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Particle Acceleration in Gamma-Ray Bursts

Published online by Cambridge University Press:  19 September 2016

J.G. Kirk
J.G. Kirk*
Affiliation:
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany; [email protected]

Summary

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Simple kinematic theories of particle acceleration at relativistic shocks lead to the prediction of a high-energy spectral index of −1.1 for the energy flux of synchrotron photons. However, several effects can change this picture. In this paper I discuss the effect of magnetic field generation at the shock front and, by analogy with the Crab Nebula, suggest that an intrinsic break in the injection spectrum should be expected where the electron gyro radius is comparable to that of protons thermalized by the shock.

Type
Part VII Gamma-Ray Bursters
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 475 - 482
Copyright
Copyright © Springer-Verlag 2005

References

1. Achterberg, A., Gallant, Y.A., Kirk, J.G., Guthmann, A.W.: Mon. Not. R. Astron. Soc. 328, 393 (2001)Google Scholar
2. Ballard, K.R., Heavens, A.F.: Mon. Not. R. Astron. Soc. 259, 89 (1992)Google Scholar
3. Bednarz, J., Ostrowski, M.: Phys. Rev. Lett. 80, 3911 (1998)Google Scholar
4. Begelman, M.C., Kirk, J.G.: Astrophys. J. 353, 66 (1990)Google Scholar
5. Casse, F., Lemoine, M., Pelletier, G.: Phys. Rev. D 65, 023002 (2002)Google Scholar
6. Derishev, E.V., Aharonian, F.A., Kocharovsky, V.V., Kocharovsky, V.V.: astro-ph 0301263 (2003)Google Scholar
7. Ellison, D.C., Double, G.P.: Astropart. Phys. 18, 213 (2002)CrossRefGoogle Scholar
8. Fonseca, R.A., Silva, L.O., Tonge, J.W., Mori, W.B., Dawson, J.M.: Phys. Plasmas 10, 1979 (2003)Google Scholar
9. Gallant, Y., van der Swaluw, E., Kirk, J.G., Achterberg, A.: “Modeling ple-rion spectra and their evolution.” In: Neutron Stars in Supernova Remnants. eds. Slane, P.O., Gaensler, B.M. (ASP Conf. Series: Vol. 271 2001) p. 161 Google Scholar
10. Hoshino, M., Arons, J., Gallant, Y.A., Langdon, A.B.: Astrophys. J. 390, 454 (1992)Google Scholar
11. Kirk, J.G., Duffy, P.: J. Phys. G: Nucl. Part. Phys. 25 R163 (1999)CrossRefGoogle Scholar
12. Kirk, J.G., Guthmann, A.W., Gallant, Y.A., Achterberg, A.: Astrophys. J. 542, 235 (2000)Google Scholar
13. Kirk, J.G., Skjaeraasen, O.: Astrophys. J. 591, 366 (2003)Google Scholar
14. Lemoine, M., Pelletier, G.: Astrophys. J. 589, L73 (2003)Google Scholar
15. Lyubarsky, Y.: astro-ph 0306435 (2003)Google Scholar
16. Malkov, M., Drury, L.O’C.: Rep. Prog. Phys. 64, 429 (2001)CrossRefGoogle Scholar
17. Medvedev, M.V., Loeb, A.: Astrophys. J. 526, 679 (1999)CrossRefGoogle Scholar
18. Ostrowski, M.: Mon. Not. R. Astron. Soc. 264, 248 (1993)CrossRefGoogle Scholar
19. Ostrowski, M., Bednarz, J.: Astron. Astrophys. 394, 1141 (2002)Google Scholar
20. Panaitescu, A., Kumar, P.: Astrophys. J. 571, 779 (2002)CrossRefGoogle Scholar
21. Sakai, J., Nakayama, T., Kazimura, Y., Bulanov, S.: J. Phys. Soc. Japan 69, 2503 (2000)CrossRefGoogle Scholar
22. Silva, L.O., Fonseca, R.A., Tonge, J.W., Dawson, J.M., Mori, W.B., Medvedev, M.V.. astro-ph 0307500 (2003)Google Scholar
23. Stern, B.E.: astro-ph 0301384 (2003)Google Scholar
24. Willingale, R., Aschenbach, B., Griffiths, R.G., Sembay, S., Warwick, R.S., Becker, W., Abbey, A.F., Bonnet-Bidaud, J.M.: Astron. Astrophys. 365, L212 (2001)Google Scholar
25. Yang, T.Y.B., Gallant, Y., Arons, J., Langdon, A.B.: Phys. Fluids 5, 3369 (1993)CrossRefGoogle Scholar
26. Yang, T.Y.B., Arons, J., Langdon, A.B.: Phys. Plasmas l, 3059 (1994)CrossRefGoogle Scholar