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Jose Luis Blázquez-Salcedo

Researcher at Complutense University of Madrid

Publications -  77
Citations -  2296

Jose Luis Blázquez-Salcedo is an academic researcher from Complutense University of Madrid. The author has contributed to research in topics: Neutron star & Black hole. The author has an hindex of 20, co-authored 72 publications receiving 1670 citations. Previous affiliations of Jose Luis Blázquez-Salcedo include University of Oldenburg.

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Black holes, gravitational waves and fundamental physics: a roadmap.

Leor Barack, +205 more
TL;DR: A comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress can be found in this article, where the authors present a concise, yet comprehensive overview.
Journal ArticleDOI

Black holes, gravitational waves and fundamental physics: a roadmap

Leor Barack, +231 more
TL;DR: A comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress can be found in this article, which is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'.
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Perturbed black holes in Einstein-dilaton-Gauss-Bonnet gravity: Stability, ringdown, and gravitational-wave emission

TL;DR: In this article, the topological Gauss-Bonnet invariant coupled to a dilaton was shown to be stable against both axial and polar perturbations, and the quasinormal modes of black holes can be excited during collisions involving black holes.
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Radial perturbations of the scalarized Einstein-Gauss-Bonnet black holes

TL;DR: In this article, the axial perturbations of spontaneously scalarized black holes in the Gauss-Bonnet model were studied and the spectrum of the quasinormal modes by time evolution was determined by solving the associated time-independent eigenvalue problem.
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Radial perturbations of the scalarized EGB black holes

TL;DR: In this article, the radial perturbations of scalarized EGB black holes were studied and the stability of the solutions on the fundamental branch, whose scalar field has no radial nodes, depends on the particular choice of the coupling function between the scalar fields and the Gauss-Bonnet invariant.