Re-parameterization invariance of FRW model: Supervariable and BRST approaches

IF 2.8 3区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS Nuclear Physics B Pub Date : 2025-02-03 DOI:10.1016/j.nuclphysb.2025.116816
B. Chauhan, R. Tripathi
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Abstract

We perform the Becchi-Rouet-Stora-Tyutin (BRST) quantization of a (0+1)-dimensional cosmological Friedmann-Robertson-Walker (FRW) model. This quantization leverages the classical infinitesimal and continuous re-parameterization symmetry transformations of the system. To derive the nilpotent re-parameterization invariant BRST-anti-BRST symmetry transformations for the scale factor and corresponding momentum variables present in the cosmological FRW model, we employ the modified Bonora-Tonin supervariable approach (MBTSA) to BRST formalism. Through this approach, we also establish the BRST-anti-BRST invariant Curci-Ferrari (CF)-type restriction for this cosmological re-parameterization invariant model. Further, we obtain the off-shell nilpotent quantum BRST-anti-BRST symmetry transformations for other variables within the model using the (anti-)chiral supervariable approach (ACSA) to BRST formalism. Within the framework of ACSA, the CF-type restriction is demonstrated through two key aspects: (i) the invariance of the coupled Lagrangians under symmetry transformations, and (ii) the absolute anti-commutativity of the conserved BRST-anti-BRST charges. Notably, applying the MBTSA to a physical cosmological system, specifically a one-dimensional one, constitutes a novel contribution to this work. Additionally, in the application of ACSA, we restrict our analysis to (anti-)chiral super expansions of supervariables, leading to the unique observation of the absolute anti-commutativity of the conserved BRST-anti-BRST charges. Moreover, we highlight that the CF-type restriction demonstrates a universal nature, remaining consistent across any re-parameterization invariant models in general D-dimensional spacetime.
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FRW模型的再参数化不变性:超变量和BRST方法
我们执行了一个(0+1)维宇宙学弗里德曼-罗伯逊-沃克(FRW)模型的贝克-路-斯托-图丁(BRST)量子化。这种量化利用了系统的经典无穷小和连续的再参数化对称变换。为了推导出宇宙FRW模型中存在的尺度因子和相应动量变量的幂零再参数化不变BRST-反BRST对称变换,我们将改进的Bonora-Tonin超变量方法(MBTSA)应用于BRST形式化。通过这种方法,我们还建立了该宇宙学再参数化不变量模型的BRST-anti-BRST不变Curci-Ferrari (CF)型约束。进一步,我们利用(反)手性超变量方法(ACSA)得到了模型内其他变量的off-壳幂零量子BRST-反BRST对称变换。在ACSA的框架内,cf型约束通过两个关键方面得到证明:(i)对称变换下耦合拉格朗日量的不变性,(ii)守恒brst -反brst电荷的绝对反交换性。值得注意的是,将MBTSA应用于物理宇宙系统,特别是一维宇宙系统,对这项工作做出了新的贡献。此外,在ACSA的应用中,我们将我们的分析限制在超变量的(反)手性超展开上,从而导致了保守brst -反brst电荷的绝对反交换性的唯一观察。此外,我们强调,cf型限制显示出一种普适性,在一般的d维时空中,在任何再参数化不变模型中保持一致。
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来源期刊
Nuclear Physics B
Nuclear Physics B 物理-物理:粒子与场物理
CiteScore
5.50
自引率
7.10%
发文量
302
审稿时长
1 months
期刊介绍: Nuclear Physics B focuses on the domain of high energy physics, quantum field theory, statistical systems, and mathematical physics, and includes four main sections: high energy physics - phenomenology, high energy physics - theory, high energy physics - experiment, and quantum field theory, statistical systems, and mathematical physics. The emphasis is on original research papers (Frontiers Articles or Full Length Articles), but Review Articles are also welcome.
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