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The quark-hadron transition and hot hadronic matter in the early universe

Includes bibliographical references.

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Bibliographic Details
Main Author: Von Oertzen, Detlof Wilhelm
Other Authors: Rafelski, Johann
Format: Thesis
Language:English
Published: Department of Physics 2015
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access_status_str Open Access
author Von Oertzen, Detlof Wilhelm
author2 Rafelski, Johann
author_browse Rafelski, Johann
Von Oertzen, Detlof Wilhelm
author_facet Rafelski, Johann
Von Oertzen, Detlof Wilhelm
author_sort Von Oertzen, Detlof Wilhelm
collection Thesis
description Includes bibliographical references.
format Thesis
id oai:open.uct.ac.za:11427/15904
institution University of Cape Town (South Africa)
language eng
last_indexed 2026-06-10T12:34:10.861Z
license_str Not specified — see source repository
provenance_str_mv Harvested via OAI-PMH from UCTD — University of Cape Town Open Access Repository
publishDate 2015
publishDateRange 2015
publishDateSort 2015
publisher Department of Physics
publisherStr Department of Physics
record_format dspace
source_str UCTD — University of Cape Town Open Access Repository
spelling oai:open.uct.ac.za:11427/15904 The quark-hadron transition and hot hadronic matter in the early universe Von Oertzen, Detlof Wilhelm Rafelski, Johann Cleymans, Jean Quarks Hadrons Nuclear astrophysics Theoretical Physics Includes bibliographical references. Various calculations· of the evolution of the hadron gas in the early universe are carried out. To determine the starting point for the evolution equations a phase transition between the quark-gluon plasma phase and the hadron gas phase is constructed. A simple calculation leads to an estimate of the chemical potential of baryons at the quark-hadron phase transition in the early universe. We investigate how the transition temperature depends on the equations of state for the bagged quark and the hadron phase. A particle density evolution model is introduced which predicts the temperature at which particle species drop out of equilibrium (freeze-out) in an expanding universe. We then construct dynamical evolution equations to describe the reactions of interacting pions and photons. In order to model a more realistic hadron gas, we include kaons and finally nucleons and hyperons into the model universe. The results indicate that this type of model should be extended to include more interacting particle species and that a more realistic evolution model is dependent on obtaining accurate reaction cross-sections. 2015-12-20T15:43:50Z 2015-12-20T15:43:50Z 1987 Master Thesis Masters MSc http://hdl.handle.net/11427/15904 eng application/pdf Department of Physics Faculty of Science University of Cape Town
spellingShingle Quarks
Hadrons
Nuclear astrophysics
Theoretical Physics
Von Oertzen, Detlof Wilhelm
The quark-hadron transition and hot hadronic matter in the early universe
thesis_degree_str Master's
title The quark-hadron transition and hot hadronic matter in the early universe
title_full The quark-hadron transition and hot hadronic matter in the early universe
title_fullStr The quark-hadron transition and hot hadronic matter in the early universe
title_full_unstemmed The quark-hadron transition and hot hadronic matter in the early universe
title_short The quark-hadron transition and hot hadronic matter in the early universe
title_sort quark hadron transition and hot hadronic matter in the early universe
topic Quarks
Hadrons
Nuclear astrophysics
Theoretical Physics
url http://hdl.handle.net/11427/15904
work_keys_str_mv AT vonoertzendetlofwilhelm thequarkhadrontransitionandhothadronicmatterintheearlyuniverse
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