Page:The principle of relativity (1920).djvu/192

From Wikisource
Jump to navigation Jump to search
This page needs to be proofread.

sign δ corresponds to a passage from a point of the geodetic curve sought-for to a point of the contiguous curve, both lying on the same surface λ.

Then (20) can be replaced by

        { λ_3
        { [integral]δω dλ = 0
(20a) { λ_1
        {
        { ω^2 = g_{μν}(dx_μ/dλ)(dx_ν/dλ)

But

δω = (1/ω){1/2([part]g_{μν}/[part]x_σ) · (dx_μ/dλ) · (dx_ν/dλ) · δx

  + g_{μν}(dx_μ/dλ)δ(dx_ν/dλ)}

So we get by the substitution of δω in (20a), remembering that

δ(dx_ν/dλ) = (d/dλ)(δx_ν)

after partial integration,

        { λ_3
        { [integral] dλ k_σ δx_σ = 0
(20b) { λ_1
        {
        { where k_σ = (d/dλ){(g_{μν}/ω) · (dx_μ/dλ)} - (1/(2ω))([part]g_{μν}/[part]x

            ×(dx_μ/dλ) · (dx_ν/dλ).