Maqola

Cosmological test of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si211.svg" display="inline" id="d1e1497"> <mml:mfrac> <mml:mrow> <mml:mi>σ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>θ</mml:mi> </mml:mrow> </mml:mfrac> </mml:math> as function of scale factor in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si3.svg" display="inline" id="d1e1507"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> framework

Himanshu ChaudharyDepartment of Applied Mathematics, Delhi Technological University, Delhi 110042, IndiaAditya KaushikDepartment of Applied Mathematics, Delhi Technological University, Delhi 110042, IndiaAnkita KohliDepartment of Applied Mathematics, Delhi Technological University, Delhi 110042, India

2023lv

Ochiq kirish: yoʻq

ABI

Annotatsiya

Annotatsiya mavjud emas.

Identifikatorlar

DOI: 10.1016/j.newast.2023.102044

Iqtiboslar va manbalar

10 ta iqtibos0 ta foydalanilgan manba