{"total":24,"items":[{"citing_arxiv_id":"2605.30405","ref_index":64,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Toward a Phenomenologically Acceptable Quantum Cyclic Universe","primary_cat":"gr-qc","submitted_at":"2026-05-28T17:45:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A finite-dimensional quantum model with commensurable energy eigenvalues and minimum-entropy initial condition yields exact periodicity and a distinguished entropy minimum that may represent the Big Bang while suppressing Boltzmann Brains.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.22951","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Amorphous Radial Frustration and Water-Like Anomalies in a Ramp-Shoulder Fluid","primary_cat":"cond-mat.soft","submitted_at":"2026-05-21T18:27:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Molecular dynamics of a ramp-shoulder fluid shows water-like anomalies arising from cooperative radial restructuring and amorphous radial frustration rather than shell competition alone.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Effective interaction potentialU CS and corresponding force (inset) as a function of the reduced interparticle distancer ∗ ij. For fluids and amorphous phases,C s2(r) converges at large distances, whereas crystalline phases display divergent behavior due to long-range translational order 28,29. The translational order parameter was calculated as τ= 1 ξc Z ξc 0 |g(ξ)−1|dξ,(6) 7 while the coordination number was obtained from Ncoord(r) = 4πρ Z r 0 g(r′)r′2dr′,(7) where the upper integration limit was chosen at the first or successive minima ofg(r), depending on the number of coordination shells considered. The susceptibility associated with translational order was computed as χτ = \u0012 ∂τ ∂P \u0013 T ,(8) which measures the variation of translational order under compression."},{"citing_arxiv_id":"2605.16587","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"3d QFT IR divergences as UV divergences in 4d Holographic Cosmology","primary_cat":"hep-th","submitted_at":"2026-05-15T19:45:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"In a 3d toy model for holographic cosmology, a mass term preserving generalized conformal structure permits 2-loop computations that indicate possible IR finiteness beyond perturbation theory, corresponding to UV finiteness without singularities in the 4d dual.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13890","ref_index":28,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes","primary_cat":"gr-qc","submitted_at":"2026-05-12T06:01:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"External quadrupolar distortion imprints on orbital dynamics and accretion structure in thin disks around deformed compact objects, with the radiating region's outer edge tied to the radiation-to-gas pressure transition.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"seed q-metric is asymptotically flat, the distorted geometry obtained in this way is, in general, only locally valid. In pro- late spheroidal coordinates 1 the corresponding line element takes the form ds2 =− x−1 x+1 !1+α e2 ˆψ dt2 (1) +M 2(x2 −1) x+1 x−1 !1+α e−2 ˆψ \" x2 −1 x2 −y 2 !α(2+α) e2ˆγ dx2 x2 −1 + dy2 1−y 2 ! +(1−y 2)dϕ 2 # . wheret∈(−∞,+∞),x∈(1,+∞),y∈[−1,1], andϕ∈ [0,2π) andα∈(−1,∞) is the deformation parameter in the q-metric. HereMis the Schwarzschild mass parameter ap- pearing in the metric and equals the physical mass when α=0. For generalα,M ADM =(1+α)M. Since the seed q-metric contribution has already been written explicitly in Equation 1, the functions ˆψand ˆγencode only the external distortion field (Faraji 2022). They are given by ˆψ= ∞X n=1 βnRnPn \u0012 xy R \u0013 ,(2) and ˆγ= ∞X n=1 βn(1+α) n−1X l=0 h (−1) n−l+1(x+y)−x+y i RlPl + ∞X n,k=1 nkβ nβk n+k Rn+k (PnPk −P n−1Pk−1) ,(3) whereβ n ∈Rare constants characterizing the external multi- polar distortion,P n denotes the Legendre polynomial of de- green, and Pn ≡P n \u0012 xy R \u0013 ,R= q x2 +y 2 −1.(4) By construction, setting ˆψ=0 and ˆγ=0 recov- ers the q-metric, whereas the additional limitα=0 yields the Schwarzschild solution. The transformation to Schwarzschild-like coordinates is x= r M −1,y=cosθ,(5) 1 Prolate spheroidal coordinates are obtained by rotating the two- dimensional elliptic coordinates about the focal axis of the ellipse. Analytic thin disks and rings3 so that the domainx>1 corresponds to the exterior region r>2M. This metric has a central curvature singularity at x=−1 (orr=0), as well as an additional singularity ap- pears atx=1 (orr=2M), and the norm of the time-like Killing vector at this latter vanishes. However, outside this hypersurface, there exists no additional horizon. Neverthe- less, considering a relatively small quadrupole moment, a physically interior solution can cover this hypersurface, since it is closely place to the central singularity (Quevedo 2011a). Besides, o"},{"citing_arxiv_id":"2605.10000","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Diamond membranes: platform for photonic and opto-mechanical applications","primary_cat":"physics.optics","submitted_at":"2026-05-11T05:24:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Thin diamond membranes are fabricated and tested as a versatile platform for photonic and optomechanical devices, with IR grating dichroism changes, femtosecond laser cutting, and polarization-dependent light modeling shown.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05720","ref_index":45,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Localized efficient in-vacuum loading of $\\sim$0.1-10 $\\mu$m spherical and plate-like particles into optical traps using a pulled glass capillary","primary_cat":"physics.optics","submitted_at":"2026-05-07T06:09:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A piezoelectric-driven glass capillary launcher enables localized, high-efficiency (up to 93%) in-vacuum loading of silica spheres, nanodiamonds, and plate-like particles into single-beam, dual-beam, and standing-wave optical traps.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03270","ref_index":23,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Can phaseless auxiliary-field quantum Monte Carlo with broken symmetry trials describe iron-sulfur clusters?","primary_cat":"physics.chem-ph","submitted_at":"2026-05-05T01:51:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Improving broken-symmetry trial wavefunctions in phaseless AFQMC for Fe-S clusters can worsen energy accuracy until high fidelity, linked to measurement trial selection and suggesting error cancellation in HF-based results.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.26045","ref_index":1,"ref_count":2,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Euclidean volume fluctuations in de Sitter quantum gravity","primary_cat":"hep-th","submitted_at":"2026-04-28T18:30:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"From the de Sitter partition function in various approximations, the volume probability distribution concentrates around the classical value but shifts to favor smaller universes as quantum effects increase.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.25035","ref_index":3,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"The Thermodynamics of Cosmological Horizons and Their Holographic Description in de Sitter Space","primary_cat":"hep-th","submitted_at":"2026-04-27T22:35:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A universal first law of thermodynamics for de Sitter cosmological horizons defines entropy in the holographic dual at future infinity as a function of boundary pressure and angular momentum from the Brown-York stress tensor.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"can immediately see that the pressure in the intermediate regionIcannot be related by eq.(D.65) to entropy of any of theH 1 orH 2 as discussed in section 5.1. - 45 - References [1] J. M. Maldacena,Non-Gaussian features of primordial fluctuations in single field inflationary models,JHEP05(2003) 013, [astro-ph/0210603]. [2] J. Kluson,Remark about dS / CFT correspondence,Class. Quant. Grav.20(2003) 2131-2146, [hep-th/0302008]. [3] E. Witten,Quantum gravity in de Sitter space, inStrings 2001: International Conference, 6, 2001.hep-th/0106109. [4] A. Strominger,The dS / CFT correspondence,JHEP10(2001) 034, [hep-th/0106113]. [5] M. Spradlin and A. Volovich,Vacuum states and the S matrix in dS / CFT,Phys. Rev. D 65(2002) 104037, [hep-th/0112223]. [6] V. Balasubramanian, J. de Boer and D."},{"citing_arxiv_id":"2604.22086","ref_index":34,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Tantalum Damascene Coplanar Waveguide Resonators Fabricated Using 300 mm Scale Processes","primary_cat":"quant-ph","submitted_at":"2026-04-23T21:38:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Tantalum damascene resonators on 300 mm wafers show modest loss reduction by replacing sidewall oxides with metal-substrate interfaces via buried oxide simulation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.21408","ref_index":72,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Holographic complexity of conformal fields in global de Sitter spacetime","primary_cat":"hep-th","submitted_at":"2026-04-23T08:22:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Holographic complexity of CFTs in global dS_d is computed via volume and action prescriptions in AdS foliation and brane setups, then compared to results from static and Poincare patches.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"We expect the presence of Einstein-Hilbert term to affect the complexity in a non-trivial way as the intersection of the two null surfaces of WDW patch which happens at the brane will give a non-zero contribution. Also if we consider fluctuating (backreacting) brane, then we might also see some nontrivial quantum gravity effects as observed in the case of - 26 - AdS [72]. There remain several open questions and interesting avenues of further investigations. In particular, it would be interesting to understand how notions such as the Lloyd bound should be reformulated, or possibly modified, in de Sitter spacetime where the number of degrees of freedom is exponentially increasing, i.e. does the exponential growth of com-"},{"citing_arxiv_id":"2604.17966","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"TPS-CalcBench: A Benchmark and Diagnostic Evaluation Framework for LLM Analytical Calculation Competence in Hypersonic Thermal Protection System Engineering","primary_cat":"cs.AI","submitted_at":"2026-04-20T08:46:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"TPS-CalcBench is a new benchmark and evaluation framework that tests LLMs on analytical calculations in hypersonic aerodynamics and gas dynamics, using dual-track scoring and interventions to detect physically invalid reasoning.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.17541","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":true,"paper_title":"Anisotropic Electrostatic-Elastic Softening and Stability in Charged Colloidal Crystals","primary_cat":"cond-mat.soft","submitted_at":"2026-04-19T17:03:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Derives closed-form critical electrostatic-elastic coupling values for the onset of homogeneous instability along [100], [110], and [111] directions in cubic colloidal crystals by renormalizing the elastic tensor with a scalar λ_g obtained from Poisson-Boltzmann theory.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.27824","ref_index":98,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Holographic duality from a four-fermion interaction: emergent AdS$_3$/CFT$_2$, D-branes, and Einstein gravity","primary_cat":"hep-th","submitted_at":"2026-03-29T19:30:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The bosonic AdS3/CFT2 duality emerges from the Gross-Neveu model via higher-spin composites and fluctuations in competing spin-0 and spin-1 condensates that define the radial bulk coordinate.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.25797","ref_index":122,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Dark energy from string theory: an introductory review","primary_cat":"hep-th","submitted_at":"2026-03-26T18:05:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"String theory imposes constraints on dark energy but permits various construction attempts for de Sitter vacua and single-field exponential quintessence models despite obstructions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"ries over anti-de Sitter backgrounds are considered defined non-perturbatively, thanks to the holographic duality, by the adequate conformal field theories living on the boundary. From that perspective, one may wonder whether quantum gravity on a de Sitter spacetime could be defined in the same (non-perturbative) fashion, through a putative dS/CFT correspon- dence [120, 121, 122]. This also turns out to be difficult to realise. To start with, because of the isometry group of de Sitter, the (would-be) dual CFT is Euclidian, typically with non- unitary representations of the conformal group, or complex conformal weights. 10 Regarding the boundary where the field theory should live, there are several proposals: a first one is the"},{"citing_arxiv_id":"2603.20913","ref_index":15,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Horizon Edge Partition Functions in $\\Lambda>0$ Quantum Gravity","primary_cat":"hep-th","submitted_at":"2026-03-21T18:55:08+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Horizon edge mode spectra in de Sitter and Nariai spacetimes exhibit universal shift symmetries that produce novel symmetry breaking in one-loop partition functions.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"sitter space, inThe Davis Meeting on Cosmic Inflation (2003) arXiv:astro-ph/0305037. [13] E. Witten, Quantum gravity in de Sitter space, inStrings 2001: International Conference(2001) arXiv:hep-th/0106109. [14] D. Anninos, T. Bautista, and B. M¨ uhlmann, The two- sphere partition function in two-dimensional quantum gravity, JHEP09, 116, arXiv:2106.01665 [hep-th]. [15] E. Coleman, E. A. Mazenc, V. Shyam, E. Silverstein, R. M. Soni, G. Torroba, and S. Yang, De Sitter mi- crostates from T T+ Λ 2 and the Hawking-Page transi- tion, JHEP07, 140, arXiv:2110.14670 [hep-th]. [16] D. Anninos and B. M¨ uhlmann, The semiclassical grav- itational path integral and random matrices (toward a microscopic picture of a dS 2 universe), JHEP12, 206,"},{"citing_arxiv_id":"2602.19812","ref_index":52,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"dS$^4$ Metamorphosis","primary_cat":"hep-th","submitted_at":"2026-02-23T13:12:14+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.06113","ref_index":226,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography","primary_cat":"hep-th","submitted_at":"2026-02-05T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Deformations of the double-scaled SYK model via finite-cutoff holography produce Krylov complexity as wormhole length and realize Susskind's stretched horizon proposal through targeted T² deformations in the high-energy spectrum.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.15228","ref_index":2,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"De Sitter Momentum Space","primary_cat":"hep-th","submitted_at":"2026-01-21T18:03:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"A Kontorovitch-Lebedev-Fourier momentum space is constructed for de Sitter QFT where the dS frequency labels unitary representations, making equations algebraic and propagators simple like in flat space.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.03779","ref_index":15,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Cosmological Entanglement Entropy from the von Neumann Algebra of Double-Scaled SYK & Its Connection with Krylov Complexity","primary_cat":"hep-th","submitted_at":"2025-11-05T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Algebraic entanglement entropy from type II1 algebras in double-scaled SYK is matched via triple-scaling limits to Ryu-Takayanagi areas in (A)dS2, reproducing Bekenstein-Hawking and Gibbons-Hawking formulas for specific regions while depending on Krylov complexity of the Hartle-Hawking state.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Hayden, M. Headrick and A. Maloney,Holographic Mutual Information is Monogamous, Phys. Rev. D87(2013) 046003 [1107.2940]. [13] M. Headrick and T. Takayanagi,A Holographic proof of the strong subadditivity of entanglement entropy,Phys. Rev. D76(2007) 106013 [0704.3719]. [14] A. Strominger,The dS / CFT correspondence,JHEP10(2001) 034 [hep-th/0106113]. [15] E. Witten,Quantum gravity in de Sitter space, inStrings 2001: International Conference, 6, 2001 [hep-th/0106109]. [16] J.M. Maldacena,Non-Gaussian features of primordial fluctuations in single field inflationary models,JHEP05(2003) 013 [astro-ph/0210603]. [17] A. Lewkowycz, J. Liu, E. Silverstein and G. Torroba,TTand EE, with implications for (A)dS"},{"citing_arxiv_id":"2509.04974","ref_index":7,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Minkowski Space holography and Radon transform","primary_cat":"hep-th","submitted_at":"2025-09-05T09:57:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Relates free scalar in Minkowski space to codimension-two sphere field via Radon transform to dS/EAdS slice and bulk reconstruction, with Mellin modes as generalized hypergeometric functions via Lee-Pomeransky method.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.16436","ref_index":75,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"QFT in Klein space","primary_cat":"hep-th","submitted_at":"2025-05-22T09:26:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Authors construct canonical and path-integral quantizations for QFT in Klein space using extra modes, deriving correlation functions that match Minkowski space via analytical continuation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.11553","ref_index":58,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Holographic entanglement entropy and complexity for the cosmological braneworld model","primary_cat":"hep-th","submitted_at":"2025-05-15T15:59:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Time-dependent holographic entanglement entropy and complexity are computed perturbatively for braneworld FLRW universes with radiation, matter, and exotic matter by using time-dependent brane positions in black brane bulk geometries.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.03068","ref_index":13,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"M\\\"obius randomness in the Hartle-Hawking state","primary_cat":"hep-th","submitted_at":"2025-05-05T23:22:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The Hartle-Hawking state for toroidal quantum cosmologies is expressed in the Langlands decomposition as a sum over zeta zeros whose near-singularity dynamics follow the Hilbert-Pólya Hamiltonian and as a Möbius average of CFT partition functions.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Hellerman, A. Lepage-Jutier, A. Maloney, D. Radicevic, and S. Shenker,Topology of Future Infinity in dS/CFT, JHEP 11 (2013) 026, [arXiv:1306.6629]. [11] G. Conti and T. Hertog,Two wave functions and dS/CFT on S1 × S2, JHEP 06 (2015) 101, [arXiv:1412.3728]. [12] G. J. Turiaci and C.-H. Wu,The wavefunction of a quantumS1 × S2 universe, arXiv:2503.14639. [13] E. Witten,Quantum gravity in de Sitter space, inStrings 2001: International Conference, 6, 2001. hep-th/0106109. [14] A. Strominger,The dS / CFT correspondence, JHEP 10 (2001) 034, [hep-th/0106113]. [15] A. Strominger,Inflation and the dS / CFT correspondence, JHEP 11 (2001) 049, [hep-th/0110087]. [16] J. M. Maldacena,Non-Gaussian features of primordial fluctuations in single field"}],"limit":50,"offset":0}