Abstract
We present a model in which the breakdown of conformal symmetry of a quantumstress-tensor due to the trace anomaly is related to a cosmological effect in agravitational model. This is done by characterizing the traceless part of thequantum stress-tensor in terms of the stress-tensor of a conformal invariantclassical scalar field. We introduce a conformal frame in which the anomaloustrace is identified with a cosmological constant. In this conformal frame weestablish the Einstein field equations by connecting the quantum stress-tensorwith the large-scale distribution of matter in the universe.
Similar content being viewed by others
REFERENCES
Birrell, N. D., and Davies, P. C.W. Quantum Fields in Curved Space (Cambridge University Press, Cambridge, 1982).
Salehi, H. (1998). Int. J. Theor. Phys. 37, 1253.
Wald, R. M. (1978). Commun. Math. Phys. 54, 1 (1977); Phys. Rev. D 17, 1477.
Hawking, S. W., and Ellis, G. F. R. The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, 1973).
Deser, S. (1970). Ann. Phys. 59, 248.
Parker, L. (1973). Phys. Rev. D 7, 976.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Salehi, H., Bisabr, Y. Conformal Anomaly and Large-ScaleGravitational Coupling. International Journal of Theoretical Physics 39, 1241–1244 (2000). https://doi.org/10.1023/A:1003634719325
Issue Date:
DOI: https://doi.org/10.1023/A:1003634719325