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Calzetta, E.A.; Hu, B.L. "Influence action and decoherence of hydrodynamic modes" (1999) Physical Review D - Particles, Fields, Gravitation and Cosmology. 59(6)
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Abstract:

We derive an influence action for the heat diffusion equation and from its spectral dependence show that long wavelength hydrodynamic modes are more readily decohered. The result is independent of the details of the microscopic dynamics, and follows from general principles alone. © 1999 The American Physical Society.

Registro:

Documento: Artículo
Título:Influence action and decoherence of hydrodynamic modes
Autor:Calzetta, E.A.; Hu, B.L.
Filiación:Department of Physics and IAFE, University of Buenos Aires, Argentina
Department of Physics, University of Maryland, College Park, Maryland, 20742-4111, United States
Año:1999
Volumen:59
Número:6
DOI: http://dx.doi.org/10.1103/PhysRevD.59.065018
Título revista:Physical Review D - Particles, Fields, Gravitation and Cosmology
Título revista abreviado:Phys Rev D Part Fields Gravit Cosmol
ISSN:15507998
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v59_n6_p_Calzetta

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Citas:

---------- APA ----------
Calzetta, E.A. & Hu, B.L. (1999) . Influence action and decoherence of hydrodynamic modes. Physical Review D - Particles, Fields, Gravitation and Cosmology, 59(6).
http://dx.doi.org/10.1103/PhysRevD.59.065018
---------- CHICAGO ----------
Calzetta, E.A., Hu, B.L. "Influence action and decoherence of hydrodynamic modes" . Physical Review D - Particles, Fields, Gravitation and Cosmology 59, no. 6 (1999).
http://dx.doi.org/10.1103/PhysRevD.59.065018
---------- MLA ----------
Calzetta, E.A., Hu, B.L. "Influence action and decoherence of hydrodynamic modes" . Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 59, no. 6, 1999.
http://dx.doi.org/10.1103/PhysRevD.59.065018
---------- VANCOUVER ----------
Calzetta, E.A., Hu, B.L. Influence action and decoherence of hydrodynamic modes. Phys Rev D Part Fields Gravit Cosmol. 1999;59(6).
http://dx.doi.org/10.1103/PhysRevD.59.065018