Interaction between modified Chaplygin gas and ghost dark energy in the presence of extra dimensions

Abstract

In this paper, we consider three different models of dark energy in higher dimensional space-time and discuss about some cosmological parameters numerically. The first model is a single component universe including viscous varying modified Chaplygin gas. In the second model, we consider two-component universe including viscous varying modified Chaplygin gas and ghost dark energy. In the third model, we consider another two-component universe including viscous modified cosmic Chaplygin gas and ghost dark energy. In the cases of two-component fluids we also consider possibility of interaction between components.

Stability and interacting f(T, T ) gravity with modified Chaplygin gas

“…1 and 2 show us that free parameters of the modified Chaplygin gas (A and B) and the interacting term (b) play a very important role to confirm the accelerated expansion of the universe (the obtained results are consistent with [50,51]). …”

“…In order to describe dark energy model, numerous studies have been performed in isotropic space-time such as scalar fields (quintessence, phantom, tachyon and etc.) [6][7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23], modified gravity models [24][25][26][27][28][29][30][31], holographic models [32][33][34][35][36][37][38][39][40], interacting models [41][42][43][44][45][46][47][48][49][50][51][52], bouncing model [53][54][55...…”

Observational constraints on the extended Chaplygin gas inflation

“…Then, Lu et al (2008) (Lu et al 2011). In order to obtain more suitable evolution of the universe, an interaction is often assumed, so there are several works about interacting modified Chaplygin gas (Chattopadhyay and Debnath 2010; Jamil and Debnath 2011; Khurshudyan et al 2014a). Similar to the generalized Chaplygin gas, it is possible to reconsider constant parameters B in the equation of state as variable (Chakraborty and Debnath 2010;Bhadra and Debnath 2012a, 2012b, 2012cDeng 2011;Ranjit et al 2013aRanjit et al , 2013b.…”

Interacting Quintessence Dark Energy Models in Lyra Manifold

“…It is found that a suitable interaction can help to alleviate the coincidence problem. Different interacting models of dark energy have been investigated [7][8][9][10][11][12][13][14]. Alternative models of dark energy suggest a dynamical form of dark energy, which at least in an effective level, can originate from a variable cosmological constant [15], or from various fields, such is a canonical scalar field [16]- [20] (quintessence), a phantom field [21]- [19], or quintom [29]- [42].…”