corner
corner

Phys. Rev. D 40, 1876–1885 (1989)

Observer-dependent quantum vacua in curved space. II

Download: PDF (416 kB) Buy this article Export: BibTeX or EndNote (RIS)

Mario A. Castagnino
Instituto de Astronomía y Física del Espacio, Casilla de Correo 67, Suc. 28, Ciudad Universitaria, 1428 Buenos Aires, Argentina and Instituto de Física de Rosario, Consejo Nacional de Investigaciones Científicas y Técnicas-Universidad Nacional de Rosario, Av. Pellegrini 250, 2000 Rosario, Argentina

Jorge B. Sztrajman
Instituto de Astronomía y Física del Espacio, Casilla de Correo 67, Suc. 28, Ciudad Universitaria, 1428 Buenos Aires, Argentina and Area de Físico-Matemática, Ciclo Básico Común, Universidad de Buenos Aires, Ciudad Universitaria, Pabellón II, 1428 Buenos Aires, Argentina

Received 12 May 1987; revised 30 May 1989; published in the issue dated 15 September 1989

An observer-dependent Hamiltonian is introduced in order to describe massless spin-1 particles in curved space-times. The vacuum state is defined by means of Hamiltonian diagonalization and minimization, which turns out to be equivalent criteria. This method works in an arbitrary geometry, although a condition on the fluid of observers is required. Computations give the vacua commonly accepted in the literature.

© 1989 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.40.1876
DOI:
10.1103/PhysRevD.40.1876
PACS: