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Scalar boson stars have attracted attention as simple models for exploring the nonlinear dynamics of a large class of ultra compact and black hole mimicking objects. Here, we study the impact of interactions in the scalar matter making up…

广义相对论与量子宇宙学 · 物理学 2023-06-14 Nils Siemonsen , William E. East

We study the geodesic motion of test particles in the space-time of non-compact boson stars. These objects are made of a self-interacting scalar field and -- depending on the scalar field's mass -- can be as dense as neutron stars or even…

广义相对论与量子宇宙学 · 物理学 2013-08-21 Valeria Diemer , Keno Eilers , Betti Hartmann , Isabell Schaffer , Catalin Toma

The quasinormal modes of relativistic compact objects encode important information about the gravitational response associated with astrophysical phenomena. Detecting such oscillations would provide us with a unique understanding of the…

广义相对论与量子宇宙学 · 物理学 2016-04-20 Caio F. B. Macedo , Vitor Cardoso , Luís C. B. Crispino , Paolo Pani

We study {\it analytically} the physical and mathematical properties of spatially regular massless scalar field configurations which are non-minimally coupled to the electromagnetic field of a spherically symmetric charged reflecting shell.…

广义相对论与量子宇宙学 · 物理学 2021-06-16 Shahar Hod

We investigate the boson star with the self-interacting scalar field as a model of galactic halos. The model has slightly increasing rotation curves and allows wider ranges of the mass($m$) and coupling($\lambda$) of the halo dark matter…

高能物理 - 唯象学 · 物理学 2010-11-19 Jae-weon Lee , In-guy Koh

We propose that stable boson stars generically fall within an infinite-parameter family of solutions that oscillate on any number of non-commensurate frequencies. We numerically construct two-frequency solutions and explore their parameter…

广义相对论与量子宇宙学 · 物理学 2019-10-02 Matthew Choptuik , Ramon Masachs , Benson Way

It has recently been revealed that dyonic black-hole spacetimes of a quasitopological non-linear electrodynamic field theory may be characterized by discrete radial regions with the property $dg_{tt}(r)/dr=0$ in which spherically symmetric…

广义相对论与量子宇宙学 · 物理学 2026-05-15 Shahar Hod

A new solution to the coupled gravitational and scalar field equations for a condensed boson field is found in Newtonian approximation. The solution is axially symmetric, but not spherically symmetric. For N particles the mass of the object…

天体物理学 · 物理学 2009-10-28 B. Schupp , J. J. van der Bij

Topological stars are regular, horizonless solitons arising from dimensional compactification of Einstein-Maxwell theory in five dimensions, which could describe qualitative properties of microstate geometries for astrophysical black holes.…

广义相对论与量子宇宙学 · 物理学 2025-02-10 Alexandru Dima , Marco Melis , Paolo Pani

We study a self-gravitating ultralight dark matter condensate (a boson star) hosting a central black hole, in the nonrelativistic limit, which we refer to as a boson star black hole (BS-BH) system. We numerically solve the equations of…

广义相对论与量子宇宙学 · 物理学 2026-05-14 Amitayus Banik , Jeong Han Kim , Xing-Yu Yang

Solitonic boson stars (SBS) are compact shell-like objects with an inside having a nearly constant value of scalar field bounded by a thin shell where the scalar field rapidly changes. While the spherically symmetric SBS can be described by…

广义相对论与量子宇宙学 · 物理学 2024-04-08 Nikolay Sukhov

Axions and axion-like particles are a leading model for the dark matter in the Universe; therefore, dark matter halos may be boson stars in the process of collapsing. We examine a class of static boson stars with a non-minimal coupling to…

宇宙学与河外天体物理 · 物理学 2017-11-22 Jeremy Heyl , Matthew W. Choptuik , David Shinkaruk

We study boson star configurations with generic, but not non-topological, self-interaction terms, i.e. we do not restrict ourselves just to consider the standard $\lambda |\psi|^4$ interaction but more general U(1)-symmetry-preserving…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Franz E. Schunck , Diego F. Torres

We consider charged boson stars and study their effect on the structure of the vacuum. For very compact particle like ``stars", with constituent mass $m_{*}$ close to the Planck mass $m_{Pl}$, i.e. $m_{*}^{2} = {\cal O} (\alpha…

天体物理学 · 物理学 2019-08-17 P. Jetzer , P. Liljenberg , B. -S. Skagerstam

We investigate the complete family of (aligned) Robinson-Trautman spacetimes sourced by conformally invariant non-linear electrodynamics in $D$ dimensions in the presence of an arbitrary cosmological constant. After presenting general…

广义相对论与量子宇宙学 · 物理学 2021-12-24 David Kokoška , Marcello Ortaggio

We give good approximate analytic solutions for spherical charged boson stars in the large scalar-self-coupling limit in general relativity. We show that if the charge $e$ and mass $m$ of the scalar field nearly satisfy the critical…

广义相对论与量子宇宙学 · 物理学 2018-03-29 Nahomi Kan , Kiyoshi Shiraishi

Binary boson stars can be used to model the nonlinear dynamics and gravitational wave signals of merging ultracompact, but horizonless, objects. However, doing so requires initial data satisfying the Hamiltonian and momentum constraints of…

广义相对论与量子宇宙学 · 物理学 2023-12-05 Nils Siemonsen , William E. East

Spherical clusters of SU(2) BPS monopoles are investigated here. A large class of monopole solutions is found using an abelian approximation, where the clusters are spherically symmetric, although exact solutions cannot have this symmetry…

高能物理 - 理论 · 物理学 2013-05-30 N. S. Manton

We construct and explore the complex structures of boson stars, drawing inspiration from similar configurations of non-topological solitons in Minkowski space. These "molecular states" of boson stars have a multipolar structure and both…

广义相对论与量子宇宙学 · 物理学 2024-12-04 Víctor Jaramillo , Shuang-Yong Zhou

We analyze the dynamics of a gravitational bounded cloud of generic bosons or a boson star in the non-relativistic regime, assuming from the very beginning that the boson star is in a Bose-Einstein condensed state. Also, we have taken into…

广义相对论与量子宇宙学 · 物理学 2024-11-05 Jorge Mastache , Elías Castellanos , Guillermo Chacón-Acosta