Interacting quintessence
We demonstrate that a suitable coupling between a quintessence scalar field and a pressureless cold dark matter (CDM) fluid leads to a constant ratio of the energy densities of both components which is compatible with an accelerated expansion of the Universe. © 2001 Elsevier Science B.V. All rights...
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| Publicado: |
2001
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v521_n3-4_p133_Zimdahl http://hdl.handle.net/20.500.12110/paper_03702693_v521_n3-4_p133_Zimdahl |
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