A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe
We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1982 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
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| Übergeordnetes Werk: |
in: Chinese Astronomy and Astrophysics - Amsterdam : Elsevier, 6(1982), 3, Seite 243-247 |
| Übergeordnetes Werk: |
volume:6 ; year:1982 ; number:3 ; pages:243-247 |
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| 520 | |a We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. | ||
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(DE-627)NLEJ180314505 (DE-599)GBVNLZ180314505 DE-627 ger DE-627 rakwb eng A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe 1982 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Guo Han-ying oth Zou Zhen-long oth in Chinese Astronomy and Astrophysics Amsterdam : Elsevier 6(1982), 3, Seite 243-247 (DE-627)NLEJ180305603 (DE-600)2020472-3 0275-1062 nnns volume:6 year:1982 number:3 pages:243-247 http://linkinghub.elsevier.com/retrieve/pii/0275-1062(82)90031-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 6 1982 3 243-247 |
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(DE-627)NLEJ180314505 (DE-599)GBVNLZ180314505 DE-627 ger DE-627 rakwb eng A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe 1982 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Guo Han-ying oth Zou Zhen-long oth in Chinese Astronomy and Astrophysics Amsterdam : Elsevier 6(1982), 3, Seite 243-247 (DE-627)NLEJ180305603 (DE-600)2020472-3 0275-1062 nnns volume:6 year:1982 number:3 pages:243-247 http://linkinghub.elsevier.com/retrieve/pii/0275-1062(82)90031-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 6 1982 3 243-247 |
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(DE-627)NLEJ180314505 (DE-599)GBVNLZ180314505 DE-627 ger DE-627 rakwb eng A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe 1982 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Guo Han-ying oth Zou Zhen-long oth in Chinese Astronomy and Astrophysics Amsterdam : Elsevier 6(1982), 3, Seite 243-247 (DE-627)NLEJ180305603 (DE-600)2020472-3 0275-1062 nnns volume:6 year:1982 number:3 pages:243-247 http://linkinghub.elsevier.com/retrieve/pii/0275-1062(82)90031-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 6 1982 3 243-247 |
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(DE-627)NLEJ180314505 (DE-599)GBVNLZ180314505 DE-627 ger DE-627 rakwb eng A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe 1982 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Guo Han-ying oth Zou Zhen-long oth in Chinese Astronomy and Astrophysics Amsterdam : Elsevier 6(1982), 3, Seite 243-247 (DE-627)NLEJ180305603 (DE-600)2020472-3 0275-1062 nnns volume:6 year:1982 number:3 pages:243-247 http://linkinghub.elsevier.com/retrieve/pii/0275-1062(82)90031-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 6 1982 3 243-247 |
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(DE-627)NLEJ180314505 (DE-599)GBVNLZ180314505 DE-627 ger DE-627 rakwb eng A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe 1982 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Guo Han-ying oth Zou Zhen-long oth in Chinese Astronomy and Astrophysics Amsterdam : Elsevier 6(1982), 3, Seite 243-247 (DE-627)NLEJ180305603 (DE-600)2020472-3 0275-1062 nnns volume:6 year:1982 number:3 pages:243-247 http://linkinghub.elsevier.com/retrieve/pii/0275-1062(82)90031-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 6 1982 3 243-247 |
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in Chinese Astronomy and Astrophysics 6(1982), 3, Seite 243-247 volume:6 year:1982 number:3 pages:243-247 |
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A finite temperature λφ^4 model and A De Sitter - Friedmann transition in the early universe |
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We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. |
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We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. |
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We have analysed the finite temperature λφ^4 model in the Robertson Walker metric, taking into consideration spontaneous symmetry breaking, particle production and symmetry recovery through phase transition under a high temperature, and found that it is possible to have a cosmological model free of singularities. Such a model begins in the singularity-free, horizon-free, Beltrami-Anti-de Sitter state. Continual production of particles keeps on raising its temperature until a critical temperature T"C is reached, when a phase change takes place, and the universe is transformed into a radiation-dominated, thermally-expanding Friedmann state. This phase transition corresponds to a big-bang without, however, an antecedent singularity. |
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