Consider a massless relativistic particle approaching a potential step of height V _ 0 with energy E _ 0 and momentum p.
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They are known as radio bubbles, because they appear as emitters of radio waves due to the relativistic particles in the bubble.
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One interpretation of the paradox is that a potential step cannot reverse the direction of the group velocity of a massless relativistic particle.
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Radio relics can be divided into two main groups : Cluster radio shocks or radio gischt are large elongated, often relativistic particles.
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The free Lagrangian is the Taylor expansion of free Lagrangian of two relativistic particles to second order in " v ".
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In 1967 he published the first specific suggestion that strongly magnetized neutron stars could release their rotational energy and produce a large flow of relativistic particles.
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:I believe what you may be refering to is the issue with relativistic particles that carry momentum despite the rest mass of such particles being zero.
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:: : Just making sure the information above is clear, the Dirac equation is used to describe relativistic particles that have spin 1 / 2.
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This world-tube describes the region of non-covariance of the relativistic collective variables and puts a theoretical limit for the localization of relativistic particles.
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Maxwell Boltzmann statistics can be used to extend that distribution to particles with a different energy momentum relation, such as relativistic particles ( Maxwell J�ttner distribution ).
