Symbol y_2
is part of the quantity the equation computes from the expression on the right.
Read this term in its guide →Published equation contexts
An exact analytic evaluation, not a simulation, fixes the scale this actually requires. Take three clocks stacked vertically at heights -h , 0 , and +h near Earth’s surface, giving two edges = - and = - . Their difference is an exact finite-difference identity up to a Taylor remainder of order : . For Earth modelled as a point mass, = -GM/r gives a radial second derivative of magnitude 2GM/ and, since is harmonic in vacuum, transverse second derivatives of magnitude GM/ with the opposite sign — a trace-free tensor in the exact ratio 2:{-1}:{-1} . With the standard gravitational parameter G =…
is part of the quantity the equation computes from the expression on the right.
Read this term in its guide →phi_,zz is one of the signed contributions combined to compute the quantity on the left.
Read this term in its guide →O is one of the signed contributions combined to compute the quantity on the left.
Read this term in its guide →is one of the signed contributions combined to compute the quantity on the left.
Read this term in its guide →Read it with the definitions, units, and assumptions supplied by the article.
A symbol can carry a different meaning in another article. Each occurrence keeps its own guide and term definitions.
Equation 123 · Evolutionary Physics
This equation states an equality: the expressions on both sides have the same value under the article’s assumptions.
An exact analytic evaluation, not a simulation, fixes the scale this actually requires. Take three clocks stacked vertically at heights -h , 0 , and +h near Earth’s surface, giving two edges = - and = - . Their difference is an exact finite-difference identity up to a Taylor remainder of order : . For Earth modelled as a point mass, = -GM/r gives a radial second derivative of magnitude 2GM/ and, since is harmonic in vacuum, transverse second derivatives of magnitude GM/ with the opposite sign — a trace-free tensor in the exact ratio 2:{-1}:{-1} . With the standard gravitational parameter G =…