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Abstract:

We show that the "turbulent" particle spectra found in numerical simulations of the behavior of matter fields during reheating admit a simple interpretation in terms of hydrodynamic models of the reheating period. We predict a particle number spectrum n k∝k -α with α∼2 for k→0. © 2002 The American Physical Society.

Registro:

Documento: Artículo
Título:Reheating and turbulence
Autor:Graña, M.; Calzetta, E.
Filiación:Department of Physics, University of California at Santa Barbara, Santa Barbara, CA 93106, United States
Physics Department, University of Buenos Aires, Buenos Aires, Argentina
Palabras clave:article; heating; hydrodynamics; mathematical analysis; molecular interaction; prediction; simulation; theoretical model; turbulent flow
Año:2002
Volumen:65
Número:6
DOI: http://dx.doi.org/10.1103/PhysRevD.65.063522
Título revista:Physical Review D
Título revista abreviado:-
ISSN:05562821
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v65_n6_p_Grana

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Citas:

---------- APA ----------
Graña, M. & Calzetta, E. (2002) . Reheating and turbulence. Physical Review D, 65(6).
http://dx.doi.org/10.1103/PhysRevD.65.063522
---------- CHICAGO ----------
Graña, M., Calzetta, E. "Reheating and turbulence" . Physical Review D 65, no. 6 (2002).
http://dx.doi.org/10.1103/PhysRevD.65.063522
---------- MLA ----------
Graña, M., Calzetta, E. "Reheating and turbulence" . Physical Review D, vol. 65, no. 6, 2002.
http://dx.doi.org/10.1103/PhysRevD.65.063522
---------- VANCOUVER ----------
Graña, M., Calzetta, E. Reheating and turbulence. -. 2002;65(6).
http://dx.doi.org/10.1103/PhysRevD.65.063522