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Compact bosonic field configurations, or boson stars, are promising dark matter candidates which have been invoked as an alternative description for the supermassive compact objects in active galactic nuclei. Boson stars can be comparable…

广义相对论与量子宇宙学 · 物理学 2013-09-26 Caio F. B. Macedo , Paolo Pani , Vitor Cardoso , Luís C. B. Crispino

We investigate the possible gravitational redshift values for boson stars with a self-interaction, studying a wide range of possible masses. We find a limiting value of z_lim \simeq 0.687 for stable boson star configurations. We can exclude…

天体物理学 · 物理学 2015-05-13 Franz E. Schunck , Andrew R. Liddle

Dark matter may be in the form of non-baryonic structures such as compact subhalos and boson stars. Structures weighing between asteroid and solar masses may be discovered via gravitational microlensing, an astronomical probe that has in…

宇宙学与河外天体物理 · 物理学 2020-04-15 Djuna Croon , David McKeen , Nirmal Raj

We consider galaxy halos formed by dark matter bosons with mass in the range of about a few tens or hundreds eV. A major part of the particles is in a noncondensed state and described under the Thomas-Fermi approach. Derived equations are…

星系天体物理 · 物理学 2021-12-08 Iskander G. Abdullin , Vladimir A. Popov

We use the flexibility of the concept of a fermion-boson star to explore different configurations, ranging from objects of atomic size and masses of the order $10^{18}$ g, up to objects of galactic masses and gigantic halos around a smaller…

天体物理学 · 物理学 2009-11-07 Alfredo B. Henriques , Luis E. Mendes

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

Observations of the Sgr A* region in the galactic center confirm the presence of a large amount of matter in a small volume, leading to the consensus that a black hole exists there. However, dynamical observations cannot rule out the…

广义相对论与量子宇宙学 · 物理学 2013-01-09 Amitai Y. Bin-Nun

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

We explore whether supermassive non-baryonic stars (in particular boson, mini-boson and non-topological soliton stars) might be at the center of some galaxies, with special attention to the Milky Way. We analyze, from a dynamical point of…

天体物理学 · 物理学 2009-10-31 Diego F. Torres , S. Capozziello , G. Lambiase

We discuss boson stars as possible gravitational lenses and study the lensing effect by these objects made of scalar particles. The mass and the size of a boson star may vary from an individual Newtonian object similar to the Sun to the…

天体物理学 · 物理学 2009-10-30 Mariusz P. Dabrowski , Franz E. Schunck

If the dark matter particles are axions, gravity can cause them to coalesce into axion stars, which are stable gravitationally bound systems of axions. In the previously known solutions for axion stars, gravity and the attractive force…

高能物理 - 唯象学 · 物理学 2016-09-20 Eric Braaten , Abhishek Mohapatra , Hong Zhang

We study equilibrium configurations of boson stars in the framework of a class scalar-tensor theories of gravity with massive gravitational scalar (dilaton). In particular we investigate the influence of the mass of the dilaton on the boson…

广义相对论与量子宇宙学 · 物理学 2009-10-31 P. Fiziev , S. Yazadjiev , T. Boyadjiev , M. Todorov

In a recent work (Torres, Capozziello and Lambiase, Physical Review D62, 104012 (2000)), it was shown that a supermassive boson star could provide an alternative model for the galactic center, usually assumed as a black hole. Here we…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Diego F. Torres , S. Capozziello , G. Lambiase

Boson stars coupled to Einstein's general relativity possess some features similar to gravastars, such as the anisotropy in principal pressures and relatively large compactness ($\mu_{max} = 0.32$). However, no matter how large the…

广义相对论与量子宇宙学 · 物理学 2015-12-18 Anja Marunovic

Light bosonic fields may suffer an instability around a rotating compact object. This process, known as superradiance, leads to the exponential amplification of the field around a black hole or neutron star, while the spin of the central…

高能物理 - 唯象学 · 物理学 2026-03-16 Francesca Chadha-Day

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

A fraction of light scalar dark matter, especially axions, may organize into Bose-Einstein condensates, gravitationally bound clumps, "boson stars", and be present in large number in galactic halos today. We compute the expected number of…

高能物理 - 唯象学 · 物理学 2022-06-22 Kohei Fujikura , Mark P. Hertzberg , Enrico D. Schiappacasse , Masahide Yamaguchi

Compact objects occupy a pivotal role in the exploration of Nature. The interest spans from the role of compact objects in astrophysics to their detection through various methods (gravitational waves interferometry, microlensing, imaging).…

广义相对论与量子宇宙学 · 物理学 2023-01-13 Luca Visinelli

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

We study equilibrium configurations of boson stars in the framework of general scalar-tensor theories of gravitation. We analyse several possible couplings, with acceptable weak field limit and, when known, nucleosynthesis bounds, in order…

广义相对论与量子宇宙学 · 物理学 2011-09-09 Diego F. Torres
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