Modelling the IDV Emissions of the BL Lac Objects with a Langevin Type Stochastic Differential Equation
In this paper, we introduce a simplified model for explaining the observations of optical intra-day variability (IDV) of the BL Lac Objects. We assume that the source of the IDV are the stochastic oscillations of an accretion disk around a supermassive black hole. The stochastic fluctuations on the vertical direction of the accretion disk are described by using a Langevin type equation with a damping term and a random, white noise type force. Furthermore, preliminary numerical simulation results are presented, which are based on the numerical analysis of the Langevin stochastic differential equation.
C.S.Leung J.Y.Wei T.Harko Z.Kovacs
National Astronomical Observatories,Chinese Academy of Sciences,20A Datun Road,Chaoyang District,Bei Department of Physics and Center for Theoretical and Computational Physics,The University of Hong Ko
国际会议
International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)
广州
英文
189-192
2010-09-20（万方平台首次上网日期，不代表论文的发表时间）