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This presentation by Dr. Yacoub I. Anini explores the Limiting Curvature Hypothesis, proposing that spacetime curvature possesses a maximum threshold. It examines the vast differences in gravitational force across celestial bodies, from Earth to primordial black holes. The hypothesis suggests that as curvature approaches this limit, spacetime behaves according to De Sitter geometry. Additionally, it discusses novel formulations of Lagrangian mechanics and the implications for gravitational fields, cosmology, and non-singular black holes.
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The Limiting Curvaturehypothesis A new principle of physics Dr. Yacoub I. Anini
Is there a limit to the strength of gravitational force? • The surface gravity of the earth : 9.8 m/s² • The surface gravity of the sun : 270 m/s² • The surface gravity of a white dwarf : 5000,000 m/s² • The surface gravity of a neutron star: • 5,000,000,000,00 m/s² • The surface gravity of a stellar black hole: • 2,000,000,000,000 m/s² • The surface gravity of a premordial black hole • 7,000,000,000,000,000,000,000,000,000,000,0 m/s²
The limiting curvature hypothesis • The curvature of spacetime (all curvature invariants) at any point have a maximum limiting value. Moreover, when the the curvature approaches its limiting value, The spacetime geometry approaches The perfectly regular de sitter geometry.
The Lagrangian • It is possible to implement the limiting Curvature hypothesis by introducing the following lagrangian: L = (R + Λ/2 ) – (Λ/2)(√1 - R²/Λ²), where R is the Ricci scalar curvature and Λ is the limiting value of the curvature.
The contracted field equations • -R -Λ (1 – U ) = -8π G T, • U = √(1- R²/Λ²) • Introducing the following notation : • Β =R/Λ • γ = 8πG (T/Λ) • The contracted field equations take the form • 2β² + 2(1-γ)β + γ² - 2 γ = 0
Expressing β in terms of γ Β = - ½ (1 – γ ) ±½√1 - γ² + 2γ It is clear that if β is to be real then there will Be a limit on the allowed values of γ (1-√2 ) < γ < (1+ √2 )
By varying the gravitational action with respect to the metric we obtainthe new field equations • Gμν - ¼ [1 - √(1- R²/Λ²)] gμν = - 8π G Tμν
Spaces of constant curvature • Writing the field equation for A homogeneous and isotropic space • The cosmological Case
The limiting geometry • The limiting gravitational state • The limiting value of curvature • The limiting state of matter • The limiting value of density
Some Cosmological solutions • The limiting de sitter geometry • The radiation filled universe • The matter filled universe • The general case ( radiation + matter )
Spherically symmetric solutions • Writing the field equations for spherically Symmetric solutions • Non- singular black holes
The numerical value of the limiting curvature • Low curvature limiting value (effective gravity theory) • Planck –scale limiting curvature (quantum Gravity scale)
Spherically Symmatric solutions • Non- Singular Black Holes
references • Collapse to a Black Hole (Movie)_files • Falling to the Singularity of the Black Hole (Movie)_files • Sphere collapsing to a black hole_files
White Holes and Wormholes.htm • paper.pdf • Falling to the Singularity of the Black Hole (Movie).htm
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