Observing black hole phase transitions in extended phase space and holographic thermodynamics approaches from optical features

บทความในวารสาร


ผู้เขียน/บรรณาธิการ


กลุ่มสาขาการวิจัยเชิงกลยุทธ์


รายละเอียดสำหรับงานพิมพ์

รายชื่อผู้แต่งPromsiri C.; Horinouchi W.; Hirunsirisawat E.

ผู้เผยแพร่SpringerOpen

ปีที่เผยแพร่ (ค.ศ.)2025

ชื่อย่อของวารสารEPJC

Volume number85

Issue number5

นอก1434-6044

eISSN1434-6052

URLhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-105004208019&doi=10.1140%2fepjc%2fs10052-025-14221-x&partnerID=40&md5=154dbc8520f25e69386ea9854c3d6adb

ภาษาEnglish-Great Britain (EN-GB)


ดูบนเว็บไซต์ของสำนักพิมพ์


บทคัดย่อ

The phase transitions of charged Anti-de Sitter (AdS) black holes are characterized by studying null geodesics in the vicinity of the critical curve of photon trajectories around black holes as well as their optical appearance as the black hole images. In the present work, the critical parameters including the orbital half-period τ, the angular Lyapunov exponent λL, and the temporal Lyapunov exponent γL are employed to characterize black hole phase transitions within both the extended phase space and holographic thermodynamics frameworks. Under certain conditions, we observe multi-valued function behaviors of these parameters as functions of bulk pressure and temperature in the respective approaches. We propose that τ,λL, and γL can serve as order parameters due to their discontinuous changes at first-order phase transitions. To validate this, we provide detailed analytical calculations demonstrating that these optical critical parameters follow scaling behavior near the critical phase transition point. Notably, the critical exponents for these parameters are found to be 1/2, consistent with those of the van der Waals fluid. Our findings suggest that static and distant observers can study black hole thermodynamics by analyzing the images of regions around the black holes. © The Author(s) 2025.


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อัพเดทล่าสุด 2025-15-07 ถึง 00:00