来自 LHAASO 源的中微子的冰立方结果和展望

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Journal of High Energy Astrophysics Pub Date : 2024-07-02 DOI:10.1016/j.jheap.2024.07.001
Ke Fang, Francis Halzen
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引用次数: 0

摘要

我们简要回顾了冰立方中微子天文台在发现宇宙中微子十年后取得的主要成果。我们强调了多信使观测的重要性,其中最突出的是发现了来自我们银河系的中微子。我们模拟了银河宇宙射线与星际介质相互作用产生的银河面通量,并讨论了通过结合中微子和伽马射线观测来理解银河面 TeV-PeV 辐射的前景。我们提请注意一个有趣的事实,即来自银河系的中微子通量并不是中微子天空的主要特征,这与任何其他波长的光不同。最后,我们回顾了通过面对银河源的中微子和伽马射线发射(包括LHAASO观测到的那些)来识别PeVatrons的尝试。最后,我们讨论了从 LHAASO 的银河系外瞬态源伽马射线暴 221009A 中搜索中微子的问题。
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IceCube results and perspective for neutrinos from LHAASO sources

We briefly review the main results of the IceCube Neutrino Observatory one decade after the discovery of cosmic neutrinos. We emphasize the importance of multimessenger observations, most prominently for the discovery of neutrinos from our own Galaxy. We model the flux from the Galactic plane produced by Galactic cosmic rays interacting with the interstellar medium and discuss the perspectives of understanding the TeV-PeV emission of the Galactic plane by combining neutrino and gamma-ray observations. We draw attention to the interesting fact that the neutrino flux from the Galaxy is not a dominant feature of the neutrino sky, unlike the case in any other wavelength of light. Finally, we review the attempts to identify PeVatrons by confronting the neutrino and gamma-ray emission of Galactic sources, including those observed by LHAASO. We end with a discussion of searches for neutrinos from LHAASO's extragalactic transient source gamma-ray burst 221009A.

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来源期刊
Journal of High Energy Astrophysics
Journal of High Energy Astrophysics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
9.70
自引率
5.30%
发文量
38
审稿时长
65 days
期刊介绍: The journal welcomes manuscripts on theoretical models, simulations, and observations of highly energetic astrophysical objects both in our Galaxy and beyond. Among those, black holes at all scales, neutron stars, pulsars and their nebula, binaries, novae and supernovae, their remnants, active galaxies, and clusters are just a few examples. The journal will consider research across the whole electromagnetic spectrum, as well as research using various messengers, such as gravitational waves or neutrinos. Effects of high-energy phenomena on cosmology and star-formation, results from dedicated surveys expanding the knowledge of extreme environments, and astrophysical implications of dark matter are also welcomed topics.
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