标量张量引力的准palatini公式

IF 5.9 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Sotirios Karamitsos
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引用次数: 0

摘要

帕拉蒂尼公式已经成功地发展了几个可供选择的引力理论。众所周知,帕拉蒂尼公式和度量公式在最小耦合标量张量模型中是等效的,但非最小标量张量模型可能导致物理上不同的理论,这取决于底层的公式。一旦选定了一个模型,所选择的公式就是离散的,因此,将其推广为连续的,预计会产生更广泛的行动。为此,我们提出了“准Palatini”公式,这是一种在给定模型的度量公式和Palatini公式之间进行插值的方法,可以产生连续的模型族。我们将准帕拉蒂尼公式应用于希格斯暴胀、诱导引力暴胀和斯塔宾斯基暴胀,并演示了这如何导致势的变形,并对可观测值产生切实的影响。我们还讨论了如何将不同动作之间的插值扩展到标量-扭转和标量-非度量模型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Quasi-Palatini formulation of scalar-tensor gravity
The Palatini formulation has been successful in the development of several alternative theories of gravity. It is well understood that the Palatini and metric formulations are equivalent in minimally coupled scalar-tensor models, but nonminimal scalar-tensor models can lead to physically distinct theories depending on the underlying formulation. Once a model has been selected, the choice of formulation is a discrete one, and so promoting it to be continuous is expected to give rise to a wider class of actions. To this end, we propose the “quasi-Palatini” formulation, a method for interpolating between the metric and Palatini formulations for a given model that gives rise to a continuous family of models. We apply the quasi-Palatini formulation to Higgs inflation, induced gravity inflation, and Starobinsky inflation, and demonstrate how this leads to a deformation of the potential with a tangible effect on the observables. We also discuss how the interpolation between different actions can be extended to scalar-torsion and scalar-nonmetricity models.
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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