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Ignacy Sawicki

Researcher at Academy of Sciences of the Czech Republic

Publications -  61
Citations -  10691

Ignacy Sawicki is an academic researcher from Academy of Sciences of the Czech Republic. The author has contributed to research in topics: Dark energy & General relativity. The author has an hindex of 38, co-authored 61 publications receiving 9349 citations. Previous affiliations of Ignacy Sawicki include Heidelberg University & African Institute for Mathematical Sciences.

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Models of f(R) Cosmic Acceleration that Evade Solar-System Tests

TL;DR: In this paper, the authors study a class of metric-variation models that accelerates the expansion without a cosmological constant and satisfies both cosmologically and solar-system tests in the small-field limit of the parameter space.
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Cosmology and Fundamental Physics with the Euclid Satellite

Luca Amendola, +81 more
TL;DR: Euclid is a European Space Agency medium-class mission selected for launch in 2020 within the cosmic vision 2015-2025 program as discussed by the authors, which will explore the expansion history of the universe and the evolution of cosmic structures by measuring shapes and red-shift of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky.
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Strong Constraints on Cosmological Gravity from GW170817 and GRB 170817A.

TL;DR: It is shown that the detection of an electromagnetic counterpart to the gravitational-wave signal from the merger of two neutron stars allows for stringent constraints on general scalar-tensor and vector-Tensor theories, while allowing for an independent bound on the graviton mass in bimetric theories of gravity.
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Imperfect Dark Energy from Kinetic Gravity Braiding

TL;DR: In this paper, the authors introduce a large class of scalar-tensor models with interactions containing the second derivatives of the scalar field but not leading to additional degrees of freedom.
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Large scale structure of f(R) gravity

TL;DR: In this paper, the evolution of linear cosmological perturbations in f(R) models of accelerated expansion in the physical frame where the gravitational dynamics are fourth order and the matter is minimally coupled is studied.