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Publication Date:
February 2007
ISSN:
1437-4358
DOI:
10.1515/JNETDY.2007.002

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Editor-in-Chief: Keller, Jürgen U.

Ed. by Michaelides, Efstathios E. / Muschik, Wolfgang

Editorial Board Member: Andresen, Bjarne / Bejan, Adrian / Brüggemann, Dieter / Buchholz, Rainer / Dinkelacker, Friedrich / Do, Duong / Groll, Manfred / Gross, Joachim / Hoffmann, Karl-Heinz / Kalliadasis, Serafim / Kjelstrup, S. / Lebon, Georgy / Maugin, G. A. / Raffa, Robert B. / Rubi, J. Miguel / Scholl, Stephan / Steinchen, Annie / Stockar, Urs / Verhas, Jozsef / Winter, Roland / Zaman, Muhammad / Ahlborn, Boye / Bedeaux, Dick / Fox, Ronald F. / Kizilova, Natalya / Kollmann, W. / Ricard, Jacques / Sieniutycz, Stanislaw / Velarde, M.G. / Papenfuss, Christina / Stark, Holger

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Rank 25 out of 52 in category Thermodynamics in the 2011 Thomson Reuters Journal Citation Report/Science Edition.

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On the Fluctuation-Dissipation Theorem for Convective Processes

Alan J McKane1 / Federico Vázquez2 / 3

Citation Information: Journal of Non-Equilibrium Thermodynamics. Volume 32, Issue 1, Pages 29–40, ISSN (Print) 0340-0204, DOI: 10.1515/JNETDY.2007.002, February 2007

Publication History:
Received:
2006-05-17
Accepted:
2006-06-29
Published Online:
2007-02-22

Abstract

When making the connection between the thermodynamics of irreversible processes and the theory of stochastic processes through the fluctuation–dissipation theorem, it is necessary to invoke a postulate of the Einstein–Boltzmann type. For convective processes hydrodynamic fluctuations must be included; the velocity is a dynamical variable and although the entropy cannot depend directly on the velocity, δ2 S will depend on velocity variations. Some authors do not include velocity variations in δ2 S, and so have to introduce a non-thermodynamic function which replaces the entropy and does depend on the velocity. At first sight, it seems that the introduction of such a function requires a generalisation of the Einstein–Boltzmann relation to be invoked. We review the reason why it is not necessary to introduce such a function, and therefore why there is no need to generalise the Einstein–Boltzmann relation in this way. We then obtain the fluctuation–dissipation theorem, which shows some differences as compared with the non-convective case. We also show that δ2 S is a Liapunov function when it includes velocity fluctuations.

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