Discussion Overview
The discussion revolves around the limits of gravitational influence in both Newtonian gravity and General Relativity (GR), particularly in the context of dark energy and its effects on gravitational fields. Participants explore theoretical implications and the nature of gravitational propagation over vast distances.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
Main Points Raised
- Some participants assert that under Newtonian gravity, the gravitational influence has no limits except for the speed of causality and the age of the object, suggesting that the Sun's influence could extend to 4.6 billion light-years.
- Others clarify that in Newtonian mechanics, gravitational fields propagate instantaneously, while in GR, changes propagate at the speed of light.
- A participant questions whether the gravitational field in GR is also infinite, leading to a discussion about the necessity of infinite time for propagation.
- Some propose that dark energy might act as an anti-gravity effect, potentially limiting the propagation of gravitational fields at longer distances.
- Another participant argues that any effect of dark energy would manifest as a change in spacetime curvature, which is inherently linked to the gravitational field in GR.
- There is a suggestion that dark energy does not flatten the universe but produces a different type of spacetime curvature that does not cancel out the effects of gravitational fields.
- One participant expresses uncertainty about the understanding of dark energy, noting that some scientists believe it could be an unknown force while others think it indicates incompleteness in gravitational theory.
- The discussion includes a rephrasing of the original question regarding whether gravity may be attenuated differently at large distances compared to smaller scales, with a focus on the interaction between two distant stars in both Newtonian and GR frameworks.
- Another participant emphasizes that stars must be formed from existing matter, suggesting that gravitational interactions at large distances are influenced by the historical distribution of matter.
Areas of Agreement / Disagreement
Participants express multiple competing views regarding the nature of gravitational influence, the role of dark energy, and the propagation of gravitational fields in GR. The discussion remains unresolved with no consensus on these complex topics.
Contextual Notes
Participants acknowledge limitations in understanding dark energy and its implications for gravitational fields, as well as the dependence on historical matter distribution for gravitational interactions at large distances.