Gravitating solitons and black holes with synchronised hair in the four dimensional O(3) sigma-model
We consider the O(3) non-linear sigma-model, composed of three real scalar fields with a standard kinetic term and with a symmetry breaking potential in four space-time dimensions. We show that this simple, geometrically motivated model, admits both self-gravitating, asymptotically flat, non-topolog...
| Autor principal: | |
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| Outros Autores: | , , |
| Formato: | article |
| Idioma: | eng |
| Publicado em: |
2019
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| Assuntos: | |
| Texto completo: | http://hdl.handle.net/10773/26023 |
| País: | Portugal |
| Oai: | oai:ria.ua.pt:10773/26023 |