Fast collisionless reconnection in electron-positron plasmas

被引:73
作者
Bessho, Naoki [1 ]
Bhattacharjee, A.
机构
[1] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
[2] Univ New Hampshire, Ctr Magnet Self Org, Inst Study Earth Oceans & Space, Durham, NH 03824 USA
关键词
D O I
10.1063/1.2714020
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Magnetic reconnection in electron-positron (pair) plasmas is studied by two-dimensional, electromagnetic, particle-in-cell simulations. In pair plasmas, the Hall current does not appear because there is no scale separation between ion and electron motion. Simulations show that fast reconnection is realized in both nonrelativistic and relativistic regimes. It is demonstrated that the divergence of the electron and positron pressure tensors essentially plays the role of an effective collisionless resistivity in realizing fast reconnection. Since there is no Hall current in pair plasmas, there is no quadrupolar structure in the out-of-plane magnetic field. Particle acceleration by reconnection is investigated. Major sites of particle acceleration are the regions in the vicinity of X lines, where ultrarelativistic particles are generated by the reconnection electric field. (C) 2007 American Institute of Physics.
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页数:9
相关论文
共 62 条
[1]   Collisionless reconnection in an electron-positron plasma [J].
Bessho, N ;
Bhattacharjee, A .
PHYSICAL REVIEW LETTERS, 2005, 95 (24)
[2]   Current singularities: Drivers of impulsive reconnection [J].
Bhattacharjee, A ;
Germaschewski, K ;
Ng, CS .
PHYSICS OF PLASMAS, 2005, 12 (04) :1-11
[3]  
Birn J, 2001, J GEOPHYS RES-SPACE, V106, P3715, DOI 10.1029/1999JA900449
[4]   Geospace Environment Modeling (GEM) magnetic reconnection challenge: Resistive tearing, anisotropic pressure and Hall effects [J].
Birn, J ;
Hesse, M .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2001, 106 (A3) :3737-3750
[5]   KINEMATICS OF RELATIVISTIC MAGNETIC RECONNECTION [J].
BLACKMAN, EG ;
FIELD, GB .
PHYSICAL REVIEW LETTERS, 1994, 72 (04) :494-497
[6]   Two fluid effects on three-dimensional reconnection in the Swarthmore Spheromak Experiment with comparisons to space data [J].
Brown, M. R. ;
Cothran, C. D. ;
Fung, J. .
PHYSICS OF PLASMAS, 2006, 13 (05)
[7]   MAGNETICALLY STRIPED RELATIVISTIC MAGNETOHYDRODYNAMIC WINDS - THE CRAB-NEBULA REVISITED [J].
CORONITI, FV .
ASTROPHYSICAL JOURNAL, 1990, 349 (02) :538-545
[8]   Hall current effects in dynamic magnetic reconnection solutions [J].
Craig, IJD ;
Heerikhuisen, J ;
Watson, PG .
PHYSICS OF PLASMAS, 2003, 10 (08) :3120-3130
[9]   Fully kinetic simulations of undriven magnetic reconnection with open boundary conditions [J].
Daughton, William ;
Scudder, Jack ;
Karimabadi, Homa .
PHYSICS OF PLASMAS, 2006, 13 (07)
[10]   Rapid magnetic reconnection in the Earth's magnetosphere mediated by whistler waves [J].
Deng, XH ;
Matsumoto, H .
NATURE, 2001, 410 (6828) :557-560