Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Feola, Pasquale"'
In the framework of scalar-tensor gravity, we consider non-flat interacting quintessence cosmology where a scalar field is interacting with dark matter. Such a scalar field can be a standard or a phantom one. We use the Noether Symmetry Approach to o
Externí odkaz:
http://arxiv.org/abs/2307.02355
Autor:
Feola, Pasquale, Forteza, Xisco Jimenez, Capozziello, Salvatore, Cianci, Roberto, Vignolo, Stefano
Publikováno v:
Phys. Rev. D 101, 044037 (2020)
Within the framework of $f(R)=R+\alpha R^2$ gravity, we study realistic models of neutron stars, using equations of state compatible with the LIGO constraints. i.e. APR4, MPA1, SLy, and WW1. By numerically solving modified Tolman-Oppenheimer-Volkoff
Externí odkaz:
http://arxiv.org/abs/1909.08847
Autor:
FEOLA, PASQUALE
The aim of this thesis is to study the possible astrophysical and cosmological applications of Extended Theories of Gravity. In particular, Neutron Stars are studied, both on astrophysical and cosmological scale where, at cosmological level, they can
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11134b75fccdd5e3aeb5a96c672d9933
http://hdl.handle.net/11567/1006198
http://hdl.handle.net/11567/1006198
Autor:
Feola, Pasquale, Forteza, Xisco Jimenez, Capozziello, Salvatore, Cianci, Roberto, Vignolo, Stefano
Within the framework of $f(R)=R+��R^2$ gravity, we study realistic models of neutron stars, using equations of state compatible with the LIGO constraints. i.e. APR4, MPA1, SLy, and WW1. By numerically solving modified Tolman-Oppenheimer-Volkoff e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dedcafca386d88dc2b075ef052a81c54