充分获取超新星轴子信息
高能物理 - 唯象学
2024-01-04 v2 高能天体物理现象
摘要
与核子耦合的类轴子粒子(ALPs)可能从超新星(SN)核心大量发射。我们将既有的自由流ALPs限制扩展到这些ALPs与核物质强相互作用而被囚禁于SN核心的情形。对于强相互作用ALPs，我们还扩展了基于SN 1987A时刻Kamiokande-II中微子探测器中无ALP诱导信号的约束。我们发现综合不同论证，SNe排除了ALP—核子耦合(对应ALP质量)的取值。值得注意的是，对于标准QCD轴子模型，SN约束排除了所有的取值。该结果排除了当前与未来宇宙学巡天探测由热暗物质QCD轴子质量所致任何信号的可能性。
引用
@article{arxiv.2306.01048,
title = {Getting the most on supernova axions},
author = {Alessandro Lella and Pierluca Carenza and Giampaolo Co' and Giuseppe Lucente and Maurizio Giannotti and Alessandro Mirizzi and Thomas Rauscher},
journal= {arXiv preprint arXiv:2306.01048},
year = {2024}
}
备注
15 pages, 7 figures. Matches the version published on PRD. Changes: we employed a different benchmark SN model with respect to the previous version, accounting for a 1D treatment of convection. We added a new section to discuss the uncertainties on the SN bounds. We added an additional section to analyze SN bounds on canonical QCD axion models