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Ish: Kerr–Newman black holes in Weyl–Cartan theory: Shadows and EHT constraints

1. Shadows and optical appearances of black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si157.svg" display="inline" id="d1e2760"><mml:msup><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math> gravity

   Khadije Jafarzade, Sanjar Shaymatov, Mubasher Jamil

   MaqolaCosmology and Gravitation TheoriesAstroparticle Physics20252 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000587

2. Influence of quantum correction on Kerr black hole in effective loop quantum gravity via shadows and EHT results

   Muhammad Ali Raza, M. Zubair, Farruh Atamurotov +1

   MaqolaNoncommutative and Quantum Gravity TheoriesThe European Physical Journal C20252 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000834