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相关论文: Boson stars in massive dilatonic gravity

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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

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 phenomenological features and stability of boson stars in massless and massive scalar-tensor theory of gravity with Damour-Esposito-Farese coupling. This coupling between the tensor and scalar sectors of the theory leads to a…

广义相对论与量子宇宙学 · 物理学 2024-07-29 Tamara Evstafyeva , Roxana Rosca-Mead , Ulrich Sperhake , Bernd Brugmann

We review particle-like configurations of complex scalar field, localized by gravity, so-called boson stars. In the simplest case, these solutions posses spherical symmetry, they may arise in the massive Einstein-Klein-Gordon theory with…

广义相对论与量子宇宙学 · 物理学 2022-04-14 Yakov Shnir

Spherically symmetric configurations of the non-interacting massive complex scalar field, representing non-rotating boson stars, are considered within the framework of the modified torsion based $f(T)$ gravity, with $f(T) = T + \alpha \,…

广义相对论与量子宇宙学 · 物理学 2020-10-19 Saša Ilijić , Marko Sossich

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

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

We study boson stars in a theory of complex scalar field coupled to Einstein gravity with the potential: $V(|\Phi|) := m^{2} |\Phi|^2 +2 \lambda |\Phi|$ (where $m^2$ and $\lambda$ are positive constant parameters). This could be considered…

高能物理 - 理论 · 物理学 2016-05-24 Sanjeev Kumar , Usha Kulshreshtha , Daya Shankar Kulshreshtha

Boson stars consist of a system of self-gravitating scalar fields which form a macroscopic quantum state and are a possible dark matter candidate. In this paper, we address the existence of boson stars in Brans-Dicke gravity. We show that…

天体物理学 · 物理学 2009-10-22 Mark A. Gunderson , Lars Gerhard Jensen

We study solutions for boson stars in multiscalar theory. We start with simple models with N scalar theories. Our purpose is to study the models in which the mass matrix of scalars and the scalar couplings are given by an extended method of…

广义相对论与量子宇宙学 · 物理学 2010-02-15 Nahomi Kan , Kiyoshi Shiraishi

We study boson shells and boson stars in a theory of complex scalar field coupled to the $U(1)$ gauge field $A_{\mu}$ and Einstein gravity with the potential: $V(|\Phi|) := \frac{1}{2} m^{2} \left(|\Phi|+ a \right)^2$. This could be…

高能物理 - 理论 · 物理学 2016-06-08 Sanjeev Kumar , Usha Kulshreshtha , Daya Shankar Kulshreshtha

Boson stars in zero-, one-, and two-node equilibrium states are modeled numerically within the framework of Scalar-Tensor Gravity. The complex scalar field is taken to be both massive and self-interacting. Configurations are formed in the…

广义相对论与量子宇宙学 · 物理学 2009-10-30 G. L. Comer , Hisa-aki Shinkai

The properties of compact stars made of massive bosons with a repulsive selfinteraction mediated by vector mesons are studied within the mean-field approximation and general relativity. We demonstrate that there exists a scaling property…

天体物理学 · 物理学 2010-04-21 Pratik Agnihotri , Juergen Schaffner-Bielich , Igor N. Mishustin

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

A model of static boson-fermion star with spherical symmetry based on the scalar-tensor theory of gravity with massive dilaton field is investigated numerically. Since the radius of star is \textit{a priori} an unknown quantity, the…

数值分析 · 数学 2025-10-20 T. L. Boyadjiev , M. D. Todorov , P. P. Fiziev , S. S. Yazadjiev

We study numerically the gravitational field of a star made of massive and neutral string states for the case in which the dilaton is massive. The solution exhibits very simple scaling properties in the dilaton mass. There is no horizon and…

高能物理 - 理论 · 物理学 2009-10-22 M. Fabbrichesi , R. Iengo

We make a detailed study of boson star configurations in Jordan--Brans--Dicke theory, studying both equilibrium properties and stability, and considering boson stars existing at different cosmic epochs. We show that boson stars can be…

广义相对论与量子宇宙学 · 物理学 2011-08-11 Diego F Torres , Franz E Schunck , Andrew R Liddle

We analyse the (thermo)dynamics of the scalar degrees of freedom in the scalar boson stars through the dark matter density under extreme conditions. The boson stars are studied in terms of a dark scalar sector in such a way this sector…

高能物理 - 唯象学 · 物理学 2024-06-04 G. A. Kozlov

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

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 compare…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Franz E Schunck , Andrew R Liddle
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