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Ish: Wormholes versus black holes: quasinormal ringing at early and late times

1. Dehnen-type dark matter wormholes in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg" display="inline" id="d1e414"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi mathvariant="script">L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> action

   Abdelghani Errehymy, Orhan Dönmez, Bobur Turimov +3

   MaqolaCosmology and Gravitation TheoriesAnnals of Physics20254 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000267

2. Global monopole induced wormholes in power-law gravity: stability and physical viability

   M. Yousaf, H. Asad, Kashif Ammar Yasir +3

   MaqolaCosmology and Gravitation TheoriesThe European Physical Journal C20253 iqtibos

   ABIABI:AkademIndex/openalex/2025.article.000369