Quick proton decay and astrophysics
Article
First Online:
Received:
Accepted:
- 40 Downloads
Abstract
Protons of energy 109 GeV and 104 GeV accelerating by the magnetic field of very strongly magnetized neutron stars and of extreme Kerr-Newmann black holes (respectively) may undergo instantaneous decay.
Keywords
gravitation thermodynamics Unruh effect cosmic rays neutron stars black holes magnetarsReferences
- Davies, P.C.W.: Physics Letters B 101, 399 (1981).CrossRefADSGoogle Scholar
- Duncan, R.C. and Thompson, C.: Astronomical Journal 392 L9 (1992).Google Scholar
- Duncan, R.C. and Thompson, C.: “Magnetars” in: Proceedings of a March 1995 Astrophysics Conference in La Jolla, California, pp. 112–117 (1995).Google Scholar
- Ibrahim, Alaa I., Markwardt, C.B., Swank, J.H., Ransom, S., Roberts, M., Kaspi, V., Woods, P.M., Safi–Harb, S., Balman, S., Parke, W.C., Kouveliotou, C., Hurley, K, and Cline, T.: The Astrophysical Journal 609, L21 (2004).CrossRefADSGoogle Scholar
- Kouveliotou, C., Dieters, S., Strohmayer, T., Von Paradijs, J., Fishman, G.J., Meegan, C.A., Hurley, K., Kommers, J., Smoth, I., Frail, D. and Murakami, T.: Nature 393, 235 (1998).CrossRefADSGoogle Scholar
- Massa, C.: Astrophysics and Space Science 271, 365, and references therein (2000).Google Scholar
- Misner, C., Thorne, K.S. and Wheeler, J.A.: Gravitation (W.H. Freeman and Company, San Francisco); see Ch. 33, Sec. 3, pp. 891–892 (1973).Google Scholar
- Rosu, H.: International Journal of Modern Physics 3, 545 (1994).ADSGoogle Scholar
- Unruh, W.G.: Physical Review, D 14, 870 (1976).CrossRefADSGoogle Scholar
Copyright information
© Springer Science+Business Media, Inc. 2006