We present the constraints on the Massive Graviton Dark Matter scenario (MGCDM) using the cosmological observations, including type Ia supernovae (SNe Ia), Gamma Ray Bursts (GRB), Observational Hubble Parameter Data (OHD), Cosmic Microwave Background shift parameter, and the Radial Baryon Acoustic Oscillation. In order to compare the goodness of the data samples and their combinations, we adopt the Fisher matrix analysis and the figure of merit (FoM) diagnostic. Based on the constraint results, we further discuss the cosmic age problem in MGCDM. The calculation shows that the universe in MGCDM frame is older than that in standard Lambda CDM model, but the cosmic age crisis is still unresolved with just an alleviation.
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Nanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Peoples R ChinaNanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Zhang, Cun
Cui, Ming-Yang
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Nanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Peoples R ChinaNanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Cui, Ming-Yang
Feng, Lei
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Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Peoples R ChinaNanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Feng, Lei
Fan, Yi-Zhong
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Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Peoples R ChinaNanjing Univ, Sch Phys, Nanjing 210092, Peoples R China
Fan, Yi-Zhong
Ren, Zhong-Zhou
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Nanjing Univ, Sch Phys, Nanjing 210092, Peoples R ChinaNanjing Univ, Sch Phys, Nanjing 210092, Peoples R China