Cosmological expansion and local physics

Abstract

The interplay between cosmological expansion and local attraction in a gravitationally bound system is revisited in various regimes. First, weakly gravitating Newtonian systems are considered, followed by various exact solutions describing a relativistic central object embedded in a Friedmann universe. It is shown that the ``all or nothing'' behaviour recently discovered (i.e., weakly coupled systems are comoving while strongly coupled ones resist the cosmic expansion) is limited to the de Sitter background. New exact solutions are presented which describe black holes perfectly comoving with a generic Friedmann universe. The possibility of violating cosmic censorship for a black hole approaching the Big Rip is also discussed.

17 pages, LaTeX, to appear in Phys. Rev. D

References in corpus (71)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• Phantom Energy and Cosmic Doomsday
• Cosmological Results from High-z Supernovae
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
• Quantum deSitter cosmology and phantom matter
• Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
• General Laws of Black-Hole Dynamics
• The phantom menaced: constraints on low-energy effective ghosts
• Black hole mass decreasing due to phantom energy accretion
• 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at z>0.7
• Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
• Phantom cosmologies
• Dynamical Horizons: Energy, Angular Momentum, Fluxes and Balance Laws
• Quasi-Local Gravitational Energy
• The Collision of Two Black Holes
• The Fate of Bound Systems in Phantom and Quintessence Cosmologies
• Varying Alpha in a More Realistic Universe
• Expanding Confusion: common misconceptions of cosmological horizons and the superluminal expansion of the Universe
• Superquintessence
• The fundamental definition of 'radial velocity'
• Generalized phantom energy
• Born-Infeld Quantum Condensate as Dark Energy in the Universe
• A Preliminary Indication of Evolution of Type Ia Supernovae from their Risetimes
• Phantom Inflation and Primordial Perturbation Spectrum
• Local and Global Variations of The Fine Structure Constant
• Relic Dark energy from Trans-Planckian Regime
• A point mass in an isotropic universe. Existence, uniqueness and basic properties
• Phantom Cosmologies
• Phantom-like GCG and the constraints of its parameters via cosmological dynamics
• The influence of the cosmological expansion on local systems
• Inhomogeneous Gravity
• Phantom cosmology with general potentials
• Phantom with Born-Infield type Lagrangian
• Phantom k-essence cosmologies
• Phantom Field with O(N) Symmetry in Exponential Potential
• How to Test Stringy Dark Energy?
• Future Evolution of Structure in an Accelerating Universe
• Attractor Behavior of Phantom Cosmology
• Born-Infeld-type phantom on the brane world
• A point mass in an isotropic universe: III. The region $R\le 2m$
• Metric of a tidally distorted, nonrotating black hole
• Modified Dispersion Relations from Closed Strings in Toroidal Cosmology
• Cosmology with a Nonlinear Born-Infeld type Scalar Field
• Reissner-Nordström Metric in the Friedman-Robertson-Walker Universe
• Evolution of gravitational orbits in the expanding universe
• Cosmological perturbations on local systems
• The Evolution of Universe with th B-I Type Phantom Scalar Field
• Upper limits on the size of a primordial black hole
• Growth of primordial black holes in a universe containing a massless scalar field
• Joining the Hubble Flow: Implications for Expanding Space
• Cosmological Evolution of Black Holes in Brans-Dicke Gravity
• Non-existence of self-similar solutions containing a black hole in a universe with a stiff fluid or scalar field or quintessence
• The Local Effects of Cosmological Variations in Physical 'Constants' and Scalar Fields I. Spherically Symmetric Spacetimes
• Solutions to the tethered galaxy problem in an expanding universe and the observation of receding blueshifted objects
• Local Experiments See Cosmologically Varying Constants
• Qualitative Analysis of Universes with Varying Alpha
• Black Holes in Non-flat Backgrounds: the Schwarzschild Black Hole in the Einstein Universe
• Axially symmetric Einstein-Straus models
• Arbitrary Dimensional Schwarzschild-FRW Black Holes
• The Local Effects of Cosmological Variations in Physical 'Constants' and Scalar Fields II. Quasi-Spherical Spacetimes
• Expansion-induced contribution to the precession of binary orbits
• Influence of the cosmological expansion on small systems
• Super-horizon primordial black holes
• Constraints on the Detectability of Cosmic Topology from Observational Uncertainties
• Cosmological Black Holes
• Williams et al. Reply (to the Comment by Dumin on "Progress in Lunar Laser Ranging Tests of Relativistic Gravity")
• Disks in Expanding FRW Universes

Cited by in corpus (130)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Influence of global cosmological expansion on local dynamics and kinematics
• Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energy
• The Clustering Evolution of Primordial Black Holes
• Does the mass of a black hole decrease due to the accretion of phantom energy
• The effect of a massive object on an expanding universe
• Gauge k-vortices
• The little sibling of the big rip singularity
• On the generalization of McVittie's model for an inhomogeneity in a cosmological spacetime
• The effect of an expanding universe on massive objects
• The Jebsen-Birkhoff theorem in alternative gravity
• Making sense of the bizarre behaviour of horizons in the McVittie spacetime
• Turnaround radius in an accelerated universe with quasi-local mass
• Cosmologically coupled compact objects: a single parameter model for LIGO--Virgo mass and redshift distributions
• Eliminating the LIGO bounds on primordial black hole dark matter
• How the expansion of the universe determines the causal structure of McVittie spacetimes
• Local conditions separating expansion from collapse in spherically symmetric models with anisotropic pressures
• First-order thermodynamics of Horndeski gravity
• What is the fate of a black hole embedded in an expanding universe?
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• Eddington-Born-Infeld cosmology: a cosmographic approach, a tale of doomsdays and the fate of bound structures
• Particle and photon orbits in McVittie spacetimes
• The Hawking temperature of expanding cosmological black holes
• Black Holes in the Universe: Generalized Lemaitre-Tolman-Bondi Solutions
• Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
• Quantum corrections to the gravitational potentials of a point source due to conformal fields in de Sitter
• The charged McVittie spacetime
• Accretion of phantom scalar field into a black hole
• Cosmological coupling of nonsingular black holes
• Time dependent black holes and scalar hair
• Cosmological black holes and white holes with time-dependent mass
• Dissimilar Donuts in the Sky? Effects of a Pressure Singularity on the Circular Photon Orbits and Shadow of a Cosmological Black Hole
• Are quantization rules for horizon areas universal?
• Comparing two approaches to Hawking radiation of Schwarzschild-de Sitter black holes
• Realistic fluids as source for dynamically accreting black holes in a cosmological background
• An analysis of the Sultana-Dyer cosmological black hole solution of the Einstein equations
• Transition dynamics in the ${\Lambda }_{\mathrm{s}}$CDM model: Implications for bound cosmic structures
• Searching for dynamical black holes in various theories of gravity
• Constraints on the cosmological coupling of black holes from Gaia
• Separating expansion and collapse in general fluid models with heat flux
• Phantom Inflation in Little Rip
• Horndeski meets McVittie: A scalar field theory for accretion onto cosmological black holes
• DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
• Cosmological black holes from self-gravitating fields
• Dark Energy Accretion onto a Black Hole in an Expanding Universe
• A Lemaitre-Tolman-Bondi cosmological wormhole
• Evolving Black Holes in Inflation
• Clifton's spherical solution in f(R) vacuo harbours a naked singularity
• Quasi-local masses and cosmological coupling of black holes and mimickers
• Black Hole Thermodynamics with Dynamical Lambda
• Implications of cosmologically coupled black holes for pulsar timing arrays
• First law of thermodynamics for dynamical apparent horizons and the entropy of Friedmann universes
• Origin and growth of primordial black holes
• Astrophysical black holes in screened modified gravity
• Geodesics of McVittie Spacetime with a Phantom Cosmological Background
• Dynamical apparent horizons in inhomogeneous Brans-Dicke universes
• Quantum thermodynamics of de Sitter space
• The fate of bound systems through Sudden Future Singularities
• Gravitational orbits in the expanding universe revisited
• Positive neutrino masses with DESI DR2 via matter conversion to dark energy
• Black holes in realistic branes: black string-like objects?
• Weighing Milky Way and Andromeda in an expanding $\Lambda$CDM Universe: Decreasing the Local Group mass
• Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass
• The Hawking-Page-like Phase Transition from FRW Spacetime to McVittie Black Hole
• Hawking-Like Radiation as Tunneling from a Cosmological Black Hole in Modified Gravity: Semiclassical Approximation and Beyond
• A dual null formalism for the collapse of fluids in a cosmological background
• Preserving quantum information in $f(Q)$ cosmology
• Observational implications of cosmologically coupled black holes
• Conformally Schwarzschild cosmological black holes
• The Cosmological Model with a Wormhole and Hawking Temperature near Apparent Horizon
• Black Hole in a Radiation-Dominated Universe
• Generalized McVittie geometry in Horndeski gravity with matter
• Velocity and velocity bounds in static spherically symmetric metrics
• Time dependent embedding of spherically symmetric Rindler-like spacetime
• Navigating the asteroid field: New evaporation constraints for primordial black holes as dark matter
• A note on geodesics in inhomogeneous expanding spacetimes
• Holography and black holes in asymptotically flat FLRW
• Catastrophic fate of Schwarzschild black holes in a thermal bath
• Supermassive gravitinos and giant primordial black holes
• Simultaneous baldness and cosmic baldness and Kottler spacetime
• On the time dependent Schwarzschild - de Sitter spacetime
• Charged black holes in expanding Einstein-de Sitter universes
• Evolution of black holes through a nonsingular cosmological bounce
• Exact cosmological black hole solutions in Scalar Tensor Vector Gravity
• Equation of State for a van der Waals Universe during Reissner-Nordstrom Expansion
• Dynamical model for primordial black holes
• Propagation of gravitational waves in an expanding background in the presence of a point mass
• Cosmological expansion and local systems: a Lemaître-Tolman-Bondi model
• Turnaround physics beyond spherical symmetry
• Point mass Cosmological Black Holes
• Non-minimally coupled electromagnetic fields and observable implications for primordial black holes
• Survival of black holes through a cosmological bounce
• Local Hubble Expansion: Current State of the Problem
• A Locally Anisotropic Metric for Matter in an Expanding Universe: I. The Ansatz and the Modified Newton Law
• Direct Detection of Universal Expansion by Holonomy in the McVittie Spacetime
• Consistency of the mass variation formula for black holes accreting cosmological fluids
• Relatively complicated? Using models to teach general relativity at different levels
• Horizons and singularity in Clifton's spherical solution of f(R) vacuum
• Hawking radiation and thermodynamics of dynamical black holes in phantom dominated universe
• Entropy of cosmological black holes and generalized second law in phantom energy-dominated universe
• Trapping Horizons in the Sultana-Dyer Space-Time
• McVittie-Plummer Spacetime: Plummer Sphere Immersed in the FLRW Universe
• Evolving black hole horizons in General Relativity and alternative gravity
• Matching McVittie spacetimes
• On cosmological expansion and local physics
• Exact solution for a black hole embedded in a nonstatic dust-filled universe
• Black Hole solutions in a cosmological spacetime background
• Planetary motion on an expanding locally anisotropic background
• Solar System, Astrophysics, and Cosmology from the Derivative Expansion
• Cosmological black holes are not described by the Thakurta metric: LIGO-Virgo bounds on PBHs remain unchanged
• A bound system in the expanding universe with modified holographic Ricci dark energy and dark matter
• Local Peculiar Motions in McVittie and LTB Spacetimes
• Multiscale Cosmic Curvature: from Local Structures to Cosmology
• Spherically symmetric solutions in a FRW background
• Cold Collapse and Bounce of an FLRW Cloud
• New time-dependent solutions of viable Horndeski gravity
• Micro-cosmos model of a nucleon
• Embedding black holes and other inhomogeneities in the universe in various theories of gravity: a short review
• Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
• Black holes in a bouncing universe
• The perturbed FLRW metric on all scales: Newtonian limit and top-hat collapse
• The generalized Lemaitre-Tolman-Bondi solutions with nonzero pressure in modeling the cosmological black holes
• Gravitational Field of a Rotating Mass on an Expanding Universe
• Self-dual solitons in a Born-Infeld baby Skyrme model
• The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
• Back reaction of the gravitational radiation on the metric of spacetime
• Islands in Simulated Cosmos: Probing the Hubble Flow around Groups and Clusters
• Cosmological inhomogeneities, primordial black holes, and a hypothesis on the death of the universe
• Dynamical axisymmetric compact objects in General Relativity
• Naked Singularity in the Sultana-Dyer Space-Time