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Boson stars, hypothetical astrophysical objects bound by the self-gravity of a scalar field, have been widely studied as a type of exotic compact object that is horizonless and provides a testing ground for physics beyond the Standard…

广义相对论与量子宇宙学 · 物理学 2025-12-23 Yu Miyauchi , Takahiro Tanaka

There is increasing numerical evidence that scalar fields can form long-lived quasi-bound states around black holes. Recent perturbative and numerical relativity calculations have provided further confirmation in a variety of physical…

广义相对论与量子宇宙学 · 物理学 2017-07-19 Alejandro Escorihuela-Tomàs , Nicolas Sanchis-Gual , Juan Carlos Degollado , José A. Font

Ultralight boson is one of the potential candidates for dark matter. If exists, it can be generated by a rapidly rotating black hole via superradiance, extracting the energy and angular momentum of the black hole and forming a boson cloud.…

广义相对论与量子宇宙学 · 物理学 2023-09-15 Yao Guo , Wenjie Zhong , Yiqiu Ma , Daiqin Su

Boson stars arise as solutions of a massive complex scalar field coupled to gravity. A variety of scalar potentials, giving rise to different types of boson stars, have been studied in the literature. Here we study instead the effect of…

广义相对论与量子宇宙学 · 物理学 2023-11-17 Pablo A. Cano , Ludovico Machet , Charlotte Myin

Many gravitational phenomena that lie at the core of our understanding of the Universe have not yet been directly observed. An example in this sense is the boson star that has been proposed as an alternative to some compact objects…

There is accumulating evidence that (fundamental) scalar fields may exist in Nature. The gravitational collapse of such a boson cloud would lead to a boson star (BS) as a new type of a compact object. Similarly as for white dwarfs and…

天体物理学 · 物理学 2019-04-03 Franz E. Schunck , Eckehard W. Mielke

In a certain class of scalar-Gauss-Bonnet gravity, the black holes and the neutron stars can undergo spontaneous scalarization -- a strong gravity phase transition triggered by a tachyonic instability due to the nonminimal coupling between…

广义相对论与量子宇宙学 · 物理学 2021-10-18 Hao-Jui Kuan , Daniela D. Doneva , Stoytcho S. Yazadjiev

We report simulations regarding tidal disruption clouds orbiting spherically symmetric compact boson stars in two different regimes. First we consider clouds in three different bound orbits close to the boson star and analyze the mechanisms…

高能天体物理现象 · 物理学 2021-06-18 Matheus C. Teodoro , Lucas G. Collodel , Jutta Kunz

In this paper, we study the evolutions of a self-gravitating cloud of bosonic dark matter with finite angular momentum and self-interaction. This is achieved by using the sixth-order pseudospectral operator splitting method to solve the…

宇宙学与河外天体物理 · 物理学 2023-11-22 Kuldeep J. Purohit , Pravin Kumar Natwariya , Jitesh R. Bhatt , Prashant K. Mehta

Scalar particles are a common prediction of many beyond the Standard Model theories. If they are light and cold enough, there is a possibility they may form Bose-Einstein condensates, which will then become gravitationally bound. These…

宇宙学与河外天体物理 · 物理学 2016-10-19 Eric Cotner

We study the spontaneous scalarization of spherically symmetric, asymptotically flat boson stars in the $(\alpha {\cal R} + \gamma {\cal G}) \phi^2$ scalar-tensor gravity model. These compact objects are made of a complex valued scalar…

广义相对论与量子宇宙学 · 物理学 2019-10-02 Yves Brihaye , Betti Hartmann

This work studies the formation and growth of boson stars and their surrounding miniclusters by gravitational condensation using non-linear dynamical numerical methods. Fully dynamical attractive and repulsive self-interactions are also…

宇宙学与河外天体物理 · 物理学 2021-10-27 Jiajun Chen , Xiaolong Du , Erik W. Lentz , David J. E. Marsh , Jens C. Niemeyer

Black holes with masses $\approx 1\, M_{\odot}$ cannot be produced via stellar evolution. A popular scenario of their formation involves transmutation of neutron stars - by accumulation of dark matter triggering gravitational collapse in…

高能物理 - 唯象学 · 物理学 2022-03-28 Raghuveer Garani , Dmitry Levkov , Peter Tinyakov

Ultralight scalars can extract rotational energy from astrophysical black holes through superradiant instabilities, forming macroscopic boson clouds. This process is most efficient when the Compton wavelength of the boson is comparable to…

广义相对论与量子宇宙学 · 物理学 2019-05-17 Emanuele Berti , Richard Brito , Caio F. B. Macedo , Guilherme Raposo , Joao Luis Rosa

We study the transition of charged boson stars from sub- to super-criticality. This transition is defined as that choice of coupling constants for which the Coulomb repulsion of two individual bosons (that make up the star) exactly cancels…

广义相对论与量子宇宙学 · 物理学 2023-09-04 Yves Brihaye , Betti Hartmann

We investigate the gravitational evolution of dark matter halos made up of a massless bosonic field. The coupled Einstein-Klein-Gordon equations are solved numerically, showing that such a boson halo is stable and can be formed under a…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Jayashree Balakrishna , Franz E. Schunck

One class of competitive candidates for dark matter is ultralight bosons. If they exist, these bosons may form long-lived bosonic clouds surrounding rotating black holes via superradiant instabilities, acting as sources of gravity and…

广义相对论与量子宇宙学 · 物理学 2021-10-08 Adrian Ka-Wai Chung , Joseph Gais , Mark H. Y. Cheung , Tjonnie G. F. Li

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

The present surge for the astrophysical relevance of boson stars stems from the speculative possibility that these compact objects could provide a considerable fraction of the non-baryonic part of dark matter within the halo of galaxies.…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Eckehard W. Mielke , Franz E. Schunck

We study numerical evolutions of an initial cloud of self-gravitating bosonic dark matter with finite angular momentum and self-interaction in kinetic regime. It is demonstrated that such a system can undergo gravitational condensation and…

宇宙学与河外天体物理 · 物理学 2022-12-29 Kuldeep J. Purohit , Pravin Kumar Natwariya , Jitesh R. Bhatt , Prashant K. Mehta
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