Conformal Gravity: Understanding Attractive & Repulsive Forces

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SUMMARY

The paper "Attractive and Repulsive Gravity" by Philip Mannheim (2000) introduces the theory of conformal gravity, which modifies the Einstein-Hilbert action to allow for MOND-like gravity at galactic scales and eliminates singularities associated with the big bang and black holes by introducing repulsive gravity under dense energy conditions. This theory posits a "big time zero bounce" instead of a big bang, suggesting a unique origin for the universe and addressing the cosmological constant problem. While it aligns closely with general relativity (GR) and lacks independent support, conformal gravity presents a compelling alternative to prevailing cosmological models and offers insights into the nature of gravity.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with the Einstein-Hilbert action
  • Knowledge of Modified Newtonian Dynamics (MOND)
  • Basic concepts of cosmology and the cosmological constant
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  • Research the implications of conformal gravity on cosmological models
  • Explore the relationship between conformal gravity and Loop Quantum Gravity (LQG)
  • Investigate the concept of vacuum energy in cosmology
  • Examine alternative cosmological theories, such as Quasi-Steady State cosmology
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The discussion is beneficial for theoretical physicists, cosmologists, and researchers interested in alternative theories of gravity and the implications for the universe's origin and structure.

ohwilleke
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The paper "Attractive and Repulsive Gravity", http://arxiv.org/PS_cache/gr-qc/pdf/0001/0001011.pdf by Philip Mannheim (2000) sets out at some length his theory of conformal gravity.

He starts by breaking the evidence in support of GR into those that flow from its geometric nature, which he seeks to preserve, and those which flow from the form of the Einstein-Hilbert action. He notes that his amendment of the EH action can make possible a MOND like gravity at galactic scales, eliminates the big bang and black hole singularities by making gravity repulsive in the presence of very dense energy sources and in the cosmological limit, and resolves a number of issues associated with the cosmological constant problem. It also states that at galactic and cosmological scales that there is a Machian component to gravity (i.e. the force of gravity is in part a function of the aggregate mass of the universe). Since it flows closely from the GR equations it is theoretically "well behaved".

It proposes rather than a big bang, a big time zero bounce from a minimum finite radius in which the universe has a maximal temperature (possiblity eliminating the issue of inflation), because beneath that radius the repulsive aspect of gravity overcomes other forces. It suggests that under this theory, the low ratio of matter to a running cosmological constant in the Omega sum is inevitable regardless of initial condition, rather than a coincidence.

Of particular interest to those looking to derive a quantum gravity, he accepts a figure for vacuum energy from cosmology, and uses that conclusion to determine that the gravitational constant must be deeply wrong.

While this theory has little independent support (i.e. it does not differ from GR where it reduces to GR, does not differ greatly from MOND where it reduces to MOND, does not differ from Newtonian gravity where it reduces to Newtonian gravity, and fits cosmological data by design rather than prediction) it should stand as a significant alternative to either cosmological constant cold dark matter models (the prevailing paradigm), or Relativistic MOND models (the main alternative at the galactic scale), or alternative cosmologies such as those of Arp (Quasi-Steady State).

The conclusions reached are not dramatically different from those of LQG, and indeed resemble LQG also in that LQG theorists sometimes see gravity as a counterpoint to QCD which like Mannheim's conformal gravity changes from repulsive to attractive at different distance scales.
 
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Overall, Mannheim's conformal gravity presents an interesting and thought-provoking alternative to the current theories of gravity. By preserving the geometric nature of general relativity while also addressing issues such as the cosmological constant problem and the big bang singularity, this theory offers a unique perspective on the nature of gravity and its effects on the universe.

One particularly intriguing aspect of this theory is the idea of a big time zero bounce, which suggests a different origin for the universe than the commonly accepted big bang theory. This could potentially lead to a better understanding of the early universe and its evolution.

However, as noted, this theory currently lacks independent support and its predictions are not significantly different from other existing theories in certain regimes. Therefore, more research and evidence is needed to fully evaluate the validity and potential of conformal gravity. But as a significant alternative to current theories, it is certainly worth further exploration and consideration.
 

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