Dirac-star-plus-wormhole configurations

2025

Full text Open access: Gold Metadata (CSL-JSON)
DOI 10.1088/1742-6596/3089/1/012007
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

Abstract We study configurations consisting of a gravitating linear spinor field and a massless ghost scalar field providing a nontrivial spacetime topology. For such a mixed system, we have constructed two families of asymptotically flat asymmetric solutions describing localized configurations (Dirac stars) possessing a wormhole topology. The physical properties of such systems are completely determined by the values of the spinor frequency and the throat parameter. For a fixed value of the latter, we have compared mass curves for the two families of solutions and revealed considerable differences in their behavior and physical properties of the systems under consideration (the configurations may be regular or singular and possess one or two throats, as well as they may contain possible event horizons).