Abstract
The energy momentum tensor of a scalar field is considered as being that of a perfect fluid with equation of statep=p(ρ). In the extreme case that the field energy is purely kinetic,p=p, whereas if it is purely potential,p=−ρ.
References
Birrell, N. D. and Davies, P. C. W.: 1982,Quantum Fields in Curved Space, Cambridge University Press, Cambridge.
Weinberg, S.: 1972,Gravitation and Cosmology, Wiley, New York.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Madsen, M.S. A note on the equation of state of a scalar field. Astrophys Space Sci 113, 205–207 (1985). https://doi.org/10.1007/BF00650285
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650285