Primordial black hole formation during a strongly coupled crossover
Primordial black hole formation during a strongly coupled crossover
复制标题
DOI：
10.1103/physrevd.107.l041301
复制
发表时间：
2022-11
影响因子：
5
通讯作者：
A. Escrivá;Javier G. Subils
中科院分区：
文献类型：
--
作者：
A. Escrivá;Javier G. Subils
原始黑洞的最终质量分布对宇宙状态方程在功率谱所能达到的尺度上是敏感的。出于在几个超越标准模型理论，其中一些是强耦合的相变的存在，我们分析了生产的原始黑洞在这种相变过程中，我们使用规范/引力对偶模型。我们专注于（通常被认为是物理上无趣的）相变只是一个平滑的交叉的情况下。我们发现在[10^{-16}，10 ^{-6}]M_{\odot}$中的$M_{\rm{PBH}}\中，原初黑洞的产生增强。
The final mass distribution of primordial black holes is sensitive to the equation of state of the Universe at the scales accessible by the power spectrum. Motivated by the presence of phase transitions in several beyond the Standard Model theories, some of which are strongly coupled, we analyze the production of primordial black holes during such phase transitions, which we model using the gauge/gravity duality. We focus in the (often regarded as physically uninteresting) case for which the phase transition is just a smooth crossover. We find an enhancement of primordial black hole production in the range $M_{\rm{PBH}}\in[10^{-16},10^{-6}]M_{\odot}$.