Three-dimensional and four-dimensional scalar, vector, tensor cosmological fluctuations and the cosmological decompositi
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Three-dimensional and four-dimensional scalar, vector, tensor cosmological fluctuations and the cosmological decomposition theorem Matthew G. Phelps1 · Asanka Amarasinghe1 · Philip D. Mannheim1 Received: 12 May 2020 / Accepted: 10 October 2020 © Springer Science+Business Media, LLC, part of Springer Nature 2020
Abstract In cosmological perturbation theory it is convenient to use the scalar, vector, tensor basis as defined according to how these components transform under threedimensional rotations. In attempting to solve the fluctuation equations that are automatically written in terms of gauge-invariant combinations of these components, the equations are taken to break up into separate scalar, vector and tensor sectors, the decomposition theorem. Here, without needing to specify a gauge, we solve the fluctuation equations exactly for some standard cosmologies, to show that in general the various gauge-invariant combinations only separate at a higher-derivative level. To achieve separation at the level of the fluctuation equations themselves one has to assume boundary conditions for the higher-derivative equations. While spatially asymptotic boundary conditions suffice for fluctuations around a de Sitter background or a spatially flat Robertson–Walker background, for fluctuations around a spatially non-flat Robertson–Walker background one additionally has to require that the fluctuations be well-behaved at the origin. We show that in certain cases the gauge-invariant combinations themselves involve both scalars and vectors. For such cases there is no decomposition theorem for the individual scalar, vector and tensor components themselves as that would violate gauge invariance, but for the gauge-invariant combinations there still can be. Given the lack of manifest covariance (though not of covariance itself) in defining a basis with respect to three-dimensional rotations, we introduce an alternate scalar, vector, tensor basis whose components are defined according to how they transform under four-dimensional general coordinate transformations. With this basis the fluctuation equations greatly simplify, and while one can again break them up into separate gauge-invariant sectors at the higher-derivative level, in general we find that even with boundary conditions we do not obtain a decomposition theorem in which the fluctuations separate at the level of the fluctuation equations themselves. Keywords Cosmological perturbation theory · Decomposition theorem · Four dimensional formalism
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Contents 1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 The three-dimensional scalar, vector, tensor basis . . . . . . . . . . . . . . . . . . . . . . . . 1.2 The decomposition theorem . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.3 Robertson–Walker considerations . . . . . . . . . . . . . . . . . . . . . . .
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