官僚统治 发表于 2025-3-28 14:34:46
http://reply.papertrans.cn/25/2423/242222/242222_41.png不真 发表于 2025-3-28 22:01:49
http://reply.papertrans.cn/25/2423/242222/242222_42.pngNOT 发表于 2025-3-29 02:42:31
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http://reply.papertrans.cn/25/2423/242222/242222_44.png里程碑 发表于 2025-3-29 08:57:35
https://doi.org/10.1385/1597451304asinormal frequencies. We apply these results to the calculation of quasinormal frequencies associated with gravitational perturbations of d-dimensional spherically symmetric black holes with string corrections. We do this for two distinct limits: the eikonal limit and the asymptotic limit.Diuretic 发表于 2025-3-29 13:00:18
http://reply.papertrans.cn/25/2423/242222/242222_46.pngNADIR 发表于 2025-3-29 16:09:21
978-3-031-55100-0The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl长处 发表于 2025-3-29 23:12:22
http://reply.papertrans.cn/25/2423/242222/242222_48.pngindubitable 发表于 2025-3-30 03:52:13
https://doi.org/10.1007/978-981-19-0928-3e irregular. Therefore, in order to derive novel and physically interesting solutions that describe compact objects one needs to address generalised gravitational theories. One popular class of such theories is the Einstein-scalar-Gauss-Bonnet (EsGB) theory with a general coupling function between tGRE 发表于 2025-3-30 07:01:09
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