中文

MACHOs: The Plot Thickens

天体物理学 2007-05-23 v1 高能物理 - 唯象学

摘要

We discuss the implications of the recent upward revision of the LMC microlensing rate by the MACHO Collaboration. We conclude: (i) A good case for the existence of baryonic dark matter in the halo has been made; (ii) The case for the existence of cold dark matter is unaffected and still compelling; and (iii) The Galactic halo is still an excellent place to search for cold dark matter particles (e.g., axions or neutralinos).

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引用

@article{arxiv.astro-ph/9601168,
  title  = {MACHOs: The Plot Thickens},
  author = {Michael S. Turner and Evalyn I. Gates and Geza Gyuk},
  journal= {arXiv preprint arXiv:astro-ph/9601168},
  year   = {2007}
}

备注

6 pages, two figures, postscript