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Ish: Modeling Compact Object Mergers GW190814 and GW200210 and Other Self-bound Compact Stars with Dark Matter Induced by Gravitational Decoupling and Its Significance to the Mass Gap

1. 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

   S. K. Maurya, Abdelghani Errehymy, Y. Saginayev +4

   MaqolaCosmology and Gravitation TheoriesPhysics of the Dark Universe20251 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000793

2. Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics

   S. Khan, Javlon Rayimbaev, Inomjon Ibragimov +3

   MaqolaPulsars and Gravitational Waves ResearchPhysica Scripta20250 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000653

3. Mass-Gap Strange Quark Stars in Vegh-Type Massive Gravity with Gravitationally Decoupled Dark Matter

   Shahid Hussain Gurmani, Saadia Mumtaz, G. D. AÇAN Yildiz +3

   PreprintCosmology and Gravitation TheoriesSSRN Electronic Journal20260 iqtibos

   ABIABI:AkademIndex/openalex/2026.preprint.001387