中文

强磁场下 H$_2^{+}$ 分子离子:基态

天体物理学 2008-11-26 v1

摘要

presented for magnetic field ranging from 04.414×1013G0 - 4.414 \times 10^{13} G. The present study is focused on the question of the existence of the molecular ion H2+H_2^{+} in a magnetic field. As a tool, a variational method with an optimization of the form of the vector potential (optimal gauge fixing) is used. It is shown that in the domain of applicability of the non-relativistic approximation the system (ppe)(ppe) in the Born-Oppenheimer approximation has a well-pronounced minimum in the total energy at a finite interproton distance for B1011GB \lesssim 10^{11} G, thus manifesting the existence of H2+H_2^{+}. For B1011GB \gtrsim 10^{11} G and large inclinations (of the molecular axis with respect to the magnetic line) the minimum disappears and hence the molecular ion H2+H_2^{+} does not exist. It is shown that the most stable configuration of H2+H_2^{+} always corresponds to protons situated along the magnetic line. With magnetic field growth the ion H2+H_2^{+} becomes more and more tightly bound and compact, and the electronic distribution evolves from a two-peak to a one-peak pattern. The domain of inclinations where the H2+H_2^{+} ion exists reduces with magnetic field increase and finally becomes 0o25o0^o - 25^o at B=4.414×1013GB = 4.414 \times 10^{13} G. Phase transition type behavior of variational parameters for some interproton distances related to the beginning of the chemical reaction H2+H+pH_2^{+} \leftrightarrow H + p is found.

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引用

@article{arxiv.astro-ph/0212463,
  title  = {$H_2^{+}$ molecular ion in a strong magnetic field: ground state},
  author = {J. C. Lopez Vieyra and A. V. Turbiner},
  journal= {arXiv preprint arXiv:astro-ph/0212463},
  year   = {2008}
}

备注

RevTeX 4, 36 pages, 19 Figs. (figures 14-18 should be requested from the authors)