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• W3100589330 endingPage "011" @default.
• W3100589330 startingPage "011" @default.
• W3100589330 abstract "We apply a parametric reconstruction method to a homogeneous, isotropic and spatially flat Friedmann-Robertson-Walker (FRW) cosmological model filled of a fluid of dark energy (DE) with constant equation of state (EOS) parameter interacting with dark matter (DM)@. The reconstruction method is based on expansions of the general interaction term and the relevant cosmological variables in terms of Chebyshev polynomials which form a complete set orthonormal functions. This interaction term describes an exchange of energy flow between the DE and DM within dark sector. To show how the method works we do the reconstruction of the interaction function expanding it in terms of only the first six Chebyshev polynomials and obtain the best estimation for the coefficients of the expansion assuming three models: (a) a DE equation of the state parameter w = −1 (an interacting cosmological Λ), (b) a DE equation of the state parameter w = constant with a dark matter density parameter fixed, (c) a DE equation of the state parameter w = constant with a free constant dark matter density parameter to be estimated, and using the Union2 SNe Ia data set from ``The Supernova Cosmology Project'' (SCP) composed by 557 type Ia supernovae. In both cases, the preliminary reconstruction shows that in the best scenario there exist the possibility of a crossing of the noninteracting line Q = 0 in the recent past within the 1σ and 2σ errors from positive values at early times to negative values at late times. This means that, in this reconstruction, there is an energy transfer from DE to DM at early times and an energy transfer from DM to DE at late times. We conclude that this fact is an indication of the possible existence of a crossing behavior in a general interaction coupling between dark components." @default.
• W3100589330 created "2020-11-23" @default.
• W3100589330 creator A5027554396 @default.
• W3100589330 creator A5088088676 @default.
• W3100589330 date "2012-04-12" @default.
• W3100589330 modified "2023-09-25" @default.
• W3100589330 title "Reconstruction of the interaction term between dark matter and dark energy using SNe Ia" @default.
• W3100589330 cites W1500512830 @default.
• W3100589330 cites W1514867752 @default.
• W3100589330 cites W1565645298 @default.
• W3100589330 cites W1650341083 @default.
• W3100589330 cites W1853767801 @default.
• W3100589330 cites W1861505357 @default.
• W3100589330 cites W1964180654 @default.
• W3100589330 cites W1965656673 @default.
• W3100589330 cites W1966378325 @default.
• W3100589330 cites W1967442617 @default.
• W3100589330 cites W1970614242 @default.
• W3100589330 cites W1975029831 @default.
• W3100589330 cites W1975763473 @default.
• W3100589330 cites W1977458260 @default.
• W3100589330 cites W1978249170 @default.
• W3100589330 cites W1978959454 @default.
• W3100589330 cites W1982996481 @default.
• W3100589330 cites W1983622660 @default.
• W3100589330 cites W1986118179 @default.
• W3100589330 cites W1986539017 @default.
• W3100589330 cites W1991952254 @default.
• W3100589330 cites W1993883701 @default.
• W3100589330 cites W1994770854 @default.
• W3100589330 cites W1999908579 @default.
• W3100589330 cites W2001809798 @default.
• W3100589330 cites W2001900257 @default.
• W3100589330 cites W2003686608 @default.
• W3100589330 cites W2004937381 @default.
• W3100589330 cites W2007572894 @default.
• W3100589330 cites W2009904318 @default.
• W3100589330 cites W2016362844 @default.
• W3100589330 cites W2019344527 @default.
• W3100589330 cites W2023875957 @default.
• W3100589330 cites W2026189783 @default.
• W3100589330 cites W2030178578 @default.
• W3100589330 cites W2032284587 @default.
• W3100589330 cites W2032659990 @default.
• W3100589330 cites W2032901690 @default.
• W3100589330 cites W2033219410 @default.
• W3100589330 cites W2033427171 @default.
• W3100589330 cites W2034585440 @default.
• W3100589330 cites W2036121739 @default.
• W3100589330 cites W2038283991 @default.
• W3100589330 cites W2038998752 @default.
• W3100589330 cites W2039439567 @default.
• W3100589330 cites W2039504999 @default.
• W3100589330 cites W2040384286 @default.
• W3100589330 cites W2044206295 @default.
• W3100589330 cites W2045719640 @default.
• W3100589330 cites W2048426097 @default.
• W3100589330 cites W2050573442 @default.
• W3100589330 cites W2051054281 @default.
• W3100589330 cites W2051901943 @default.
• W3100589330 cites W2056173066 @default.
• W3100589330 cites W2057351095 @default.
• W3100589330 cites W2058257480 @default.
• W3100589330 cites W2060566384 @default.
• W3100589330 cites W2061881867 @default.
• W3100589330 cites W2061994992 @default.
• W3100589330 cites W2062105538 @default.
• W3100589330 cites W2065743072 @default.
• W3100589330 cites W2065971829 @default.
• W3100589330 cites W2066510363 @default.
• W3100589330 cites W2067083584 @default.
• W3100589330 cites W2068373320 @default.
• W3100589330 cites W2069855398 @default.
• W3100589330 cites W2071357776 @default.
• W3100589330 cites W2073603601 @default.
• W3100589330 cites W2073832139 @default.
• W3100589330 cites W2075884494 @default.
• W3100589330 cites W2079422567 @default.
• W3100589330 cites W2080206322 @default.
• W3100589330 cites W2082050761 @default.
• W3100589330 cites W2082619498 @default.
• W3100589330 cites W2083330797 @default.
• W3100589330 cites W2084251777 @default.
• W3100589330 cites W2084375583 @default.
• W3100589330 cites W2086436511 @default.
• W3100589330 cites W2086657196 @default.
• W3100589330 cites W2087753835 @default.
• W3100589330 cites W2090235855 @default.
• W3100589330 cites W2093519520 @default.
• W3100589330 cites W2096942305 @default.
• W3100589330 cites W2097549518 @default.
• W3100589330 cites W2099179623 @default.
• W3100589330 cites W2099464295 @default.
• W3100589330 cites W2099827831 @default.
• W3100589330 cites W2103906554 @default.
• W3100589330 cites W2106766431 @default.
• W3100589330 cites W2108905599 @default.
• W3100589330 cites W2110957533 @default.

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