Scalaron tunneling and the fate of antisymmetric tensor fields in F(R) gravity

Paul, Tanmoy; SenGupta, Soumitra

doi:10.1088/1361-6382/abb926

Cited by 2 publications

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“…Apart from the above procedure, a different non-dynamical method, in particular by the effect of the quantum tunneling of the scalaron field, was proposed in the context of F(R) gravity to explain the imperceptible signatures of the antisymmetric tensor fields in the present universe [123]. The demonstration goes as follows : the scalar degree of freedom associated with F(R) gravity, known as scalaron field, is generally endowed within a potential which in turn depends on the form of F(R).…”

Section: A Different Non-dynamical Methods For the Suppression Of Antisymmetric Tensor Fields By The "Scalaron Tunneling"mentioning

confidence: 99%

Antisymmetric Tensor Fields in Modified Gravity: A Summary

Paul

2020

Symmetry

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We provide various aspects of second rank antisymmetric Kalb–Ramond (KR) field in modified theories of gravity. The KR field energy density is found to decrease with the expansion of our universe at a faster rate in comparison to radiation and matter components. Thus as the universe evolves and cools down, the contribution of the KR field on the evolutionary process reduces significantly, and at present it almost does not affect the universe evolution. However the KR field has a significant contribution during early universe; in particular, it affects the beginning of inflation as well as increases the amount of primordial gravitational radiation and hence enlarges the value of tensor-to-scalar ratio in respect to the case when the KR field is absent. In regard to the KR field couplings, it turns out that in four dimensional higher curvature inflationary model the couplings of the KR field to other matter fields is given by 1/MPl (where MPl is known as the “reduced Planck mass” defined by MPl=18πG with G is the “Newton’s constant”) i.e., same as the usual gravity–matter coupling; however in the context of higher dimensional higher curvature model the KR couplings get an additional suppression over 1/MPl. Thus in comparison to the four dimensional model, the higher curvature braneworld scenario gives a better explanation of why the present universe carries practically no footprint of the Kalb–Ramond field. The higher curvature term in the higher dimensional gravitational action acts as a suitable stabilizing agent in the dynamical stabilization mechanism of the extra dimensional modulus field from the perspective of effective on-brane theory. Based on the evolution of KR field, one intriguing question can be—“sitting in present day universe, how do we confirm the existence of the Kalb–Ramond field which has considerably low energy density (with respect to the other components) in our present universe but has a significant impact during early universe?” We try to answer this question by the phenomena “cosmological quantum entanglement” which indeed carries the information of early universe. Finally, we briefly discuss some future perspectives of Kalb–Ramond cosmology at the end of the paper.

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Section: A Different Non-dynamical Methods For the Suppression Of Antisymmetric Tensor Fields By The "Scalaron Tunneling"mentioning

confidence: 99%