We investigate regular rotating black holes predicted by asymptotically safe gravity, where the Newton constant varies with energy scale and modifies the near horizon geometry. These solutions remain asymptotically flat and avoid central singularities while differing from the classical Kerr spacetime in the strong field region. We compute the radiative efficiency of thin accretion disks and the jet power from the Blandford Znajek mechanism, both of which depend on the deformation parameter of the model. The predictions are compared with observational estimates for six stellar mass black holes. For systems with low or moderate spin the model reproduces the data within reported uncertainties, while rapidly spinning sources such as GRS 1915 105 present tensions and point to a restricted deformation range or the need for additional physics. The results show that quantum corrections confined to the strong gravity regime can still leave detectable imprints on high energy astrophysical processes. Radiative and jet based diagnostics therefore provide a promising method to test the geometry near the horizon and to explore possible signatures of quantum gravity in observations.
Swampland Conjectures through ACT Observations: Observational Signatures of Radiative-Corrected Inflation
University of Mazandaran（马赞德兰大学）；Damghan University（达姆甘大学）；Canadian Quantum Research Center（加拿大量子研究中心）；Khazar University（哈扎尔大学）；Chitkara University Institute of Engineering and Technology, Chitkara University（奇特卡拉大学工程技术学院，奇特卡拉大学）；Eastern Mediterranean University（东地中海大学）
Greybody Factors, Absorption Cross Sections and Hawking Radiation of Holonomy-Corrected Schwarzschild Black Holes
University of Hradec Králové（赫拉德茨克拉洛韦大学）；Kimyo International University in Tashkent（塔什干金学院国际大学）；New Uzbekistan University（新乌兹别克斯坦大学）；National University of Uzbekistan（乌兹别克斯坦国立大学）；Ulugh Beg Astronomical Institute（乌鲁伯格天文研究所）；University of Tashkent for Applied Sciences（塔什干应用科学大学）；Tashkent State Technical University（塔什干国立技术大学）
Bardeen spacetime as quantum corrected black hole: Grey-body factors and quasinormal modes of gravitational perturbations
University of Hradec Králové（赫拉德茨克拉洛韦大学）；Tashkent International University of Education（塔什干国际教育学院）；University of Tashkent for Applied Sciences（塔什干应用科学大学）；National University of Uzbekistan（乌兹别克斯坦国立大学）；New Uzbekistan University（新乌兹别克斯坦大学）；Tashkent State Technical University（塔什干国立技术大学）；Kimyo International University in Tashkent（塔什干化学国际大学）；Mamun University（马蒙大学）
Dymnikova-Schwinger quantum-corrected slowly rotating wormholes: Photon and spinning particle dynamics
University of KwaZulu-Natal（夸祖鲁-纳塔尔大学）；Khazar University（哈扎尔大学）；University Hassan II（哈桑二世大学）；Ibn Tofail University（伊本·图费勒大学）；Abdus Salam International Centre for Theoretical Physics（阿卜杜斯·萨拉姆理论物理国际中心）；Ulugh Beg Astronomical Institute（乌鲁伯格天文研究所）；Central Asian University（中亚大学）；Imam Mohammad Ibn Saud Islamic University (IMSIU)（伊玛目穆罕默德·伊本·沙特伊斯兰大学）；Kimyo International University in Tashkent（塔什干基莫国际大学）
