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Иш: Role of three coupling parameters on maximum mass and stability: Theoretical insights into relativistic massive compact objects in mass gap under <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si334.svg" display="inline" id="d1e10703"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> action
Cosmological inflation in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1354" altimg="si9.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:mi>T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity
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Мақола20186 иқтибосABIBeyond the cosmological standard model
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Мақола20146 иқтибосABIBlack holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi mathvariant="double-struck">Q</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math> gravity
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Мақола20205 иқтибосABI