Abstract
Applying the Hamilton-Jacobi method, we investigate particles’ tunneling behavior in a spherically symmetric spacetime with dark matter. The tunneling rate and Hawking temperature at the event horizon are obtained. The result shows that the dark matter parameter β has an important influence on the Hawking temperature and the tunneling rate.
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References
Hawking, S.W.: Nature 30, 248 (1974)
Hawking, S.W.: Commun. Math. Phys. 43(3), 199 (1975)
Li, R., Ren, J.R., Shi, D.F.: Phys. Lett. B 670(4–5), 446 (2009)
Zhao, Z.: Chin. Phys. Lett. 9(9), 401 (1992)
Wu, S.Q., Jiang, Q.Q.: J. High Energy Phys. 0603, 079 (2006)
Robinson, S.P.: Phys. Rev. Lett. 95, 011303 (2005)
Parikh, M.K.: Phys. Rev. Lett. 85, 5042 (2000)
Srinivasan, K., Padmanabhan, T.: Phys. Rev. D 60(2), 24007 (1999)
Chen, D.Y., Yang, S.Z.: Gen. Relativ. Gravit. 39, 1503 (2007)
Chen, D.Y., Yang, S.Z.: Mod. Phys. Lett. A 22, 2611 (2007)
Chen, D.Y., Yang, S.Z.: Int. J. Mod. Phys. A 22, 5173 (2007)
Chen, D.Y., Yang, S.Z.: Int. J. Mod. Phys. D 16, 1295 (2007)
Chen, D.Y., Yang, S.Z.: New J. Phys. 9, 252 (2007)
Kerner, R., Mann, R.B.: Phys. Rev. D 73, 104010 (2006)
Kerner, R., Mann, R.B.: Phys. Lett. B 665, 277 (2008)
Chen, D.Y., Jiang, Q.Q., Zu, X.T.: Phys. Lett. B 665, 106 (2008)
Jiang, Q.Q.: Phys. Rev. D 78, 044009 (2008)
Lin, K., Yang, S.Z.: Phys. Rev. D 79, 064035 (2009)
Yang, S.Z., Lin, K.: Sci. China 40(4), 507 (2010)
Heydari-Fard, M., Razmi, H., Sepangi, H.R.: Phys. Rev. D 76, 066002 (2007)
Shahab, S., Hami, R.S.: Int. J. Mod. Phys. D 20, 77 (2011)
del Campo, S.: Phys. Rev. D 66, 123513 (2002)
Joao, R.G., Dolan, S.R.: Phys. Rev. D 85, 044043 (2012)
Yale, A., Mann, R.B.: arXiv:0808.2820 (2008)
Acknowledgement
This work was supported by the National Foundation of china under Grant No. 11178018.
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Li, GP., Zhou, YG. & Zu, XT. Particles’ Tunneling in Spherically Symmetric Spacetimes with Dark Matter. Int J Theor Phys 52, 4025–4031 (2013). https://doi.org/10.1007/s10773-013-1716-y
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DOI: https://doi.org/10.1007/s10773-013-1716-y