Reconstruction of the Cosmic Equation of State for High Redshift

We investigate the possibilities of reconstructing the cosmic equation of state (EoS) for high redshift. In order to obtain general results, we use two model-independent approaches. The first reconstructs the EoS using comoving distance and the second makes use of the Hubble parameter data. To implement the first method, we use a recent set of Gamma-Ray Bursts (GRBs) measures. To implement the second method, we generate simulated data using the Sandage-Loeb ($SL$) effect; for the fiducial model, we use the $\Lambda CDM$ model. In both cases, the statistical analysis is conducted through the Gaussian processes (non-parametric). In general, we demonstrate that this methodology for reconstructing the EoS using a non-parametric method plus a model-independent approach works appropriately due to the feasibility of calculation and the ease of introducing a priori information ($H_ {0}$ and $\Omega_{m0}$). In the near future, following this methodology with a higher number of high quality data will help obtain strong restrictions for the EoS.Comment: 9 pages, 5 figure

Interacting photon-baryon fluid, warm dark matter and the first acoustic peak

The Reduced Relativistic Gas (RRG) model was introduced by A. Sakharov in 1965 for deriving the cosmic microwave background (CMB) spectrum. It was recently reinvented by some of us to achieve an interpolation between the radiation and dust epochs in the evolution of the Universe. This model circumvents the complicated structure of the Boltzmann-Einstein system of equations and admits a transparent description of warm-dark-matter effects. It is extended here to include, on a phenomenological basis, an out-of-equilibrium interaction between radiation and baryons which is supposed to account for relevant aspects of pre-recombination physics in a simplified manner. Furthermore, we use the tight-coupling approximation to explore the influence of both this interaction and of the RRG warmness parameter on the anisotropy spectrum of the CMB. The predictions of the model are very similar to those of the {\Lambda}CDM model if both the interaction and the dark-matter warmness parameters are of the order of $10^{-4}$ or smaller. As far as the warmness parameter is concerned, this is in good agreement with previous estimations on the basis of results from structure formation.Comment: 10 pages and 4 figure

Black hole shadow of a rotating polytropic black hole by the Newman--Janis algorithm without complexification

In this work, starting from a spherically symmetric polytropic black hole, a rotating solution is obtained by following the Newman--Janis algorithm without complexification. Besides studying the horizon, the static conditions and causality issues of the rotating solution, we obtain and discuss the shape of its shadow. Some other physical features as the Hawking temperature and emission rate of the rotating polytropic black hole solution are also discussed.Comment: 9 pages, 2 figures, some references adde

Facilitating Social Media and Offline Political Engagement During Electoral Cycles: Using Social Cognitive Theory to Explain Political Action Among Hispanics and Latinos

This is an Accepted Manuscript of an article published by Taylor & Francis in Mass Communication and Society on July 9th, 2018, available online: http://www.tandfonline.com/10.1080/15205436.2018.1484489.Two interacting forces are subtly shifting the nature of American democracy—the public’s increased use of social media for political information and meaningful changes in the demographic characteristics of the country. This study specifically examined ways in which social media use for political purposes could leverage greater offline political participation among Hispanics and Latinos—a rapidly growing segment of the population. Using social cognitive theory, this study evaluated features of users’ social media network and social media behaviors that can facilitate greater political participation both online and offline. Results indicate that individuals’ social media network expression and social media political expression experiences influence users’ social media political efficacy, social media political expression, and eventually their offline political engagement. Special attention is given to the role of social media political efficacy in promoting broad forms of social media political expression and offline engagement for Hispanics and Latinos