Discussion Overview
The discussion revolves around the concept of inertial frames in relation to the Milky Way's gravitational influence, particularly referencing Erwin Schrödinger's 1925 paper. Participants explore the implications of gravitational potential on inertial frames, the historical context of Schrödinger's claims, and the current understanding of reference frames in astronomy.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
- Historical
Main Points Raised
- Some participants question the relationship between gravitational potential and rotation-free inertial frames, suggesting they may be fundamentally different concepts.
- One participant argues that if the gravitational potential is dominated by the Milky Way, then local frames may be influenced by its rotation, leading to frame-dragging effects.
- Another participant highlights that the common view is that distant stellar systems contribute more significantly to gravitational potential than nearby ones, challenging Schrödinger's assertion.
- A later reply emphasizes the historical context of Schrödinger's work, noting that he lacked knowledge about the size of the Milky Way and the universe at the time of writing.
- Participants discuss the transition in astronomy from using stars to extra-galactic sources for defining non-rotating reference frames, citing changes in methodology since the 1990s.
- One participant mentions the Lense-Thirring effect as a classic example of calculating frame dragging using General Relativity.
Areas of Agreement / Disagreement
Participants express differing views on the relationship between gravitational potential and inertial frames, with no consensus reached on the implications of Schrödinger's claims or the current understanding of reference frames in astronomy.
Contextual Notes
Some limitations include the historical context of Schrödinger's paper, the evolving understanding of gravitational influences, and the unresolved compatibility of relativity with Mach's principle.