Destabilization of neutron stars by type I dimension bubbles

E. I. Guendelman, J. R. Morris

Research output: Contribution to journalArticlepeer-review

3 Scopus citations


An inhomogeneous compactification of a higher-dimensional spacetime can result in the formation of type I dimension bubbles, i.e., nontopological solitons which tend to absorb and entrap massive particle modes. We consider possible consequences of a neutron star that harbors such a soliton. The astrophysical outcome depends upon the model parameters for the dimension bubble, with a special sensitivity to the bubble's energy scale. For relatively small energy scales, the bubble tends to rapidly consume the star without forming a black hole. For larger energy scales, the bubble grows to a critical mass, then forms a black hole within the star, which subsequently causes the remaining star to collapse. It is possible that the latter scenario is associated with core collapse explosions and gamma ray bursts.

Original languageEnglish
Pages (from-to)194-198
Number of pages5
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Issue number3-4
StatePublished - 24 Feb 2005


  • Dimension bubble
  • Nontopological solitons

ASJC Scopus subject areas

  • Nuclear and High Energy Physics


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