On the Schwinger limit attainability with extreme power lasers
On the Schwinger limit attainability with extreme power lasers
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