Growing classical and quantum entropies in the early universe
Following the idea that the global and local arrow of time has a cosmological origin, we define an entropy in the classical and in the quantum periods of the universe evolution. For the quantum period a semi-classical approach is adopted, modelling the universe with Wheeler-De Witt equation and usin...
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2010
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00207748_v49_n1_p171_Ardenghi http://hdl.handle.net/20.500.12110/paper_00207748_v49_n1_p171_Ardenghi |
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paper:paper_00207748_v49_n1_p171_Ardenghi2023-06-08T14:41:57Z Growing classical and quantum entropies in the early universe Decoherence Entropy Quantum universe Following the idea that the global and local arrow of time has a cosmological origin, we define an entropy in the classical and in the quantum periods of the universe evolution. For the quantum period a semi-classical approach is adopted, modelling the universe with Wheeler-De Witt equation and using WKB. By applying the self-induced decoherence to the state of the universe it is proved that the quantum universe becomes a classical one. This allows us to define a conditional entropy which, in our simplified model, is proportional to e2γt where γ is the dumping factor associated with the interaction potential of the scalar fields. Finally we find both Gibbs and thermodynamical entropy of the universe based in the conditional entropy. © Springer Science+Business Media, LLC 2009. 2010 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00207748_v49_n1_p171_Ardenghi http://hdl.handle.net/20.500.12110/paper_00207748_v49_n1_p171_Ardenghi |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Decoherence Entropy Quantum universe |
spellingShingle |
Decoherence Entropy Quantum universe Growing classical and quantum entropies in the early universe |
topic_facet |
Decoherence Entropy Quantum universe |
description |
Following the idea that the global and local arrow of time has a cosmological origin, we define an entropy in the classical and in the quantum periods of the universe evolution. For the quantum period a semi-classical approach is adopted, modelling the universe with Wheeler-De Witt equation and using WKB. By applying the self-induced decoherence to the state of the universe it is proved that the quantum universe becomes a classical one. This allows us to define a conditional entropy which, in our simplified model, is proportional to e2γt where γ is the dumping factor associated with the interaction potential of the scalar fields. Finally we find both Gibbs and thermodynamical entropy of the universe based in the conditional entropy. © Springer Science+Business Media, LLC 2009. |
title |
Growing classical and quantum entropies in the early universe |
title_short |
Growing classical and quantum entropies in the early universe |
title_full |
Growing classical and quantum entropies in the early universe |
title_fullStr |
Growing classical and quantum entropies in the early universe |
title_full_unstemmed |
Growing classical and quantum entropies in the early universe |
title_sort |
growing classical and quantum entropies in the early universe |
publishDate |
2010 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00207748_v49_n1_p171_Ardenghi http://hdl.handle.net/20.500.12110/paper_00207748_v49_n1_p171_Ardenghi |
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1768545218844426240 |