The Galilei-covariant tensor formulation is a method for treating non-relativistic physics using the extended Galilei group as the representation group of the theory. It is constructed in the light cone of a five dimensional manifold.
Takahashi et. al., in 1988, began a study of Galilean symmetry, where an explicitly covariant non-relativistic field theory could be developed. The theory is constructed in the light cone of a (4,1) Minkowski space.[1][2][3][4] Previously, in 1985, Duval et. al. constructed a similar tensor formulation in the context of Newton–Cartan theory.[5] Some other authors also have developed a similar Galilean tensor formalism.[6][7]
Galilean Manifold
The Galilei transformations are
where stands for the three-dimensional Euclidean rotations,
is the relative velocity determining Galilean boosts, a stands for spacial translations and b, for time translations. Consider a free mass particle
; the mass shell relation is given by
.
We can then define a 5-vector, , with
.
Thus, we can define a scalar product of the type
where
is the metric of the space-time, and .[3]
Extended Galilei Algebra
A five dimensional Poincaré algebra leaves the metric invariant,
We can write the generators as
The non-vanishing commutation relations will then be rewritten as
An important Lie subalgebra is
is the generator of time translations (Hamiltonian), Pi is the generator of spatial translations (momentum operator),
is the generator of Galilean boosts, and
stands for a generator of rotations (angular momentum operator). The generator
is a Casimir invariant and
is an additional Casimir invariant. This algebra is isomorphic to the extended Galilean Algebra in (3+1) dimensions with
, The central charge, interpreted as mass, and
.[citation needed]
The third Casimir invariant is given by , where
is a 5-dimensional analog of the Pauli–Lubanski pseudovector.[citation needed]
Bargmann structures
In 1985 Duval, Burdet and Kunzle showed that four-dimensional Newton–Cartan theory of gravitation can be reformulated as Kaluza–Klein reduction of five-dimensional Einstein gravity along a null-like direction. The metric used is the same as the Galilean metric but with all positive entries
This lifting is considered to be useful for non-relativistic holographic models.[8] Gravitational models in this framework have shown to precisely calculate the mercury precession.
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