In his short essay, “How Great Equations Survive,” Nobel laureate physicist Steven Weinberg argues that though equations survive through scientific change, they are reinterpreted in light of the developments of theory. “The equations of General Relativity,” he argues, “have undergone a similar reinterpretation.” Weinberg devotes attention to the point that “the equations” are of the type known as “second order differential equations." This means "that the equations were assumed by Einstein to involve only rates of change of the fields (first derivatives) and rates of change of rates of change (second derivatives) but not rates of higher order.” This he sees as something of a reasonable idealization. “I don’t know,” he writes, “any place where Einstein explains the motivation for this assumption.”

“Today,” Weinberg continues, “General Relativity is widely (though not universally regarded as another effective field theory, useful only for distances much larger than about 10 (to the -33rd) centimeters, and particle energies much less than an energy equivalent to the mass of 10 (to the 19th) protons. No one today would (or at least no one should) take seriously any consequence of General Relativity for shorter distances or larger energies.”

“The more important an equation is,” he writes, “the more we have to be alert to changes in its significance.” It seems then that the meaning of the equations in Einstein’s original papers is different from the meaning attributed to them as an “effective field theory.”

See, Weinberg 2009, “How Great Equations Survive,” in Lake Views, pp. 54-55.

From the Wikipedia:

The Einstein field equations (EFE) may be written in the form:

(This failed to reproduce, but see the link below.)

where is the Ricci curvature tensor, is the metric tensor, is the cosmological constant, is Newton’s gravitational constant, is the speed of light in vacuum, is the scalar curvature and is the stress-energy tensor.

The EFE is a tensor equation relating a set of symmetric 4x4 tensors. Each tensor has 10 independent components. The four Bianchi identities reduce the number of independent equations from 10 to 6, leaving the metric with four gauge fixing degrees of freedom, which correspond to the freedom to choose a coordinate system.

See: https://en.wikipedia.org/wiki/Einstein_field_equations#Mathematical_form

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