Broad histogram: an overview

The Broad Histogram is a method allowing the direct calculation of the energy degeneracy g(E). This quantity is independent of thermodynamic concepts such as thermal equilibrium. It only depends on the distribution of allowed (micro) states along the energy axis, but not on the energy changes between the system and its environment. Once one has obtained g(E), no further effort is needed in order to consider different environment conditions, for instance, different temperatures, for the same system. The method is based on the exact relation between g(E) and the microcanonical averages of certain macroscopic quantities Nup and Ndn . For an application to a particular problem, one needs to choose an adequate instrument in order to determine the averages < Nup (E) > and < Ndn(E) >, as functions of energy. Replacing the usual fixed-temperature canonical by the fixed-energy microcanonical ensemble, new subtle concepts emerge. The temperature, for instance, is no longer an external parameter controlled by the user. Instead, the microcanonical temperature Tm(E) is a function of energy defined from g(E) itself, being thus an internal (environment independent) characteristic of the system. Accordingly, all microcanonical averages are functions of E. The present text is an overview of the method. Some features of the microcanonical ensemble are also discussed, as well as some clues towards the deffinition of efficient Monte Carlo microcanonical sampling rules.

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Main Author: Oliveira,Paulo Murilo Castro de
Format: Digital revista
Language:English
Published: Sociedade Brasileira de Física 2000
Online Access:http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332000000100022
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spelling oai:scielo:S0103-973320000001000222001-10-17Broad histogram: an overviewOliveira,Paulo Murilo Castro deThe Broad Histogram is a method allowing the direct calculation of the energy degeneracy g(E). This quantity is independent of thermodynamic concepts such as thermal equilibrium. It only depends on the distribution of allowed (micro) states along the energy axis, but not on the energy changes between the system and its environment. Once one has obtained g(E), no further effort is needed in order to consider different environment conditions, for instance, different temperatures, for the same system. The method is based on the exact relation between g(E) and the microcanonical averages of certain macroscopic quantities Nup and Ndn . For an application to a particular problem, one needs to choose an adequate instrument in order to determine the averages < Nup (E) > and < Ndn(E) >, as functions of energy. Replacing the usual fixed-temperature canonical by the fixed-energy microcanonical ensemble, new subtle concepts emerge. The temperature, for instance, is no longer an external parameter controlled by the user. Instead, the microcanonical temperature Tm(E) is a function of energy defined from g(E) itself, being thus an internal (environment independent) characteristic of the system. Accordingly, all microcanonical averages are functions of E. The present text is an overview of the method. Some features of the microcanonical ensemble are also discussed, as well as some clues towards the deffinition of efficient Monte Carlo microcanonical sampling rules.info:eu-repo/semantics/openAccessSociedade Brasileira de FísicaBrazilian Journal of Physics v.30 n.1 20002000-03-01info:eu-repo/semantics/articletext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332000000100022en10.1590/S0103-97332000000100022
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libraryname SciELO
language English
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author Oliveira,Paulo Murilo Castro de
spellingShingle Oliveira,Paulo Murilo Castro de
Broad histogram: an overview
author_facet Oliveira,Paulo Murilo Castro de
author_sort Oliveira,Paulo Murilo Castro de
title Broad histogram: an overview
title_short Broad histogram: an overview
title_full Broad histogram: an overview
title_fullStr Broad histogram: an overview
title_full_unstemmed Broad histogram: an overview
title_sort broad histogram: an overview
description The Broad Histogram is a method allowing the direct calculation of the energy degeneracy g(E). This quantity is independent of thermodynamic concepts such as thermal equilibrium. It only depends on the distribution of allowed (micro) states along the energy axis, but not on the energy changes between the system and its environment. Once one has obtained g(E), no further effort is needed in order to consider different environment conditions, for instance, different temperatures, for the same system. The method is based on the exact relation between g(E) and the microcanonical averages of certain macroscopic quantities Nup and Ndn . For an application to a particular problem, one needs to choose an adequate instrument in order to determine the averages < Nup (E) > and < Ndn(E) >, as functions of energy. Replacing the usual fixed-temperature canonical by the fixed-energy microcanonical ensemble, new subtle concepts emerge. The temperature, for instance, is no longer an external parameter controlled by the user. Instead, the microcanonical temperature Tm(E) is a function of energy defined from g(E) itself, being thus an internal (environment independent) characteristic of the system. Accordingly, all microcanonical averages are functions of E. The present text is an overview of the method. Some features of the microcanonical ensemble are also discussed, as well as some clues towards the deffinition of efficient Monte Carlo microcanonical sampling rules.
publisher Sociedade Brasileira de Física
publishDate 2000
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332000000100022
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