{"title":"History of a Particle Bounded to the Cosmological LTB Black Hole Surrounded by the Quintom Field","authors":"Sareh Eslamzadeh, Saheb Soroushfar","doi":"arxiv-2409.11318","DOIUrl":null,"url":null,"abstract":"This paper provides a complete set of analytic time-varying geodesic\nequations of the LTB black hole surrounded by the Quintom field. Indeed, we\nprobe the evolution of the effective potential of such a black hole and\npossible photon orbits on cosmic epochs. We deduce that passing time in the\naccelerated universe from the early to late time epochs causes the peak of\neffective potential to decrease and shift to small radii, while the possibility\nof forming a stable orbit increases. Besides, four situations including:\nterminating bound orbit, stable orbit, scattering flyby orbit, and terminating\nescape orbit have been illustrated in some cosmic time slices. Moreover,\nchanging orbits with time from the early universe to the late time epochs have\nbeen investigated. Furthermore, the stability of orbits and ISCO have been\nanalyzed.","PeriodicalId":501067,"journal":{"name":"arXiv - PHYS - High Energy Physics - Phenomenology","volume":"188 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Physics - Phenomenology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.11318","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
This paper provides a complete set of analytic time-varying geodesic
equations of the LTB black hole surrounded by the Quintom field. Indeed, we
probe the evolution of the effective potential of such a black hole and
possible photon orbits on cosmic epochs. We deduce that passing time in the
accelerated universe from the early to late time epochs causes the peak of
effective potential to decrease and shift to small radii, while the possibility
of forming a stable orbit increases. Besides, four situations including:
terminating bound orbit, stable orbit, scattering flyby orbit, and terminating
escape orbit have been illustrated in some cosmic time slices. Moreover,
changing orbits with time from the early universe to the late time epochs have
been investigated. Furthermore, the stability of orbits and ISCO have been
analyzed.