supported by the Open Research Program of the Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences
It is expected that there should be a spectral cutoff at the high energy end of emission from a prompt gamma-ray burst (GRB), due to, e.g. γγ absorption and/or a high energy cutoff in the electron distribution. We...
supported by the National Natural Science Foundation of China (Grant Nos. 10873009 and 11033002);the National Basic Research Program of China (973 Program;No. 2007CB815404)
We present broadband (radio, optical, X-ray and GeV) fits to the afterglow light curves and spectra of three long-duration gamma-ray bursts (GRBs 080916C, 090902B, and 090926A) detected by the Gamma-Ray Burst Moni...
supported by National Natural Science Foundation of China (Grant No.30727002);National High-Tech Research and Development Program of China (2006AA02Z343)
Bursts are electrical spikes firing with a high frequency, which are the most important property in synaptic plasticity and information processing in the central nervous system. However, bursts are difficult to identi...
In this paper, we present a new analytical model for TCP Reno, and thismethod can also be used in other versions of TCP. The first order two-state Markovian model is usedto describe the wireless link, so as to deal wi...