Relativistic rotational kinetic energy

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SUMMARY

The discussion centers on the formula for rotational kinetic energy in the context of relativistic velocities. The initial formula, E = 1/2 * L * w, where L is angular momentum and w is angular velocity, is deemed insufficient for relativistic scenarios. The correct approach involves using the total energy formula E² = m²c⁴ + p²c², leading to the kinetic energy expression KE = mc²(√(1 + γ²v²/c²) - 1). This highlights the importance of using rest mass and incorporating the Lorentz factor (γ) for accurate calculations in relativistic physics.

PREREQUISITES
  • Understanding of angular momentum (L = p * r)
  • Familiarity with angular velocity (w = v / r)
  • Knowledge of relativistic mass and the Lorentz factor (γ)
  • Basic principles of special relativity and energy-momentum relations
NEXT STEPS
  • Study the derivation of the total energy formula E² = m²c⁴ + p²c²
  • Learn about the Lorentz factor (γ) and its implications in relativistic physics
  • Explore the concept of relativistic kinetic energy and its applications
  • Investigate the relationship between linear momentum and angular momentum in relativistic contexts
USEFUL FOR

Physicists, students of advanced mechanics, and anyone interested in the implications of special relativity on rotational dynamics.

johne1618
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Hi,

I was wondering if the formula for rotational energy:

E = 1/2 * L * w

where L is the angular momentum and w is the angular velocity,
is actually correct for relativistic velocities.

Using

L = p * r

and

w = v / r

where

p = the linear momentum = m * v

We get:

E = 1/2 * (m * v * r) * (v/r)

I would have thought that this expression is correct up to relativistic velocity as the expressions for linear momentum, p = m * v, and angular velocity, w = v / r, do not require relativistic modification provided that we acknowledge that m increases as v -> c.

As a corollary, as v -> c, it seems that the maximum rotational energy of a system is:

E = 1/2 * m c^2 (i.e. half the total mass/energy of the system)

John
 
Last edited:
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Kinetic energy is not a particularly useful concept in special relativity. Neither is the 'relativistic mass.' Always use the rest mass and put in the factors of γ explicitly. The exact formula for the total energy of a particle is E2 = m2c4 + p2c2 where p = γmv. This can be written

E = mc2 √(1 + γ2v2/c2)

The kinetic energy will be the total E minus the rest energy:

KE = mc2(√(1 + γ2v2/c2) - 1)

This is still exact. For circular motion, just put in v = ω/r.
 

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