Stationary scalar hair on a reflecting compact star is unstable when the scalar frequency is small, with ω²/m² ≤ 1/3.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
On instabilities of stationary scalar field configurations supported by reflecting compact stars
Stationary scalar hair on a reflecting compact star is unstable when the scalar frequency is small, with ω²/m² ≤ 1/3.