具有韦利边界的宇宙中宇宙演化的大爆炸核合成约束

IF 4.8 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Teodora M. Matei, Cristian A. Croitoru, Tiberiu Harko
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引用次数: 0

摘要

我们研究了在大爆炸核合成(BBN)框架中爱因斯坦引力场方程中包含边界项所产生的影响。特别地,我们考虑了宇宙边界用Weyl型几何来描述的可能性。利用在FLRW度规下得到的具有Weylian边界的宇宙的广义Friedmann方程,可以构造三个不同的宇宙模型。宇宙演化由耗散标量场和来自边界的Weyl向量决定。通过对广义能量守恒方程进行适当的拆分,得到了几种宇宙学情景。在本工作中,我们利用BBN数据获得了这些模型的相关约束。特别是,对后热暴胀时代出现的BBN的影响将通过理论评估残余核(氢、氘、氦-3、氦-4和锂-7)的测量丰度来检验。我们首先考虑原始质量分数估计值,以及它们由于冻结温度变化而产生的偏差,这些偏差对由修正的弗里德曼方程得到的有效能量密度施加了上限。因此,辐射等离子体与标准能量密度的偏差受到氦-4原子核丰度的限制。其次,通过使用PRyMordial软件包进行数值分析,我们将考虑上限,借助该软件包,我们通过在考虑的修正重力框架内评估热核率来计算轻元素的原始丰度。最后,MCMC分析将验证具有韦利边界贡献的宇宙学模型,并对宇宙的初始条件施加相关约束。该方法在python代码genesys中实现,该代码可在GitHub上获得。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Big Bang Nucleosynthesis constraints on the cosmological evolution in a Universe with a Weylian boundary

We investigate the effects that arise from the inclusion of boundary terms in the Einstein gravitational field equations in the Big Bang Nucleosynthesis (BBN) framework. In particular, we consider the possibility that the boundary of the Universe is described by a Weyl type geometry. With the help of the generalized Friedmann equations for a Universe with a Weylian boundary, obtained for a Friedmann–Lemaitre–Robertson–Walker FLRW metric, three distinct cosmological models can be constructed. The cosmological evolution is determined by a dissipative scalar field, and by the Weyl vector coming from the boundary. Several cosmological scenarios are obtained via the appropriate splitting of the generalized energy conservation equation. In the present work we obtain relevant constraints on these models by using the BBN data. In particular, the effects on the BBN that arise in the post warm-inflationary era will be examined by theoretically evaluating the measured abundances of relic nuclei (Hydrogen, Deuterium, Helium-3, Helium-4, and Lithium-7). We consider firstly the primordial mass fraction estimates, and their deviations due to changes in the freezing temperature, which impose an upper limit on the effective energy density obtained from the modified Friedmann equations. The deviation from the standard energy density of the radiative plasma is therefore constrained by the abundances of the Helium-4 nuclei. Secondly, an upper limit will be considered in a numerical analysis performed through the usage of the PRyMordial software package, with the help of which we calculate the primordial abundances of the light elements by evaluating the thermonuclear rates within the considered modified gravity framework. Finally, an MCMC analysis will validate the cosmological model with Weylian boundary contributions, imposing relevant constraints on the initial conditions of the cosmos. The methodology is implemented in the python code genesys, which is available on GitHub.

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来源期刊
The European Physical Journal C
The European Physical Journal C 物理-物理:粒子与场物理
CiteScore
8.10
自引率
15.90%
发文量
1008
审稿时长
2-4 weeks
期刊介绍: Experimental Physics I: Accelerator Based High-Energy Physics Hadron and lepton collider physics Lepton-nucleon scattering High-energy nuclear reactions Standard model precision tests Search for new physics beyond the standard model Heavy flavour physics Neutrino properties Particle detector developments Computational methods and analysis tools Experimental Physics II: Astroparticle Physics Dark matter searches High-energy cosmic rays Double beta decay Long baseline neutrino experiments Neutrino astronomy Axions and other weakly interacting light particles Gravitational waves and observational cosmology Particle detector developments Computational methods and analysis tools Theoretical Physics I: Phenomenology of the Standard Model and Beyond Electroweak interactions Quantum chromo dynamics Heavy quark physics and quark flavour mixing Neutrino physics Phenomenology of astro- and cosmoparticle physics Meson spectroscopy and non-perturbative QCD Low-energy effective field theories Lattice field theory High temperature QCD and heavy ion physics Phenomenology of supersymmetric extensions of the SM Phenomenology of non-supersymmetric extensions of the SM Model building and alternative models of electroweak symmetry breaking Flavour physics beyond the SM Computational algorithms and tools...etc.
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