Luca Amendola

Luca Amendola


Research Focus & Metrics

Academic Career Length

38Years (1989-Present)

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

Representative Publications

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24 July 2000 in Physical Review D
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LALuca Amendola
Luca Amendola
A new component of the cosmic medium, a light scalar field or “quintessence,” has been proposed recently to explain cosmic acceleration with a dynamical cosmological constant. Such a field is expected to be coupled explicitly to ordinary matter, unless some unknown symmetry prevents it. I investigate the cosmological consequences of a coupled quintessence (CQ) model, assuming an exponential potential and a linear coupling. This model is conformally equivalent to Brans-Dicke Lagrangians with any power-law potential. I evaluate the density perturbations on the cosmic microwave background and on the galaxy distribution at the present and derive bounds on the coupling constant from the comparison with observational data. A novel feature of CQ is that during the matter dominated era the scalar field has a finite and almost constant energy density. This epoch, denoted as φMDE, is a saddle point in the dynamical phase space. The φMDE is responsible of several differences with respect to uncoupled quintessence: the multipole spectrum of the microwave background is tilted at large angles, the acoustic peaks are shifted, their amplitude is changed, and the present 8 Mpc/h density variance is diminished. The present data constrain the dimensionless coupling constant to |β|<~0.1 assuming Ωm=0.3 and a primordial fluctuation slope ns=1.

12 April 2018 in Living Reviews in Relativity
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TGThe Euclid Theory Working Group
The Euclid Theory Working Group
LALuca Amendola
Luca Amendola
SAStephen Appleby
Stephen Appleby
AAAnastasios Avgoustidis
Anastasios Avgoustidis
DBDavid Bacon
David Bacon
TZTom Zlosnik
Tom Zlosnik
Euclid is a European Space Agency medium-class mission selected for launch in 2020 within the cosmic vision 2015–2025 program. The main goal of Euclid is to understand the origin of the accelerated expansion of the universe. Euclid will explore the expansion history of the universe and the evolution of cosmic structures by measuring shapes and red-shifts of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky. Although the main driver for Euclid is the nature of dark energy, Euclid science covers a vast range of topics, from cosmology to galaxy evolution to planetary research. In this review we focus on cosmology and fundamental physics, with a strong emphasis on science beyond the current standard models. We discuss five broad topics: dark energy and modified gravity, dark matter, initial conditions, basic assumptions and questions of methodology in the data analysis. This review has been planned and carried out within Euclid’s Theory Working Group and is meant to provide a guide to the scientific themes that will underlie the activity of the group during the preparation of the Euclid mission.

2 September 2013 in Living Reviews in Relativity
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LALuca Amendola
Luca Amendola
SAStephen Appleby
Stephen Appleby
DBDavid Bacon
David Bacon
TBTessa Baker
Tessa Baker
MBMarco Baldi
Marco Baldi
TZTom Zlosnik
Tom Zlosnik
Euclid is a European Space Agency medium-class mission selected for launch in 2019 within the Cosmic Vision 2015–2025 program. The main goal of Euclid is to understand the origin of the accelerated...

6 April 2007 in Physical Review D
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LALuca Amendola
Luca Amendola
RGRadouane Gannouji
Radouane Gannouji
DPDavid Polarski
David Polarski
STShinji Tsujikawa
Shinji Tsujikawa
We derive the conditions under which dark energy models whose Lagrangian densities f are written in terms of the Ricci scalar R are cosmologically viable. We show that the cosmological behavior of f(R) models can be understood by a geometrical approach consisting of studying the m(r) curve on the (r,m) plane, where m≡Rf,RR/f,R and r≡−Rf,R/f with f,R≡df/dR. This allows us to classify the f(R) models into four general classes, depending on the existence of a standard matter epoch and on the final accelerated stage. The existence of a viable matter-dominated epoch prior to a late-time acceleration requires that the variable m satisfies the conditions m(r)≈+0 and dm/dr>−1 at r≈−1. For the existence of a viable late-time acceleration we require instead either (i) m=−r−1, (3−1)/2<m≤1 and dm/dr<−1 or (ii) 0<m≤1 at r=−2. These conditions identify two regions in the (r,m) space, one for the matter era and the other for the acceleration. Only models with an m(r) curve that connects these regions and satisfies the requirements above lead to an acceptable cosmology. The models of type f(R)=αR−n and f=R+αR−n do not satisfy these conditions for any n>0 and n<−1 and are thus cosmologically unacceptable. Similar conclusions can be reached for many other examples discussed in the text. In most cases the standard matter era is replaced by a cosmic expansion with scale factor a∝t1/2. We also find that f(R) models can have a strongly phantom attractor but in this case there is no acceptable matter era.

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.

10 June 2010
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LALuca Amendola
Luca Amendola
STShinji Tsujikawa
Shinji Tsujikawa
Dark energy, the mysterious cause of the accelerating expansion of the universe, is one of the most important fields of research in astrophysics and cosmology today. Introducing the theoretical ideas, observational methods and results, this textbook is ideally suited to graduate courses on dark energy, and will also supplement advanced cosmology courses. Providing a thorough introduction to this exciting field, the textbook covers the cosmological constant, quintessence, k-essence, perfect fluid models, extra-dimensional models, and modified gravity. Observational research is reviewed, from the cosmic microwave background to baryon acoustic oscillations, weak lensing and cluster abundances. Every chapter ends with problems, with full solutions provided, and any calculations are worked through step-by-step.