2003
DOI: 10.1086/377391
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Understanding the Time-Asymmetry of Radiation

Abstract: I discuss the nature of the puzzle about the time-asymmetry of radiation and argue that its most common formulation is flawed. As a result, many proposed solutions fail to solve the real problem. I discuss a recent proposal of Mathias Frisch as an example of the tendency to address the wrong problem. I go on to suggest that the asymmetry of radiation, like the asymmetry of thermodynamics, results from the initial state of the universe.

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Cited by 28 publications
(17 citation statements)
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“…31 The experimental results reported in Angelopoulos et al (1998) give a direct demonstration of time reversal invariance in the sense that they do not (as earlier results did) appeal to observed CP violation and the CP T theorem. 32 T mech := m R d u u (x z). 33 An exception to the rule will be mentioned shortly.…”
Section: Notesmentioning
confidence: 99%
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“…31 The experimental results reported in Angelopoulos et al (1998) give a direct demonstration of time reversal invariance in the sense that they do not (as earlier results did) appeal to observed CP violation and the CP T theorem. 32 T mech := m R d u u (x z). 33 An exception to the rule will be mentioned shortly.…”
Section: Notesmentioning
confidence: 99%
“…a charge-current distribution J , satisfying r J = 0, is speci…ed, and one seeks to …nd the corresponding solution to the Maxwell equations. One could add a second well-de…ned problem: an external electromagnetic …eld ext F and a nonelectromagnetic force nem F are speci…ed, and one seeks to find the worldline z ( ) of a point mass carrying charge q by using the Lorentz force law and solving the resultant equation of motionma = q( ext F u ) + nem F(23)And combining the two also leads to a harmonious situation in that (i) the coupled Maxwell-Lorentz equations have a well-posed initial value problem and (ii) the total stress-energy tensor, consisting of the sum of the stressenergy tensor of the electromagnetic …eld and the mechanical stress-energy tensor of the particle,32 is conserved.Unfortunately, equation(23)is empirically inadequate, for accelerated charges radiate and, as a result, they experience a damping force that is not re ‡ected in (23). 33 The generally accepted equation of motion describing this phenomenon for a point charge in Minkowski spacetime is called the Lorentz-Dirac equation:ma = q( ext F u ) + nem F ext F u ) + nem F + 2 3 q 2 ( + u u ) _ awhere a := a a is the magnitude of the four-vector acceleration and is the Minkowski metric.…”
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confidence: 99%
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“…The account in the book is a revised version of Frisch's (2000). I have argued against this solution elsewhere (North 2003), but let me say a few things about it here.…”
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confidence: 99%