我們回顧並討論全像暗能量的觀點，並且研究將全像暗能量放入Brans-Dicke宇宙學的情況，觀察Brans-Dicke耦合常數對全像參數的影響。使用182顆Ia類超新星的觀測資料擬合此模型，我們發現最佳擬合給出的狀態參數會跨過負一，這和標準宇宙學中的全像暗能量行為類似，因此違反弱能條件的要求。

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