Physical properties of class I compact star model for linear and Starobinsky <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1207" altimg="si25.svg"> <mml:mrow> <mml:mo>−</mml:mo> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> functions
Ksh. Newton SinghDepartment of Mathematics, Jadavpur University, Kolkata 700032, IndiaS. K. MauryaDepartment of Mathematical and Physical Sciences, College of Arts and Sciences, University of Nizwa, Nizwa, Sultanate of OmanAbdelghani ErrehymyLaboratory of High Energy Physics and Condensed Matter (LPHEMaC), Department of Physics, Faculty of Sciences Aïn Chock, University of Hassan II, B.P. 5366 Mâarif, Casablanca 20100, MoroccoFarook RahamanDepartment of Mathematics, Jadavpur University, Kolkata 700032, IndiaM. DaoudDepartment of Physics, Faculty of Sciences, University of Ibn Tofail, B.P. 133, Kenitra 14000, Morocco
2020lv
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