2022
DOI: 10.1007/jhep07(2022)103
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Nonlocality of quantum matter corrections and cosmological constant running

Abstract: Semiclassical loop corrections to the gravitational action include various terms with zero, two, and four derivatives of the metric as well as nonlocal form factors for these terms. Contributions to some of these terms could be confused with others on a specific metric background or for a particular gauge fixing. We present a critical analysis of the recent works where the tensor structure and the number of derivatives in the action of gravity were not properly taken into account. Taking these relevant aspects… Show more

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Cited by 3 publications
(3 citation statements)
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“…Recently, similar observations were done, e.g., in [26,56,57]). This situation confirms the general expectation that there cannot be physical running of the cosmological constant term, detectable by means of flat-space calculations, as discussed in [2] and more recently in [44]. Let us stress that this does not mean that the cosmological constant running is impossible in general, it just cannot be detected in the flat-space calculations [3].…”
Section: Implications For the Cosmological Constant Problemsupporting
confidence: 86%
See 1 more Smart Citation
“…Recently, similar observations were done, e.g., in [26,56,57]). This situation confirms the general expectation that there cannot be physical running of the cosmological constant term, detectable by means of flat-space calculations, as discussed in [2] and more recently in [44]. Let us stress that this does not mean that the cosmological constant running is impossible in general, it just cannot be detected in the flat-space calculations [3].…”
Section: Implications For the Cosmological Constant Problemsupporting
confidence: 86%
“…In particular, this issue was described in detail, exactly as a reaction to the attribution of the part of the gravitational form factor to the cosmological constant in [45]. It reality, the corresponding terms appear as part of the expansion of the nonlocal form factors of the R µν R µν and R 2 terms and have no direct relation to the cosmological constant term [44].…”
Section: Jhep07(2023)097mentioning
confidence: 99%
“…In this subsection we will use a more physical scheme, in spirit similar to the discussions in [79,[81][82][83][84][85][86][87], noting that the functions C…”
Section: An Alternative Renormalization Schemementioning
confidence: 99%