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Quantum Gravity

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REFERENCES 343Kiefer, C. (2001a). Path integrals in quantum cosmology. In Fluctuating pathsand fields (ed. W. Janke, A. Pelster, H.-J. Schmidt, and M. Bachmann),pp. 729–40. World Scientific, Singapore.Kiefer, C. (2001b). Hawking radiation from decoherence. Class. <strong>Quantum</strong> Grav.,18, L151–4.Kiefer, C. (2003a). <strong>Quantum</strong> aspects of black holes. In The galactic black hole(ed. H. Falcke and F. W. Hehl), pp. 207–25. Institute of Physics Publishing,Bristol.Kiefer, C. (2003b). On the interpretation of quantum theory—from Copenhagento the present day. In Time, quantum and information (ed. L. Castell andO. Ischebeck), pp. 291–9. Springer, Berlin.Kiefer, C. (2004a). Is there an information-loss problem for black holes? InDecoherence and entropy in complex systems (ed. H.-T. Elze). Lecture Notesin Physics 633. Springer, Berlin.Kiefer, C. (2004b). Hawking temperature from quasi-normal modes. Class. <strong>Quantum</strong>Grav., 21, L123–7.Kiefer, C. (2006). <strong>Quantum</strong> gravity: general introduction and recent developments.Ann. Phys. (Leipzig), 8th series, 129–48.Kiefer, C. and Louko, J. (1999). Hamiltonian evolution and quantization forextremal black holes. Ann. Phys. (Leipzig), 8thseries,8, 67–81.Kiefer, C. and Singh, T. P. (1991). <strong>Quantum</strong> gravitational correction terms tothe functional Schrödinger equation. Phys. Rev. D, 44, 1067–76.Kiefer, C. and Wipf, A. (1994). Functional Schrödinger equation for fermionsin external gauge fields. Ann. Phys. (NY), 236, 241–85.Kiefer, C. and Weber, C. (2005). On the interaction of mesoscopic quantumsystems with gravity. Ann. Phys. (Leipzig), 8th series, 253–78.Kiefer, C. and Zeh, H. D. (1995). Arrow of time in a recollapsing quantumuniverse. Phys. Rev. D, 51, 4145–53.Kiefer, C., Lück, T., and Moniz, P. (2005). Semiclassical approximation to supersymmetricquantum gravity. Phys. Rev. D, 72, 045006 [19 pages].Kiefer, C., Müller-Hill, J., and Vaz, C. (2006a). Classical and quantum Lemaître–Tolman–Bondi model for the nonmarginal case. Phys. Rev. D, 73, 044025 [13pages].Kiefer, C., Polarski, D., and Starobinsky, A. A. (1998). <strong>Quantum</strong>-to-classicaltransition for fluctuations in the early universe. Int. J. Mod. Phys. D, 7, 455–62.Kiefer, C., Polarski, D., and Starobinsky, A. A. (2000). Entropy of gravitonsproduced in the early universe. Phys. Rev. D, 62, 043518 [6 pages].Kimberly, D. and Magueijo, J. (2005). Phenomenological quantum gravity.http://arxiv.org/abs/gr-qc/0502110 [23 pages] (cited on December 15, 2006).Kodama, H. (1990). Holomorphic wavefunction of the universe. Phys. Rev. D,42, 2548–65.Kokkotas, K. D. and Schmidt, B. G. (1999). Quasi-normal modes of stars andblack holes. Living Rev. Relativity, 2, 2. URL (cited on February 24, 2006):

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