Registro completo de metadatos
Campo DC | Valor | Lengua/Idioma |
---|---|---|
dc.creator | Chimento, Luis Pascual | - |
dc.creator | Forte, Mónica | - |
dc.creator | Richarte, Martín Gustavo | - |
dc.date | 2017-06-12T19:55:06Z | - |
dc.date | 2017-06-12T19:55:06Z | - |
dc.date | 2013-01 | - |
dc.date | 2017-06-09T14:15:14Z | - |
dc.date.accessioned | 2019-04-29T15:42:06Z | - |
dc.date.available | 2019-04-29T15:42:06Z | - |
dc.date.issued | 2013-01 | - |
dc.identifier | Chimento, Luis Pascual; Forte, Mónica; Richarte, Martín Gustavo; Self-interacting holographic dark energy; World Scientific; Modern Physics Letters A: Particles And Fields; Gravitation; Cosmology And Nuclear Physics; 28; 1; 1-2013; 1-16; 1250235 | - |
dc.identifier | 0217-7323 | - |
dc.identifier | http://hdl.handle.net/11336/18007 | - |
dc.identifier | 1793-6632 | - |
dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/299909 | - |
dc.description | We investigate a spatially flat Friedmann–Robertson–Walker (FRW) universe where dark matter exchanges energy with a self-interacting holographic dark energy (SIHDE). Using the χ 2 -statistical method on the Hubble function, we obtain a critical redshift that seems to be consistent with both BAO and CMB data. We calculate the theoretical distance modulus for confronting with the observational data of SNe Ia for small redshift z ≤ 0.1 and large redshift 0.1 ≤ z ≤ 1.5. The model gets accelerated faster than the ΛCDM one and it can be a good candidate to alleviate the coincidence problem. We also examine the age crisis at high redshift associated with the old quasar APM 08279+5255. | - |
dc.description | Fil: Chimento, Luis Pascual. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina | - |
dc.description | Fil: Forte, Mónica. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina | - |
dc.description | Fil: Richarte, Martín Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina | - |
dc.format | application/pdf | - |
dc.format | application/pdf | - |
dc.language | eng | - |
dc.publisher | World Scientific | - |
dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1142/S0217732312502355 | - |
dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0217732312502355 | - |
dc.rights | info:eu-repo/semantics/restrictedAccess | - |
dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
dc.source | reponame:CONICET Digital (CONICET) | - |
dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
dc.source | instacron:CONICET | - |
dc.source.uri | http://hdl.handle.net/11336/49100 | - |
dc.subject | INTERACTING DARK SECTOR | - |
dc.subject | HOLOGRAPHIC DARK ENERGY | - |
dc.subject | OLD QUASAR | - |
dc.subject | Otras Ciencias Físicas | - |
dc.subject | Ciencias Físicas | - |
dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
dc.title | Self-interacting holographic dark energy | - |
dc.type | info:eu-repo/semantics/article | - |
dc.type | info:eu-repo/semantics/publishedVersion | - |
dc.type | info:ar-repo/semantics/articulo | - |
Aparece en las colecciones: | CONICET |
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