Lina Zhang, Qiyuan Pan, Yun Soo Myung, De-Cheng Zou
{"title":"巴丁黑洞的自发标量化","authors":"Lina Zhang, Qiyuan Pan, Yun Soo Myung, De-Cheng Zou","doi":"arxiv-2409.11669","DOIUrl":null,"url":null,"abstract":"We study the spontaneous scalarization of Bardeen black holes, whose\ntachyonic instability triggers the formation of scalarized charged black holes\n(SCBHs). In this case, we find infinite ($n=0,1,2,\\cdots$) branches of SCBHs\nwith magnetic charge $g$. The $n = 0$ branch of SCBHs can be found for the\ncoupling parameter $\\alpha \\geq \\alpha_{n=0}(g)$ with both quadratic (1-$\\alpha\n\\varphi^2$) and exponential ($e^{-\\alpha \\varphi^2}$) couplings, where\n$\\alpha_{n=0}(g)$ represents the threshold of tachyonic instability for the\nBardeen black holes. Furthermore, it is shown that the $n = 0$ branch for both\ncouplings is stable against radial perturbations. This stability shows that\nthis branch can be used for further observational implications.","PeriodicalId":501041,"journal":{"name":"arXiv - PHYS - General Relativity and Quantum Cosmology","volume":"263 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Spontaneous scalarization of Bardeen black holes\",\"authors\":\"Lina Zhang, Qiyuan Pan, Yun Soo Myung, De-Cheng Zou\",\"doi\":\"arxiv-2409.11669\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We study the spontaneous scalarization of Bardeen black holes, whose\\ntachyonic instability triggers the formation of scalarized charged black holes\\n(SCBHs). In this case, we find infinite ($n=0,1,2,\\\\cdots$) branches of SCBHs\\nwith magnetic charge $g$. The $n = 0$ branch of SCBHs can be found for the\\ncoupling parameter $\\\\alpha \\\\geq \\\\alpha_{n=0}(g)$ with both quadratic (1-$\\\\alpha\\n\\\\varphi^2$) and exponential ($e^{-\\\\alpha \\\\varphi^2}$) couplings, where\\n$\\\\alpha_{n=0}(g)$ represents the threshold of tachyonic instability for the\\nBardeen black holes. Furthermore, it is shown that the $n = 0$ branch for both\\ncouplings is stable against radial perturbations. This stability shows that\\nthis branch can be used for further observational implications.\",\"PeriodicalId\":501041,\"journal\":{\"name\":\"arXiv - PHYS - General Relativity and Quantum Cosmology\",\"volume\":\"263 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-18\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - General Relativity and Quantum Cosmology\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.11669\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - General Relativity and Quantum Cosmology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11669","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We study the spontaneous scalarization of Bardeen black holes, whose
tachyonic instability triggers the formation of scalarized charged black holes
(SCBHs). In this case, we find infinite ($n=0,1,2,\cdots$) branches of SCBHs
with magnetic charge $g$. The $n = 0$ branch of SCBHs can be found for the
coupling parameter $\alpha \geq \alpha_{n=0}(g)$ with both quadratic (1-$\alpha
\varphi^2$) and exponential ($e^{-\alpha \varphi^2}$) couplings, where
$\alpha_{n=0}(g)$ represents the threshold of tachyonic instability for the
Bardeen black holes. Furthermore, it is shown that the $n = 0$ branch for both
couplings is stable against radial perturbations. This stability shows that
this branch can be used for further observational implications.