Phase space structure of symmetric teleparallel theory of gravity

IF 3.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Classical and Quantum Gravity Pub Date : 2025-01-07 DOI:10.1088/1361-6382/ada197
Dalia Saha and Abhik Kumar Sanyal
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Abstract

The ‘generalized symmetric teleparallel gravity’ (GSTG) does not admit diffeomorphic invariance, since the auxiliary field as well as the shift vector act as non-propagating dynamical variables carrying 1/2 degrees of freedom each. We show that in a minisuperspace model, which is devoid of the shift vector, the problem is alleviated for locally Lorentz invariant GSTG theory, and diffeomorphic invariance is established at least for one connection. However, the eerie structure of the Hamiltonian constructed even in the background of spatially flat isotropic and homogeneous Robertson–Walker space-time, can not be maneuvered. In contrast, the other two spatially flat connections containing an arbitrary time dependent function, doesʼnt admit non-linear extension to ‘symmetric teleparallel equivalent to general relativity’ (STEGR). We therefore construct the phase-space structure with three different spatially flat connections for the ‘Lorentz invariant’ linear-scalar–vector–tensor GSTG action. Diffeomorphic invariance is established and the associated Hamiltonians are found to be well behaved for all the three cases.
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对称遥平行引力理论的相空间结构
“广义对称远平行引力”(GSTG)不承认微分不变性,因为辅助场和位移向量作为非传播的动态变量,每个都携带1/2个自由度。我们证明了在没有位移向量的极小超空间模型中,局部Lorentz不变GSTG理论的问题得到了缓解,并且至少有一个连接的微分不变性得到了建立。然而,即使在空间平面各向同性和均匀的罗伯逊-沃克时空背景下,哈密顿量的怪异结构也无法被操纵。相比之下,其他两个空间平面连接包含任意时间相关函数doesʼnt允许非线性扩展到“对称远平行等效于广义相对论”(STEGR)。因此,我们为“洛伦兹不变量”线性-标量-矢量-张量GSTG作用构造了具有三种不同空间平面连接的相空间结构。建立了微分同胚不变性,并发现相关的哈密顿量在这三种情况下都表现良好。
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来源期刊
Classical and Quantum Gravity
Classical and Quantum Gravity 物理-天文与天体物理
CiteScore
7.00
自引率
8.60%
发文量
301
审稿时长
2-4 weeks
期刊介绍: Classical and Quantum Gravity is an established journal for physicists, mathematicians and cosmologists in the fields of gravitation and the theory of spacetime. The journal is now the acknowledged world leader in classical relativity and all areas of quantum gravity.
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