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Volumn 390, Issue 9, 2011, Pages 1546-1574

Brownian particles with long- and short-range interactions

Author keywords

Brownian particles; Generalized thermodynamics; Kinetic theory; Long range interactions; Nonlinear mean field FokkerPlanck equations

Indexed keywords

BIOCHEMISTRY; BROWNIAN MOVEMENT; COLLOIDS; FOKKER PLANCK EQUATION; FREE ENERGY; HYDRODYNAMICS; KINETIC THEORY; KINETICS; PROBABILITY DISTRIBUTIONS; SUSPENSIONS (FLUIDS);

EID: 79952105141     PISSN: 03784371     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.physa.2010.12.018     Document Type: Article
Times cited : (45)

References (83)
  • 1
    • 0042602166 scopus 로고    scopus 로고
    • Dynamics and Thermodynamics of Systems with Long-Range Interactions
    • Springer Berlin
    • T. Dauxois, S. Ruffo, E. Arimondo, M. Wilkens, Dynamics and Thermodynamics of Systems with Long-Range Interactions Lectures Notes in Physics vol. 602 2002 Springer Berlin
    • (2002) Lectures Notes in Physics , vol.602
    • Dauxois, T.1    Ruffo, S.2    Arimondo, E.3    Wilkens, M.4
  • 2
    • 67650775732 scopus 로고    scopus 로고
    • Dynamics and Thermodynamics of Systems with Long-Range Interactions: Theory and Experiments
    • A. Campa, A. Giansanti, G. Morigi, F. Sylos Labini, Dynamics and Thermodynamics of Systems with Long-Range Interactions: Theory and Experiments AIP Conf. Proc. vol. 965 2008 122
    • (2008) AIP Conf. Proc. , vol.965 , pp. 122
    • Campa, A.1    Giansanti, A.2    Morigi, G.3    Sylos Labini, F.4
  • 27
    • 85087602095 scopus 로고    scopus 로고
    • Collapse and evaporation of a canonical self-gravitating gas
    • World Scientific Singapore
    • C. Sire, and P.H. Chavanis Collapse and evaporation of a canonical self-gravitating gas Proceedings of the 12th Marcel Grossmann Meeting 2010 World Scientific Singapore arXiv:1003.1118
    • (2010) Proceedings of the 12th Marcel Grossmann Meeting
    • Sire, C.1    Chavanis, P.H.2
  • 38
    • 79952103798 scopus 로고    scopus 로고
    • P.H. Chavanis, and C. Sire arXiv:1009.2884
    • P.H. Chavanis, and C. Sire arXiv:1009.2884
  • 52
    • 79952106817 scopus 로고    scopus 로고
    • note
    • The usual thermodynamic limit N → + ∞ with N V fixed is not relevant for systems with long-range interactions that are generically spatially inhomogeneous, and it must be reconsidered. If we write the potential of interaction as u (| r - r ′ | ) = k u (| r - r ′ | ) where k is the coupling constant, then the appropriate thermodynamic limit for long-range interactions corresponds to N → + ∞ in such a way that the coupling constant k ∼ 1 N → 0 while the volume of the system remains fixed: V ∼ 1. This is called the Kac prescription [17]. In that limit, we have an extensive scaling of the energy E ∼ N and of the entropy S ∼ N (while the temperature T ∼ 1 is intensive), but the system remains fundamentally non-additive [4].
  • 55
    • 79952106437 scopus 로고    scopus 로고
    • note
    • This shift in density ρ (r ) - ρ ̄ is similar to the one arising in the modified Newtonian model studied in [80].
  • 58
    • 79952107558 scopus 로고    scopus 로고
    • This is not always the case. For example, the free energy associated with the Smoluchowski-Poisson system describing self-gravitating Brownian particles is not bounded from below [48]. In that case, the system can experience an isothermal collapse. However, there also exists long-lived metastable states (local minima of free energy at fixed mass) on which the system can settle [26]
    • This is not always the case. For example, the free energy associated with the SmoluchowskiPoisson system describing self-gravitating Brownian particles is not bounded from below [48]. In that case, the system can experience an isothermal collapse. However, there also exists long-lived metastable states (local minima of free energy at fixed mass) on which the system can settle [26].
  • 65
    • 79952100388 scopus 로고    scopus 로고
    • This is the case, for example, in chemotaxis where the number of particles (bacteria, cells, ...) can be relatively small.
    • This is the case, for example, in chemotaxis where the number of particles (bacteria, cells,...) can be relatively small.
  • 71
    • 79952102433 scopus 로고    scopus 로고
    • Note, however, that changing the initial condition from experiment to experiment may allow to explore a wider diversity of states and reconstruct the density probability (B.1)
    • Note, however, that changing the initial condition from experiment to experiment may allow to explore a wider diversity of states and reconstruct the density probability (B.1).
  • 78
    • 79952105639 scopus 로고    scopus 로고
    • note
    • The non-commutation of the limits t → + ∞ and N → + ∞ that we discuss here is different from the one reported by Latora et al. [81] in relation to quasi stationary states (QSSs). These authors consider isolated Hamiltonian systems with long-range interactions, in the absence of metastable states, and discuss the difference between QSSs (steady states of the Vlasov equation [82]) obtained when the N → + ∞ limit is taken before the t → + ∞ limit and statistical equilibrium states (global entropy maxima) obtained when the t → + ∞ limit is taken before the N → + ∞ limit. Here, we consider overdamped Brownian systems with long-range interactions and discuss the difference between metastable states (local free energy minima) obtained when the N → + ∞ limit is taken before the t → + ∞ limit and strict statistical equilibrium states (global free energy minima) obtained when the t → + ∞ limit is taken before the N → + ∞ limit. A more detailed discussion is provided in Appendix C.
  • 79
    • 79952102511 scopus 로고    scopus 로고
    • note
    • This is particularly true for self-gravitating systems for which there is no global minimum of free energy due to gravitational collapse. Yet, the system can be found in a metastable state (local minimum of free energy) that can persist for a very long time of the order of e N [50]. On longer timescales, the system undergoes gravitational collapse. In that case, it cannot return to a metastable state since the barrier of free energy becomes infinite.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.