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20032025
most citedDensity Perturbations in the Early Universe

2 citations · 5 across the 7 of their papers we have counts for

collaborators

7 papers

gr-qc2025

Earliest Structures in the Universe can be explained by a Relativistic Cosmological Perturbation Theory

Pieter G. Miedema

A relativistic cosmological perturbation theory for the Friedmann-Lemaître-Robertson-Walker universe is presented that explains the masses and formation times of the first structur…

gr-qc2016

Structure Formation in the Early Universe

P. G. Miedema

The evolution of the perturbations in the energy density and the particle number density in a flat Friedmann-Lemaitre-Robertson-Walker universe in the radiation-dominated era and i…

gr-qc2014★ 1 cited

General Relativistic Evolution Equations for Density Perturbations in Closed, Flat and Open FLRW Universes

P. G. Miedema

It is shown that the decomposition theorems of York, Stewart and Walker for symmetric spatial second-rank tensors, such as the perturbed metric tensor and perturbed Ricci tensor, a…

gr-qc2011★ 1 cited

Relativistic Cosmological Perturbation Theory and the Evolution of Small-Scale Inhomogeneities

P. G. Miedema

It is shown that a first-order relativistic perturbation theory for the open, flat or closed Friedmann-Lemaitre-Robertson-Walker universe admits one, and only one, gauge-invariant…

gr-qc2010

Manifestly Covariant Gauge-invariant Cosmological Perturbation Theory

P. G. Miedema, W. A. van Leeuwen

It is shown that a first-order cosmological perturbation theory for the open, flat and closed Friedmann-Lemaître-Robertson-Walker universes admits one, and only one, gauge-invarian…

gr-qc2008★ 1 cited

Structure Formation independent of Cold Dark Matter

P. G. Miedema

It is shown that a first-order cosmological perturbation theory for Friedmann-Lemaitre-Robertson-Walker universes admits one and only one gauge-invariant variable which describes t…