Muhammad Danish Sultan , Shahid Chaudhary , Talha Anwar , Asifa Ashraf , Ali M. Mubaraki , Farruh Atamurotov , Awatef Abidi
{"title":"热相变,蒸发,和黑洞的阴影在扩展重力与弦物质","authors":"Muhammad Danish Sultan , Shahid Chaudhary , Talha Anwar , Asifa Ashraf , Ali M. Mubaraki , Farruh Atamurotov , Awatef Abidi","doi":"10.1016/j.dark.2025.102077","DOIUrl":null,"url":null,"abstract":"<div><div>The thermodynamics and quantum nature of black holes remain central to advancing our understanding of gravity, quantum mechanics, and high-energy physics. Motivated by the inadequacy of classical electrodynamics in extreme gravitational regimes and inspired by string theory’s prediction of extended matter structures, this work explores the rich interplay between nonlinear electrodynamics (NLED) and a surrounding cloud of strings on black hole physics. We present a novel class of regular AdS black holes within the framework of Einstein gravity, modified by both magnetic NLED sources and a cloud of strings, and perform an extensive investigation into their thermodynamic behavior, evaporation dynamics, and observational characteristics. A key motivation is to uncover whether exotic fields and high-energy corrections can alter classical predictions and stabilize black holes against evaporation. Our analysis reveals several striking results: (i) the deviation parameter <span><math><mi>k</mi></math></span>, magnetic charge <span><math><mi>g</mi></math></span>, and string cloud parameter <span><math><mi>a</mi></math></span> act as regulators of black hole thermodynamics, significantly suppressing Hawking radiation and extending black hole lifetimes; (ii) Joule–Thomson expansion shows that increasing <span><math><mi>k</mi></math></span> and <span><math><mi>a</mi></math></span> enhances thermal stability by eliminating heating phases and broadening cooling regions; (iii) quantum gravity corrections to entropy induce richer and more complex phase transitions than those in classical models, with the HPEM thermodynamic geometry consistently identifying critical points; (iv) scalar perturbation and greybody factor analyses indicate stronger damping and reduced radiation escape under higher <span><math><mi>k</mi></math></span>, <span><math><mi>a</mi></math></span>, or <span><math><mi>g</mi></math></span>, suggesting suppressed quasinormal modes and observable deviations in gravitational wave signatures; and (v) the black hole shadow radius shrinks under the influence of all three parameters, opening new possibilities for observational constraints via horizon-scale imaging.</div></div>","PeriodicalId":48774,"journal":{"name":"Physics of the Dark Universe","volume":"50 ","pages":"Article 102077"},"PeriodicalIF":6.4000,"publicationDate":"2025-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Thermal phase transitions, evaporation, and shadows of regular black holes in extended gravity with stringy matter\",\"authors\":\"Muhammad Danish Sultan , Shahid Chaudhary , Talha Anwar , Asifa Ashraf , Ali M. Mubaraki , Farruh Atamurotov , Awatef Abidi\",\"doi\":\"10.1016/j.dark.2025.102077\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The thermodynamics and quantum nature of black holes remain central to advancing our understanding of gravity, quantum mechanics, and high-energy physics. Motivated by the inadequacy of classical electrodynamics in extreme gravitational regimes and inspired by string theory’s prediction of extended matter structures, this work explores the rich interplay between nonlinear electrodynamics (NLED) and a surrounding cloud of strings on black hole physics. We present a novel class of regular AdS black holes within the framework of Einstein gravity, modified by both magnetic NLED sources and a cloud of strings, and perform an extensive investigation into their thermodynamic behavior, evaporation dynamics, and observational characteristics. A key motivation is to uncover whether exotic fields and high-energy corrections can alter classical predictions and stabilize black holes against evaporation. Our analysis reveals several striking results: (i) the deviation parameter <span><math><mi>k</mi></math></span>, magnetic charge <span><math><mi>g</mi></math></span>, and string cloud parameter <span><math><mi>a</mi></math></span> act as regulators of black hole thermodynamics, significantly suppressing Hawking radiation and extending black hole lifetimes; (ii) Joule–Thomson expansion shows that increasing <span><math><mi>k</mi></math></span> and <span><math><mi>a</mi></math></span> enhances thermal stability by eliminating heating phases and broadening cooling regions; (iii) quantum gravity corrections to entropy induce richer and more complex phase transitions than those in classical models, with the HPEM thermodynamic geometry consistently identifying critical points; (iv) scalar perturbation and greybody factor analyses indicate stronger damping and reduced radiation escape under higher <span><math><mi>k</mi></math></span>, <span><math><mi>a</mi></math></span>, or <span><math><mi>g</mi></math></span>, suggesting suppressed quasinormal modes and observable deviations in gravitational wave signatures; and (v) the black hole shadow radius shrinks under the influence of all three parameters, opening new possibilities for observational constraints via horizon-scale imaging.</div></div>\",\"PeriodicalId\":48774,\"journal\":{\"name\":\"Physics of the Dark Universe\",\"volume\":\"50 \",\"pages\":\"Article 102077\"},\"PeriodicalIF\":6.4000,\"publicationDate\":\"2025-09-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physics of the Dark Universe\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S2212686425002705\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of the Dark Universe","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2212686425002705","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Thermal phase transitions, evaporation, and shadows of regular black holes in extended gravity with stringy matter
The thermodynamics and quantum nature of black holes remain central to advancing our understanding of gravity, quantum mechanics, and high-energy physics. Motivated by the inadequacy of classical electrodynamics in extreme gravitational regimes and inspired by string theory’s prediction of extended matter structures, this work explores the rich interplay between nonlinear electrodynamics (NLED) and a surrounding cloud of strings on black hole physics. We present a novel class of regular AdS black holes within the framework of Einstein gravity, modified by both magnetic NLED sources and a cloud of strings, and perform an extensive investigation into their thermodynamic behavior, evaporation dynamics, and observational characteristics. A key motivation is to uncover whether exotic fields and high-energy corrections can alter classical predictions and stabilize black holes against evaporation. Our analysis reveals several striking results: (i) the deviation parameter , magnetic charge , and string cloud parameter act as regulators of black hole thermodynamics, significantly suppressing Hawking radiation and extending black hole lifetimes; (ii) Joule–Thomson expansion shows that increasing and enhances thermal stability by eliminating heating phases and broadening cooling regions; (iii) quantum gravity corrections to entropy induce richer and more complex phase transitions than those in classical models, with the HPEM thermodynamic geometry consistently identifying critical points; (iv) scalar perturbation and greybody factor analyses indicate stronger damping and reduced radiation escape under higher , , or , suggesting suppressed quasinormal modes and observable deviations in gravitational wave signatures; and (v) the black hole shadow radius shrinks under the influence of all three parameters, opening new possibilities for observational constraints via horizon-scale imaging.
期刊介绍:
Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact.
The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.