scholarly journals Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity

2021 ◽  
Vol 104 (6) ◽  
Author(s):  
Daris Samart ◽  
Bhuddhanubhap Silasan ◽  
Phongpichit Channuie
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Interacting Dark Energy

scholarly journals Interacting dark energy and dark matter: Observational constraints from cosmological parameters

2007 ◽  
Vol 778 (1-2) ◽  
pp. 69-84 ◽  
Author(s):  
Bin Wang ◽  
Jiadong Zang ◽  
Chi-Yong Lin ◽  
Elcio Abdalla ◽  
S. Micheletti
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Cosmological Parameters ◽  
Observational Constraints ◽  
Interacting Dark Energy

scholarly journals Large-scale instability in interacting dark energy and dark matter fluids

2008 ◽  
Vol 2008 (07) ◽  
pp. 020 ◽  
Author(s):  
Jussi Väliviita ◽  
Elisabetta Majerotto ◽  
Roy Maartens
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Large Scale ◽  
Interacting Dark Energy

scholarly journals Bianchi Type-I Dark Energy Cosmology with Power-Law Relation in Brans-Dicke Theory of Gravitation

2018 ◽  
Vol 2018 ◽  
pp. 1-11 ◽  
Author(s):  
S. D. Katore ◽  
D. V. Kapse
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Power Law ◽  
Bianchi Type ◽  
Type I ◽  
Field Equations ◽  
Coincidence Problem ◽  
Bianchi Type I ◽  
Interacting Dark Energy ◽  
Theory Of Gravitation

We have studied the interacting and non-interacting dark energy and dark matter in the spatially homogenous and anisotropic Bianchi type-I model in the Brans-Dicke theory of gravitation. The field equations have been solved (i) by using power-law relation and (ii) by assuming scale factor in terms of redshift. Here we have considered two cases of an interacting and non-interacting dark energy scenario and obtained general results. It has been found that for suitable choice of interaction between dark energy and dark matter we can avoid the coincidence problem which appears in the ΛCDM model. Some physical aspects and stability of the models are discussed in detail. The statefinder diagnostic pair, i.e., {r,s}, is adopted to differentiate our dark energy models.

scholarly journals Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids

2021 ◽  
Vol 2021 (03) ◽  
pp. 085
Author(s):  
Jose Beltrán Jiménez ◽  
Dario Bettoni ◽  
David Figueruelo ◽  
Florencia A. Teppa Pannia ◽  
Shinji Tsujikawa
Keyword(s):  
Dark Matter ◽  
Dark Energy ◽  
Lagrangian Description ◽  
Interacting Dark Energy ◽  
Perfect Fluids
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