Radiation back reaction in classical electrodynamics

In summary, radiation back reaction in classical electrodynamics refers to the effect of emitted radiation on the motion of a charged particle. This phenomenon occurs when a charged particle accelerates, creating an electromagnetic field and subsequently emitting radiation. The emitted radiation carries away energy and momentum from the particle, causing it to experience a reaction force in the opposite direction. This back reaction can have significant impacts on the dynamics of charged particles, particularly in systems with high acceleration and strong electromagnetic fields. Understanding radiation back reaction is crucial in various areas of physics, including astrophysics and accelerator technologies.
  • #1
HomogenousCow
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I've been doing some research on the topic of radiation reaction force/self force in classical electrodynamics and although there are some discussions on the internet I would like direct answers to these following questions:

  1. Is there a rigorous and universally accepted treatment of radiation reaction force in classical electrodynamics for point particles? If so what was the breakthrough that solved the issues plaguing the seminal works such as pre-acceleration and runaway solutions?
  2. If we couple Maxwell's equations to a dynamical extended body, such as a charged fluid, do the resulting equations suffer from the typical issues encountered with point sources? And if not, does this treatment predict radiation reaction force that is physically reasonable?
  3. Is classical electrodynamics coupled to fluid dynamics a mathematically sound theory? As in, are there results on the existence and uniqueness of solutions in this theory.
 
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HomogenousCow said:
If so what was the breakthrough that solved the issues plaguing the seminal works such as pre-acceleration and runaway solutions?
There is no such breakthrough. Those issues remain unresolved.

HomogenousCow said:
If we couple Maxwell's equations to a dynamical extended body, such as a charged fluid, do the resulting equations suffer from the typical issues encountered with point sources? And if not, does this treatment predict radiation reaction force that is physically reasonable?
Extended bodies with charge densities that are everywhere finite are physically reasonable.

HomogenousCow said:
Is classical electrodynamics coupled to fluid dynamics a mathematically sound theory? As in, are there results on the existence and uniqueness of solutions in this theory.
I don’t know, but I am not aware of problems like those with classical point particles.
 
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  • #3
HomogenousCow said:
Is classical electrodynamics coupled to fluid dynamics a mathematically sound theory? As in, are there results on the existence and uniqueness of solutions in this theory.
I don't know if existence and uniqueness has been settled (I really doubt it), but a 30-second google search yielded some interesting hits like
https://www.jstor.org/stable/20209485
http://wrap.warwick.ac.uk/66955/
This is more in the realm of mathematics than physics, in that few physicists probably have the tools (or inclination) to make much progress on that front.

Even if those issues haven't been resolved, fluid models of plasmas have been pretty successful at describing physical phenomena. So have the more accurate kinetic models that can be used to derive fluid models by taking velocity-space moments.

jason
 
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  • #4
According to "numerical studies" the best we have on the classical level concerning the radiation-reaction problem is the Landau-Lifshitz approximation to the Lorentz-Abraham-Dirac equation. For a nice treatment, see

C. Nakhleh, The Lorentz-Dirac and Landau-Lifshitz equations from the perspective of
modern renormalization theory, Am. J. Phys 81, 180 (2013),
https://dx.doi.org/10.1119/1.4773292.
https://arxiv.org/abs/1207.1745

K. Lechner, Classical Electrodynamics, Springer International Publishing AG, Cham
(2018), https://doi.org/10.1007/978-3-319-91809-9
 
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  • #5
In his derivation, Lechner states on page 467, "Ultimately the Lorentz Dirac equation must be postulated."
 
  • #6
But the LAD equation is not the solution! The Landau-Lifshitz approximation is much better. A quantum-Langevin approach (at least for the non-relativistic case) suggests that the real matter is a non-Markovian description on the classical level, which avoids all the problems of the LAD equation right away. For this, see

G. W. Ford, J. T. Lewis and R. F. O’Connell, Quantum
Langevin equation, Phys. Rev. A 37, 4419 (1988),
https://doi.org/10.1103/PhysRevA.37.4419

or

https://doi.org/10.1016/0375-9601(91)90054-C
 

FAQ: Radiation back reaction in classical electrodynamics

What is radiation back reaction in classical electrodynamics?

Radiation back reaction refers to the effect that the emission of electromagnetic radiation has on the motion of a charged particle. When a charged particle accelerates, it emits radiation, and this emission carries momentum and energy away from the particle, influencing its subsequent motion. This effect is described by the self-interaction of the particle with its own electromagnetic field.

How is the radiation reaction force described mathematically?

The radiation reaction force in classical electrodynamics is commonly described by the Abraham-Lorentz force. This force can be expressed as \( \mathbf{F}_{\text{rad}} = \frac{\mu_0 q^2}{6 \pi c} \frac{d^3 \mathbf{r}}{dt^3} \), where \( q \) is the charge of the particle, \( \mu_0 \) is the permeability of free space, \( c \) is the speed of light, and \( \frac{d^3 \mathbf{r}}{dt^3} \) is the third time derivative of the particle's position, also known as the "jerk."

What are some problems associated with the classical description of radiation reaction?

The classical description of radiation reaction, particularly the Abraham-Lorentz force, leads to several issues. One major problem is the occurrence of "runaway solutions," where a particle's acceleration increases exponentially without bound. Another issue is "pre-acceleration," where a particle appears to start accelerating before the force is applied. These non-physical solutions suggest limitations in the classical theory and the need for more refined models or quantum mechanical treatments.

How does the Landau-Lifshitz equation address the issues with the Abraham-Lorentz force?

The Landau-Lifshitz equation is an alternative formulation that aims to mitigate the issues associated with the Abraham-Lorentz force. It provides a perturbative solution that avoids runaway solutions and pre-acceleration by considering the radiation reaction force as a small correction to the motion of the particle. This equation is more stable and physically realistic for most practical scenarios involving radiation reaction.

How does quantum electrodynamics (QED) handle radiation back reaction?

Quantum electrodynamics (QED) provides a more comprehensive framework for dealing with radiation back reaction by incorporating quantum effects. In QED, the interaction between charged particles and the electromagnetic field is treated probabilistically, and the emission of radiation is described by the exchange of virtual photons. This approach inherently avoids the classical problems of runaway solutions and pre-acceleration, as it accounts for the discrete nature of radiation emission and the quantization of the electromagnetic field.

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