Boson-star formation by classical instability

Details Boson-star formation by classical instability Boson-star formation by classical instability

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..41.2998g&link_type=abstract

Physical Review D (Particles and Fields), Volume 41, Issue 10, 15 May 1990, pp.2998-3002

Physics

12

Scientific paper

A new mechanism to form boson and minisoliton stars is proposed. These
objects could be generated by the second-order phase transition due to
the ground-state instability of a gravitational interacting scalar
field. It is shown that this process manifests itself as a conventional
gravitational collapse.

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