Abstract
A general-relativistic formalism describing a system of self-gravitating charged bosons is given. It describes the system at zero as well as at finite temperature and chemical potential. A phase transition (Bose-Einstein condensation) occurs at some critical temperature.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Bilić and Nikolić (2000) Bilić N., Nikolić H. (2000): Nucl. Phys. B 590, 575
Friedberg et al. (1987) Friedberg R., Lee T.D., Pang Y. (1987): Phys. Rev. D 35, 3640
Haber and Weldon (1982) Haber H.E., Weldon H.A. (1982): Phys. Rev. D 25, 502
Hawking (1979) Hawking S.W. (1979): in General relativity: An Einstein centenary survey, edited by Hawking S.W. and Israel W. (Cambridge University Press, Cambridge)
Kapusta (1989) Kapusta J.I. (1989): Finite-temperature field theory (Cambridge University Press, Cambridge)
Mielke and Schunck (2000) Mielke E.W., Schunck F.E. (2000): Nucl. Phys. B 564, 185
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2003 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Nikolić, H. (2003). Self-gravitating Bosons at Finite Temperature. In: Trampetić, J., Wess, J. (eds) Particle Physics in the New Millennium. Lecture Notes in Physics, vol 616. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-36539-7_41
Download citation
DOI: https://doi.org/10.1007/3-540-36539-7_41
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-00711-1
Online ISBN: 978-3-540-36539-6
eBook Packages: Springer Book Archive