Massless scalar field 2026-10-14
A free real scalar field with zero mass has the displayed wave equation in Minkowski spacetime. In curved spacetime its dynamics also depend on curvature coupling: a minimally coupled massless scalar field and a conformally coupled scalar field need not have the same cosmological modes.
The displayed action functional contains no mass term and no curvature coupling. Its Euler-Lagrange field equation is . In a flat FLRW metric, a Fourier mode obeys in four dimensions. The expansion can therefore freeze these modes; the curvature term of a conformally coupled scalar field changes that conclusion.
For the FLRW metric in conformal time, , and . The equation for a minimally coupled massless scalar field is consequently
For a Fourier mode of comoving wavevector , the Laplacian contributes , where . Thus
Since , this yields
The absence of a curvature-coupling term is material: a conformally coupled scalar field obeys a different mode equation.
For a scalar operator of dimension in a boundary theory of dimension , the AdS scalar mass--dimension relation gives
in unit-radius . In Poincare coordinates,
so the free Klein-Gordon equation is
This mass is exactly that of a conformally coupled scalar field in four-dimensional anti-de Sitter spacetime. The Weyl transformation
therefore maps the equation to the flat half-space wave equation
The Euler-Lagrange equation is
After a spatial Fourier transform and the change to conformal time, , this becomes
For the exact de Sitter spacetime scale factor , one has . Setting therefore cancels both the friction term and the effective mass term, leaving
This is the special cancellation for a conformally coupled scalar field.
Varying the scalar action and Fourier transforming the spatial coordinates gives the Klein-Gordon equation
In de Sitter spacetime, and , so
Direct substitution shows that and are independent solutions. Hence
The mass value is the one that gives a conformally coupled scalar field in four-dimensional de Sitter spacetime.