Influence action and decoherence of hydrodynamic modes
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...
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1999
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| LEADER | 08441caa a22011897a 4500 | ||
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| 001 | PAPER-19692 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205103.0 | ||
| 008 | 190411s1999 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-17044417574 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Calzetta, E.A. | |
| 245 | 1 | 0 | |a Influence action and decoherence of hydrodynamic modes |
| 260 | |c 1999 | ||
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a 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. |l eng | |
| 593 | |a Department of Physics and IAFE, University of Buenos Aires, Argentina | ||
| 593 | |a Department of Physics, University of Maryland, College Park, Maryland, 20742-4111, United States | ||
| 700 | 1 | |a Hu, B.L. | |
| 773 | 0 | |d 1999 |g v. 59 |k n. 6 |p Phys Rev D Part Fields Gravit Cosmol |x 15507998 |t Physical Review D - Particles, Fields, Gravitation and Cosmology | |
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| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.59.065018 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_15507998_v59_n6_p_Calzetta |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v59_n6_p_Calzetta |y Registro en la Biblioteca Digital |
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