Constraining a one-dimensional wave-type gravitational wave parameter through the shadow of M87* via Event Horizon Telescope

Abstract

During the glorious success of the EHT in providing the first image of a black hole, numerous papers have been published about the effect of different astrophysical environments on black hole geometry. Motivated by the work on how gravitational wave affects the shadow of a Schwarzschild black hole [Eur. Phys. J. C 10.1140/epjc/s10052-021-09287-2], we extend it by considering a quantum correction on the black hole through the extended uncertainty principle (EUP). Along with this correction, we probe the gravitational wave's effect on the null geodesics, and photonsphere, and find constraints to the gravitational wave parameter $\epsilon$ using the black hole shadow of M87* for some given test value for the gravitational wave frequency $\sigma$. Not only that some nodes were found in the light trajectory, but the general behavior of paths changes in a periodic way as the time $t$ progresses. These patterns then confirm the chaotic formation of the shadow seen by some remote observer. Finally, the constraint that we find for $\epsilon$ is $10^{-10}$ orders of magnitude for the effect of the gravitational wave to be seen at a distance of $D=16.8$ Mpc. As a consequence of such a value for $\epsilon$, another result reveals that while there is are gravitational wave effect on the shadow perceived at $D$, the deviations on the photonsphere are nearly non-existent. Apart from Earth-based detectors for gravitational waves, the study implies the possibility of an alternative detection method especially if a gravitational wave source is near a lone black hole.

arXiv comment10 pages, 6 figures

References in corpus (62)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
• First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
• Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• Tests of General Relativity with GW170817
• Influence of a plasma on the shadow of a spherically symmetric black hole
• Constraints on black-hole charges with the 2017 EHT observations of M87*
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Black hole shadow in an expanding universe with a cosmological constant
• Black holes with a cosmological constant in bumblebee gravity
• Shadow, lensing, quasinormal modes, greybody bounds and neutrino propagation by dyonic ModMax black holes
• Probing a nonlinear electrodynamics black hole with thin accretion disk, shadow and deflection angle with M87* and Sgr A* from EHT
• Shadows and gravitational weak lensing by the Schwarzschild black hole in the string cloud background with quintessential field
• Solutions of the Einstein equations for a black hole surrounded by a galactic halo
• Shadows of Sgr A${}^{\ast }$ Black Hole Surrounded by Superfluid Dark Matter Halo
• An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• Testing dynamical torsion effects on the charged black hole's shadow, deflection angle and greybody with M87* and Sgr. A* from EHT
• Modelling the Sgr A* Black Hole Immersed in a Dark Matter Spike
• Testing Horndeski Gravity from EHT Observational Results for Rotating Black Holes
• Dehnen halo effect on a black hole in an ultra-faint dwarf galaxy
• Dark matter effect on the weak deflection angle by black holes at the center of Milky Way and M87 galaxies
• Shadow and weak deflection angle of extended uncertainty principle black hole surrounded with dark matter
• Testing Generalized Einstein-Cartan-Kibble-Sciama Gravity using Weak Deflection Angle and Shadow Cast
• Extended Uncertainty Principle Black Holes
• Black Hole Shadow in Symmergent Gravity
• Shadow cast of non-commutative black holes in Rastall gravity
• Black holes in galactic centers: quasinormal ringing, grey-body factors and Unruh temperature
• Chaotic shadow of a non-Kerr rotating compact object with quadrupole mass moment
• Quasiperiodic oscillations, weak field lensing and shadow cast around black holes in Symmergent gravity
• Weak Deflection Angle of Extended Uncertainty Principle Black Holes
• Testing Symmergent gravity through the shadow image and weak field photon deflection by a rotating black hole using the M87${}^{\ast }$ and Sgr. A${}^{\ast }$ results
• A study on black hole shadows in asymptotically de Sitter spacetimes
• Constraints on Barrow entropy from M87* and S2 star observations
• Primordial Gravitational Wave Signals in Modified Cosmologies
• Deflection angle and shadow of the Reissner-Nordström black hole with higher-order magnetic correction in Einstein-nonlinear-Maxwell fields
• Investigating effects of dark matter on photon orbits and black hole shadows
• Chaos in black holes surrounded by gravitational waves
• Quantum effects on the black hole shadow and deflection angle in presence of plasma
• Black holes surrounded by Einstein clusters as models of dark matter fluid
• Rotating dirty black hole and its shadow
• Black Hole Shadows in Verlinde's Emergent Gravity
• Generalized Extended Uncertainty Principle Black Holes: Shadow and lensing in the macro- and microscopic realms
• Search for gravitational-wave signals associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo
• Shadow of a Schwarzschild black hole surrounded by a Bach-Weyl ring
• Gravitational ringing and superradiant instabilities of the Kerr-like black holes in a dark matter halo
• Black hole shadow with a cosmological constant for cosmological observers
• Orbits of light rays in scale-dependent gravity: Exact analytical solutions to the null geodesic equations
• EUP-corrected thermodynamics of BTZ black hole
• Weak Deflection angle and Shadow by Tidal Charged Black Hole
• Quantum corrections to the quasinormal modes of the Schwarzschild black hole
• Effect of gravitational wave on shadow of a Schwarzschild black hole
• Shadow of quantum extended Kruskal black hole and its super-radiance property
• Orbits of light rays in (1+2)-dimensional Einstein-power-Maxwell gravity: Exact analytical solution to the null geodesic equations
• Geodesic analysis and black hole shadows on a general non--extremal rotating black hole in five--dimensional gauged supergravity
• Strongly Magnetized Hot QCD Matter and Stochastic Gravitational Wave Background
• Investigating bounds on the extended uncertainty principle metric through astrophysical tests
• Constraints on extended gravity models through gravitational wave emission
• Effect of quantum deformed black hole on BH shadow in two-dimensional Dilaton gravity
• Effects of Extended Uncertainty Principle on the Relativistic Coulomb Potential

Cited by in corpus (12)

• Investigating the Connection between Generalized Uncertainty Principle and Asymptotically Safe Gravity in Black Hole Signatures through Shadow and Quasinormal Modes
• Constraints on charged Symmergent black hole from shadow and lensing
• Event Horizon Telescope observations exclude compact objects in baseline mimetic gravity
• Quasinormal modes-shadow correspondence for rotating regular black holes
• Shadow and deflection angle of asymptotic, magnetically-charged, non-singular black hole
• Primordial regular black holes as all the dark matter. II. Non-time-radial-symmetric and loop quantum gravity-inspired metrics
• Primordial regular black holes as all the dark matter. I. Time-radial-symmetric metrics
• Shadow and greybody bounding of a regular scale-dependent black hole solution
• Nonlinearly charged black holes: Shadow and Thin-accretion disk
• Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
• Asymptotically-Flat Black Hole Solutions in Symmergent Gravity
• Shadow Ringing of Black Holes from Photon Sphere Quasinormal Modes