Time-Dependent Gravitational Constant Reconciling Historic Equations with Modern Observations

Abstract: The gravitational constant (G) is one of the fundamental parameters governing cosmic evolution, yet the possibility of its time variation has been widely debated in gravitational physics, cosmology, and modified gravity theories. While Newtonian and Einsteinian gravity assume G is constant, several theoretical models—including scalar-tensor theories, extra-dimensional frameworks, and quantum gravity corrections—suggest that G may evolve over cosmological timescales. This paper revisits the time-dependent gravitational constant hypothesis, exploring its implications for cosmic expansion, large-scale structure formation, and gravitational wave propagation. We examine how historic equations, including those from Newton’s law of universal gravitation and Einstein’s field equations, can be reconciled with modern observational constraints from pulsar timing, cosmic microwave background anisotropies, and precision gravitational wave data. Additionally, we investigate whether higher-dimensional gravity, scalar fields, or emergent spacetime models could naturally lead to a varying G, without violating existing experimental bounds. Key Highlights: Reviewing historical equations for gravity in light of possible time-dependence of G. Theoretical models predicting a variable G, including scalar-tensor and extra-dimensional theories. Observational constraints from pulsars, gravitational waves, and cosmological expansion. Implications for dark energy, cosmic acceleration, and modified gravity theories. Potential experimental tests in next-generation gravitational physics research. By integrating insights from classical gravity, quantum field theory, and observational astrophysics, this work presents a refined framework for exploring the time evolution of G, offering potential experimental pathways for testing variations in fundamental constants. Keywords: Gravitational constant, time-dependent gravity, scalar-tensor theories, extra dimensions, quantum gravity, cosmic evolution, modified gravity, pulsar timing, gravitational waves, fundamental physics.

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-03-16
DOI
https://doi.org/10.5281/zenodo.15036190
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
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article

Time-Dependent Gravitational Constant Reconciling Historic Equations with Modern Observations

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Time-Dependent Gravitational Constant Reconciling Historic Equations with Modern Observations

article en

Abstract

Abstract: The gravitational constant (G) is one of the fundamental parameters governing cosmic evolution, yet the possibility of its time variation has been widely debated in gravitational physics, cosmology, and modified gravity theories. While Newtonian and Einsteinian gravity assume G is constant, several theoretical models—including scalar-tensor theories, extra-dimensional frameworks, and quantum gravity corrections—suggest that G may evolve over cosmological timescales. This paper revisits the time-dependent gravitational constant hypothesis, exploring its implications for cosmic expansion, large-scale structure formation, and gravitational wave propagation. We examine how historic equations, including those from Newton’s law of universal gravitation and Einstein’s field equations, can be reconciled with modern observational constraints from pulsar timing, cosmic microwave background anisotropies, and precision gravitational wave data. Additionally, we investigate whether higher-dimensional gravity, scalar fields, or emergent spacetime models could naturally lead to a varying G, without violating existing experimental bounds. Key Highlights: Reviewing historical equations for gravity in light of possible time-dependence of G. Theoretical models predicting a variable G, including scalar-tensor and extra-dimensional theories. Observational constraints from pulsars, gravitational waves, and cosmological expansion. Implications for dark energy, cosmic acceleration, and modified gravity theories. Potential experimental tests in next-generation gravitational physics research. By integrating insights from classical gravity, quantum field theory, and observational astrophysics, this work presents a refined framework for exploring the time evolution of G, offering potential experimental pathways for testing variations in fundamental constants. Keywords: Gravitational constant, time-dependent gravity, scalar-tensor theories, extra dimensions, quantum gravity, cosmic evolution, modified gravity, pulsar timing, gravitational waves, fundamental physics.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 62%
Cosmology and Gravitation Theories
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