GRB 970228 and its associated supernova within the EMBH model

R. Ruffini; M. G. Bernardini; C. L. Bianco; A. Corsi; S. S. Xue; P. Chardonnet; F. Fraschetti

doi:10.1142/9789812704030_0355

GRB 970228 and its associated supernova within the EMBH model

R. Ruffini, M. G. Bernardini, C. L. Bianco, A. Corsi, S. S. Xue, P. Chardonnet, F. Fraschetti

Physics

Research output: Chapter in Book/Report/Conference proceeding › Chapter › peer-review

Abstract

The λ-ray burst of 1997 February 28 is analyzed within the Electromagnetic Black Hole model. We first estimate the value of the total energy deposited in the dyadosphere, M_dyaa nd the amount of baryonic matter left over by the EMBH progenitor star, B = M_BC ²/E_dya- We then consider the role of the interstellar medium number density n_jsMand of the ratio R between the effective emitting area and the total surface area of the 7-ray burst source, in reproducing the prompt emission and the X-ray afterglow of this burst. Some considerations are also done concerning the possibility of explaining, within the theory, the observed evidence for a supernova in the optical afterglow.

Original language	English
Title of host publication	The Tenth Marcel Grossmann Meeting
Subtitle of host publication	On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories
Publisher	World Scientific Publishing Co.
Pages	2465-2467
Number of pages	3
Volume	3
ISBN (Electronic)	9789812704030
ISBN (Print)	9789812566676
DOIs	https://doi.org/10.1142/9789812704030_0355
State	Published - Jan 1 2006

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Ruffini, R., Bernardini, M. G., Bianco, C. L., Corsi, A., Xue, S. S., Chardonnet, P., & Fraschetti, F. (2006). GRB 970228 and its associated supernova within the EMBH model. In The Tenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (Vol. 3, pp. 2465-2467). World Scientific Publishing Co.. https://doi.org/10.1142/9789812704030_0355

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title = "GRB 970228 and its associated supernova within the EMBH model",

abstract = "The λ-ray burst of 1997 February 28 is analyzed within the Electromagnetic Black Hole model. We first estimate the value of the total energy deposited in the dyadosphere, Mdyaa nd the amount of baryonic matter left over by the EMBH progenitor star, B = MBC 2/Edya- We then consider the role of the interstellar medium number density njsMand of the ratio R between the effective emitting area and the total surface area of the 7-ray burst source, in reproducing the prompt emission and the X-ray afterglow of this burst. Some considerations are also done concerning the possibility of explaining, within the theory, the observed evidence for a supernova in the optical afterglow.",

author = "R. Ruffini and Bernardini, {M. G.} and Bianco, {C. L.} and A. Corsi and Xue, {S. S.} and P. Chardonnet and F. Fraschetti",

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doi = "10.1142/9789812704030_0355",

language = "English",

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Ruffini, R, Bernardini, MG, Bianco, CL, Corsi, A, Xue, SS, Chardonnet, P & Fraschetti, F 2006, GRB 970228 and its associated supernova within the EMBH model. in The Tenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories. vol. 3, World Scientific Publishing Co., pp. 2465-2467. https://doi.org/10.1142/9789812704030_0355

GRB 970228 and its associated supernova within the EMBH model. / Ruffini, R.; Bernardini, M. G.; Bianco, C. L. et al.
The Tenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories. Vol. 3 World Scientific Publishing Co., 2006. p. 2465-2467.

Research output: Chapter in Book/Report/Conference proceeding › Chapter › peer-review

TY - CHAP

T1 - GRB 970228 and its associated supernova within the EMBH model

AU - Ruffini, R.

AU - Bernardini, M. G.

AU - Bianco, C. L.

AU - Corsi, A.

AU - Xue, S. S.

AU - Chardonnet, P.

AU - Fraschetti, F.

PY - 2006/1/1

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N2 - The λ-ray burst of 1997 February 28 is analyzed within the Electromagnetic Black Hole model. We first estimate the value of the total energy deposited in the dyadosphere, Mdyaa nd the amount of baryonic matter left over by the EMBH progenitor star, B = MBC 2/Edya- We then consider the role of the interstellar medium number density njsMand of the ratio R between the effective emitting area and the total surface area of the 7-ray burst source, in reproducing the prompt emission and the X-ray afterglow of this burst. Some considerations are also done concerning the possibility of explaining, within the theory, the observed evidence for a supernova in the optical afterglow.

AB - The λ-ray burst of 1997 February 28 is analyzed within the Electromagnetic Black Hole model. We first estimate the value of the total energy deposited in the dyadosphere, Mdyaa nd the amount of baryonic matter left over by the EMBH progenitor star, B = MBC 2/Edya- We then consider the role of the interstellar medium number density njsMand of the ratio R between the effective emitting area and the total surface area of the 7-ray burst source, in reproducing the prompt emission and the X-ray afterglow of this burst. Some considerations are also done concerning the possibility of explaining, within the theory, the observed evidence for a supernova in the optical afterglow.

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SN - 9789812566676

VL - 3

SP - 2465

EP - 2467

BT - The Tenth Marcel Grossmann Meeting

PB - World Scientific Publishing Co.

ER -

Ruffini R, Bernardini MG, Bianco CL, Corsi A, Xue SS, Chardonnet P et al. GRB 970228 and its associated supernova within the EMBH model. In The Tenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories. Vol. 3. World Scientific Publishing Co. 2006. p. 2465-2467 doi: 10.1142/9789812704030_0355

GRB 970228 and its associated supernova within the EMBH model

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