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SCIENCE CHINA Physics, Mechanics & Astronomy, Volume 61 , Issue 3 : 030011(2018) https://doi.org/10.1007/s11433-017-9131-9

Probing the sign-changeable interaction between dark energy and dark matter with current observations

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  • ReceivedOct 14, 2017
  • AcceptedNov 6, 2017
  • PublishedJan 11, 2018
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Abstract


Acknowledgment

This work was supported by the National Natural Science Foundation of China (Grant Nos. 11522540, and 11690021), the National Program for Support of Top-Notch Young Professionals, and the Provincial Department of Education of Liaoning (Grant No. L2012087).


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  • Figure 1

    (Color online) The 1$\sigma$ and 2$\sigma$ confidence level contours in the $b_0$-$b_\text{e}$ plane, for the six I$\Lambda$CDM models, by using CMB+BAO+SN+$H_{0}$. (a)$\Lambda$CDM1; (b) $\Lambda$CDM2; (c) $\Lambda$CDM3; (d) $\Lambda$CDM4; (e) $\Lambda$CDM5; (f) $\Lambda$CDM6.

  • Figure 2

    (Color online) The 1$\sigma$ and 2$\sigma$ confidence level contours in the $\Omega_m$-$h$ plane, for the six I$\Lambda$CDM models, by using CMB+BAO+SN+$H_{0}$. (a)$\Lambda$CDM1; (b) $\Lambda$CDM2; (c) $\Lambda$CDM3; (d) $\Lambda$CDM4; (e) $\Lambda$CDM5; (f) $\Lambda$CDM6.

  • Figure 3

    (Color online) The reconstructed evolutionary histories for $b(z)$ in the six I$\Lambda$CDM models. The black solid line represents the 1$\sigma$ uncertainties. The blue dashed line in each plot denotes the noniteracting line. (a) $\Lambda$CDM1; (b) $\Lambda$CDM2; (c) $\Lambda$CDM3; (d) $\Lambda$CDM4; (e) $\Lambda$CDM5; (f) $\Lambda$CDM6.

  • Table 1   Fitting results of the parameters with best-fit values as well as 1$\sigma$ errors in all the I$\Lambda$CDM models
    Parameter I$\Lambda$CDM1 I$\Lambda$CDM2 I$\Lambda$CDM3 I$\Lambda$CDM4 I$\Lambda$CDM5 I$\Lambda$CDM6
    $\Omega_{\rm~m}$ $0.3152^{+0.0085}_{-0.0091}$ $0.3150^{+0.0092}_{-0.0089}$ $0.3140^{+0.0089}_{-0.0060}$ $0.3143^{+0.0088}_{-0.0092}$ $0.3164^{+0.0074}_{-0.0103}$ $0.3137^{+0.0100}_{-0.0080}$
    $b_0$ $-0.3295^{+0.3518}_{-0.2599}$ $-0.4148^{+0.4517}_{-0.3603}$ $-0.5296^{+0.3429}_{-0.3467}$ $-0.2922^{+0.2725}_{-0.1957}$ $-0.3115^{+0.3036}_{-0.3980}$ $-0.4012^{+0.3944}_{-0.2795}$
    $b_\text{e}$ $1.4079^{+1.0358}_{-1.4708}$ $1.8372^{+1.6063}_{-1.9337}$ $0.8647^{+0.5487}_{-0.5485}$ $0.9848^{+0.6698}_{-0.9005}$ $1.1329^{+1.5331}_{-1.0766}$ $1.4669^{+1.0740}_{-1.4104}$
    $h$ $0.6798^{+0.0107}_{-0.0119}$ $0.6788^{+0.0104}_{-0.0110}$ $0.7016^{+0.0224}_{-0.0235}$ $0.6843^{+0.0123}_{-0.0150}$ $0.6786^{+0.0136}_{-0.0098}$ $0.6822^{+0.0097}_{-0.0130}$
    $\chi^2_{\rm~min}$ $698.35$ $698.31$ $697.35$ $698.09$ $698.17$ $698.19$
qqqq

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