基于爱因斯坦-高斯-庞内引力的宇宙学模型中的残余引力波

IF 0.4 4区物理与天体物理 Q4 PHYSICS, NUCLEAR

Physics of Atomic Nuclei Pub Date : 2025-10-09 DOI:10.1134/S1063778825600939

G. D. Manucharyan, I. V. Fomin, V. O. Gladyshev, V. L. Kauts

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引用次数: 0

摘要

考虑了宇宙动力学方程的一类特殊解，这类解暗示了广义相对论框架下暴胀模型与爱因斯坦-高斯-邦纳引力之间的解析联系。分析了通过直接观测遗迹引力波来验证该模型的可能性，这些遗迹引力波的频谱由模型参数决定。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Relic Gravitational Waves in Cosmological Models Based on Einstein–Gauss–Bonnet Gravity

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Relic Gravitational Waves in Cosmological Models Based on Einstein–Gauss–Bonnet Gravity

A special class of solutions of the equations of cosmological dynamics implying analytic connection between inflationary models in the framework of general relativity and Einstein–Gauss–Bonnet gravity is considered. The possibility of verification of such models by direct observation of relic gravitational waves, the spectrum of which is determined by the parameters of the model was analyzed.

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来源期刊

Physics of Atomic Nuclei 物理-物理：核物理

CiteScore

0.60

自引率

25.00%

发文量

审稿时长

3-6 weeks

期刊介绍： Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.