Mass loss and longevity of gravitationally bound oscillating scalar lumps (oscillatons) in D dimensions

G. Fodor, P. Forgács, Márk Mezei

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

Spherically symmetric oscillatons (also referred to as oscillating soliton stars) i.e. gravitationally bound oscillating scalar lumps are considered in theories containing a massive self-interacting real scalar field coupled to Einstein's gravity in 1+D dimensional spacetimes. Oscillations are known to decay by emitting scalar radiation with a characteristic time scale which is, however, extremely long, it can be comparable even to the lifetime of our universe. In the limit when the central density (or amplitude) of the oscillaton tends to zero (small-amplitude limit) a method is introduced to compute the transcendentally small amplitude of the outgoing waves. The results are illustrated in detail on the simplest case, a single massive free scalar field coupled to gravity.

Original languageEnglish
Article number064029
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume81
Issue number6
DOIs
Publication statusPublished - Mar 23 2010

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scalars
gravitation
universe
solitary waves
stars
life (durability)
oscillations
decay
radiation

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

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