Einstein presents the field equations of general relativity
node
After eight years of work Einstein presented the final form of the gravitational field equations to the Prussian Academy of Sciences in Berlin in November 1915, describing gravity as the curvature of spacetime by mass and energy rather than as a force. The equations are nonlinear and were expected to resist exact solution; the immediate successes were the perihelion precession of Mercury, computed by Einstein himself, and the prediction of light deflection later tested in 1919. Everything in this Journey is a consequence of these equations, and the first of those consequences arrived within weeks.
A node is not a place. Drawing it on a map would assert something about the world that no stored fact supports.
Read in · 1
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 2
- Schwarzschild radiusconcerns
- Gravitational wavesconcerns
Assembled narrative · 1
Assembled from 21 blocks · 1 evidence · 19 related
- Story
- After eight years of work Einstein presented the final form of the gravitational field equations to the Prussian Academy of Sciences in Berlin in November 1915, describing gravity as the curvature of spacetime by mass and energy rather than as a force. The equations are nonlinear and were expected to resist exact solution; the immediate successes were the perihelion precession of Mercury, computed by Einstein himself, and the prediction of light deflection later tested in 1919. Everything in this Journey is a consequence of these equations, and the first of those consequences arrived within weeks.
- Knowledge
- Schwarzschild radius
- Gravitational waves
- Einstein presents the field equations of general relativity
- Connections
- Schwarzschild radius
- Gravitational waves
- Karl Schwarzschild
- The event horizon
- The photon sphere and the shadow
- Time dilation near a horizon
- Tidal stretching near a black hole
- Einstein presents the field equations of general relativity
- Schwarzschild solves the field equations for a point mass
- Einstein presents the field equations of general relativity
- GW150914 - two black holes merge and the signal reaches Earth
- The detection is announced and published
- Evidence
- The first exact solution of the Einstein field equations for the vacuum outside a spherical mass, containing the radius now named for its author. V55 VERIFICATION BASIS: the paper was NOT consulted in this session - WebFetch was refused by the network egress proxy for every host attempted and the WebSearch budget was exhausted before authoring began. Title, venue and page range are given from the author's recall of a canonical citation and must be checked.
Observed changes · 0
No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.
Actions
/atlas?object=EVT_EINSTEIN_FIELD_EQUATIONS_1915&experience=EVT_EINSTEIN_FIELD_EQUATIONS_1915