Discussion Overview
The discussion revolves around whether a gravitational field generated by a mass (A) influences that same mass (A) in addition to affecting other masses (B). The scope includes theoretical considerations in classical and relativistic physics, as well as implications in quantum theory.
Discussion Character
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants propose that mass A cannot be accelerated by the gravitational field it generates.
- Others argue that extended sources can self-interact, citing examples such as the pressure in the Earth's core due to gravitational influences.
- A participant mentions that point sources in classical physics lead to singularities and require quantum theory for proper description.
- One participant suggests that the symmetry of the situation is important, noting that both masses A and B exert forces on each other through their respective fields.
- In a relativistic context, it is suggested that the gravitational field does influence the originating mass, drawing parallels to electromagnetic radiation reaction and its unresolved issues in point particle theory.
- Another participant highlights that gravitational waves can affect the motion of their sources, referencing the Hulse-Taylor pulsar as an example.
Areas of Agreement / Disagreement
Participants express differing views on whether a mass can be influenced by its own gravitational field, with some asserting it cannot while others suggest that it can under certain conditions. The discussion remains unresolved with multiple competing perspectives.
Contextual Notes
The discussion touches on limitations related to classical versus quantum descriptions of gravitational fields, as well as the implications of relativistic effects and the challenges of singularities in point mass scenarios.