Scalar stars and lumps with AdS or dS cores

Cadoni, M.; Oi, M.; Pitzalis, M.; Sanna, A. P.

doi:10.1103/physrevd.109.084031

Phys. Rev. D

2024

DOI: 10.1103/physrevd.109.084031

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Scalar stars and lumps with AdS or dS cores

M. Cadoni,

M. Oi,

M. Pitzalis

et al.

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2024

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References 127 publications

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Gravitating Scalarons with Inverted Higgs Potential

Chew,

Lim

2024

Universe

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Previously, a class of regular and asymptotically flat gravitating scalar solitons (scalarons) has been constructed in the Einstein–Klein–Gordon (EKG) theory by adopting a phantom field with Higgs-like potential where the kinetic term has the wrong sign and the scalaron possesses the negative Arnowitt–Deser–Misner (ADM) mass as a consequence. In this paper, we demonstrate that the use of the phantom field can be avoided by inverting the Higgs-like potential in the EKG system when the kinetic term has a proper sign, such that the corresponding gravitating scalaron can possess the positive ADM mass. We systematically study the basic properties of the gravitating scalaron, such as the ADM mass, the energy conditions, the geodesics of test particles, etc. Moreover, we find that it can be smoothly connected to the counterpart hairy black hole solutions from our recent work in the small horizon limit.

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Gravitating Scalarons with Inverted Higgs Potential

Chew,

Lim

2024

Universe

View full text Add to dashboard Cite

show abstract

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Scalar stars and lumps with AdS or dS cores

Cited by 1 publication

References 127 publications

Gravitating Scalarons with Inverted Higgs Potential

Gravitating Scalarons with Inverted Higgs Potential

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