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From Wikipedia, the free encyclopedia
宇宙學常數問題,或稱真空災變(英語:Vacuum catastrophe),是當今物理學界中待解決的謎團之一,是指理論與觀察之間的一個巨大落差:根據量子場論的推算,真空中的零點能量應該非常龐大,但實際觀測到的真空能量值卻小得多,兩者相差極大。由於真空能量值是計算宇宙學常數的一個關鍵值,若對真空能量的估算出現偏差,整個宇宙模型也會隨之不同。[1]
雖然該能量的理論值依據不同的理論條件(例如普朗克能量上限)而有所變化,但科學家在計算後仍然發現兩者之間的差距高達50到120個數量級。[2][3] 物理學界認為這漾的差異是科學史上理論與實驗最嚴重的不符,[2]甚至有人稱之為「物理學史上最差勁的理論預測」。[4]
Beyond the Standard Model |
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![]() Simulated Large Hadron Collider CMS particle detector data depicting a Higgs boson produced by colliding protons decaying into hadron jets and electrons |
Standard Model |
Evidence |
Theories |
Experiments |
Beyond the Standard Model |
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![]() Simulated Large Hadron Collider CMS particle detector data depicting a Higgs boson produced by colliding protons decaying into hadron jets and electrons |
Standard Model |
Evidence |
Theories |
Experiments |
In cosmology, the cosmological constant problem or vacuum catastrophe is the substantial disagreement between the observed values of vacuum energy density (the small value of the cosmological constant) and the much larger theoretical value of zero-point energy suggested by quantum field theory.
Depending on the Planck energy cutoff and other factors, the quantum vacuum energy contribution to the effective cosmological constant is calculated to be between 50 and as many as 120 orders of magnitude greater than has actually been observed,[1][2] a state of affairs described by physicists as "the largest discrepancy between theory and experiment in all of science"[1] and "the worst theoretical prediction in the history of physics".[3]