Abstract
The analytic solution of a static spherical symmetrical Proca black hole is discussed in this paper. As in the massive vector field, Proca black hole can be considered as the analogy of RN background plus a perturbation with the same order as μ 2 due to the mass of vector particle μ satisfying μ 2 ≪ 1. Through the action of Proca field, we find the analytic form with the first and arbitrary order approximation. Furthermore, we divide the results into 3 groups according to the real zero solutions of the background (i.e., spacetime in massless vector field). Finally we analyze the Hawking radiation of such black hole, which is significant for constructing black hole thermodynamic.
Similar content being viewed by others
References
Hawking, S.W.: Nature 248, 30 (1974)
Hawking, S.W.: Commun. Math. Phys. 43, 199 (1975)
Kraus, P., Wilczek, F.: Nucl. Phys. B 433, 403 (1995). arXiv:9408003 [gr-qc]
Robinson, S.P., Wilczek, F.: Phys. Rev. Lett. 95, 011303 (2005). arXiv:0502074 [gr-qc]
Iso, S., Umetsu, H., Wilczek, F.: Phys. Rev. D 74, 044017 (2006). arXiv:0606018 [hep-th]
Parikh, M.K., Wilczek, F.: Phys. Rev. Lett. 85, 5042 (2000). arXiv:9907001 [hep-th]
Parikh, M.K.: Int. J. Mod. Phys. D 13, 2355 (2004). arXiv:0405160 [hep-th]
Parikh, M.K.: The Tenth Marcel Grossmann Meeting. In: Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF) (2006). arXiv:http://www.worldscientific.com/worldscibooks/10.1142/6033 [hep-th]
Zhang, J.Y., Zhao, Z.: Phys. Lett. B 638, 110 (2006). arXiv:0512153 [gr-qc]
Srinivasan, K., Padmanabhan, T.: Phys. Rev. D 60, 24007 (1999)
Akhmedov, E.T., Akhmedova, V., Singleton, D.: Phys. Lett. B 642, 124 (2006)
Angheben, M., Nadalini, M., Vanzo, L., Zerbini, S.: J. High Energy Phys. 0505, 014 (2005)
Shankaranarayanan, S., Padmanabhan, T., Srinivasan, K.: Class. Quant. Grav. 19, 2671 (2002)
Cai, R.G., Cao, L.M., Hu, Y.P.: J. High Energy Phys. 0808, 090 (2008)
Banerijee, R., Majhi, B.R.: J. High. Energy Phys. 0806, 095 (2008)
Majhi, B.R.: Phys. Rev. D 79, 044005 (2009)
Modak, S.K.: Phys. Lett. B 671, 167 (2009)
Lin, K., Yang, S.Z.: Europhys. Lett. 82, 20006 (2009)
Lin, K., Yang, S.Z.: Int. J. Theor. Phys. 48, 2920 (2009)
Lin, K., Yang, S.Z.: Chin. Phys. B 20, 110403 (2011)
Torii, T., Maeda, K.-I., Tachizawa, T.: Phys. Rev. D 51, 1510 (1995). arXiv:9406013 [gr-qc]
Torii, T., Maeda, K.: Phys. Rev. D 48, 1643 (1993)
Galtsov, D.V., Volkov, M.S.: Phys. Lett. A 162, 144 (1992)
Straumann, N., Zhou, Z.-H.: Phys. Lett. B 234, 33 (1990)
Zhou, Z.-H., Straumann, N.: Nucl. Phys. B 234, 180 (1991)
Bizon, P.: Phys. Lett. B 259, 53 (1991)
Bizon, P., Wald, R.M.: Phys. Lett. B 259, 173 (1991)
Heusler, M., Droz, S., Straumann, N.: Phys. Lett. B 271, 61 (1991)
Bizon, P. Acta Phys. Polon B 25, 877 (1994). arXiv:9402016 [gr-qc]
Gibbons, G.W., Maeda, K.: Nucl. Phys. B 298, 741 (1988)
Garfinkle, D., Horowitz, G.T., Strominger, A.: Phys. Rev. D 43, 3140 (1991)
Hawking, S.W.: Nature 248, 30 (1974)
Hawking, S.W.: Commun. Math. Phys. 43, 199 (1975)
Damoar, T., Ruffini, R.: Phys. Rev. D 14, 332 (1976)
Yang, S.Z., Lin, K., Li, J.: Hawking radiation of black hole in Einstein-Proca theory. Int. J. Theor. Phys. (2014) doi:10.1007/s10773-013-1968-6
Lin, K., Yang, S.Z.: Chin. Phys. B 20, 110403 (2011)
Tu, L.C., Shao, C.C., Luo, J.: Phys. Lett. A 352, 267 (2006)
Acknowledgments
This work was supported by National Natural Science Foundation of China No. 11205254, No. 11178018 and No. 11075224, and the Natural Science Foundation Project of CQ CSTC 2011BB0052, and the Fundamental Research Funds for the Central Universities CQDXWL-2013-010,CDJZR12160015 and CDJRC10300003.
Author information
Authors and Affiliations
Corresponding author
Appendix
Appendix
In the appendix, for the case 1, case 2, case 3 mentioned in Section 2, we list the perturbation functions Ñ (r) and à 0 (r) with corresponding subscripts respectively. Here we only retain the coefficients of δ.
Case 1
\(1+\frac {Q^{2}}{r^{2}}-\frac {2M}{r}+\frac {r^{2}\Lambda }{3}=\frac {\Lambda }{3r^{2}}(r-r_{1})(r-r_{2})(r-r_{3})(r-r_{4})\):
Case 2
\(1+\frac {Q^{2}}{r^{2}}-\frac {2M}{r}+\frac {r^{2}\Lambda }{3}=\frac {\Lambda }{3r^{2}}(r-r_{1})(r-r_{2})(r^{2}+ar+b)\):
Case 3
\(1+\frac {Q^{2}}{r^{2}}-\frac {2M}{r}+\frac {r^{2}\Lambda }{3}=\frac {\Lambda }{3r^{2}}(r^{2}+ar+b)(r^{2}+cr+d)\):
Rights and permissions
About this article
Cite this article
Zhong, Y., Li, J. & Lin, K. An Analytic Approximation for Researching Tunneling Rate from Black Hole in Proca Field. Int J Theor Phys 53, 3035–3045 (2014). https://doi.org/10.1007/s10773-014-2099-4
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-014-2099-4