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On the Schwinger limit attainability with extreme power lasers

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Radiation friction effects<br />

du 2e<br />

ds 3c<br />

<br />

2<br />

2<br />

mec <br />

eFu <br />

g<br />

The radiation friction force in <strong>the</strong> Landau-Lifshitz form is given by<br />

Retaining <strong>the</strong> main order terms, we obtain equation for <strong>the</strong> x-component of <strong>the</strong> electron<br />

momentum<br />

2<br />

dpx 2 px re<br />

rad0 a (2 t)<br />

, rad<br />

<br />

dt m c 3<br />

Its solution is<br />

<br />

2 <br />

2<br />

2e<br />

Fe g u u F F u F u F u u<br />

3 2 <br />

3mec <br />

x<br />

mec <br />

<br />

p (0) m c m c<br />

p ( t) , p ( t)<br />

<br />

x e e<br />

x t<br />

2<br />

mec rad0px(0) a (2t ') dt '<br />

0<br />

x<br />

t<br />

2<br />

rad0lasa0 L. D. Landau, and E. M. Lifshitz, The Classical Theory of Fields, Pergamon, 1975<br />

I. Pomeranchuk, “Maximum Energy that Primary Cosmic-ray Electrons Can Acquire on <strong>the</strong> Surface of <strong>the</strong> Earth as a Result of Radiation in <strong>the</strong> Earth's Magnetic<br />

Field”, J. Phys. USSR, 2, 65 – 69, 1940<br />

e

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