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Иш: Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics
Equations of state for supernovae and compact stars
Micaela Oertel, Matthias Hempel, T. Klähn +1
Мақола20173 иқтибосABIProperties of the Binary Neutron Star Merger GW170817
B. P. Abbott, R. Abbott, T. D. Abbott +96
Мақола20193 иқтибосABIRole of complexity on the minimal deformation of black holes
Z. Yousaf, Kazuharu Bamba, Bander Almutairi +2
Мақола20243 иқтибосABIGravastars in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e273" altimg="si5.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>R</mml:mi> <mml:mo>,</mml:mo> <mml:mi>G</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity
M.Z. Bhatti, Z. Yousaf, A. Rehman
Мақола20202 иқтибосABIExact EGB models for spherical static perfect fluids
Sudan Hansraj, Brian Chilambwe, Sunil D. Maharaj
Мақола20152 иқтибосABI