Dark matter signatures of black holes with Yukawa potential

Abstract

This study uses a nonsingular Yukawa--modified potential to obtain a static and spherically symmetric black hole solution with a cosmological constant. Such Yukawa--like corrections are encoded in two parameters, $\alpha$ and $\lambda$, that modify Newton's law of gravity in large distances, and a deformation parameter ${\ell }_0$, which plays an essential role in short distances. The most significant effect is encoded in $\alpha$, which modifies the total black hole mass with an extra mass proportional to $\alpha M$, mimicking the dark matter effects at large distances from the black hole. On the other hand, the effect due to $\lambda$ is small for astrophysical values. We scrutinize the \textit{quasinormal} frequencies and shadows associated with a spherically symmetric black hole and the thermodynamical behavior influenced by the Yukawa potential. In particular, the thermodynamics of this black hole displays a rich behavior, including possible phase transitions. We use the WKB method to probe the \textit{quasinormal} modes of massless scalar, electromagnetic, and gravitational field perturbations. In order to check the influence of the parameters on the shadow radius, we consider astrophysical data to determine their values, incorporating information on an optically thin radiating and infalling gas surrounding a black hole to model the black hole shadow image. In particular, we consider Sgr A* black hole as an example and we find that its shadow radius changes by order of $10^{-9}$, meaning that the shadow radius of a black hole with Yukawa potential practically gives rise to the same result encountered in the Schwarzschild black hole. Also, in the eikonal regime, using astrophysical data for Yukawa parameters, we show that the value of the real part of the QNMs frequencies changes by $10^{-18}$.

arXiv comment24 pages in double column, 13 figures and 5 tables

References in corpus (99)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• Modified Gravity and Cosmology
• f(R) theories
• Extended Theories of Gravity
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Quasinormal modes of black holes and black branes
• First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
• Resummation of Massive Gravity
• Quasinormal modes of black holes: from astrophysics to string theory
• f(T) teleparallel gravity and cosmology
• Geodesic stability, Lyapunov exponents and quasinormal modes
• Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
• Quintom Cosmology: Theoretical implications and observations
• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
• Black Hole Shadows, Photon Rings, and Lensing Rings
• Calculating black hole shadows: Review of analytical studies
• Shadows and strong gravitational lensing: a brief review
• Can dark matter be a Bose-Einstein condensate?
• Shadows of Kerr black holes with scalar hair
• Testing the rotational nature of the supermassive object M87* from the circularity and size of its first image
• Measurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow
• Shadow of rotating regular black holes
• Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
• Black-bounce to traversable wormhole
• Quasinormal modes of black holes. The improved semianalytic approach
• Modified teleparallel theories of gravity
• Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
• Teleparallel Theories of Gravity: Illuminating a Fully Invariant Approach
• Are eikonal quasinormal modes linked to the unstable circular null geodesics?
• Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope
• Shapes and Positions of Black Hole Shadows in Accretion Disks and Spin Parameters of Black Holes
• The Current Ability to Test Theories of Gravity with Black Hole Shadows
• Theory of Dark Matter Superfluidity
• Black holes with scalar hair in light of the Event Horizon Telescope
• Black hole shadow in an asymptotically-flat, stationary, and axisymmetric spacetime: The Kerr-Newman and rotating regular black holes
• Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
• Can the supermassive objects at the centers of galaxies be traversable wormholes? The first test of strong gravity for mm/sub-mm VLBI facilities
• Conditions for the cosmological viability of the most general scalar-tensor theories and their applications to extended Galileon dark energy models
• Phase-Space analysis of Teleparallel Dark Energy
• Local-Group tests of dark-matter Concordance Cosmology: Towards a new paradigm for structure formation
• Connection between black-hole quasinormal modes and lensing in the strong deflection limit
• Wormhole Shadows
• MOND and the "Dearth of Dark Matter in Ordinary Elliptical Galaxies"
• Dynamical behavior in $f(T,T_G)$ cosmology
• Modified Gravity Black Holes and their Observable Shadows
• Incidences between points and lines on a two-dimensional variety
• Testing General Relativity with the Event Horizon Telescope
• Quasinormal Modes of Black Holes Surrounded by Dark Matter and Their Connection with the Shadow Radius
• Phase-space analysis of Horava-Lifshitz cosmology
• A class of black holes in dRGT massive gravity and their thermodynamical properties
• EHT constraint on the ultralight scalar hair of the M87 supermassive black hole
• Shadows of Sgr A${}^{\ast }$ Black Hole Surrounded by Superfluid Dark Matter Halo
• The Kiselev black hole is neither perfect fluid, nor is it quintessence
• Velocity dispersion around ellipticals in MOND
• Quantum Corrected Black Holes from String T-Duality
• Imprints of Dark Matter on Black Hole Shadows using Spherical Accretions
• Corrected form of the first law of thermodynamics for regular black holes
• Dynamical analysis of generalized Galileon cosmology
• Thermodynamics of a class of regular black holes with a generalized uncertainty principle
• Further clarification on quasinormal modes/circular null geodesics correspondence
• Scaling Solutions and reconstruction of Scalar Field Potentials
• Dynamical features of scalar-torsion theories
• Analytical correspondence between shadow radius and black hole quasinormal frequencies
• Shadow images of Kerr-like wormholes
• Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
• Observational Constraints on New Exact Inflationary Scalar-field Solutions
• Destruction of Refractory Carbon in Protoplanetary Disks
• Black hole shadow as a standard ruler in cosmology
• Retrolensing by two photon spheres of a black-bounce spacetime
• Quasinormal frequencies of self-dual black holes
• Gravitational signatures of a non--commutative stable black hole
• Einstein's Theory of Gravity and the Problem of Missing Mass
• Thermodynamics and evaporation of a modified Schwarzschild black hole in a non--commutative gauge theory
• Exploring antisymmetric tensor effects on black hole shadows and quasinormal frequencies
• Gravity Modification with Yukawa-type Potential: Dark Matter and Mirror Gravity
• The MOND Fundamental Plane
• Analytical Solutions in a Cosmic String Born-Infeld-dilaton Black Hole Geometry: Quasinormal Modes and Quantization
• Gravitational traces of bumblebee gravity in metric-affine formalism
• Thermal analysis of photon-like particles in rainbow gravity
• Observational constraints on Yukawa cosmology and connection with black hole shadows
• Decomposition of total stress-energy for the generalised Kiselev black hole
• Thermodynamical properties of an ideal gas in a traversable wormhole
• Dark Matter in Galaxies: evidences and challenges
• Bi-scalar modified gravity and cosmology with conformal invariance
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• Implications of a Simpson-Visser solution in Verlinde's framework
• Thermodynamic schemes of charged BTZ-like black holes in arbitrary dimensions
• Dark Universe Phenomenology from Yukawa Potential?
• Thermodynamical properties of a deformed Schwarzschild black hole via Dunkl generalization
• Conservation laws and Exact Solutions in Brans-Dicke Cosmology with a Scalar Field
• de Sitter versus anti-de Sitter in Horndeski-like gravity
• On existence of a possible Lorentz invariant modified gravity in Weitzenböck spacetime
• Addressing the Hubble tension in Yukawa cosmology?
• Apparent Dark Matter Inspired by Einstein Equation of State
• Gravitational perturbation of traversable wormhole

Cited by in corpus (16)

• How does non-metricity affect particle creation and evaporation in bumblebee gravity?
• Effects of non-commutative geometry on black hole properties
• Particle creation and evaporation in Kalb-Ramond gravity
• Particle production induced by a Lorentzian non-commutative spacetime
• A Non-Commutative Kalb-Ramond Black Hole
• Thermodynamics, Weak Gravitational Lensing, and Parameter Estimation of a Schwarzschild Black Hole Immersed in Hernquist Dark Matter Halo
• Properties of an axisymmetric Lorentzian non-commutative black hole
• Non-commutativity in Hayward spacetime
• Remarks on a nonlinear electromagnetic extension in AdS Reissner-Nordström spacetime
• Quantum-corrected Schwarzschild AdS black hole surrounded by quintessence: Thermodynamics and Shadows
• Gravitational signatures of a nonlinear electrodynamics in $f(R,T)$ gravity
• Analysis of a nonlinear electromagnetic generalization of the Reissner-Nordström black hole
• Black holes surrounded by massive vector fields in Kaluza-Klein gravity
• Axisymmetric black hole in a non-commutative gauge theory: classical and quantum gravity effects
• Imprints of non-commutativity on charged black holes
• Black Hole Solutions in Dark Photon Models with Higher Order Corrections