The Primordial Density Perturbation

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Planck 2018 results (2020, methodology): “, Lynden-Bell et al. 1988; Tully et al. 2008). Estimates of the corrections required to obtain the motion of the Galactic centre relative to the CMB and the motion of the centre of mass of the Local Group relative to the CMB were given by Kogut et al. (1993), and have seldom been revisited since the”
Primordial black holes—perspectives in gravitational wave astronomy (2018, background): “ty perturbations, which are classied as the scalar-type, evolve independently of the gravitational waves (GWs), which are classied as the tensor-type, at the linear order in the perturbation (e.g., [194]). This independence no longer holds beyond the linear order, and the GWs are sourced by the dens”
Possible signals of vacuum dynamics in the Universe (2017, background): “…VACUUM Despite the theory of cosmological perturbations has been discussed at length in several specialized textbooks, see e.g. (Peebles 1993; Liddle & Lyth 2000, 2009; Dodelson 2003), the dynamical character of the vacuum produces some changes on the standard equations which are worth…”
Phenomenology of the Lense-Thirring effect in the solar system (2010, methodology): “The inflationary scenario predicts cosmological models in which the Universe undergoes a brief phase of a very rapid expansion in early times (Lyth and Liddle 2009).”