## Neutrino-cooled Accretion Model with Magnetic Coupling for X-ray Flares in GRBs    [PDF]

Yang Luo, Wei-Min Gu, Tong Liu, Ju-Fu Lu
The neutrino-cooled accretion disk, which was proposed to work as the central engine of gamma-ray bursts, encounters difficulty in interpreting the X-ray flares after the prompt gamma-ray emission. In this paper, the magnetic coupling between the inner disk and the central black hole is taken into consideration. For mass accretion rates around \$0.001 \sim 0.1 M_{\sun} s^{-1}\$, our results show that the luminosity of neutrino annihilation can be significantly enhanced due to the coupling effects. As a consequence, after the gamma-ray emission, a remnant disk with mass \$M_{disk} \la 0.5 M_{\sun}\$ may power most of the observed X-ray flares with the rest frame duration less than 100 seconds. In addition, a comparison between the magnetic coupling process and the Blandford-Znajek mechanism is shown on the extraction of black hole rotational energy.
View original: http://arxiv.org/abs/1306.6690