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Is There a Relation between Duration and Eiso in Gamma-Ray Bursts?

Published online by Cambridge University Press:  21 February 2013

Shu-Jin Hou ,
Tong Liu ,
Da-Bin Lin ,
Xue-Feng Wu  and
Ju-Fu Lu
Shu-Jin Hou
Affiliation:
Department of Physics and Institute of Theoretical Physics and Astrophysics, University Xiamen, Fujian 361005, China email: [email protected] Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected]
Tong Liu
Affiliation:
Department of Physics and Institute of Theoretical Physics and Astrophysics, University Xiamen, Fujian 361005, China email: [email protected]
Da-Bin Lin
Affiliation:
Department of Physics and Institute of Theoretical Physics and Astrophysics, University Xiamen, Fujian 361005, China email: [email protected]
Xue-Feng Wu
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected]
Ju-Fu Lu
Affiliation:
Department of Physics and Institute of Theoretical Physics and Astrophysics, University Xiamen, Fujian 361005, China email: [email protected]
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Abstract

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The system of accretion disk and black hole is usually considered as the central engine of Gamma-ray Bursts (GRBs). It is usually thought that the disk in the central engine of GRBs is the advection-dominated accretion disk, which is developed from a massive (mass Mdisk) torus at radius rdisk. We find a positive correlation between the isotropic gamma-ray energy Eiso and duration (so-called T90) for GRBs. We interpret this correlation within the advection-dominated accretion disk model, associating Eiso and T90 with Mdisk and viscous timescale respectively.

Keywords

Gamma-ray: burstsaccretion, accretion disksblack hole physics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 223 - 224
Copyright
Copyright © International Astronomical Union 2013

References

Gehrels, N., Ramirez-Ruiz, E., & Fox, D. B. 2009, ARA&A, 47, 567Google Scholar
Kouveliotou, C., Meegan, C. A., Fishman, G. J., et al. 2001, ApJ, 413, 101CrossRefGoogle Scholar
Liu, T., Gu, W. M., Xue, L., & Lu, J. F. 2007, ApJ, 661, 1025CrossRefGoogle Scholar
Narayan, R., Piran, T., & Kumar, P. 2001, ApJ, 557, 949CrossRefGoogle Scholar
Popham, R., Woosley, S. E., & Fryer, C. 1999, ApJ, 518, 356CrossRefGoogle Scholar