从 NANOGrav 15 年数据中重建通胀潜能:使用非邦奇-戴维斯初始条件的稳健研究

IF 10.2 4区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Journal of High Energy Astrophysics Pub Date : 2024-10-09 DOI:10.1016/j.jheap.2024.10.003
Sayantan Choudhury
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引用次数: 0

摘要

我们讨论了以一种与模型无关的方式重构典型单场慢滚暴胀的一般类暴胀势背后的理论框架。非邦奇戴维斯(NBD)初始条件是确定势的结构和适应最近在 NANOGrav 中观测到的蓝色倾斜张量功率谱特征的重要选择。利用重构技术,我们找到了支持蓝色倾斜张量功率谱的有利参数空间。通过使用新的场偏移公式,我们还保持了膨胀中 EFT 方程的有效性,同时还检查了亚普朗克场值的必要条件和充分条件。我们发现重建的势显示出拐点行为,这与高能物理有更深的联系。
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Reconstructing inflationary potential from NANOGrav 15-year data: A robust study using Non-Bunch Davies initial condition
We discuss the theoretical framework behind reconstruction of a generic class of inflationary potentials for canonical single-field slow-roll inflation in a model-independent fashion. The Non-Bunch Davies (NBD) initial condition is an essential choice to determine the structure of potential and to accommodate the blue-tilted tensor power spectrum feature recently observed in NANOGrav. Using the reconstruction technique we found the favoured parameter space which supports blue tilted tensor power spectrum. The validity of the EFT prescription in inflation is also maintained through the use of a new field excursion formula while keeping the necessary and sufficient conditions on the sub-Planckian field values in check. We find that the reconstructed potential display inflection point behaviour, which has deeper connection with high energy physics.
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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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