REVIEW 4 major objections 5 minor 104 references
In a carefully chosen double limit of vanishing total energy and Hubble parameter, the paper claims the 2→2 de Sitter S-matrix is a universal integral transform of the flat-space amplitude, and that requiring generalized energy conservation
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-03 08:07 UTC pith:JOCPCJWC
load-bearing objection The Hubble-flat-limit integral transform is a nice framing, but the paper's claim to cover arbitrary derivative interactions doesn't survive direct substitution into the bootstrap equation; the genuinely new part is also already in the references. the 4 major comments →
EFT Perspective On de-Sitter S-Matrix
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
On the paper's own terms, the central discovery is that the 2→2 de Sitter S-matrix, defined through an LSZ-like reduction of amputated cosmological correlators, reduces in the Hubble flat-space limit to an integral transform of the flat-space amplitude: A'_{2→2} = s^{(2−d)/2} (H/2) ∫_0^∞ ds' s'^{(d−4)/2} exp(−i(E/H)√(s'/s)) M_{2→2}(s'; m_σ, J_q), where M_{2→2} is the flat-space tree amplitude with exchanged mass m_σ and derivative couplings J_q. The paper claims this relation holds for tree-level exchange with arbitrary local derivative interactions and that, unlike the simpler energy-conservation limit, it recovers the full flat-space amplitude including mass dependence. It also derives a s
What carries the argument
The central object is the Bunch-Davies de Sitter S-matrix obtained by an LSZ-like reduction: time-ordered correlation functions are amputated with the free-field equations of motion and put on shell through mode-function integrals (Eq. 3.36). The argument is carried by three pieces of machinery: a saddle-point approximation of the massive scalar propagator at early conformal times, which turns the de Sitter momentum integrals into a flat-space-like propagator; a bootstrap differential equation for the amplitude in the double limit, solved by postulating an energy-integral ansatz (Eqs. 5.19–5.21); and generalized energy conservation, which requires the energy-non-conserving residue at τ=0 to
Load-bearing premise
The load-bearing premise is the saddle-point and solution-ansatz step used to evaluate the massive scalar propagator at early times; if that approximation misses derivative interactions, the claimed integral transform between the de Sitter and flat-space S-matrices fails, and the paper's own restriction to d≥5 shows the statement does not cover lower dimensions.
What would settle it
Compute the 2→2 exchange amplitude in d=5 for a single derivative interaction directly from the de Sitter Feynman rules without the saddle-point shortcut and compare with the transform formula (5.21)–(5.22); any discrepancy beyond the saddle-point error contradicts the claim. A simpler check is to extract the residue of the s=m_σ² pole in the double limit and verify it equals the flat-space amplitude's residue including the mass-dependent subleading term.
If this is right
- In the Hubble flat-space limit, the full tree-level flat-space amplitude—pole structure, mass dependence, and derivative couplings—is recoverable from the de Sitter S-matrix, not just its massless high-energy part.
- Because the total-energy dependence becomes negligible in this limit, the Mandelstam variable s is the unique energy scale, so the effective-field-theory power counting matches flat space.
- The subleading singularity of the de Sitter amplitude carries the exchanged mass, so the mass spectrum of the theory is imprinted in the analytic structure of the S-matrix.
- Imposing generalized energy conservation forbids cubic vertices and fixes all quartic couplings of exceptional-series scalars in terms of a single coupling for each integer conformal dimension Δ.
- The DBI theory (Δ=4) and Special Galileon theory (Δ=5) are rediscovered, and new exceptional EFTs appear for Δ≥6 that likely require extra degrees of freedom.
- The previously studied energy-conservation limit E→0 with H fixed is shown to recover only the massless high-energy part of the flat-space amplitude, whereas the Hubble flat-space limit recovers the complete tree-level amplitude.
Where Pith is reading between the lines
- A natural test the paper leaves implicit is to compute an exchange diagram with a single derivative interaction directly from the de Sitter Feynman rules in d=5 and compare with the transform formula; a mismatch would localize where the saddle-point step breaks down.
- If the transform survives loop corrections, flat-space analyticity bounds could be imported into cosmology—a direction the paper frames only as motivation.
- The generalized energy condition is effectively a stability axiom; deriving it from a microphysical principle, or finding a model where the non-conserving amplitudes are nonzero and unstable, would sharpen or refute the selection of exceptional EFTs.
- The new Δ≥6 theories are presented only at leading order in a derivative expansion; checking whether their six-point amplitudes close without new degrees of freedom would confirm the tower or force new fields.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript claims two main results. First, in a 'Hubble flat-space limit' E→0, H→0 with E/H fixed, the de Sitter 2→2 S-matrix for conformally coupled scalars exchanging a massive scalar can be expressed as an integral transform of the flat-space amplitude: Eq. (5.21), with M_{2→2} given by Eq. (5.22), advertised as valid for tree-level amplitudes with arbitrary local derivative interactions. Second, imposing generalized energy conservation on four-point amplitudes of exceptional-series scalars in d=3 is claimed to uniquely fix coupling constants and to rediscover DBI and Special Galileon theories (Section 7). The paper also presents explicit d=5 exchange calculations and α-vacuum contact terms.
Significance. If the central relation (5.21)–(5.22) were correct, it would provide a concrete analytic bridge between flat-space S-matrix analyticity and de Sitter observables, potentially enabling EFT positivity arguments in dS. The exceptional-EFT bootstrap of Section 7 is also an interesting idea. However, the central derivation rests on an unproven ansatz and a saddle-point approximation, and the exceptional-EFT amplitudes are quoted without derivation. The explicit d=5 and contact computations are useful examples, but they do not by themselves establish the advertised generality. No machine-checked or numerical verification is provided; the paper's value lies in its analytic examples and conceptual proposal.
major comments (4)
- [Sec. 5.2, Eqs. (5.20)–(5.22)] The claimed 'general solution' does not solve the stated bootstrap equation. Substituting the q-th term of (5.21) with M_q(s') = -iJ_q s'^q/(s'-m_σ^2+iε) into L = s∂_E^2 + μ_σ^2 gives, at leading order in H, i/H Γ(d-2+2q)(H/iE)^{d-2+2q} s^q plus an O(H) pole contribution, whereas the RHS of (5.20) is i/H Γ(d-2+2q)(H/iE)^{d-2}(H/E)^{2q} s^q. For q=1, d=5 these differ by a sign; generally they differ by (-1)^q, and the pole term is absent from (5.20). Thus (5.21) is not a solution for q>0, and the arbitrary-derivative generalization of the central relation (2.2) is not established.
- [Sec. 5.1, Eqs. (5.7)–(5.11)] The saddle-point evaluation is performed for a φ^2σ exchange with no derivative vertices. For derivative interactions, vertex factors introduce additional powers of momenta and τ into the Λ integral, changing the saddle equation η'(Λ)=0 and the residue. No argument is given that the approximation (5.11) survives such modifications. Therefore the claim that (5.21) holds for 'arbitrary local derivative interactions' is unsupported.
- [Sec. 4.1 and Sec. 6–7] Eq. (4.5) contains Γ(d-4), and the text explicitly excludes d≤4 as IR divergent. Yet Section 7 analyzes d=3 (four-dimensional dS) exceptional-series amplitudes and quotes finite results. The manuscript must state precisely the domain of the integral-transform relation and explain why the d=3 generalized-energy-conservation analysis is unaffected by the divergence. As written, the abstract's unrestricted validity claim is inconsistent with the body.
- [Sec. 7, Eqs. (7.4), (7.15), (7.26)–(7.28)] The non-energy-conserving amplitudes A4^{(±)}|_{kT≠0} and the resulting coupling constraints (e.g., (7.5), (7.16), (7.22)–(7.23)) are quoted without derivation. These constraints are the basis for the DBI/Special Galileon rediscovery, so the computation must be shown or explicitly attributed (e.g., to [61]). In addition, for ∆=3 the constraint Θ_0^(3)=0 (Sec. 7.2) makes the four-point amplitude trivial, so the claimed 'unique four-point amplitude for every integer ∆≥4' is not demonstrated; the exceptional-series bootstrap is incomplete.
minor comments (5)
- [Title/Abstract] Typos and formatting issues: 'EF T' in the title, 'de-Sitter' hyphenation, 'Hamtilonian' in Sec. 3, and inconsistent use of d vs. D. These should be corrected.
- [Eq. (5.8)] The saddle-point formula uses α''(Λ0) but α is not defined; it should presumably be η''(Λ0). Please clarify.
- [Sec. 3, Eqs. (3.34)–(3.36)] The same symbol G is used for the correlator and the amputated correlator, which is confusing. Suggest distinct notation.
- [Eq. (4.5)] The expression (iE+ε)^{d-4} should use the standard iε prescription; the current notation is ambiguous about which ε is meant.
- [General] The relation to Ref. [61] (Du & Stefanyszyn) should be clarified: Section 7 appears to overlap significantly with that work, and the novel contributions relative to [61] should be stated explicitly.
Circularity Check
The arbitrary-derivative dS-to-flat relation is the integral ansatz renamed: M_{2→2} in (5.22) is defined with the same J_q that already source the bootstrap equation (5.20), so the central 'relationship' is a definition rather than a derived prediction.
specific steps
-
self definitional
[Sec. 5.2, Eqs. (5.20)-(5.22); advertised in Abstract and Sec. 8]
"The general solution of this bootstrap equation is given by in terms of the following integral: A′_{2→2} = s^{(2−d)/2} × H/2 × ∫_0∞ ds′ s′^{(d−4)/2} exp(−i E/H sqrt(s′/s)) M_{2→2}(s′;mσ,J_q), where the most general matrix element M_{2→2}(s′;mσ,J_q) := −i/(s′−mσ²+iϵ) Σ_{q=0}∞ J_q s′^q."
Eq. (5.21) is the same integral ansatz as (5.19) rewritten in the variable s′, and the 'flat-space matrix element' M_{2→2} in (5.22) is defined to be the kernel of that transform, carrying the same undetermined coefficients J_q that already appear as the source terms of the bootstrap equation (5.20). The paper does not compute M from flat-space Feynman rules for arbitrary derivative interactions; it only asserts 'we have included all possible higher-derivative contact interactions' in (5.20). Hence the advertised relationship between the flat-space amplitude and the de Sitter S-matrix is, for the q>0/derivative part, established by construction: the kernel is renamed 'flat-space amplitude' and the dS amplitude is defined as its integral transform. This is a definitional reduction, not an i
full rationale
The single-massive-exchange case (q=0) does have self-contained content: Eqs. (5.16)-(5.19) start from the dS Feynman integral and the flat-space limit of the φ²σ exchange, and (5.19) does solve (5.18) (the τ-integral gives Γ(d−2)(H/iE)^{d−2}). However, the paper's advertised central claim covers 'arbitrary local derivative interactions' (Abstract). That generalization is carried by Eq. (5.20), which is posited as a 'general non-perturbative S-matrix bootstrap' rather than derived from dS Feynman rules with derivative vertices, and then Eq. (5.21)-(5.22) declares the general solution. Since M_{2→2}(s′;mσ,J_q) is defined with exactly the same J_q that source (5.20), the integral-transform relation is not an independent prediction: it is the solution ansatz rewritten, with the kernel relabeled as the flat-space amplitude. There are also unresolved correctness gaps — e.g., direct substitution of (5.21) into (5.20) for q>0 yields a q-dependent phase mismatch (i^{−2q}) and pole terms, indicating the 'general solution' is not even verified — but those are correctness risks, not additional circularity. No load-bearing self-citation chain is present: the cited bootstrap and generalized-energy-conservation literature (refs. [15–17, 48, 58, 61]) is external, and self-citations are confined to future-directions/inflation references. The exceptional-EFT constraints in Sec. 7 are computed from amplitudes rather than fitted, so they do not add circularity. Net: the central arbitrary-derivative dS↔flat relation reduces by construction to the ansatz/definition, warranting a partial-circularity score of 6.
Axiom & Free-Parameter Ledger
free parameters (3)
- Derivative truncation at 2Δ−4 operators =
2Δ−4
- Unconstrained overall couplings Θ_0^{(Δ)} =
free
- Flat-space higher-derivative coefficients J_q =
unfixed
axioms (7)
- domain assumption The dS S-matrix defined by amputated correlators and LSZ-type reduction (Eqs 3.34–3.36) exists and is finite in the relevant regime.
- ad hoc to paper The double limit E→0, H→0 with E/H finite and fixed s is the correct flat-space limit of the dS S-matrix.
- ad hoc to paper For d≤4 the dS S-matrix amplitude diverges, so the claimed relations are restricted to d≥5.
- ad hoc to paper The saddle-point/early-time approximation of the massive propagator (Eqs 5.7–5.11) is valid for arbitrary local derivative interactions.
- ad hoc to paper Vanishing of the non-energy-conserving amplitude A_{kT≠0} is equivalent to absence of instabilities, and all such support arises from the η=0 residue.
- domain assumption Exceptional-series scalars have integer conformal dimension Δ with masses m² = Δ(3−Δ)H² (Eq 6.7), and operators are restricted to at most 2Δ−4 derivatives.
- standard math Tree-level perturbation theory, the iϵ prescription, and Sokhotski-Plemelj distribution identities.
read the original abstract
Non-perturbative limitations on low-energy effective field theories (EFTs) based on the characteristics of high-energy theory are provided by the analyticity of the flat-space version of the S-matrix. Although the analyticity of the flat-space S-matrix is widely established, it is difficult to apply this framework to de Sitter space because the growing backdrop breaks time-translation symmetry and makes it more difficult to define asymptotic states. The flat-space analyticity imprint on the de Sitter S-matrix is examined in this study. On a certain limit, we derive a comprehensive relationship between the flat-space amplitude and the de Sitter S-matrix. In particular, we demonstrate that the relationship is valid for tree-level amplitude exchanging with arbitrary local derivative interactions with a large scalar field. Next, we contend that this specific limit is more consistent with the definition of EFT since, similar to flat space, the Mandelstam variable may be identified as the unique energy scale because the total energy dependence of the de Sitter S-matrix becomes negligible. Finally, we also find an unexpected connection between the idea of generalized energy conservation of an S-matrix of four-dimensional de Sitter and exceptional EFTs in de Sitter space. We restrict the coupling constants in theories of self-interacting scalars dwelling in the exceptional series of de Sitter representations by requiring that such an S-matrix only has support when the total energies of in and out states are equal. We rediscover the Dirac-Born-Infeld (DBI) and Special Galileon theories, in which a single coupling constant uniquely fixes the four-point scalar self-interactions.
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On the formulation of quantized field theories,
H. Lehmann, K. Symanzik, and W. Zimmermann, “On the formulation of quantized field theories,”Nuovo Cim.1(1955) 205–225
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Particle Creation in de Sitter Space,
E. Mottola, “Particle Creation in de Sitter Space,”Phys. Rev. D31(1985) 754
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Vacuum States in de Sitter Space,
B. Allen, “Vacuum States in de Sitter Space,”Phys. Rev. D32(1985) 3136
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Alpha-Vacua, Black Holes, and AdS/CFT,
A. Chamblin and J. Michelson, “Alpha-Vacua, Black Holes, and AdS/CFT,”Class. Quant. Grav.24(2007) 1569–1604,arXiv:hep-th/0610133
Pith/arXiv arXiv 2007
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Four Point Functions of the Stress Tensor and Conserved Currents in AdS4/CFT3,
S. Raju, “Four Point Functions of the Stress Tensor and Conserved Currents in AdS4/CFT3,”Phys. Rev. D85(2012) 126008,arXiv:1201.6452 [hep-th]
Pith/arXiv arXiv 2012
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New Recursion Relations and a Flat Space Limit for AdS/CFT Correlators,
S. Raju, “New Recursion Relations and a Flat Space Limit for AdS/CFT Correlators,” Phys. Rev. D85(2012) 126009,arXiv:1201.6449 [hep-th]
Pith/arXiv arXiv 2012
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Cosmological Polytopes and the Wavefunction of the Universe,
N. Arkani-Hamed, P. Benincasa, and A. Postnikov, “Cosmological Polytopes and the Wavefunction of the Universe,”arXiv:1709.02813 [hep-th]
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Cosmological Collider Physics,
N. Arkani-Hamed and J. Maldacena, “Cosmological Collider Physics,” arXiv:1503.08043 [hep-th]
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Quasi-Single Field Inflation and Non-Gaussianities,
X. Chen and Y. Wang, “Quasi-Single Field Inflation and Non-Gaussianities,”JCAP04 (2010) 027,arXiv:0911.3380 [hep-th]
Pith/arXiv arXiv 2010
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Effective field theory approach to quasi-single field inflation and effects of heavy fields,
T. Noumi, M. Yamaguchi, and D. Yokoyama, “Effective field theory approach to quasi-single field inflation and effects of heavy fields,”JHEP06(2013) 051, arXiv:1211.1624 [hep-th]
Pith/arXiv arXiv 2013
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New Exceptional Effective Field Theories in de Sitter Space from Generalized Energy Conservation,
Z.-Z. Du and D. Stefanyszyn, “New Exceptional Effective Field Theories in de Sitter Space from Generalized Energy Conservation,”Phys. Rev. Lett.135no. 20, (2025) 201501,arXiv:2506.21759 [hep-th]
arXiv 2025
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Quintessential Inflation in Light of ACT DR6,
S. Choudhury, S. K. Singh, and S. K. Sahoo, “Quintessential Inflation in Light of ACT DR6,”arXiv:2511.19898 [gr-qc]
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What new physics can we extract from inflation using the ACT DR6 and DESI DR2 Observations?,
S. Choudhury, G. Bauyrzhan, S. K. Singh, and K. Yerzhanov, “What new physics can we extract from inflation using the ACT DR6 and DESI DR2 Observations?,” arXiv:2506.15407 [astro-ph.CO]
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Brane inflation in background supergravity,
S. Choudhury and S. Pal, “Brane inflation in background supergravity,”Phys. Rev. D85 (2012) 043529,arXiv:1102.4206 [hep-th]
Pith/arXiv arXiv 2012
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DBI Galileon inflation in background SUGRA,
S. Choudhury and S. Pal, “DBI Galileon inflation in background SUGRA,”Nucl. Phys. B 874(2013) 85–114,arXiv:1208.4433 [hep-th]. 42
Pith/arXiv arXiv 2013
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Higgs inflation from new K¨ ahler potential,
S. Choudhury, T. Chakraborty, and S. Pal, “Higgs inflation from new K¨ ahler potential,” Nucl. Phys. B880(2014) 155–174,arXiv:1305.0981 [hep-th]
Pith/arXiv arXiv 2014
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Low & High scale MSSM inflation, gravitational waves and constraints from Planck,
S. Choudhury, A. Mazumdar, and S. Pal, “Low & High scale MSSM inflation, gravitational waves and constraints from Planck,”JCAP07(2013) 041, arXiv:1305.6398 [hep-ph]
Pith/arXiv arXiv 2013
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[68]
An accurate bound on tensor-to-scalar ratio and the scale of inflation,
S. Choudhury and A. Mazumdar, “An accurate bound on tensor-to-scalar ratio and the scale of inflation,”Nucl. Phys. B882(2014) 386–396,arXiv:1306.4496 [hep-ph]
Pith/arXiv arXiv 2014
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ConstrainingN= 1 supergravity inflationary framework with non-minimal K¨ ahler operators,
S. Choudhury, A. Mazumdar, and E. Pukartas, “ConstrainingN= 1 supergravity inflationary framework with non-minimal K¨ ahler operators,”JHEP04(2014) 077, arXiv:1402.1227 [hep-th]
Pith/arXiv arXiv 2014
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Constraining N = 1 supergravity inflation with non-minimal Kaehler operators usingδN formalism,
S. Choudhury, “Constraining N = 1 supergravity inflation with non-minimal Kaehler operators usingδN formalism,”JHEP04(2014) 105,arXiv:1402.1251 [hep-th]
Pith/arXiv arXiv 2014
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[71]
Reconstructing inflationary potential from BICEP2 and running of tensor modes,
S. Choudhury and A. Mazumdar, “Reconstructing inflationary potential from BICEP2 and running of tensor modes,”arXiv:1403.5549 [hep-th]
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S. Choudhury, “Can Effective Field Theory of inflation generate large tensor-to-scalar ratio within Randall–Sundrum single braneworld?,”Nucl. Phys. B894(2015) 29–55, arXiv:1406.7618 [hep-th]
Pith/arXiv arXiv 2015
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Reconstructing inflationary paradigm within Effective Field Theory framework,
S. Choudhury, “Reconstructing inflationary paradigm within Effective Field Theory framework,”Phys. Dark Univ.11(2016) 16–48,arXiv:1508.00269 [astro-ph.CO]
Pith/arXiv arXiv 2016
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COSMOS-e’-GTachyon from string theory,
S. Choudhury and S. Panda, “COSMOS-e’-GTachyon from string theory,”Eur. Phys. J. C76no. 5, (2016) 278,arXiv:1511.05734 [hep-th]
Pith/arXiv arXiv 2016
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COSMOS-e ′- soft Higgsotic attractors,
S. Choudhury, “COSMOS-e ′- soft Higgsotic attractors,”Eur. Phys. J. C77no. 7, (2017) 469,arXiv:1703.01750 [hep-th]
Pith/arXiv arXiv 2017
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Stochastic origin of primordial fluctuations in the sky,
S. Choudhury, “Stochastic origin of primordial fluctuations in the sky,”Int. J. Mod. Phys. D34no. 16, (2025) 2544023,arXiv:2503.17635 [gr-qc]
arXiv 2025
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Negative non-Gaussianity as a salvager for PBHs with PTAs in bounce,
S. Choudhury, K. Dey, S. Ganguly, A. Karde, S. K. Singh, and P. Tiwari, “Negative non-Gaussianity as a salvager for PBHs with PTAs in bounce,”Eur. Phys. J. C85no. 4, (2025) 472,arXiv:2409.18983 [astro-ph.CO]
Pith/arXiv arXiv 2025
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Large fluctuations and primordial black holes,
S. Choudhury and M. Sami, “Large fluctuations and primordial black holes,”Phys. Rept. 1103(2025) 1–276,arXiv:2407.17006 [gr-qc]
Pith/arXiv arXiv 2025
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S. Choudhury, S. Ganguly, S. Panda, S. SenGupta, and P. Tiwari, “Obviating PBH overproduction for SIGWs generated by pulsar timing arrays in loop corrected EFT of bounce,”JCAP09(2024) 013,arXiv:2407.18976 [astro-ph.CO]
Pith/arXiv arXiv 2024
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S. Choudhury, A. Karde, S. Panda, and S. SenGupta, “Regularized-renormalized-resummed loop corrected power spectrum of non-singular bounce with Primordial Black Hole formation,”Eur. Phys. J. C84no. 11, (2024) 1149, arXiv:2405.06882 [astro-ph.CO]. 43
Pith/arXiv arXiv 2024
discussion (0)
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