is applied both parallel and perpendicular to the initial velocity.

PREREQUISITES
  • Understanding of Special Relativity concepts, particularly Lorentz transformations.
  • Familiarity with the Lorentz factor (\(\gamma\)) and its mathematical properties.
  • Basic knowledge of calculus, specifically differentiation and Taylor series expansion.
  • Experience with classical mechanics, particularly Newton's laws of motion.
NEXT STEPS
  • Study the derivation and implications of the Lorentz factor in Special Relativity.
  • Learn about Taylor series expansion and its applications in physics.
  • Research the effects of oscillatory forces on relativistic particles.
  • Explore advanced topics in relativistic dynamics, including the relationship between force and acceleration in different frames of reference.
USEFUL FOR

Students and professionals in physics, particularly those studying or working in the fields of theoretical physics, relativistic mechanics, and advanced dynamics. This discussion is beneficial for anyone looking to deepen their understanding of the mathematical treatment of forces in relativistic contexts.

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Homework Statement



Consider a particle moving at close to the speed of light with v \approx c \ \hat{z}. A small oscillatory force F(t) acts on the particle. Consider F(t) to be a first order (eg. linear) perturbation which will not effect v_o, only v_1, the first order component of v. Linearize the equation of motion and find the acceleration when F(t) is perpendicular and when F(t) is parallel to v_o.

Homework Equations



\vec{F}(t) = \dfrac{d}{dt}(\gamma m \vec{v})

The Attempt at a Solution



My trouble is with linearizing the equation.

\vec{F} = m\vec{v} \dfrac{d \gamma}{dt} + m \gamma \dfrac{d\vec{v}}{dt}

Then linearize each term so:

\vec{v} \dfrac{d \gamma}{dt} = \vec{v}_o\dot{\gamma}_o + \dfrac{d}{d \vec{v}} [\vec{v}\dot{\gamma} ] \mid_{\vec{v}= {\vec{v}_o, \dot{\gamma}= \dot{\gamma_o}}}(\vec{v} - \vec{v}_o) + \dfrac{d}{d \dot{\gamma}}[\vec{v} \dot{\gamma}] \mid_{\vec{v}= {\vec{v}_o,\dot{ \gamma}= \dot{\gamma}_o}} (\dot{\gamma} - \dot{\gamma}_o) = \vec{v}_o\dot{\gamma_o} +\dot{\gamma}_o (\vec{v} - \vec{v}_o) + \vec{v}_o(\dot{\gamma} - \dot{\gamma_o})

And then do the next term similarly. Is this the correct way to linearize?
 
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You also need to expand \gamma (and its derivative) in powers of the velocity.
 

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