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Updated: Jan 18, 2026

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通过将物质转化为暗能量的DESI DR2正中微子质量
S P Ahlen1, A Aviles2,3, B Cartwright4
1Department of Physics, Boston University, 590 Commonwealth Avenue, Boston, Massachusetts 02215, USA.
暗能量光谱仪器 (DESI) 结合了数据来测试一个模型,其中物质通过黑洞转化为暗能量. 这个模型与宇宙膨胀保持一致,并减少中微子质量张力.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 暗能量光谱仪器 (DESI) 提供了广泛的银河系外目标测量.
- 巴里昂声波振荡 (BAO) 是重要的宇宙学探测器.
研究的目的:
- 研究一种新的暗能量 (DE) 模型,涉及物质转化为宇宙学合黑洞 (CCBHs).
- 测试这个CCBH模型是否与DESI BAO数据和宇宙微波背景 (CMB) 数据集一致.
主要方法:
- 将DESI数据发布2与CMB数据集结合起来.
- 分析一个物理模型,其中DE产量与宇宙恒星形成率密度 (SFRD) 有关.
- 将模型预测与早期大爆炸核合成 (BBN) 和局部距离梯度测量进行比较.
主要成果:
- CCBH模型准确地重现了宇宙膨胀历史.
- 该模型显示与BBN baryons丰富度一致,并减轻了哈勃张力.
- 总中微子质量 (mν) 的约束放松,产生与中微子振荡实验一致的值.
结论:
- CCBH模型为标准的 ΛCDM 模型提供了一个可行的替代方案.
- 在CCBH场景中,晚期子消耗自然会导致正中微子质量.
- 这项研究突出了宇宙学模型中物质转化为暗能量转化的潜力.
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