Cosmological reconstruction and $$\Lambda $$CDM universe in $$f(Q,\,C)$$ gravity
Gaurav N. Gadbail, Avik De, P. K. Sahoo
Abstract
Abstract Symmetric Teleparallel Gravity allows for the reformulation of gravity in the form of nonmetricity by vanishing the contorsion term in the generic affine connection. Our focus is on investigating a recently proposed extension of this theory in which the Lagrangian has the form f ( Q , C ) by incorporating the boundary term C . In this work, we first use a reconstruction approach in f ( Q , C ) gravity that might admit the $$\Lambda $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>Λ</mml:mi> </mml:math> CDM expansion history. Furthermore, we perform a novel approach for cosmological reconstruction of f ( Q , C ) gravity in terms of e-folding, and it shows how any FLRW cosmology can arise from a specific f ( Q , C ) gravity. A variety of instances are provided using this approach in which f ( Q , C ) gravity is reconstructed to yield the well-known cosmic evolution: $$\Lambda $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>Λ</mml:mi> </mml:math> CDM era, acceleration/deceleration era which is equivalent to the presence of phantom and non-phantom matter, late-time acceleration with the crossing of phantom-divide line and transient phantom era.