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Center of Mathematics and Applications of University of Beira Interior
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Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
Publication . Morais, João; Bouhmadi Lopez, Mariam; Kumar, K. Sravan; Marto, João; Tavakoli, Yaser
In this paper we consider 3-form dark energy (DE) models with interactions in
the dark sector. We aim to distinguish the phenomenological interactions that
are defined through the dark matter (DM) and the DE energy densities. We do our
analysis mainly in two stages. In the first stage, we identify the
non-interacting 3-form DE model which generically leads to an abrupt late-time
cosmological event which is known as the little sibling of the Big Rip (LSBR).
We classify the interactions which can possibly avoid this late-time abrupt
event. We also study the parameter space of the model that is consistent with
the interaction between DM and DE energy densities at present as indicated by
recent studies based on BAO and SDSS data. In the later stage, we
observationally distinguish those interactions using the statefinder hierarchy parameters {S3(1),S4 (1)},{S3 (1),S5 (1)} . We also compute the growth factor parameter ε(z) for the various interactions we consider herein and use the composite null diagnostic (CND) {S3(1), ε(z)} as a tool to characterise those interactions by measuring their departures from the concordance model. In addition, we make a preliminary analysis of our model in light of the recently released data by SDSS~III on the measurement of the linear growth rate of structure.
Cosmic infinity: a dynamical system approach
Publication . Bouhmadi Lopez, Mariam; Marto, João; Morais, João; Silva, César M.
Dynamical system techniques are extremely useful to study cosmology. It turns
out that in most of the cases, we deal with finite isolated fixed points corresponding to a given
cosmological epoch. However, it is equally important to analyse the asymptotic behaviour
of the universe. On this paper, we show how this can be carried out for 3-forms model.
In fact, we show that there are fixed points at infinity mainly by introducing appropriate
compactifications and defining a new time variable that washes away any potential divergence
of the system. The richness of 3-form models allows us as well to identify normally hyperbolic
non-isolated fixed points. We apply this analysis to three physically interesting situations:
(i) a pre-inflationary era; (ii) an inflationary era; (iii) the late-time dark matter/dark energy
epoch.
Estimation of variance components in models with positive commutativity orthogonal block structure
Publication . Ferreira, Sandra S.; Ferreira, Dário; Nunes, Célia; Mexia, João T.
The article addresses alternative estimators for estimable vectors. The relative performances of the proposed estimators are studied through numerical analysis. The major motivation behind this article is providing an optimal estimator through applying simple modifications in models with Orthogonal Block Structure. In addition, an illustrative example is presented to demonstrate the efficiency and accuracy of the proposed method.
ECIR 2018: Text2Story Workshop-Narrative Extraction from Texts
Publication . Jorge, Alípio Mário Guedes; Campos, Ricardo; Jatowt, Adam; Nunes, Sergio; Rocha, Conceiçeição; Cordeiro, João; Pasquali, Arian; Mangaravite, Vitor
The 1st International Workshop on Narrative Extraction from Texts (Text2Story 2018) was held in conjunction with the 40th European Conference on Information Retrieval, ECIR 2018, Grenoble on the 26th March 2018. The workshop aimed to help foster the collaboration of researchers on a wide range of multidisciplinary issues related to the text-to-narrative- structure. The program consisted of two keynote talks, six research presentations, a poster session and a slot for demo presentations. This report briefly summarizes the workshop.
Non-Gaussianity in multiple three-form field inflation
Publication . Kumar, K. Sravan; Mulryne, David J.; Nunes, Nelson J.; Marto, João; Moniz, Paulo
In this work, we present a method for implementing the δN formalism
to study the primordial non-Gaussianity produced in multiple three-form field
inflation. Using a dual description relating three-form fields to noncanonical
scalar fields, and employing existing results, we produce expressions for the
bispectrum of the curvature perturbation in terms of three-form quantities. We
study the bispectrum generated in a two three-form field inflationary scenario
for a particular potential that for suitable values of the parameters was found
in earlier work to give values of the spectral index and ratio of tensor to
scalar perturbations compatible with current bounds. We calculate the reduced
bispectrum for this model, finding an amplitude in equilateral and orthogonal
configurations of δ(1) and in the squeezed limit of δ(10-3). We confirm, therefore, that this three-form inflationary scenario is compatible with present observational constraints.
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Funding agency
Fundação para a Ciência e a Tecnologia
Funding programme
6817 - DCRRNI ID
Funding Award Number
UID/MAT/00212/2013