Synge's world function explained
with smooth Lorentzian metric
. Let
be two points in spacetime, and suppose
belongs to a convex normal neighborhood
of
(referred to the
Levi-Civita connection associated to
) so that there exists a unique
geodesic
from
to
included in
, up to the affine parameter
. Suppose
and
. Then Synge's world function is defined as:
\sigma(x,x')=
(λ1-λ0)\int\gammag\mu\nu(z)t\mut\nudλ
where
is the tangent vector to the affinely parametrized geodesic
. That is,
is half the square of the signed geodesic length from
to
computed along the unique geodesic segment, in
, joining the two points. Synge's world function is well-defined, since the integral above is invariant under reparameterization. In particular, for
Minkowski spacetime, the Synge's world function simplifies to half the spacetime interval between the two points: it is globally defined and it takes the form
\sigma(x,x')=
η\alpha(x-x')\alpha(x-x')\beta.
Obviously Synge's function can be defined also in Riemannian manifolds and in that case it has non-negative sign. Generally speaking, Synge’s function is only locally defined and an attempt to define an extension to domains larger than convex normal neighborhoods generally leads to a
multivalued function since there may be several geodesic segments joining a pair of points in the spacetime. It is however possible to define it in a neighborhood of the diagonal of
, though this definition requires some arbitrary choice.Synge's world function (also its extension to a neighborhood of the diagonal of
) appears in particular in a number of theoretical constructions of
quantum field theory in curved spacetime. It is the crucial object used to construct a
parametrix of
Green’s functions of Lorentzian Green hyperbolic 2nd order partial differential equations in a
globally hyperbolic manifold, and in the definition of Hadamard Gaussian states.
References
- Book: Synge, John, L. . Relativity: the general theory . North-Holland . 1960 . 0-521-34400-X.
- Book: Fulling, Stephen, A. . Aspects of quantum field theory in curved space-time . CUP . 1989 . 0-521-34400-X.
- Poisson . E. . Pound . A. . Vega . I. . The Motion of Point Particles in Curved Spacetime . Living Rev. Relativ. . 14 . 7 . 2011 . 7 . 10.12942/lrr-2011-7 . 28179832 . 5255936 . 1102.0529 . 2011LRR....14....7P . free.
- Moretti . Valter . On the global Hadamard parametrix in QFT and the signed squared geodesic distance defined in domains larger than convex normal neighbourhoods . Letters in Mathematical Physics . 111 . 5 . 2021 . 130 . 10.1007/s11005-021-01464-4 . 2107.04903 . 2021LMaPh.111..130M . free.
- Moretti, Valter (2024) Geometric Methods in Mathematical Physics II: Tensor Analysis on Manifolds and General Relativity, Chapter 7. Lecture Notes Trento University (2024)