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Thursday, March 08, 2007. Is GRB 050904 a super-long burst? Is GRB 050904 a super-long burst? Comments: 16 pages, 4 figure. Submitted on Oct. 21, 2005, accepted by ApJ. Journal-ref: Astrophys.J. 646 (2005) 1098-1103. By considering synchrotron radiative process in the internal shock model and. Assuming that all internal shocks are nearly equally energetic, we analyze the. Gamma-ray burst (GRB) emission at different radii corresponding to different. Powered by performancing firefox. Time-dependent calcula...

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Lei WH's Blog | gtap.blogspot.com Reviews

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Thursday, March 08, 2007. Is GRB 050904 a super-long burst? Is GRB 050904 a super-long burst? Comments: 16 pages, 4 figure. Submitted on Oct. 21, 2005, accepted by ApJ. Journal-ref: Astrophys.J. 646 (2005) 1098-1103. By considering synchrotron radiative process in the internal shock model and. Assuming that all internal shocks are nearly equally energetic, we analyze the. Gamma-ray burst (GRB) emission at different radii corresponding to different. Powered by performancing firefox. Time-dependent calcula...

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Lei WH's Blog | gtap.blogspot.com Reviews

https://gtap.blogspot.com

Thursday, March 08, 2007. Is GRB 050904 a super-long burst? Is GRB 050904 a super-long burst? Comments: 16 pages, 4 figure. Submitted on Oct. 21, 2005, accepted by ApJ. Journal-ref: Astrophys.J. 646 (2005) 1098-1103. By considering synchrotron radiative process in the internal shock model and. Assuming that all internal shocks are nearly equally energetic, we analyze the. Gamma-ray burst (GRB) emission at different radii corresponding to different. Powered by performancing firefox. Time-dependent calcula...

INTERNAL PAGES

gtap.blogspot.com

1

Lei WH's Blog: Is GRB 050904 a super-long burst?

http://gtap.blogspot.com/2007/03/is-grb-050904-super-long-burst.html

Thursday, March 08, 2007. Is GRB 050904 a super-long burst? Is GRB 050904 a super-long burst? Comments: 16 pages, 4 figure. Submitted on Oct. 21, 2005, accepted by ApJ. Journal-ref: Astrophys.J. 646 (2005) 1098-1103. By considering synchrotron radiative process in the internal shock model and. Assuming that all internal shocks are nearly equally energetic, we analyze the. Gamma-ray burst (GRB) emission at different radii corresponding to different. Powered by performancing firefox. Inner Engine of GRB.

2

Lei WH's Blog: Magnetic acceleration of relativistic AGN jets

http://gtap.blogspot.com/2007/03/magnetic-acceleration-of-relativistic.html

Thursday, March 08, 2007. Magnetic acceleration of relativistic AGN jets. Title: Magnetic acceleration of relativistic AGN jets. Comments: Submitted to MNRAS. We present numerical simulations of axisymmetric, magnetically driven. Relativistic jets. To eliminate the dissipative effects induced by a free. Boundary with an ambient medium we assume that the flow is confined by a rigid. Wall of a prescribed shape, which we take to be $z propto r a$ (in cylindrical. Shape of the confining boundary or to the de...

3

Lei WH's Blog: Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts and Gravitational Wave Detection

http://gtap.blogspot.com/2007/03/black-hole-spin-evolution-implications.html

Thursday, March 08, 2007. Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts and Gravitational Wave Detection. Title: Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts. And Gravitational Wave Detection. Ronald E. Taam. Marc van der Sluys. Comments: 19 pages, 3 tables, 10 figures: submitted to ApJ. The evolution of the spin and tilt of black holes in compact black hole -. Neutron star and black hole - black hole binary systems is investigated via the. Is sufficie...

4

Lei WH's Blog: 10/01/2006 - 11/01/2006

http://gtap.blogspot.com/2006_10_01_archive.html

Friday, October 13, 2006. Gamma ray signatures of ultra high energy cosmic ray accelerators: electromagnetic cascade versus synchrotron radiation of secondary electrons. Title: Gamma ray signatures of ultra high energy cosmic ray accelerators: electromagnetic cascade versus synchrotron radiation of secondary electrons. Felix A. Aharonian. Comments: To appear in Astrophysics and Space Science, proceeding of "The multi messenger approach to high energy gamma ray sources", Barcelona, June 2006. 12288;&#1228...

5

Lei WH's Blog: 08/01/2006 - 09/01/2006

http://gtap.blogspot.com/2006_08_01_archive.html

Wednesday, August 30, 2006. GRBs from alternating-current jets. 65288;磁旋转不稳定性）导致环向磁场极性随机反转，典型的反转时标由磁场放大到动力学重要性的水平的时标决定。具有反转磁场特征的. 发生在空间分离重联端。在该模型中，伴生的同步辐射能被高度极化并且能够产生平滑和尖锐的光变曲线。我们注意到，作为热力学不稳定性的结果，可能在重联区产生一个冷而致密的纤维。由于对同步辐射的无束缚吸收，可能被用来解释非常硬的. The jets are powered by energy extracted electromagnetically from a rotating accretion disc and/or black hole. A bulk of the jet energy is dissipated and re-radiated in the form of GRBs, at distances. 10 13 10 14cm. Science, Nature, PRL, PR, ApJ. From Ma R. Y.). Shock...

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Lei WH's Blog

Thursday, March 08, 2007. Is GRB 050904 a super-long burst? Is GRB 050904 a super-long burst? Comments: 16 pages, 4 figure. Submitted on Oct. 21, 2005, accepted by ApJ. Journal-ref: Astrophys.J. 646 (2005) 1098-1103. By considering synchrotron radiative process in the internal shock model and. Assuming that all internal shocks are nearly equally energetic, we analyze the. Gamma-ray burst (GRB) emission at different radii corresponding to different. Powered by performancing firefox. Time-dependent calcula...

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