Discussion Overview
The discussion revolves around the relationship between pressure and gravitational potential energy in the context of Newtonian gravity. Participants explore the implications of pressure as a source of gravity, the Tolman paradox, and the integration of pressure over a static system to relate it to potential energy. The conversation includes theoretical considerations and intuitive explanations, with a focus on hydrostatic equilibrium and the mathematical representation of these concepts.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- One participant describes a method to show that in a static system, the total pressure integrated over planes is equal and opposite to the gravitational potential energy, suggesting a relationship between pressure and potential energy.
- Another participant agrees that the relationship seems intuitive, noting that in hydrostatic equilibrium, pressure balances gravitational force, leading to an expectation that the integral of pressure relates to potential energy.
- Concerns are raised about the idea of "removing a support instantly," with one participant explaining that such a model is not feasible in General Relativity due to the Bianchi identities, which do not have a counterpart in Newtonian gravity.
- Discussion includes a consideration of how sudden changes in pressure or support could be modeled differently in Newtonian versus relativistic contexts, emphasizing the constraints imposed by the nature of the gravitational framework.
- Participants express a desire for a simpler mathematical representation of the integral relating pressure and potential energy without resorting to multiple integrals along different axes.
Areas of Agreement / Disagreement
Participants generally agree on the intuitive relationship between pressure and gravitational potential energy in static systems, but there is no consensus on the implications of this relationship or the validity of certain models, particularly regarding instantaneous changes in support or pressure.
Contextual Notes
Limitations include the dependence on the assumptions of static equilibrium and the challenges in modeling instantaneous changes in pressure or support in both Newtonian and relativistic frameworks. The discussion does not resolve the complexities involved in these transitions.