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Title: Bose-Einstein condensation for interacting scalar fields in curved spacetime

Abstract

We consider the model of self-interacting complex scalar fields with a rigid gauge invariance under an arbitrary gauge group {ital G}. In order to analyze the phenomenon of Bose-Einstein condensation, finite temperature and the possibility of a finite background charge are included. Different approaches to derive the relevant high-temperature behavior of the theory are presented.

Authors:
 [1];  [2]
  1. Departament d`ECM, Facultat de Fisica, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, Catalonia (Spain)
  2. Department of Physics, University of Newcastle Upon Tyne, Newcastle Upon Tyne, United Kingdom NE1 7RU (United Kingdom)
Publication Date:
OSTI Identifier:
55213
Resource Type:
Journal Article
Journal Name:
Physical Review, D
Additional Journal Information:
Journal Volume: 51; Journal Issue: 12; Other Information: PBD: 15 Jun 1995
Country of Publication:
United States
Language:
English
Subject:
66 PHYSICS; BOSE-EINSTEIN CONDENSATION; SCALAR FIELDS; SPACE-TIME; GAUGE INVARIANCE; TEMPERATURE DEPENDENCE; CHARGES; INTERACTING BOSON MODEL

Citation Formats

Kirsten, K, and Toms, D J. Bose-Einstein condensation for interacting scalar fields in curved spacetime. United States: N. p., 1995. Web. doi:10.1103/PhysRevD.51.6886.
Kirsten, K, & Toms, D J. Bose-Einstein condensation for interacting scalar fields in curved spacetime. United States. https://doi.org/10.1103/PhysRevD.51.6886
Kirsten, K, and Toms, D J. 1995. "Bose-Einstein condensation for interacting scalar fields in curved spacetime". United States. https://doi.org/10.1103/PhysRevD.51.6886.
@article{osti_55213,
title = {Bose-Einstein condensation for interacting scalar fields in curved spacetime},
author = {Kirsten, K and Toms, D J},
abstractNote = {We consider the model of self-interacting complex scalar fields with a rigid gauge invariance under an arbitrary gauge group {ital G}. In order to analyze the phenomenon of Bose-Einstein condensation, finite temperature and the possibility of a finite background charge are included. Different approaches to derive the relevant high-temperature behavior of the theory are presented.},
doi = {10.1103/PhysRevD.51.6886},
url = {https://www.osti.gov/biblio/55213}, journal = {Physical Review, D},
number = 12,
volume = 51,
place = {United States},
year = {Thu Jun 15 00:00:00 EDT 1995},
month = {Thu Jun 15 00:00:00 EDT 1995}
}