Cosmological dark energy from the cosmic QCD phase transition and colour entanglement
Cosmological dark energy from the cosmic QCD phase transition and colour entanglement
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DOI：
10.1016/j.physletb.2005.02.008
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发表时间：
2003-07
影响因子：
4.4
通讯作者：
Shibaji Banerjee;A. Bhattacharyya;S. Ghosh;E. Ilgenfritz;S. Raha;B. Sinha;E. Takasugi;H. Toki
中科院分区：
文献类型：
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作者：
Shibaji Banerjee;A. Bhattacharyya;S. Ghosh;E. Ilgenfritz;S. Raha;B. Sinha;E. Takasugi;H. Toki
最近的天体物理观测表明，宇宙由大量负责加速宇宙膨胀的暗能量(DE)和大量负责结构形成的冷暗物质(CDM)组成。目前，对CDM和DE的起源或性质的解释似乎都需要超出基本粒子相互作用标准模型的想法。在这里，我们第一次证明了CDM和DE完全可以产生于强相互作用物理和量子纠缠的标准原理。在不需要任何可调参数的情况下，获得了与本数据定量一致的结果。
Recent astrophysical observations indicate that the universe is composed of a large amount of dark energy (DE) responsible for an accelerated expansion of the universe, along with a sizeable amount of cold dark matter (CDM), responsible for structure formation. At present, the explanations for the origin or the nature of both CDM and DE seem to require ideas beyond the standard model of elementary particle interactions. Here, for the first time, we show that CDM and DE can arise entirely from the standard principles of strong interaction physics and quantum entanglement. Quantitative agreement with the present data obtains without the need for any adjustable parameters.