On inflation and variation of the strong coupling constant
Variation of constants in the very early universe can generate inflation. We consider a scenario where the strong coupling constant was changing in time and where the gluon condensate underwent a phase transition ending the inflation. © World Scientific Publishing Company.
| Autores: | , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2007 |
| País: | Argentina |
| Recursos: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/67769 |
| Acesso em linha: | http://hdl.handle.net/11336/67769 |
| Access Level: | acceso abierto |
| Palavra-chave: | Inflation Qcd Variation of Constants https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Resumo: | Variation of constants in the very early universe can generate inflation. We consider a scenario where the strong coupling constant was changing in time and where the gluon condensate underwent a phase transition ending the inflation. © World Scientific Publishing Company. |
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