Constraining anisotropic cosmological model in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e682" altimg="si6.svg"> <mml:mrow> <mml:mi mathvariant="script" class="mathpzc">f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>ℒ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> Gravity
N.S. KavyaDepartment of P.G. Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shivamogga 577451, Karnataka, IndiaV. VenkateshaDepartment of P.G. Studies and Research in Mathematics, Kuvempu University, Shankaraghatta, Shivamogga 577451, Karnataka, IndiaSanjay MandalDepartment of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, IndiaP. K. SahooDepartment of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, India
2022lv
ABI
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