Good, MichaelAbdikamalov, Ernazar2021-07-012021-07-012020-08Good, M., & Abdikamalov, E. (2020). Radiation from an Inertial Mirror Horizon. Universe, 6(9), 131. doi:10.3390/universe60901312218-1997http://nur.nu.edu.kz/handle/123456789/5506The purpose of this study is to investigate radiation from asymptotic zero acceleration motion where a horizon is formed and subsequently detected by an outside witness. A perfectly reflecting moving mirror is used to model such a system and compute the energy and spectrum. The trajectory is asymptotically inertial (zero proper acceleration)—ensuring negative energy flux (NEF), yet approaches light-speed with a null ray horizon at a finite advanced time. We compute the spectrum and energy analytically.enAttribution-NonCommercial-ShareAlike 3.0 United StatesType of access: Open Accessacceleration radiationmoving mirrorsQFT in curved spacetimehorizonsdynamical Casimir effectblack holesHawking radiationnegative energy fluxArticle