Did the Universe Experienced a Pressure non-Crushing Type Cosmological Singularity in the Recent Past?
arXiv:2201.07647 · doi:10.1209/0295-5075/ac52dc
Abstract
In the recent literature it has been shown that the tension may be eliminated if an abrupt physics transition changed the Cepheid parameters in the near past of the Universe, nearly Myrs ago. In this letter we stress the possibility that this abrupt transition was caused by the smooth passage of our Universe through a pressure finite-time cosmological singularity. Being a non-crushing type singularity the pressure singularity can leave its imprints in the Universe, since it occurs globally and literally everywhere. We discuss how this scenario could easily be realized by gravity, with the strong energy conditions being satisfied without the need for a scalar field or specific matter fluids. We also stress the fact that the pressure singularity can affect the effective gravitational constant of gravity. Moreover, we stress the fact that pressure singularities can disrupt the trajectories of bound objects in the Universe, which is also pointed out in the literature, even in the context of general relativity. We also show numerically in a general relativistic framework that elliptic trajectories are distorted and changed to different elliptic trajectories when the Universe passes through the pressure singularity. Such a disruption of the trajectories could have tidal effects on the surface of the earth, for example on sea waters and oceans, regarding the distortion of moon's elliptic trajectory. Accordingly, the distortion of earth's trajectory around the sun could have affected climatologically earth Myrs ago.
arXiv commentEPL Accepted
References in corpus (41)
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Phantom Energy and Cosmic Doomsday
- Properties of singularities in (phantom) dark energy universe
- Tensions between the Early and the Late Universe
- Quantum deSitter cosmology and phantom matter
- The final state and thermodynamics of dark energy universe
- Cosmological Dynamics of Phantom Field
- Can the Chaplygin gas be a plausible model for dark energy?
- Sudden Future Singularities
- Quantum escape of sudden future singularity
- Constructing Phantom Cosmologies from Standard Scalar Field Universes
- The dS/CFT Correspondence and the Big Smash
- Phantom Field and the Fate of Universe
- The Fate of Bound Systems in Phantom and Quintessence Cosmologies
- Geodesic behavior of sudden future singularities
- Superquintessence
- Cosmographic bounds on the cosmological deceleration-acceleration transition redshift in gravity
- Two-field Models of Dark Energy with Equation of State Across -1
- Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
- Worse than a big rip?
- Generalized phantom energy
- New Isotropic and Anisotropic Sudden Singularities
- Singular Bouncing Cosmology from Gauss-Bonnet Modified Gravity
- Dark energy cosmology with generalized linear equation of state
- Quantum phantom cosmology
- Bouncing cosmology with future singularity from modified gravity
- A rapid transition of at as a solution of the Hubble and growth tensions
- Phantom-like GCG and the constraints of its parameters via cosmological dynamics
- On big rip singularities
- Avoidance of Big Rip In Phantom Cosmology by Gravitational Back Reaction
- Cosmic history of viable exponential gravity: Equation of state oscillations and growth index from inflation to dark energy era
- Hubble tension or a transition of the Cepheid SnIa calibrator parameters?
- Singular Inflation
- A quantitative analysis of singular inflation with scalar-tensor and modified gravity
- Sudden singularities survive massive quantum particle production
- Singular cosmological evolution using canonical and phantom scalar fields
- Tradeoff between Smoother and Sooner "Little Rip"
- The fate of bound systems through Sudden Future Singularities
- Finite time future singularities in the interacting dark sector
- Is the Hubble crisis connected with the extinction of dinosaurs?
- Big brake singularity is accommodated as an exotic quintessence field
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- Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
- Is the Observable Universe Consistent with the Cosmological Principle?
- Is Local At Odds With Dark Energy EFT?
- Finite-time Cosmological Singularities and the Possible Fate of the Universe
- Gaussian processes and effective field theory of gravity under the tension
- Multidimensionality of the Hubble tension: the roles of and
- Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant
- Early Dark Energy with Power-law F(R) Gravity
- Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
- Stepped Partially Acoustic Dark Matter, Large Scale Structure, and the Hubble Tension
- Recent advances in cosmological singularities
- Gravitational transitions via the explicitly broken symmetron screening mechanism
- Improved constraint on primordial gravitational waves in light of the Hubble tension and BICEP/Keck
- Solving the tension in Gravity through Bayesian Machine Learning
- The Unsettled Number: Hubble's Tension
- Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
- Singularity formation in asymptotically safe cosmology with inhomogeneous equation of state
- Does the fraction of dark matter diminish with early dark energy?
- On finite time singularities in scalar field dark energy models based in the RS-II Braneworld
- Hubble constant by natural selection: Evolution chips in the Hubble tension
- Cosmological singularities in gravity
- New perspectives on future rip scenarios with holographic dark energy
- Resilience and implications of adiabatic CMB cooling
- Another look on the connections of Hubble tension with the Heisenberg Uncertainty Principle
- 2D BAO vs 3D BAO: Hints for new physics?
- Equality scale-based and sound horizon-based analysis of the Hubble tension
- Type V singularities with inhomogeneous equations of state
- Solving the Hubble tension à la Ellis & Stoeger 1987
- Rips and regular future scenario with Holographic Dark Energy: A comprehensive look
- On rips and cosmological singularities in a universe merging with baby universes
- Periodic orbits and gravitational waveforms of black holes in bumblebee gravity
- Sample Variance for Supernovae Distance Measurements and the Hubble tension
- Nature-inspired optimization, the Philippine Eagle, and cosmological parameter estimation