宇宙中不连接的区域之间的相互信息的时间演变
1Department of Physics, Visva-Bharati University, Santiniketan 731235, India.
Entropy (Basel, Switzerland)
|July 29, 2023
概括
膨胀宇宙中的质量分布之间的相互信息在物质主导的时代随着时间的推移而减少,但在黑暗能量主导的时代保持不变. 这种进化与宇宙膨胀和暗能量动态有关.
科学领域:
- 宇宙学的宇宙学是什么?
- 统计力学 统计力学
- 信息理论 信息理论
背景情况:
- 相互信息量化了空间分离的系统之间的相关性.
- 了解膨胀宇宙中的信息流对于宇宙学来说至关重要.
- 宇宙膨胀和暗能量影响大规模结构的演变.
研究的目的:
- 为了研究一个膨胀的宇宙的因果连接区域中的质量分布之间的相互信息的时间演变.
- 确定控制相互信息动态的关键因素,如配置率和联合.
- 探索相互信息和宇宙加速膨胀之间的关系,特别是在暗能量模型的背景下.
主要方法:
- 对相互信息的时间演变进行分析.
- 计算配置率及其对宇宙膨胀和密度扰动的依赖.
- 检查联合在相互信息动态中的作用.
主要成果:
- 相互信息进化主要由配置率来支配.
- 联合在相互信息的演变中起到微不足道的作用.
- 在物质占主导地位的宇宙中,相互信息减少,而在兰巴达占主导地位的宇宙中则保持不变.
- 兰巴达冷暗物质 (ΛCDM) 模型和其他暗能量模型预测了相互信息的最小值,表明向暗能量主导转变.
结论:
- 这项研究揭示了在物质占主导地位的宇宙和黑暗能量占主导地位的宇宙中相互信息的不同行为.
- 相互信息动态提供了对暗能量和宇宙加速的影响的见解.
- 进一步的研究可能会揭示相互信息,暗能量和宇宙加速膨胀之间的更深层次的联系.
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