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Ivancevic_Applied-Diff-Geom

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<strong>Geom</strong>etrical Path Integrals and Their Applications 1169sidered as continuous limits of ordered discrete sets of relativistic particlesfor which the tangential velocities were excluded from the action. The authorshave proved that p−branes might be considered as continuous limitsof discrete sets of relativistic particles and that the p−brane action∫S = −γ d p+1 σ √ (−1) p g,g = det ∂xµ∂σ a∂x µ∂σ b, (6.284)is a continuous limit of sum of properly modified relativistic particle actions.Here a, b = 0, 1, . . . , p and µ = 0, 1, . . . , n where p + 1 and n + 1 are thebrane world–sheet and the bulk space dimensions respectively; g is theinduced metric determinant on the world–sheet. Strings correspond to thep = 1 case in (6.284). The modification is such that particle motions alongthe brane hypersurface become un–physical. It yields p constraints; theremaining constraint (H = 0) is a consequence of arbitrariness of ‘time’ σ 0 .The authors have also found the linear constraints in un–physical momenta,which allowed them to derive the evolution operators for the objects underconsideration from the ‘first principles’.6.6.1 A Relativistic ParticleFollowing [Golovnev and Prokhorov (2005)], we start with the simplest caseof one relativistic particle which can be formally considered as a 0−brane.Recall that the motion of free relativistic particle is defined by the well–known action∫ √S = −m 1 − −→ v 2 dt,where −→ v = d−→ x (t)dt. The canonical momentum is−→ ∂L p ≡∂ −→ v = m−→ v√1 − −→ ≡ E −→ v 2 p v ,with L being the Lagrangian, and the Hamiltonian is√H = E p = m 2 + −→ p 2 .We can write down the action in the explicitly relativistic invariant form byparametrization of the world line: x µ = x µ (σ 0 ) (usually one uses τ insteadof σ 0 ) withx µ (σ 0 ) = (t(σ 0 ), −→ x (σ 0 )),(µ = 0, . . . , n).

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