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20052023
most citedPlanck 2018 results. I. Overview and the cosmological legacy of Planck

1.7k citations · 2.7k across the 19 of their papers we have counts for

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gr-qc2023★ 48 cited

Stochastic gravitational wave background reconstruction for a non-equilateral and unequal-noise LISA constellation

Olaf Hartwig, Marc Lilley, Martina Muratore +1

We explore the impact of choosing different sets of Time-Delay Interferometry (TDI) variables for detecting and reconstructing Stochastic Gravitational Wave Background (SGWB) signa…

gr-qc2022★ 32 cited

Time delay interferometry without clock synchronisation

Olaf Hartwig, Jean-Baptiste Bayle, Martin Staab +3

Time-delay interferometry (TDI) is a data processing technique for LISA designed to suppress the otherwise overwhelming laser noise by several orders of magnitude. It is widely bel…

gr-qc2014★ 23 cited

Non-Gaussianity excess problem in classical bouncing cosmologies

Xian Gao, Marc Lilley, Patrick Peter

The simplest possible classical model leading to a cosmological bounce is examined in the light of the non-Gaussianities it can generate. Concentrating solely on the transition bet…

gr-qc2014★ 16 cited

Production of non-gaussianities in a bouncing phase

Xian Gao, Marc Lilley, Patrick Peter

We compute the level of non-gaussianities produced by a cosmological bouncing phase in the minimal non-singular setup that lies within the context of General Relativity when the ma…

gr-qc2011★ 22 cited

Observational signatures of a non-singular bouncing cosmology

Marc Lilley, Larissa Lorenz, Sebastien Clesse

We study a cosmological scenario in which inflation is preceded by a bounce. In this scenario, the primordial singularity, one of the major shortcomings of inflation, is replaced b…

gr-qc2008★ 60 cited

A classical bounce: constraints and consequences

Felipe T. Falciano, Marc Lilley, Patrick Peter

We perform a detailed investigation of the simplest possible cosmological model in which a bounce can occur, namely that where the dynamics is led by a simple massive scalar field…