@article{https://doi.org/10.48550/arxiv.1801.10534,<br/><span class="tab"></span>
  doi = {10.48550/ARXIV.1801.10534},<br/><span class="tab"></span>
  url = {https://arxiv.org/abs/1801.10534},<br/><span class="tab"></span>
  author = {Papini,<br/><span class="tab"></span> Emanuele and Landi,<br/><span class="tab"></span> Simone and Del Zanna,<br/><span class="tab"></span> Luca},<br/><span class="tab"></span>
  keywords = {Plasma Physics (physics.plasm-ph),<br/><span class="tab"></span> High Energy Astrophysical Phenomena (astro-ph.HE),<br/><span class="tab"></span> Solar and Stellar Astrophysics (astro-ph.SR),<br/><span class="tab"></span> Space Physics (physics.space-ph),<br/><span class="tab"></span> FOS: Physical sciences,<br/><span class="tab"></span> FOS: Physical sciences},<br/><span class="tab"></span>
  title = {Fast magnetic reconnection: The "ideal" tearing instability in classic,<br/><span class="tab"></span> Hall,<br/><span class="tab"></span> and relativistic plasmas},<br/><span class="tab"></span>
  publisher = {arXiv},<br/><span class="tab"></span>
  year = {2018},<br/><span class="tab"></span>
  copyright = {arXiv.org perpetual,<br/><span class="tab"></span> non-exclusive license}
}