Figure 1 from GRB 090510: A GENUINE SHORT GRB FROM A BINARY NEUTRON STAR COALESCING INTO A KERR

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GRB 090510: A GENUINE SHORT GRB FROM A BINARY NEUTRON STAR COALESCING INTO A KERR–NEWMAN BLACK HOLE

Authors: R. Ruffini, M. Muccino, Y. Aimuratov, C. L. Bianco, C. Cherubini, M. Enderli, M. Kovacevic, R. Moradi, A. V. Penacchioni, G. B. Pisani, J. A. Rueda, and Y. Wang

2016 The Astrophysical Journal 831 178.

Provider: AAS Journals

Caption: Figure 1.

Projection of the dyadotorus of a Kerr–Newman BH corresponding to selected values of the ratio E/E_c, where E_c is the critical value for vacuum polarization and E is the electric field strength. The plot assumes a black hole mass energy ﹩\mu ={M}_{\mathrm{BH}}/{M}_{\odot }=10﹩. This figure is reproduced from Cherubini et al. (2009), with their kind permission.

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