Abstract.
We study the Gaussian approximation to the quantum fluctuations of the metric of the four-dimensional anti-de Sitter spacetime. The associated massless scalar field has a quartic self-interaction, for which we construct the generating functional of the n-point correlation functions. The concomitant infrared divergence is cured by a mass renormalization provided by the cosmological constant, which is also responsible for the renormalization of the coupling constant of the field theory.
Similar content being viewed by others
References
C. Romero, J.B. Fonseca-Neto, M.L. Pucheu, Found. Phys. 42, 224 (2012) arXiv:1101.5333v1 [gr-qc]
S. Carroll, Spacetime and Geometry. An Introduction to General Relativity (Addison Wesley, San Francisco, 2004) p. 130
R. d’Inverno, Introducing Einstein’s Relativity (Oxford University Press, Oxford, 1992) p. 89
J.V. Narlikar, T. Padmanabhan, Phys. Rep. 100, 151 (1983)
L.S. Schulman, Techniques and Applications of Path Integration (J. Wiley, New York, 1981) pp. 88, 95, 96
A.D. Boozer, Eur. J. Phys. 28, 729 (2007)
L.H. Ryder, Quantum Field Theory (Cambridge University Press, Cambridge, 1996) p. 184
M. Ibison, J. Math. Phys. 48, 122501 (2007) arXiv:0704.2788 [gr-qc]
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Camargo, H.A., Gonzalez de Urreta, E.J. & Socolovsky, M. Weyl geometry, anti-de Sitter space, and \(\Phi^{4}\)-theory. Eur. Phys. J. Plus 131, 172 (2016). https://doi.org/10.1140/epjp/i2016-16172-9
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epjp/i2016-16172-9