| Full text | |
| Author(s): |
Jesus, J. F.
;
Valentim, R.
;
Escobal, A. A.
;
Pereira, S. H.
;
Benndorf, D.
Total Authors: 5
|
| Document type: | Journal article |
| Source: | Journal of Cosmology and Astroparticle Physics; v. N/A, n. 11, p. 14-pg., 2022-11-01. |
| Abstract | |
Scalar Fields (SF) have emerged as natural candidates for dark energy as quintessential or phantom fields, as they are the main ingredient of inflation theories. Instead of assuming some form for the scalar field potential, however, this work reconstructs the SF potential directly from observational data, namely, Hubble and SNe Ia data. We show that two popular forms for the SF potentials, namely, the power-law and the quadratic free-field, are compatible with the reconstructions thus obtained, at least for some choices of the priors of the matter density and curvature parameters and for some redshift intervals. (AU) | |
| FAPESP's process: | 16/09831-0 - Neutron Stars populations: bayesian statistics tools |
| Grantee: | Rodolfo Valentim da Costa Lima |
| Support Opportunities: | Regular Research Grants |
| FAPESP's process: | 21/01089-1 - Cherenkov Telescope Array: construction and first discoveries |
| Grantee: | Luiz Vitor de Souza Filho |
| Support Opportunities: | Special Projects |