American Astronomical Society, Astrophysical Journal, 2(684), p. 1477-1485, 2008
DOI: 10.1086/590425
Full text: Download
We investigate properties of the reconnecting current layer in relativistic pair plasma reconnection. We found that the current layer self-regulates its thickness when the current layer runs out current carriers, and so relativistic reconnection retains a fast reconnection rate. Constructing a steady state Sweet-Parker model, we discuss conditions for the current sheet expansion. Based on the energy argument, we conclude that the incompressible assumption is invalid in relativistic Sweet-Parker reconnection. The guide field cases are more incompressible than the anti-parallel cases, and we find a more significant current sheet expansion. ; Comment: Accepted for publication in Astrophysical Journal (to appear in vol. 685)