☆ 4.2 Review

Boson stars and oscillatons: A review

INTERNATIONAL JOURNAL OF MODERN PHYSICS D (2021)

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Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal

S. T. H. Hartman et al.

Summary: This study aims to understand the gravitational drag forces acting on massive objects moving through a self-interacting Bose-Einstein condensate at finite temperatures. By analyzing the dynamical friction in a superfluid, the research provides insights into the behavior of dark matter models and the impact of temperature on their decay times.

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Article Astronomy & Astrophysics

Oscillon preheating in full general relativity

Xiao-Xiao Kou et al.

Summary: Investigated the oscillon preheating scenario in full general relativity, and found that general-relativistic corrections can lead to the production of more and denser oscillons, potentially collapsing them into black holes in certain parameter regions.

CLASSICAL AND QUANTUM GRAVITY (2021)

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Article Astronomy & Astrophysics

Horndeski stars

Juan Barranco et al.

Summary: This study establishes the existence of time-dependent solitons in a modified gravity framework, characterized by finite energy configurations with a single continuous parameter. As the central field amplitude increases, the theory becomes strongly coupled and model-dependent. Quantum corrections do not affect the existence and properties of these solutions.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Two-scalar Bose-Einstein condensates: from stars to galaxies

Huai-Ke Guo et al.

Summary: The study focuses on the properties of Bose-Einstein Condensate (BEC) systems consisting of two scalars at stellar and galactic scales. It shows that a repulsive interaction between two scalars at stellar scales can stabilize the BEC system, leading to potential gravitational wave signals. At galactic scales, two-scalar BECs can address scaling problems.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Using space-VLBI to probe gravity around Sgr A*

C. M. Fromm et al.

Summary: This study investigates the radiation characteristics of different types of black holes around Sagittarius A* using general-relativistic magneto-hydrodynamical simulations and synthetic data comparison. The results show that the inclusion of an orbiting space antenna improves EHT's ability to distinguish between different types of rotating black holes.

ASTRONOMY & ASTROPHYSICS (2021)

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Article Astronomy & Astrophysics

Oscillons of axion-like particle: mass distribution and power spectrum

Masahiro Kawasaki et al.

Summary: In this paper, the oscillons of the pure-natural type potential are investigated through classical lattice simulation to explore key quantities necessary for phenomenological application, such as the number density of oscillons and their mass distribution.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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GW190521 as a Merger of Proca Stars: A Potential New Vector Boson of 8.7 x 10-13 eV

Juan Calderon Bustillo et al.

Summary: GW190521 is a short gravitational-wave signal interpreted as a quasicircular merger of black holes, forming a remnant black hole with a mass of about 142 solar masses. Despite the lack of visible premerger emission, further investigation is needed to understand the pre-merger dynamics and nature of the colliding objects.

PHYSICAL REVIEW LETTERS (2021)

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Article Physics, Particles & Fields

Gravitational wave spectra from oscillon formation after inflation

Takashi Hiramatsu et al.

Summary: Through numerical simulations and analysis of potential types, we find a universal feature in the shape and amplitude of emitted gravitational waves after inflation, as well as differences in the gravitational wave spectrum between two families of potentials. The number density and properties of the produced oscillons vary for each potential type. The growth rate of scalar perturbations and oscillon formation time are influenced by the small-field shape of the potential, while macroscopic properties of oscillons depend on the large-field shape.

JOURNAL OF HIGH ENERGY PHYSICS (2021)

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Article Astronomy & Astrophysics

On the linear stability of l-boson stars with respect to radial perturbations

Miguel Alcubierre et al.

Summary: This article studies the linear stability of l-boson stars with time-dependent, radial perturbations, showing the existence of stable configurations for each fixed value of the angular momentum number l, as well as unstable configurations. These results are qualitatively similar to stability results of standard boson stars with l = 0, and suggest the existence of new stable configurations that are more massive and compact than usual boson stars.

CLASSICAL AND QUANTUM GRAVITY (2021)

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Article Astronomy & Astrophysics

The imitation game: Proca stars that can mimic the Schwarzschild shadow

Carlos A. R. Herdeiro et al.

Summary: The study finds that dynamically robust spherical Proca stars can successfully mimic the shadow of a (near-)equilibrium Schwarzschild BH in an astrophysical environment, despite the absence of light rings, under certain observation conditions. Different types of bosonic stars exhibit different behaviors in terms of stability and the ability to imitate black hole characteristics, with some solutions showing potential to reproduce the ISCO of a Schwarzschild BH.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Article Astronomy & Astrophysics

Gravitational effects on oscillon lifetimes

Hong-Yi Zhang

Summary: This paper investigates the longevity of oscillons in scalar field theories with attractive self-interactions, focusing on the effects of gravity on their decay rate and lifetime. The study found that including gravitational interactions can slightly reduce the lifetime of dense oscillons under certain conditions.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Oscillon collapse to black holes

Zainab Nazari et al.

Summary: This study investigates the dynamics of pseudotopological objects called oscillons for a class of models inspired by axion-monodromy using numerical relativity simulations. It contrasts the effects of adding self-interactions with or without gravitational support, mapping out regions of parameter space where initial conditions collapse to black holes or remain pseudo-stable or disperse.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2021)

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Wave Dark Matter

Lam Hui

Summary: This paper reviews the physics and phenomenology of wave dark matter, outlining its particle physics motivations and rich phenomenology. Wave interference in dark matter leads to unique structures like vortices and solitons, with potential implications for observed astronomical phenomena. Detection experiments and theoretical predictions for wave dark matter are discussed, highlighting the importance of understanding the stochastic nature of waves in interpreting constraints and measurements.

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, VOL 59 (2021)

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Rotating boson stars using finite differences and global Newton methods

Santiago Ontanon et al.

Summary: This study investigates rotating boson star data for numerical relativity, generating seven data sets characterized by different rotation azimuthal integers using a Cartesian grid and global Newton methods. The results accurately converge with respect to resolution size and boundary extension, enabling precise calculation of global parameters such as Komar masses and angular momenta. Additionally, the study reveals both consistent results with previous literature for rotation integers [0, 2] and new findings for rotation integers l > 2, emphasizing the importance of regularization in curvilinear-based numerical relativity.

CLASSICAL AND QUANTUM GRAVITY (2021)

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A stabilization mechanism for excited fermion-boson stars

Fabrizio Di Giovanni et al.

Summary: This study numerically investigates the nonlinear stability and characteristics of excited fermion-boson stars in spherical symmetry. Contrary to purely boson stars in the excited state, a cooperative stabilization mechanism between the fermionic and bosonic constituents of these mixed stars is revealed. This stabilization mechanism appears to be a purely gravitational effect, independent of the type of matter of the companion star, in contrast to recent examples of stabilization mechanisms discussed in other contexts.

CLASSICAL AND QUANTUM GRAVITY (2021)

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Landau equation for self-gravitating classical and quantum particles: application to dark matter

Pierre-Henri Chavanis

Summary: This study develops the kinetic theory of classical and quantum particles in gravitational interaction, with a focus on the applications of quantum particle kinetic theory in the context of dark matter. The main properties of the quantum Landau equation and its implications for bosonic particles, especially in Bose-Einstein condensation, are discussed. The study also examines the relationship with the works of other researchers in the field of dark matter and Bose stars formation.

EUROPEAN PHYSICAL JOURNAL PLUS (2021)

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Beyond Schrodinger-Poisson: nonrelativistic effective field theory for scalar dark matter

Borna Salehian et al.

Summary: This paper systematically derives the SP equations and relativistic corrections from the nonlinear and fully relativistic KGE equations in an expanding universe, providing insights into deviations and applicability beyond the SP system. The method presented simplifies the analysis of scalar dark matter dynamics and accurately captures deviations from the SP system towards the full KGE case, particularly in calculating the mass-radius relationship of solitons.

JOURNAL OF HIGH ENERGY PHYSICS (2021)

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New insights into the formation and growth of boson stars in dark matter halos

Jiajun Chen et al.

Summary: This study investigates the formation and growth of boson stars and their surrounding miniclusters through gravitational condensation using nonlinear dynamical numerical methods, considering attractive and repulsive self-interactions. Strong attractive self-interactions can cause instability and collapse of boson stars, while repulsive self-interactions promote their formation and result in solutions with larger radii.

PHYSICAL REVIEW D (2021)

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Simulations of axion minihalos

Huangyu Xiao et al.

Summary: The study investigates the axion as a dark matter candidate and uses numerical simulations to analyze the formation characteristics of axion minihalos in the universe. The results suggest that the model is consistent with a certain physical model and can predict the mass function of minihalos at different redshifts, helping us understand the distribution of dark matter in the universe and its effects on cosmological microlensing and pulsar timing.

PHYSICAL REVIEW D (2021)

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Instability of rotating Bose stars

A. S. Dmitriev et al.

Summary: The study explores the stability and decay of rotating Bose stars composed of light bosonic dark matter, showing that they are unstable under certain conditions and eventually decay into a Saturn-like configuration. Only in models with strong repulsive self-interactions, the Bose star with l = 1 is stable.

PHYSICAL REVIEW D (2021)

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Jeans mass-radius relation of self-gravitating Bose-Einstein condensates and typical parameters of the dark matter particle

Pierre-Henri Chavanis

Summary: The study investigates the Jeans mass-radius relation of Bose-Einstein condensate dark matter in Newtonian gravity, showing different evolution paths and characteristics based on the self-interaction modes of bosons as the Universe expands.

PHYSICAL REVIEW D (2021)

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Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog

R. Abbott et al.

Summary: Gravitational waves are used to test general relativity in strong-field regimes, with evaluations of data consistency showing no evidence for new physics beyond general relativity. Modifying waveform parameters and constraints on Lorentz-violating coefficients have improved past limitations, while analysis of merger remnants and polarization confirms agreement with theoretical predictions.

PHYSICAL REVIEW D (2021)

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Structure of the oscillon: The dynamics of attractive self-interaction

David Cyncynates et al.

Summary: This study introduces a new formalism for computing the properties of oscillons with improved accuracy, studying their internal structure and identifying the physical mechanisms responsible for their longevity. By imposing realistic boundary conditions, a near-minimally radiating solution is naturally selected, with oscillon longevity arising from its geometry. Introducing a vocabulary for oscillon stability, new features in oscillon evolution can be predicted.

PHYSICAL REVIEW D (2021)

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Boson stars and their radial oscillations

Ben Kain

Summary: In this study, we derived and examined the pulsation equations for spherically symmetric boson stars, considering self-interacting boson stars with varying values of the self-coupling constant. By numerically evolving boson stars and Fourier transforming dynamic solutions, we independently computed radial oscillation frequencies and verified the results obtained from the pulsation equations, finding excellent agreement between the two methods.

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Alexandre Toubiana et al.

Summary: Exotic compact objects can be difficult to distinguish from black holes in the inspiral phase of binaries observed by gravitational-wave detectors, but significant differences may be present in the merger and post-merger signal. A toy model capturing the key features of binaries of exotic compact objects with low compactness was introduced to assess their detectability and distinguishability from black hole binaries. The study showed that current detectors like LISA could potentially observe exotic binaries and differentiate them from black hole binaries.

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Axion miniclusters made easy

David Ellis et al.

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Fast radio bursts from axion stars moving through pulsar magnetospheres

James H. Buckley et al.

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Nils Siemonsen et al.

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James Y. Widdicombe et al.

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Horng Sheng Chia et al.

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Ilidio Lopes et al.

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Lorenzo Annulli et al.

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Pierre-Henri Chavanis

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Relaxation times for Bose-Einstein condensation in axion miniclusters

Kay Kirkpatrick et al.

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Fabrizio Di Giovanni et al.

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Fabrizio Di Giovanni et al.

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Djuna Croon et al.

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Bradley J. Kavanagh et al.

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Luca Visinelli et al.

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Miguel Bezares et al.

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Kazunori Akiyama et al.

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Expansion in higher harmonics of boson stars using a generalized Ruffini-Bonazzola approach. Part 1. Bound states

Joshua Eby et al.

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Effective stability against superradiance of Kerr black holes with synchronised hair

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John Ellis et al.

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Gravitational radiation background from boson star binaries

Djuna Croon et al.

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Dilute and dense axion stars

Luca Visinelli et al.

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Detecting axion stars with radio telescopes

Yang Bai et al.

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Black hole formation from axion stars

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Gravitational wave signatures of highly compact boson star binaries

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Lensing and dynamics of ultracompact bosonic stars

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Gravitational wave searches for ultralight bosons with LIGO and LISA

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Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: New cosmological constraints and its detectability by LIGO

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Supermassive dark-matter Q-balls in galactic centers

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Equation of state of imbalanced cold matter from chiral perturbation theory

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CONTRASTING GALAXY FORMATION FROM QUANTUM WAVE DARK MATTER, ψDM, WITH ΛCDM, USING PLANCK AND HUBBLE DATA

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Gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale

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Astrophysical imaging of Kerr black holes with scalar hair

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Charged Proca stars

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Observing-and Imaging-Active Galactic Nuclei with the Event Horizon Telescope

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Collapse of a self-gravitating Bose-Einstein condensate with attractive self-interaction

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Boson stars in biscalar extensions of Horndeski gravity

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JETP LETTERS (2015)

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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

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A model for halo formation with axion mixed dark matter

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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2014)

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Gravitational collapse of Bose-Einstein condensate dark matter halos

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Cosmological constraints on Bose-Einstein-condensed scalar field dark matter

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Rotating boson stars in five-dimensional Einstein-Gauss-Bonnet gravity

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Models of rotating boson stars and geodesics around them: New type of orbits

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Understanding the Core-Halo Relation of Quantum Wave Dark Matter from 3D Simulations

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ACCELERATED COSMIC EXPANSION (2014)

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Improved source localization with LIGO-India

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VISHWA MIMANSA: AN INTERPRETATIVE EXPOSITION OF THE UNIVERSE. PROCEEDINGS OF THE 7TH INTERNATIONAL CONFERENCE ON GRAVITATION AND COSMOLOGY (2014)

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Chameleon dark matter stars

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Can the dark matter halo be a collisionless ensemble of axion stars?

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Charged boson stars

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Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions. I. Analytical results

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Proceedings Paper Astronomy & Astrophysics

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New models of chaotic inflation in supergravity

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Stagflation: Bose-Einstein condensation in the early universe

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Spherical boson stars as black hole mimickers

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REVEALING THE PROPERTIES OF DARK MATTER IN THE MERGING CLUSTER MACS J0025.4-1222

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Tidal love numbers of neutron stars

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Cosmic structures via Bose-Einstein condensation and its collapse

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Axion cosmology and the energy scale of inflation

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Monodromy in the CMB: Gravity waves and string inflation

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Can dark matter be a Bose-Einstein condensate?

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Neutron star observations: Prognosis for equation of state constraints

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A direct empirical proof of the existence of dark matter

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Gravitational cooling of self-gravitating bose condensates

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Scalar dark matter and cold stars

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ASTROPARTICLE PHYSICS (2006)

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Tidal coupling of a Schwarzschild black hole and circularly orbiting moon

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Rotating boson stars and Q-balls

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Particle dark matter: evidence, candidates and constraints

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Classical and quantum decay of oscillations: Oscillating self-gravitating real scalar field solitons

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Bose-Einstein condensation, dark matter and acoustic peaks

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Evolution of the Schrodinger-Newton system for a self-gravitating scalar field -: art. no. 124033

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General relativistic boson stars

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Critical collapse of a massive vector field

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Numerical studies of Φ2-oscillatons

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Fuzzy cold dark matter: The wave properties of ultralight particles

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What if dark matter is bosonic and self-interacting

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Boson stars as gravitational lenses

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