REVIEW 3 major objections 3 minor 103 references
Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime
T0 review · 3 major / 3 minor · reviewed 2026-08-11 · deepseek-v4-flash
Pith's one-line read The paper claims that in a five-dimensional teleparallel Kaluza-Klein theory, a single parity-violating coupling produces both gravitational and electromagnetic parity violation, with the exact background-independent dispersion-shift…
desk verdict A clean unification result whose central factor-6 prediction currently rests on crucial algebra the paper does not show. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the five-dimensional teleparallel parity-violating action $S_{\mathrm{TPV}}$, the simplest torsion-quadratic parity-odd scalar of the form $\eta_{AB}\hat{\varepsilon}^{\bar\mu\bar\nu\bar\rho\bar\sigma\bar\lambda}\hat{T}^A_{\bar\mu\bar\nu}\hat{T}^B_{\bar\rho\bar\sigma}n_{\bar\lambda}$, where $n_{\bar\lambda}$ is the normalized vector field pointing along the compact fifth dimension. Under the cylinder condition and the tetrad decomposition of Eq. (26), this one action carries the argument: the four-dimensional torsion supplies the Nieh-Yan term, the parity-odd torsion-squared gravitational operator, while the mixed tetrad components $\hat{T}^5_{\mu\nu}=\sqrt{2}(\phi F_{\mu\nu}+2\nabla_{[\mu}\phi\,A_{\nu]})$ supply the electromagnetic Chern-Simons term. The relative coefficient 2 between the two terms in Eq. (36) is what later produces the factor six in Eq. (44).
What would settle it
Directly recompute the full dimensional reduction of Eq. (35) without skipping the torsion-decomposition algebra and check whether the four-dimensional effective action is exactly Eq. (36); alternatively, observe a gravitational wave together with a polarized electromagnetic counterpart from the same source and test whether $\Delta\omega^2_{\mathrm{EM}}/\Delta\omega^2_{\mathrm{GW}} = 6$ over the same propagation interval.
Extended reading notes
Core claim
Restated on the paper's own terms: the five-dimensional torsion-quadratic action $S_{\mathrm{TPV}}$ in Eq. (35), built from the five-dimensional Levi-Civita tensor, two torsion two-forms, and the preferred direction $n_{\bar\lambda}$ along the compact fifth dimension, dimensionally reduces to the four-dimensional action in Eq. (36), whose only parity-violating terms are the Nieh-Yan term and the standard electromagnetic Chern-Simons term. No gravity-electromagnetism mixing, quartic electromagnetic couplings, or higher-derivative operators appear. On a flat FRW background, the gravitational sector shows velocity birefringence with dispersion $\omega_A^2 = k^2\left[1 + c\,p_A(\ln\phi)'/k\right]$, and the electromagnetic sector has $\omega_A^2 = k^2\left[1 + 6c\,p_A(\ln\phi)'/k\right]$, which together yield Eq. (44). The factor six is fixed by the tensor contraction in the five-dimensional action and does not depend on the cosmological background.
Load-bearing premise
The prediction rests on the unshown algebra that reduces Eq. (35) to exactly Eq. (36), with only the Nieh-Yan term and the electromagnetic Chern-Simons term and the stated relative coefficient 2, together with the imported quadratic actions for the tensor and vector sectors; if that reduction contains extra operators or a different relative coefficient, the factor six in Eq. (44) changes.
Editorial extensions
If this is right
- Parity violation in the gravitational and electromagnetic sectors would no longer be governed by two unrelated parameters: a single five-dimensional coupling $c$ controls both sectors.
- Joint observations of CMB polarization rotation and gravitational-wave velocity birefringence with matched propagation endpoints could test the relation directly; at leading order the rotation angle and the gravitational-wave WKB phase difference satisfy $\Delta\alpha = 3\,\Delta\Phi^{\mathrm{WKB}}_{\mathrm{GW}}$.
- The teleparallel construction avoids the ghost instability that limits the Riemannian Kaluza-Klein parity-violating model to low energies, so the 6-to-1 relation is not tied to a cutoff below which the theory must break down.
- The other parity-odd torsion contractions considered in the paper reduce to gravitational-only parity violation and are ghost-unstable, which singles out Eq. (35) as the viable operator in this class.
Reading between the lines
- If the ratio is ever measured, the exact rational factor 6 would fingerprint the single-circle teleparallel Kaluza-Klein construction; other compactifications with different extra-dimensional topology or multiple compact directions would plausibly produce a different rational factor.
- The ratio is derived at the leading-order WKB level, so a definitive test should compare full waveforms rather than only the leading dispersion relation, since nonlinear or non-eikonal corrections could modify the factor.
- Because both dispersion shifts are proportional to $(\ln\phi)'$, a stabilized Kaluza-Klein scalar field $\phi$ would erase the signals entirely; detecting the predicted correlation would therefore also probe the dynamics of the radion field between emission and observation.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper proposes a Kaluza-Klein mechanism that correlates parity violation in the gravitational and electromagnetic sectors. In Riemannian geometry, the simplest five-dimensional parity-violating curvature-squared term is reduced to a set of four-dimensional operators that includes the gravitational Chern-Simons term, which is known to suffer from a ghost instability. In teleparallel geometry, the analogous torsion-squared term is claimed to reduce to exactly two ghost-free four-dimensional operators: the Nieh-Yan term and the electromagnetic Chern-Simons term. From those operators, the authors derive helicity-dependent dispersion relations for gravitational waves (Eq. 39) and electromagnetic waves (Eq. 43), which yield the central prediction Δω²_EM = 6 Δω²_GW (Eq. 44). The paper then discusses CMB polarization rotation and GW velocity birefringence as joint observational tests, with the caveat that the two observables must share matched propagation endpoints.
Significance. If the reduction and the imported quadratic actions are correct, the paper provides a concrete, falsifiable unification scenario: a single five-dimensional parity-violating coupling controls both cosmic birefringence and GW velocity birefringence, with a background-independent numerical ratio. The teleparallel construction avoids the ghost instability of the Riemannian Chern-Simons sector, and the authors are careful about observational conventions, for example in translating the rotation angle to the factor of three rather than six in Δα = 3ΔΦ_WKB_GW. The central novelty is the factor-of-six relation; however, its validity rests on algebraic steps that are not displayed in the manuscript, so the significance is conditional on those steps being confirmed.
major comments (3)
- [Sec. V.A, Eq. (36)] Equation (36), the four-dimensional effective action obtained from Eq. (35), is asserted after substituting the torsion decomposition in Eq. (30), but the reduction is not displayed. In particular, the component T^5_{μν} = √2(φF_{μν} + 2∇_{[μ}φ A_{ν]}) in Eq. (30) contains a ∇φ∧A term whose cancellation from the reduced action is not demonstrated. Because the relative coefficient 2 between the Nieh-Yan term and the φ³F-tilde-F term in Eq. (36) directly determines the factor 6 in Eq. (44), this unshown algebra is load-bearing for the central claim and should be exhibited in full or verified by an independent check.
- [Appendix A and Secs. V.B–V.C] The quadratic actions used to obtain the central relation, Eqs. (39) and (43), are not derived in this paper. Appendix A states that the tensor-sector results are "carried over from the existing results" without rederivation, and the electromagnetic action in Eq. (43) is written down without showing the perturbative expansion of the φ³F-tilde-F term. Since the coefficient 6 in Eq. (44) depends on the contraction convention and on the time dependence of φ³, the paper should either provide the perturbative derivation or specify precisely which published results, with which conventions, yield Eqs. (39) and (43).
- [Sec. V.C and Abstract, Eq. (44)] The relation Δω²_EM = 6 Δω²_GW is characterized in the abstract and conclusions as "exact and background-independent," while Section V.C qualifies it as holding "at the level of the leading-order WKB dispersion equations." The dispersion relations in Eqs. (39) and (43) are themselves linear in c(ln φ)′/k, so the paper should either state the domain of validity consistently or show that the next-order corrections vanish identically.
minor comments (3)
- [Sec. III.B, Eqs. (20)–(21)] The Riemannian reduction leading to Eq. (21) is also summarized as "a lengthy calculation" with no intermediate steps; a brief outline of the reduction or a supplementary file would improve reproducibility, even though the Riemannian case is not the central claim.
- [Throughout] The headings contain typographical errors such as "THEOR Y" and "P ARITY VIOLA TION"; these should be corrected to "THEORY" and "PARITY VIOLATION."
- [Sec. VI, text after Eq. (47)] The sentence comparing the Planck PR4 rotation angle to c ln(ϕ0/ϕLSS) would be clearer if the sign convention for pL and pR were restated, since the rotation angle in Eq. (47) is defined with a specific ordering of ω_R and ω_L.
Circularity Check
No significant circularity: the sixfold EM/GW dispersion ratio is derived algebraically from the chosen five-dimensional action, not fitted; the self-citations that supply ghost-freeness are prior independent derivations.
full rationale
The central prediction Δω²_EM = 6Δω²_GW (Eq. 44) is a direct algebraic ratio of the dispersion shifts in Eqs. (39) and (43), both of which follow from the same 5D parity-violating action Eq. (35) after the stated dimensional reduction (Eq. (36)). No parameter is fitted to the target quantity: the ratio is independent of the coupling c and of the background evolution of a(η) and ϕ(η), so it is not an example of a fitted input being relabeled as a prediction. The reduction of Eq. (35) to Eq. (36) is asserted rather than displayed, and Appendix A states that the tensor quadratic actions are carried over from existing results rather than rederived; this makes the derivation incomplete and places the numerical factor 6 at risk if the reduction contained extra operators or a different relative coefficient, but incompleteness is not circularity. The paper does rely on prior work by its own authors for the ghost-freeness of the Nieh-Yan term and for the instability of the alternative P2, P3, P4 contractions (Refs. [74,75,92,93]), and this is load-bearing for the choice of Eq. (35) as the viable operator. However, those cited results are parameter-free perturbative analyses with assumptions that do not include the present paper's conclusions, so under the review rules they count as independent support rather than circular self-citation. No step in the derivation is defined in terms of its own output, and no known result is merely renamed: the 5D origin of the correlated NY + EM-CS terms is a genuine construction whose observable ratio is a computed consequence.
Assumptions & free parameters
free parameters (4)
- Five-dimensional PV coupling c
- Compactification length L5
- KK scalar evolution ln[phi(eta0)/phi(etaLSS)]
- Matter potential V(phi) in Appendix A
assumptions (5)
- domain assumption Spacetime is M4 x S1 with the cylinder condition d5 = 0 on all physical fields.
- domain assumption Gravity is described by teleparallel geometry in the Weitzenbock gauge, with vanishing curvature and nonmetricity.
- ad hoc to paper The five-dimensional PV action Eq. (35) is the simplest torsion-quadratic parity-odd contraction and the correct UV starting point.
- domain assumption The ghost-freeness and dispersion properties of the Nieh-Yan term follow from the previous NYTG literature.
- standard math The WKB identification of helicity dispersion shifts from the quadratic actions gives the physical propagation speeds.
Cite this review
Pith. "Pith review of Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime." pith.science (2026). https://pith.science/paper/MCFC7UZN
@misc{pith2026260809299,
author = {Pith},
title = {Pith review of: Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime},
year = {2026},
howpublished = {\url{https://pith.science/paper/MCFC7UZN}},
note = {Machine review of arXiv:2608.09299}
}
abstract
Parity violation in the gravitational and electromagnetic sectors has been extensively investigated, yet the two are conventionally treated as independent phenomena. This separation, however, may be a four-dimensional prejudice. In higher-dimensional spacetime, gravity and electromagnetism may share a common geometric origin---and so, perhaps, does their parity violation. In this paper, we pursue this idea by constructing parity-violating Kaluza-Klein models in both Riemannian and teleparallel geometries. In Riemannian geometry, the simplest five-dimensional parity-violating term reduces to several complicated four-dimensional terms, including the familiar gravitational Chern-Simons term, which suffers from a ghost instability. In teleparallel geometry, however, the result is strikingly simple. The simplest five-dimensional parity-violating term reduces to only two ghost-free terms---the familiar Nieh-Yan term and the standard electromagnetic Chern-Simons term. Remarkably, the model predicts that the helicity-dependent dispersion shift for electromagnetic waves is exactly six times that for gravitational waves, $\Delta\omega^{2}_{ EM}=6\,\Delta\omega^{2}_{GW}$, a background-independent relation. This relation offers a falsifiable test of unification through joint cosmic microwave background and gravitational wave birefringence observations.
Reference graph
Works this paper leans on
-
[1]
B. P. Abbott et al. [LIGO Scientific and Virgo], Phys. Rev. Lett. 116, no.6, 061102 (2016) doi:10.1103/PhysRevLett.116.061102 [arXiv:1602.03837 [gr-qc]]
arXiv 2016
-
[2]
B. P. Abbott et al. [LIGO Scientific and Virgo], Phys. Rev. Lett. 119, no.16, 161101 (2017) doi:10.1103/PhysRevLett.119.161101 [arXiv:1710.05832 [gr-qc]]
arXiv 2017
-
[3]
Prob- ing Primordial Gravitational Waves: Ali CMB Polarization Telescope,
H. Li, S. Y. Li, Y. Liu, Y. P. Li, Y. Cai, M. Li, G. B. Zhao, C. Z. Liu, Z. W. Li and H. Xu, et al. “Prob- ing Primordial Gravitational Waves: Ali CMB Polarization Telescope,” Natl. Sci. Rev. 6, no.1, 145-154 (2019) doi:10.1093/nsr/nwy019 [arXiv:1710.03047 [astro-ph.CO]]
arXiv 2019
-
[4]
K. Abazajian et al. [CMB-S4], Astrophys. J. 926, no.1, 54 (2022) doi:10.3847/1538-4357/ac1596 [arXiv:2008.12619 [astro-ph.CO]]
arXiv 2022
-
[5]
S. H. S. Alexander and J. Martin, Phys. Rev. D 71, 063526 (2005) doi:10.1103/PhysRevD.71.063526 [arXiv:hep- th/0410230 [hep-th]]
arXiv 2005
- [6]
-
[7]
A. Nishizawa and T. Kobayashi, Phys. Rev. D 98, no.12, 124018 (2018) doi:10.1103/PhysRevD.98.124018 [arXiv:1809.00815 [gr-qc]]
arXiv 2018
-
[8]
LIGO Scientific, Virgo and KAGRA Collaborations, Phys. Rev. X 13, 041039 (2023) doi:10.1103/PhysRevX.13.041039 [arXiv:2111.03606 [gr-qc]]
arXiv 2023
Show all 103 references
-
[9]
Z. C. Zhao, Z. Cao and S. Wang, Astrophys. J. 930, no.2, 139 (2022) doi:10.3847/1538-4357/ac62d3 [arXiv:2201.02813 [gr-qc]]
2022 arXiv
-
[10]
T. Zhu, W. Zhao, J. M. Yan, Y. Z. Wang, C. Gong and A. Wang, Phys. Rev. D 110, no.6, 064044 (2024) doi:10.1103/PhysRevD.110.064044 [arXiv:2304.09025 [gr-qc]]. 17
2024 arXiv
-
[11]
Agazie et al
G. Agazie et al. (NANOGrav Collaboration), Astrophys. J. Lett. 951, no.1, L8 (2023) doi:10.3847/2041- 8213/acdac6 [arXiv:2306.16213 [astro-ph.HE]]
2023 arXiv
-
[12]
C. Fu, J. Liu, X. Y. Yang, W. W. Yu and Y. Zhang, Phys. Rev. D 109, no.6, 063526 (2024) doi:10.1103/PhysRevD.109.063526 [arXiv:2308.15329 [astro-ph.CO]]
2024 arXiv
-
[13]
Kato and J
R. Kato and J. Soda, Phys. Rev. D 93, no.6, 062003 (2016) doi:10.1103/PhysRevD.93.062003 [arXiv:1512.09139 [gr-qc]]
2016 arXiv
-
[14]
Belgacem and M
E. Belgacem and M. Kamionkowski, Phys. Rev. D 102, no.2, 023004 (2020) doi:10.1103/PhysRevD.102.023004 [arXiv:2004.05480 [astro-ph.CO]]
2020 arXiv
-
[15]
B. Xu, H. Jiang, R. G. Cai, M. Sasaki and Y. L. Zhang, [arXiv:2604.08141 [gr-qc]]
-
[16]
J. Qiao, T. Zhu, G. Li and W. Zhao, JCAP 04, no.04, 054 (2022) doi:10.1088/1475-7516/2022/04/054 [arXiv:2110.09033 [gr-qc]]
2022 arXiv
-
[17]
Li and D
M. Li and D. Zhao, Phys. Lett. B 827, 136968 (2022) doi:10.1016/j.physletb.2022.136968 [arXiv:2108.01337 [gr- qc]]
2022
-
[18]
R. G. Cai, C. Fu and W. W. Yu, Phys. Rev. D 105, no.10, 103520 (2022) doi:10.1103/PhysRevD.105.103520 [arXiv:2112.04794 [astro-ph.CO]]
2022 arXiv
-
[19]
C. Gong, T. Zhu, R. Niu, Q. Wu, J. L. Cui, X. Zhang, W. Zhao and A. Wang, Phys. Rev. D 105, no.4, 044034 (2022) doi:10.1103/PhysRevD.105.044034 [arXiv:2112.06446 [gr-qc]]
2022 arXiv
-
[20]
M. Li, Y. Tong and D. Zhao, Phys. Rev. D 105, no.10, 104002 (2022) doi:10.1103/PhysRevD.105.104002 [arXiv:2203.06912 [gr-qc]]
2022 arXiv
-
[21]
Zhang, J
F. Zhang, J. X. Feng and X. Gao, JCAP 10, 054 (2022) doi:10.1088/1475-7516/2022/10/054 [arXiv:2205.12045 [gr-qc]]
2022 arXiv
-
[22]
Z. Li, J. Qiao, T. Liu, T. Zhu and W. Zhao, JCAP 04, 006 (2023) doi:10.1088/1475-7516/2023/04/006 [arXiv:2211.12188 [gr-qc]]
2023 arXiv
-
[23]
J. Qiao, Z. Li, T. Zhu, R. Ji, G. Li and W. Zhao, Front. Astron. Space Sci. 9, 1109086 (2023) doi:10.3389/fspas.2022.1109086 [arXiv:2211.16825 [gr-qc]]
2023
-
[24]
Cai, Phys
Y. Cai, Phys. Rev. D 107, no.6, 063512 (2023) doi:10.1103/PhysRevD.107.063512 [arXiv:2212.10893 [gr-qc]]
2023 arXiv
-
[25]
Z. Chen, Y. Yu and X. Gao, JCAP 06, 001 (2023) doi:10.1088/1475-7516/2023/06/001 [arXiv:2212.14362 [gr-qc]]
2023 arXiv
-
[26]
Zhu and Y
M. Zhu and Y. Cai, JHEP 04, 095 (2023) doi:10.1007/JHEP04(2023)095 [arXiv:2301.13502 [gr-qc]]
2023 arXiv
-
[27]
J. X. Feng, F. Zhang and X. Gao, JCAP 07, 047 (2023) doi:10.1088/1475-7516/2023/07/047 [arXiv:2302.00950 [gr-qc]]
2023 arXiv
-
[28]
H. J. Lin, T. Zhu, S. J. Zhang and A. Wang, Phys. Rev. D 108, no.4, 044005 (2023) doi:10.1103/PhysRevD.108.044005 [arXiv:2305.15733 [gr-qc]]
2023 arXiv
-
[29]
Zhang, J
F. Zhang, J. X. Feng and X. Gao, Phys. Rev. D 108, no.6, 063513 (2023) doi:10.1103/PhysRevD.108.063513 [arXiv:2307.00330 [gr-qc]]
2023 arXiv
-
[30]
J. Qiao, Z. Li, R. Ji, T. Zhu, G. Li, W. Zhao and J. Chen, JCAP 10, 066 (2023) doi:10.1088/1475-7516/2023/10/066 [arXiv:2307.12886 [gr-qc]]
2023 arXiv
-
[31]
T. C. Li, T. Zhu, W. Zhao and A. Wang, JCAP 07, 005 (2024) doi:10.1088/1475-7516/2024/07/005 [arXiv:2403.05841 [gr-qc]]
2024 arXiv
-
[32]
Zhang, J
F. Zhang, J. X. Feng and X. Gao, Phys. Rev. D 110, no.2, 023537 (2024) doi:10.1103/PhysRevD.110.023537 [arXiv:2404.02922 [gr-qc]]
2024 arXiv
-
[33]
Akama and M
S. Akama and M. Zhu, JCAP 07, 039 (2024) doi:10.1088/1475-7516/2024/07/039 [arXiv:2404.05464 [gr-qc]]
2024 arXiv
-
[34]
Z. W. Jiang, Y. Cai, F. Wang and Y. S. Piao, JHEP 09, 067 (2024) doi:10.1007/JHEP09(2024)067 [arXiv:2406.16549 [astro-ph.CO]]
2024 arXiv
-
[35]
Z. X. Xiong and D. Huang, Phys. Rev. D 111, no.8, 084020 (2025) doi:10.1103/PhysRevD.111.084020 [arXiv:2409.09382 [gr-qc]]
2025 arXiv
-
[36]
H. Xu, D. Y. Hong, Z. H. Wang and S. Y. Zhou, JCAP 01, 102 (2025) doi:10.1088/1475-7516/2025/01/102 [arXiv:2410.09794 [hep-th]]
2025 arXiv
-
[37]
B. Xu, K. Ding, H. Su, J. Chen and Y. L. Zhang, Phys. Dark Univ. 49, 101980 (2025) doi:10.1016/j.dark.2025.101980 [arXiv:2411.08691 [hep-ph]]
2025
-
[38]
H. Su, B. Xu, J. Chen, C. Liu and Y. L. Zhang, Commun. Theor. Phys. 77, 115403 (2025) doi:10.1088/1572- 9494/add1b9 [arXiv:2503.20778 [astro-ph.CO]]
2025 arXiv
-
[39]
Li and W
Z. Li and W. Zhao, JHEP 09, 187 (2025) doi:10.1007/JHEP09(2025)187 [arXiv:2504.13450 [gr-qc]]
2025
-
[40]
Y. Kang, M. Li and Y. Tong, Phys. Dark Univ. 50, 102148 (2025) doi:10.1016/j.dark.2025.102148 [arXiv:2507.03363 [gr-qc]]. 18
2025
-
[41]
C. Fu, C. Chen and Y. Wang, Phys. Rev. D 113, no.12, L121305 (2026) doi:10.1103/z6cq-trm3 [arXiv:2410.06636 [astro-ph.CO]]
2026 arXiv
-
[42]
J. X. Feng, J. Y. Fang and X. Gao, Phys. Rev. D 113, no.10, 104035 (2026) doi:10.1103/p4rb-nz6m [arXiv:2602.07430 [gr-qc]]
2026 arXiv
-
[43]
Soda and M
J. Soda and M. Takeuchi, Phys. Rev. D 113, 064044 (2026) doi:10.1103/PhysRevD.113.064044 [arXiv:2512.14063 [gr-qc]]
2026
-
[44]
J. J. Song and X. Gao, [arXiv:2607.20317 [gr-qc]]
-
[45]
Horii, T
Y. Horii, T. Murata and T. Kobayashi, Phys. Rev. D 113, 123539 (2026) doi:10.1103/PhysRevD.113.123539 [arXiv:2512.17348 [gr-qc]]
2026
-
[46]
Y. Kang, M. Li and C. Yi, Eur. Phys. J. C 86, 607 (2026) doi:10.1140/epjc/s10052-026-15828-4 [arXiv:2602.00506 [gr-qc]]
2026 arXiv
-
[47]
J. Gao, Y. Kang, M. Li and Y. Tong, Chin. Phys. C 49, no.8, 085105 (2025) doi:10.1088/1674-1137/ade49f [arXiv:2503.03119 [gr-qc]]
2025 arXiv
-
[48]
Wilczek, Phys
F. Wilczek, Phys. Rev. Lett. 58, 1799-1802 (1987) doi:10.1103/PhysRevLett.58.1799
1987 doi
-
[49]
S. M. Carroll, G. B. Field and R. Jackiw, Phys. Rev. D 41, 1231-1240 (1990) doi:10.1103/PhysRevD.41.1231
1990 doi
-
[50]
Harari and P
D. Harari and P. Sikivie, Phys. Lett. B 289, 67-72 (1992) doi:10.1016/0370-2693(92)91363-E
1992 doi
-
[51]
A. Lue, L. M. Wang and M. Kamionkowski, Phys. Rev. Lett. 83, 1506-1509 (1999) doi:10.1103/PhysRevLett.83.1506 [arXiv:astro-ph/9812088 [astro-ph]]
1999 arXiv
-
[52]
M. Li, J. Q. Xia, H. Li and X. Zhang, Phys. Lett. B 651, 357-362 (2007) doi:10.1016/j.physletb.2007.06.050 [arXiv:hep-ph/0611192 [hep-ph]]
2007 arXiv
-
[53]
Li and X
M. Li and X. Zhang, Phys. Rev. D 78, 103516 (2008) doi:10.1103/PhysRevD.78.103516 [arXiv:0810.0403 [astro- ph]]
2008 arXiv
-
[54]
M. Li, Y. F. Cai, X. Wang and X. Zhang, Phys. Lett. B 680, 118-124 (2009) doi:10.1016/j.physletb.2009.08.053 [arXiv:0907.5159 [hep-ph]]
2009 arXiv
-
[55]
Komatsu, Nature Rev
E. Komatsu, Nature Rev. Phys. 4, 452-469 (2022) doi:10.1038/s42254-022-00452-4 [arXiv:2202.13919 [astro- ph.CO]]
2022 arXiv
-
[56]
Astrophys
Planck Collaboration, Astron. Astrophys. 641, A1 (2020) doi:10.1051/0004-6361/201833880 [arXiv:1807.06205 [astro-ph.CO]]
2020 arXiv
-
[57]
Minami and E
Y. Minami and E. Komatsu, Phys. Rev. Lett. 125, no.22, 221301 (2020) doi:10.1103/PhysRevLett.125.221301 [arXiv:2011.11254 [astro-ph.CO]]
2020 arXiv
-
[58]
Diego-Palazuelos et al
P. Diego-Palazuelos et al. , Phys. Rev. Lett. 128, no.9, 091302 (2022) doi:10.1103/PhysRevLett.128.091302 [arXiv:2201.07682 [astro-ph.CO]]
2022 arXiv
-
[59]
J. R. Eskilt and E. Komatsu, Phys. Rev. D 106, no.6, 063503 (2022) doi:10.1103/PhysRevD.106.063503 [arXiv:2205.13962 [astro-ph.CO]]
2022 arXiv
-
[60]
Kaluza, Sitzungsber
T. Kaluza, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.) 1921, 966-972 (1921) [arXiv:1803.08616 [physics.hist-ph]]
1921 arXiv
- [61]
-
[62]
M. B. Green and J. H. Schwarz, Phys. Lett. B 149, 117-122 (1984) doi:10.1016/0370-2693(84)91565-X
1984 doi
-
[63]
M. J. Duff, B. E. W. Nilsson and C. N. Pope, Phys. Lett. B 163, 343-348 (1985) doi:10.1016/0370-2693(85)90293-X
1985 doi
-
[64]
M. J. Duff, B. E. W. Nilsson and C. N. Pope, Phys. Rept. 130, 1-142 (1986) doi:10.1016/0370-1573(86)90163-8
1986 doi
-
[65]
Bailin and A
D. Bailin and A. Love, Rept. Prog. Phys. 50, 1087-1170 (1987) doi:10.1088/0034-4885/50/9/001
1987 doi
-
[66]
J. M. Overduin and P. S. Wesson, Phys. Rept. 283, 303-380 (1997) doi:10.1016/S0370-1573(96)00046-4 [arXiv:gr- qc/9805018 [gr-qc]]
1997
-
[67]
Jackiw and S
R. Jackiw and S. Y. Pi, Phys. Rev. D 68, 104012 (2003) doi:10.1103/PhysRevD.68.104012 [arXiv:gr-qc/0308071 [gr-qc]]
2003 arXiv
-
[68]
Alexander and N
S. Alexander and N. Yunes, Phys. Rept. 480, 1-55 (2009) doi:10.1016/j.physrep.2009.07.002 [arXiv:0907.2562 [hep-th]]
2009 arXiv
-
[69]
S. Dyda, E. E. Flanagan and M. Kamionkowski, Phys. Rev. D 86, 124031 (2012) doi:10.1103/PhysRevD.86.124031 [arXiv:1208.4871 [gr-qc]]
2012 arXiv
-
[70]
J. W. Maluf, Annalen Phys. 525, 339-357 (2013) doi:10.1002/andp.201200272 [arXiv:1303.3897 [gr-qc]]
2013 arXiv
-
[71]
Bahamonde et al
S. Bahamonde et al. , Rept. Prog. Phys. 86, no.2, 026901 (2023) doi:10.1088/1361-6633/ac9cef [arXiv:2106.13793 [gr-qc]]
2023 arXiv
-
[72]
H. T. Nieh and M. L. Yan, J. Math. Phys. 23, 373-374 (1982) doi:10.1063/1.525379
1982 doi
-
[73]
Chandia and J
O. Chandia and J. Zanelli, Phys. Rev. D 55, 7580-7585 (1997) doi:10.1103/PhysRevD.55.7580 [arXiv:hep- 19 th/9702025 [hep-th]]
1997
-
[74]
M. Li, H. Rao and D. Zhao, JCAP 11, 023 (2020) doi:10.1088/1475-7516/2020/11/023 [arXiv:2007.08038 [gr-qc]]
2020 arXiv
-
[75]
M. Li, H. Rao and Y. Tong, Phys. Rev. D 104, no.8, 084077 (2021) doi:10.1103/PhysRevD.104.084077 [arXiv:2104.05917 [gr-qc]]
2021 arXiv
-
[76]
W. Zhao, T. Zhu, J. Qiao and A. Wang, Phys. Rev. D 101, no.2, 024002 (2020) doi:10.1103/PhysRevD.101.024002 [arXiv:1909.10887 [gr-qc]]
2020 arXiv
-
[77]
V. C. de Andrade, L. C. T. Guillen and J. G. Pereira, Phys. Rev. D 61, 084031 (2000) doi:10.1103/PhysRevD.61.084031 [arXiv:gr-qc/9909004 [gr-qc]]
2000 arXiv
-
[78]
A. L. Barbosa, L. C. T. Guillen and J. G. Pereira, Phys. Rev. D 66, 064028 (2002) doi:10.1103/PhysRevD.66.064028 [arXiv:gr-qc/0208052 [gr-qc]]
2002 arXiv
-
[79]
Bamba, S
K. Bamba, S. Nojiri and S. D. Odintsov, Phys. Lett. B 725, 368-371 (2013) doi:10.1016/j.physletb.2013.07.052 [arXiv:1304.6191 [gr-qc]]
2013 arXiv
-
[80]
C. M. Chang and W. F. Kao, Phys. Rev. D 88, 063504 (2013) doi:10.1103/PhysRevD.88.063504
2013 doi
-
[81]
C. Q. Geng, L. W. Luo and H. H. Tseng, Class. Quant. Grav. 31, 185004 (2014) doi:10.1088/0264- 9381/31/18/185004 [arXiv:1403.3161 [hep-th]]
2014 arXiv
-
[82]
C. Q. Geng, C. Lai, L. W. Luo and H. H. Tseng, Phys. Lett. B 737, 248-250 (2014) doi:10.1016/j.physletb.2014.08.055 [arXiv:1409.1018 [gr-qc]]
2014 arXiv
-
[83]
C. Q. Geng and L. W. Luo, Class. Quant. Grav. 34, no.11, 115012 (2017) doi:10.1088/1361-6382/aa6ca1 [arXiv:1612.00166 [gr-qc]]
2017 arXiv
-
[84]
Krssak, R
M. Krssak, R. J. van den Hoogen, J. G. Pereira, C. G. Boehmer and A. A. Coley, Class. Quant. Grav. 36, no.18, 183001 (2019) doi:10.1088/1361-6382/ab2e1f [arXiv:1810.12932 [gr-qc]]
2019 arXiv
-
[85]
Ferraro and F
R. Ferraro and F. Fiorini, Phys. Rev. D 75, 084031 (2007) doi:10.1103/PhysRevD.75.084031 [arXiv:gr-qc/0610067 [gr-qc]]
2007 arXiv
-
[86]
G. R. Bengochea and R. Ferraro, Phys. Rev. D 79, 124019 (2009) doi:10.1103/PhysRevD.79.124019 [arXiv:0812.1205 [astro-ph]]
2009 arXiv
-
[87]
E. V. Linder, Phys. Rev. D 81, 127301 (2010) [erratum: Phys. Rev. D 82, 109902 (2010)] doi:10.1103/PhysRevD.81.127301 [arXiv:1005.3039 [astro-ph.CO]]
2010 arXiv
-
[88]
Y. F. Cai, S. Capozziello, M. De Laurentis and E. N. Saridakis, Rept. Prog. Phys. 79, no.10, 106901 (2016) doi:10.1088/0034-4885/79/10/106901 [arXiv:1511.07586 [gr-qc]]
2016 arXiv
-
[89]
Hayashi and T
K. Hayashi and T. Shirafuji, Phys. Rev. D 19, 3524-3553 (1979) [addendum: Phys. Rev. D 24, 3312-3314 (1982)] doi:10.1103/PhysRevD.19.3524
1979 doi
-
[90]
Bahamonde, C
S. Bahamonde, C. G. Boehmer and M. Krssak, Phys. Lett. B 775, 37-43 (2017) doi:10.1016/j.physletb.2017.10.026 [arXiv:1706.04920 [gr-qc]]
2017 arXiv
-
[91]
Krssak and E
M. Krssak and E. N. Saridakis, Class. Quant. Grav. 33, no.11, 115009 (2016) doi:10.1088/0264-9381/33/11/115009 [arXiv:1510.08432 [gr-qc]]
2016 arXiv
-
[92]
M. Li, Z. Li and H. Rao, Phys. Lett. B 834, 137395 (2022) doi:10.1016/j.physletb.2022.137395 [arXiv:2201.02357 [gr-qc]]
2022
-
[93]
Rao and D
H. Rao and D. Zhao, JHEP 08, 070 (2023) doi:10.1007/JHEP08(2023)070 [arXiv:2304.07138 [gr-qc]]
2023 arXiv
-
[94]
Hohmann, L
M. Hohmann, L. Järv, M. Krššák and C. Pfeifer, Phys. Rev. D 100, no.8, 084002 (2019) doi:10.1103/PhysRevD.100.084002 [arXiv:1901.05472 [gr-qc]]
2019 arXiv
-
[95]
Hohmann, Int
M. Hohmann, Int. J. Geom. Meth. Mod. Phys. 18, no.supp01, 2140005 (2021) doi:10.1142/S0219887821400053 [arXiv:2008.12186 [gr-qc]]
2021 arXiv
-
[96]
A. A. Coley, R. J. van den Hoogen and D. D. McNutt, Class. Quant. Grav. 39, no.22, 22LT01 (2022) doi:10.1088/1361-6382/ac994a [arXiv:2205.10719 [gr-qc]]
2022 arXiv
-
[97]
Izumi and Y
K. Izumi and Y. C. Ong, JCAP 06, 029 (2013) doi:10.1088/1475-7516/2013/06/029 [arXiv:1212.5774 [gr-qc]]
2013 arXiv
-
[98]
Golovnev and T
A. Golovnev and T. Koivisto, JCAP 11, 012 (2018) doi:10.1088/1475-7516/2018/11/012 [arXiv:1808.05565 [gr-qc]]
2018 arXiv
-
[99]
Q. Wu, T. Zhu, R. Niu, W. Zhao and A. Wang, Phys. Rev. D 105, no.2, 024035 (2022) doi:10.1103/PhysRevD.105.024035 [arXiv:2110.13870 [gr-qc]]
2022 arXiv
-
[100]
Zaldarriaga and U
M. Zaldarriaga and U. Seljak, Phys. Rev. D 55, 1830-1840 (1997) doi:10.1103/PhysRevD.55.1830 [arXiv:astro- ph/9609170 [astro-ph]]
1997
-
[101]
Kamionkowski, A
M. Kamionkowski, A. Kosowsky and A. Stebbins, Phys. Rev. D 55, 7368-7388 (1997) doi:10.1103/PhysRevD.55.7368 [arXiv:astro-ph/9611125 [astro-ph]]
1997 arXiv
-
[102]
B. G. Keating, M. Shimon and A. P. S. Yadav, Astrophys. J. Lett. 762, L23 (2013) doi:10.1088/2041- 8205/762/2/L23 [arXiv:1211.5734 [astro-ph.CO]]. 20
2013 arXiv
-
[103]
Mirshekari, N
S. Mirshekari, N. Yunes and C. M. Will, Phys. Rev. D 85, 024041 (2012) doi:10.1103/PhysRevD.85.024041 [arXiv:1110.2720 [gr-qc]]
2012 arXiv
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