José Pedro Mimoso

Prof. José Pedro Mimoso

Departamento de Física, Centro de Astronomia e Astrofísica da Universidade de Lisboa, Campo Grande, Edifício C8, P-1749-016 LISBOA, Portugal
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Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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30 April 2025 in Astronomy & Astrophysics
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ECEuclid Collaboration
Euclid Collaboration
YMY. Mellier
Y. Mellier
AFAbdurro’u F
Abdurro’u F
JBJ. A. Acevedo Barroso
J. A. Acevedo Barroso
AAA. Achúcarro
A. Achúcarro
LLLler Ller
Ller Ller
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015–2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14 000 deg2 of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance.

28 August 2023 in Living Reviews in Relativity
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PAPierre Auclair
Pierre Auclair
DBDavid Bacon
David Bacon
TBTessa Baker
Tessa Baker
TBTiago Barreiro
Tiago Barreiro
NBNicola Bartolo
Nicola Bartolo
TGThe LISA Cosmology Working Group
The LISA Cosmology Working Group
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.

20 June 2025 in Physics of the Dark Universe
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Eleonora Di ValentinoEleonora Di Valentino
Eleonora Di Valentino
JSJackson Levi Said
Jackson Levi Said
ARAdam Riess
Adam Riess
APAgnieszka Pollo
Agnieszka Pollo
VPVivian Poulin
Vivian Poulin
ZDZahra Davari
Zahra Davari

5 June 2015 in Physical Review D
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Salvatore CapozzielloSalvatore Capozziello
Salvatore Capozziello
Francisco S. N. LoboFrancisco S. N. Lobo
Francisco S. N. Lobo
José Pedro MimosoJosé Pedro Mimoso
José Pedro Mimoso
In this work, we consider the further degrees of freedom related to curvature invariants and scalar fields in extended theories of gravity (ETG). These new degrees of freedom can be recast as “effective fluids” that differ in nature with respect to the standard matter fluids generally adopted as sources of the field equations. It is, thus, somewhat misleading to apply the standard general relativistic energy conditions to this effective energy-momentum tensor, as the latter contains the matter content and a geometrical quantity, which arises from the specific ETG considered. Here we explore this subtlety, extending our previous work, in particular, to cases with the contracted Bianchi identities with diffeomorphism invariance and to cases with generalized explicit curvature-matter couplings, which imply the nonconservation of the energy-momentum tensor. Furthermore, we apply the analysis to specific ETGs, such as scalar-tensor gravity and f(R) gravity. Thus, in the context of ETGs, interesting results appear such as matter that may exhibit unusual thermodynamical features, for instance, gravity that retains its attractive character in the presence of large negative pressures; or alternatively, we verify that repulsive gravity may occur for standard matter.

1 March 2014 in Physics Letters B
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Salvatore CapozzielloSalvatore Capozziello
Salvatore Capozziello
Francisco S. N. LoboFrancisco S. N. Lobo
Francisco S. N. Lobo
José Pedro MimosoJosé Pedro Mimoso
José Pedro Mimoso
We consider generalized energy conditions in modified theories of gravity by taking into account the further degrees of freedom related to scalar fields and curvature invariants. The latter are usually recast as generalized geometrical fluids that have different meanings with respect to the standard matter fluids generally adopted as sources of the field equations. More specifically, in modified gravity the curvature terms are grouped in a tensor Hab and a coupling g(Ψi) that can be reorganized in effective Einstein field equations, as corrections to the energy–momentum tensor of matter. The formal validity of such inequalities does not assure some basic requirements such as the attractive nature of gravity, so that the energy conditions have to be considered in a wider sense

25 August 2015 in The European Physical Journal C
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Tiberiu HarkoTiberiu Harko
Tiberiu Harko
Francisco S. N. LoboFrancisco S. N. Lobo
Francisco S. N. Lobo
José Pedro MimosoJosé Pedro Mimoso
José Pedro Mimoso
Diego PavónDiego Pavón
Diego Pavón