Is the cosmological dark sector better modeled by a generalized Chaplygin gas or by a scalar field?
Crossref DOI link: https://doi.org/10.1140/epjc/s10052-017-5051-y
Published Online: 2017-07-18
Published Print: 2017-07
Update policy: https://doi.org/10.1007/springer_crossmark_policy
del Campo, Sergio
Fabris, Júlio C.
Herrera, Ramón
Zimdahl, Winfried
Funding for this research was provided by:
CNPq (Brazil) and FAPES (Brazil)
Comisión Nacional de Ciencias y Tecnología
License valid from 2017-07-01