Remarks on the light ring images and the optical appearance of hairy black holes in Einstein–Maxwell-dilaton gravity

บทความในวารสาร

ผู้เขียน/บรรณาธิการ

เอกพงษ์ หิรัญสิริสวัสดิ์

กลุ่มสาขาการวิจัยเชิงกลยุทธ์

รายละเอียดสำหรับงานพิมพ์

รายชื่อผู้แต่ง: Promsiri C., Horinouchi W., Hirunsirisawat E.

ผู้เผยแพร่: SpringerOpen

ปีที่เผยแพร่ (ค.ศ.): 2024

ชื่อย่อของวารสาร: EPJC

Volume number: 84

Issue number: 9

นอก: 1434-6044

eISSN: 1434-6052

URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-85203343540&doi=10.1140%2fepjc%2fs10052-024-13258-8&partnerID=40&md5=5bbc2b4f64c4c5ab0a9f897aff4b2274

ภาษา: English-Great Britain (EN-GB)

ดูบนเว็บไซต์ของสำนักพิมพ์

บทคัดย่อ

The behaviors of null geodesics in the spherical symmetric black holes in Einstein–Maxwell-dilaton (EMD) theory with coupling function f(Φ)=e-2αΦ are meticulously analyzed. We investigate the effects of coupling constant α on the effective potential of photon trajectories within three ranges, namely 0<α<1, α=1 and α>1. We find that the thicknesses of lensing and photon rings are smaller at larger α and fixed electric charge in the unit of mass q, whereas they are larger at fixed α and larger q. This behavior can be described by using the angular Lyapunov exponent γ in the vicinity of the critical curve. Remarkably, the behaviors of photon trajectories are found to be more interesting when α>1. Namely, the radius of the black hole shadow Rs becomes to be smaller than the photon sphere radius rph when α>1 and q>q∗. Moreover, Rs goes to zero as q saturates the extremal limit, beyond which the photon orbit becomes absent. Furthermore, we construct the optical appearance of black holes surrounded by optically and geometrically thin accretion disk with three cases of Gralla–Lupsasca–Marrone (GLM) emission profile. Our results indicate that the observed flux originating from the lensing and photon rings exhibits suppression as α increases, while it undergoes amplification with the increasing parameter q. © The Author(s) 2024.

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