{"topic":"quantum-gravity","tier":"stated","total":486,"limit":50,"offset":0,"claims":[{"claim_id":2088633,"arxiv_id":"2608.09858","paper_version":1,"claim_text":"The central assertion is Eq. (91) for pure conformal quantum gravity and Eq. (100) for gravity coupled to conformal matter: C4 \\bar\\Gamma_div^(1) = 0. In words, the one-loop divergent part of the effective action is annihilated by the conformal generator in four dimensions, so the divergences are conformally invariant and no non-conformal counterterm such as R^2 is generated.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T05:24:12.218864+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"On the Renormalization in Conformal Quantum Gravity","paper_submitted_at":"2026-08-10T17:16:07+00:00"},{"claim_id":1930824,"arxiv_id":"2608.07257","paper_version":1,"claim_text":"The paper's central claim, stated on its own terms, is that after the Born-Markov and secular approximations and an explicit counterterm renormalization of the ultraviolet-divergent Lamb shift, the oscillator's reduced dynamics is exactly Lindblad for each bath state, with jump operators quadratic in the phonon operators. The universal tidal interaction $H_I = -\\frac{m}{4}\\ddot{h}_{xx}(t,0)x^2$ is quadratic in the displacement $x$, so one graviton exchanges with two mechanical phonons. In vacuum $L_V=b^2$, making $|0\\rangle$ and $|1\\rangle$ dark and preserving the coherence of the qubit they span; a coherent bath has the same dissipator plus a coherent-shift Hamiltonian that reproduces the classical geodesic-deviation equation; number and thermal baths add the excitation jump $b^{\\dagger 2}$, coupling $\\rho_{01}$ to an infinite ladder of coherences; and a squeezed bath yields the single jump operator $L_S=\\cosh r(2\\omega_m)b^2 - e^{i\\phi(2\\omega_m)}\\sinh r(2\\omega_m)b^{\\dagger 2}$, whose kernel contains one dressed dark state in each parity sector, so the mutual coherence of $|D_+\\rangle$ and $|D_-\\rangle$ is exactly preserved by the dissipator. Quantitatively, all rates are multiples of the small vacuum rate $\\gamma_V = \\frac{32}{15}t_P^2\\omega_m^3$.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:40.344781+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"The small effect of graviton-induced decoherence","paper_submitted_at":"2026-08-07T14:13:45+00:00"},{"claim_id":1797390,"arxiv_id":"2608.05973","paper_version":1,"claim_text":"The paper's central claim is that the complete three-loop five-point $\\mathcal{N}=4$ SYM amplitude admits a manifestly CK-dual integrand: 42 trivalent graph topologies, with numerators generated from two master topologies by dual Jacobi relations, at most quadratic in loop momenta, and fixed uniquely up to generalized-gauge freedom. Double copy of these numerators yields the $\\mathcal{N}=8$ supergravity integrand. At $D_c=6$, the SYM ultraviolet pole contains no double-trace term, has color dependence $N_c^3+36\\zeta_3 N_c$, and matches the two-loop five-point single-trace structure, while the SUGRA pole is the expression in Eq. (8), agreeing with the closed-string-inspired prediction for four-dimensional external states. Replacing the four-dimensional prefactors $\\gamma_{ij}$ by $D$-dimensional tree-level expressions $\\gamma^D_{ij}$ reproduces the open-string prediction for the SYM pole at generic kinematics, but for gravity the same replacement differs from the string-inspired result by the evanescent combination $E$ that vanishes in four dimensions. The paper therefore concludes that the four-dimensional representation, although complete as a four-dimensional amplitude, does not by itself determine the full integrand of the higher-dimensional theory.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:40.344781+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Three-Loop Five-Point CK-Dual Amplitudes and UV Structure in N=4 SYM and N=8 SUGRA","paper_submitted_at":"2026-08-06T12:46:44+00:00"},{"claim_id":1839920,"arxiv_id":"2608.05328","paper_version":1,"claim_text":"The central discovery claimed is that the areal-radius form of the effective polymer metric yields a two-parameter stellar structure system that reduces to the standard TOV equations when $A_\\lambda \\to 0$, and that increasing $A_\\lambda$ produces a controlled upward shift of the equilibrium sequence. For the Chandrasekhar equation of state the undeformed maximum is $1.4166\\,M_\\odot$ at radius $1010.7$ km; with the Coulomb lattice correction it is $1.3850\\,M_\\odot$ at $980.5$ km. At $A_\\lambda = 100$ these maxima rise to $1.7125\\,M_\\odot$ and $1.6907\\,M_\\odot$, with the configurations remaining inside the inverse $\\beta$ decay domain. Varying $\\eta = 0.5$ or $2$ changes $M_\\mathrm{max}$ by less than $0.1\\%$ and the radius at maximum mass by less than $0.33\\%$, so the paper identifies $A_\\lambda$, not $\\eta$, as the parameter that controls the super-Chandrasekhar displacement.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.75,"assigned_at":"2026-08-11T03:35:40.344781+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"White Dwarf Stellar Structure from Effective Polymer Geometry in Loop Quantum Gravity","paper_submitted_at":"2026-08-05T18:36:58+00:00"},{"claim_id":1841500,"arxiv_id":"2608.05292","paper_version":1,"claim_text":"On the paper's own terms, the central discovery is that the charged loop-quantum-gravity black hole is not spectrally identical to Reissner-Nordström even though it shares the same horizons and shadow radius. For massless scalar waves, the quantum parameter $b_0 > 1$ lowers the effective potential barrier, so more of the incident wave tunnels into the black hole; consequently the total absorption cross section grows with $b_0$ from the low-frequency regime up to moderate frequencies, while remaining pinned to the same black-hole area at low frequency and the same geometric capture cross section at high frequency. The numerical spectra also show an anti-correlation between peaks and troughs as $b_0$ varies: the configuration with the largest peaks has the deepest troughs. Increasing $Q/M$, by contrast, raises the barrier and suppresses absorption at all frequencies. The greybody-factor calculation shows the same two trends, with the $l \\geq 1$ partial waves reversing the $b_0$ effect in some frequency windows.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:40.344781+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Absorption spectrum and greybody factors of charged black holes in loop quantum gravity","paper_submitted_at":"2026-08-05T18:00:05+00:00"},{"claim_id":1518399,"arxiv_id":"2608.04665","paper_version":1,"claim_text":"The paper argues that, for torus universes in AdS$_3$, the $T\\bar{T}$-deformed partition function is obtained from the Wheeler–DeWitt wavefunction $\\Psi(T,m_a)$ by the kernel transform $Z_{T\\bar T}(\\lambda,m_a)=\\int_0^\\infty dT\\, K(\\lambda,T)\\Psi(T,m_a)$ with $K(\\lambda,T)=2\\sqrt{\\pi}\\,\\lambda^{1/2}e^{2\\lambda(1-\\cosh T)}$. The derivation matches the flow equation for the deformed partition function to the WdW equation in WdW time $T$, using the same shifted Maass Laplacian as the spatial operator; the physical solution is the modified Bessel function $K_{ir}(2\\lambda)$ with the $\\cos(rT)$ mode, normalized so the $\\lambda\\to\\infty$ limit gives the undeformed CFT partition function. In that limit the kernel tends to a delta function and the partition function reduces to the boundary value of the wavefunction. For finite $\\lambda$ the kernel has finite width and its center, in proper radial coordinate, sits at $\\rho_*=\\frac14\\sinh^{-1}(4\\lambda)$, so a fixed-coupling partition function is a finite-width bulk wavepacket. The inverse transform (4.3) reconstructs the exact wavefunction from the family of deformed partition functions, and the same transform, with different geometric identifications of $T=0$, applies to closed AdS$_3$ torus universes and to dS$_3$ torus universes.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T04:26:46.837720+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Wavefunctions of AdS$_3$ Universes and $T\\bar{T}$-deformed Torus Partition Functions","paper_submitted_at":"2026-08-05T10:23:10+00:00"},{"claim_id":1206024,"arxiv_id":"2608.00590","paper_version":1,"claim_text":"On the paper's own terms, the central claim is that the Gregory–Laflamme instability is a UV/IR bridge: when a black string thins to a horizon radius of order the inverse species scale, Λ_s^{-1}, gravitational effective field theory breaks down and the system must be described as a bound state of Λ_s-energy quanta. This replacement of the string scale by the species scale is asserted for general theories of quantum gravity, and it yields the prediction that a fraction of order ΔE ∼ M_pl^{d−2}/Λ_s^{d−3} of the initial black-hole mass is converted into particles of energy Λ_s, with no dependence on the number of internal dimensions. For charged black holes, the paper derives two thresholds: Q_","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:40.344781+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"IR Black Hole Instabilities Trigger Species-Scale Particle Production","paper_submitted_at":"2026-08-01T10:58:43+00:00"},{"claim_id":870933,"arxiv_id":"2607.27722","paper_version":1,"claim_text":"The central claim is that the vacuum energy density between two parallel plates in rainbow spacetime is the standard Minkowski Casimir energy times an overall factor that depends on the choice of rainbow functions. Concretely, after solving the deformed scalar field equation and relating the vacuum expectation value of the deformed energy-momentum tensor to the Green's function, the paper finds that the reduced Green's function acquires a multiplicative factor (1 + (alpha + k) E_o) relative to the Minkowski result, and that this translates into Casimir energy and force rescaled by (1 - 2 k E_o). For the first rainbow function f(E)=g(E)=1/(1 - lambda E_o/E_P), k = lambda/E_P, so the magnitude","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Vacuum fluctuations in Rainbow space-time: Study of Casimir effect","paper_submitted_at":"2026-07-30T05:58:47+00:00"},{"claim_id":897403,"arxiv_id":"2607.27337","paper_version":1,"claim_text":"On the paper's own terms, the discovery is that the vacuum-subtracted von Neumann entropy of the dual CFT state in the dressed Type-II algebra is, at leading order O(λ²), exactly one quarter of the vacuum-subtracted area of the HRT surface: ΔS(ω_h,A) = S(ρ_{\\tilde ω_h}) = (1/4)(Ar[Γ_λ,g(λ)] − Ar[Γ_0,g(0)]). This is equation (6.16). Distinctly, the proof also derives the JLMS equality — relative entropy of any bulk state with respect to the vacuum equals relative entropy of the dual CFT state — as a direct consequence of the holographic map's isometric and reconstruction properties, before any crossed-product construction is invoked.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Holography in the linearized quantum gravity regime and modular crossed product","paper_submitted_at":"2026-07-29T18:00:17+00:00"},{"claim_id":925808,"arxiv_id":"2607.26415","paper_version":1,"claim_text":"In the paper's own formulation, the generalized Bergshoeff-de Roo identification equates the auxiliary gauge-group degrees of freedom with the composite Lorentz degrees of freedom, F_{aBC} = −g E_μ^a (t_μ)_BC = E_{aBC}. Using a coset parametrization of the O(D,D+k) generalized vielbein and gauge fixings that break the extended Lorentz group to the standard one from the outset, the identified flux becomes a generalized Riemann tensor and the action takes the manifestly Lorentz-covariant form (8). Its derivative expansion up to O(α′²) is summarized by Eq. (112), which contains only three independent couplings built from the torsionful curvature R^{(+)}: R^{(+)}², (D^{(+)}R^{(+)})², and R^{(+)}","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Generalized Bergshoeff-de Roo identification in the Supergravity frame","paper_submitted_at":"2026-07-29T02:58:15+00:00"},{"claim_id":862607,"arxiv_id":"2607.26197","paper_version":1,"claim_text":"The paper's core claim is that the previously uncontrolled tensor intersections in 6d N=(1,0) supergravity are universally finite, and the bounds follow from two low-energy inputs: the gravitational anomaly vector b0 lies in the cone generated by primitive BPS strings, and distinct primitive BPS strings have non-negative mutual intersections. From these inputs the authors construct a unique lattice Zariski decomposition b0 = P + N, where N is supported on a negative-definite tensionless sector; the unit pairing b0·e = 1 then forces the coefficient of any generator in N to give Ci·e ≤ 1/αi. This yields C_-3·e ≤ 3 and C_-2·e ≤ 7 for (-2)-charges in non-Higgsable clusters, while the maximal emb","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Intersection Bounds for BPS Strings in Six-Dimensional Supergravity","paper_submitted_at":"2026-07-28T19:00:17+00:00"},{"claim_id":863295,"arxiv_id":"2607.26035","paper_version":1,"claim_text":"The central claim is that quantum mechanics and gravity both emerge from a single fractal-entanglement substrate: the paper states 'the Schrödinger equation is not postulated but derived as the geodesic equation of a particle moving in a fractal spacetime' and 'Gravity arises from the time dependence of the entanglement-induced metric, yielding Einstein gravity in the macroscopic limit.' If true, both quantum theory and general relativity would be emergent consequences of the information-theoretic geometry of an entanglement network.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Quantum Gravity from Fractal Entanglement Geometry","paper_submitted_at":"2026-07-28T17:44:26+00:00"},{"claim_id":870005,"arxiv_id":"2607.25513","paper_version":1,"claim_text":"The paper's central claim is that the 'absolute consistency criterion' (ACC)—Δs_bh > 0, the requirement that the net change in the correction to the Bekenstein-Hawking area formula be positive—is the right way to marry the gravitational-wave-validated area theorem with the generalized second law. Under this criterion, the additive expansion of the correction s_bh = s0 log S_BH + s1/S_BH + ... is constrained in its sign. For F(R) gravity, the Wald entropy formula S_bh = F'_R(R_S) A_S, together with the inverse-area expansion and the identification R_S = a/A_S, leads to the parameter inequalities F'_R(A_S^{-1}) < F'_R(0) and F''_R(0) < 0, and to further inequalities if higher-order terms are k","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Gravitational wave constraints on corrections to Bekenstein-Hawking Area Formula in classical F(R) gravity and quantum GR : implications for theory parameters","paper_submitted_at":"2026-07-28T09:51:44+00:00"},{"claim_id":844522,"arxiv_id":"2607.24930","paper_version":1,"claim_text":"The central claim is a rate formula: a coherent graviton wave packet containing N gravitons, with central frequency ω_s and bandwidth σ_ω, decays in vacuum into photon pairs at dP/dt = 3 G^2 N^2 ω_s^3 σ_ω^2/(25π), so the photon count grows as N_γ(t) ≈ G^2 N_0^2 6ω_s^3 σ_ω^2 t/(25π). Two features matter here: a single plane-wave graviton field produces no photons at leading order, and the quadratic photon-gravity coupling vanishes classically in vacuum. The process appears because the coherent state is a many-graviton superposition and because the calculation is carried to second order in the metric; the paper shows the quantum result matches a semiclassical treatment whose photon source is t","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Gravitational waves decay in vacuum","paper_submitted_at":"2026-07-27T18:00:05+00:00"},{"claim_id":879614,"arxiv_id":"2607.22412","paper_version":1,"claim_text":"The central claim is that the spinfoam construction yields a genuine quantum-gravity path integral. In three dimensions this is established: the Ponzano-Regge state sum is invariant under Pachner moves via the Biedenharn-Elliott identity, projects onto flat connections, and its 6j-symbols satisfy recursion relations that become the Wheeler-DeWitt equation in the semiclassical limit. In four dimensions, the paper argues that the EPRL vertex amplitude, built from the weak imposition of linear simplicity constraints, is the correct discrete path integral for Lorentzian quantum gravity. The construction embeds each SU(2) spin j into the SL(2,C) representation (p, k) = (γ(j+1), j), giving the Y_γ","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Les Houches lectures on Spinfoam Path Integrals","paper_submitted_at":"2026-07-24T15:28:54+00:00"},{"claim_id":883787,"arxiv_id":"2607.22037","paper_version":1,"claim_text":"The central claim is that LQC inverse-volume corrections, evaluated at second order in the slow-roll expansion, induce a prominent negative shift in n_s while leaving r almost unchanged, thereby translating the theoretical predictions of fractional power-law potentials horizontally leftward in the r–n_s plane. For the allowed ranges of the LQC parameters σ (the scale-factor exponent of the correction) and δ (its amplitude at the CMB pivot scale) listed in Tables I and II, the classically excluded potentials n = 1/3, 2/5 and 2/3 fall within the 68% and 95% confidence regions of the P-ACT-LB-BK18 dataset. The paper thus claims that strictly perturbative quantum-gravity corrections can restore","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:22.060918+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"LQC inverse volume corrections inflation driven by fractional power law potentials in light of ACT observations","paper_submitted_at":"2026-07-24T07:05:58+00:00"},{"claim_id":889783,"arxiv_id":"2607.21509","paper_version":1,"claim_text":"For a disk with an S^1 boundary of proper length ℓ in two-dimensional Λ>0 pure gravity, the genus-h contribution to the gravitational path integral takes the form W^(h)(ℓ) = κ^(2h−1) e^(−ℓ/2) Σ_{n=0}^{3h−2} ζ_n ℓ^(n+1/2), with rational coefficients ζ_n for h≥1. The paper derives genus-one and genus-two by semiclassical path integration, and genus-three through genus-six by a heat-kernel recursion; the genus-four, genus-five, and genus-six formulas are new. In the large-ℓ limit, the ratio of successive genus contributions scales as κ²ℓ³ and approaches α_h = 1/(384(1+h)), matching the behavior of two-dimensional topological gravity and its intersection numbers. The paper also argues that these","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Aspects of Closed Matricial Worlds","paper_submitted_at":"2026-07-23T16:54:54+00:00"},{"claim_id":891299,"arxiv_id":"2607.21311","paper_version":1,"claim_text":"The central claim is that diagonal R-symmetry gauging—gauge group U(1)_R+ whose generator is the sum of the usual U(1)_R and a U(1) inside the quaternionic-isometry group Sp(n_H) acting on hypermultiplets—passes all local and global anomaly tests in a much larger class of 6D (1,0) models than ordinary U(1)_R gauging, and yields supersymmetric Minkowski vacua. Concretely, the paper exhibits 706 G_1×U(1)_R+ and 1,559 G_1×G_2×U(1)_R+ anomaly-free spectra under its stated rank and charge bounds, and shows by explicit coset parametrization (rank-one ansatz on SU(n_H,2)/(U(n_H)×SU(2)_R)) that vanishing of all moment maps is achievable exactly when the gauging is diagonal, leading to C_+ = C_z' = 0","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Diagonally gauged anomaly-free 6D supergravities and their vacua","paper_submitted_at":"2026-07-23T13:33:42+00:00"},{"claim_id":895776,"arxiv_id":"2607.20867","paper_version":1,"claim_text":"The central claim: for any initial graviton state, the reduced coherence factor is D = e^{iΔΦ} Tr[ρ_g D[Δα]], where Δα is the difference of the coherent displacements induced by the two branches. In the vacuum, Γ = -ln|D| = ½N_Δ, half the mean number of gravitons the difference source would radiate. In the nonrelativistic quadrupole limit with a Gaussian closed trajectory, Γ_vac = (8/15) G m² d⁴/(ℏ c⁵ τ⁴) = (8/15)(m/m_P)^2(u/c)^4. For a general two-mode squeezed vacuum, the response is reweighted by factors between e^{-2r} and e^{2r}; for the inflationary squeezed background, the rapidly oscillating squeezing phase averages out, leaving Γ_inf = (π/20) Ω_inf (m d² H_0/ℏ)², which with Ω_inf =","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Graviton-induced which-path decoherence in matter-wave interferometry","paper_submitted_at":"2026-07-23T02:46:22+00:00"},{"claim_id":901366,"arxiv_id":"2607.20312","paper_version":1,"claim_text":"The central claim is Theorem 3.16: over a super-torsion-free (1,10|32) super-spacetime with C-field super-flux of the form (133), the lS^4-Bianchi identities dG4 = 0 and dG7 = 1/2 G4∧G4 hold if and only if the Einstein, Rarita-Schwinger, Maxwell-Chern-Simons, and duality equations of 11D supergravity hold rheonomically on superspace. Here lS^4 is the characteristic L∞-algebra with generators v3 and v6 and the single non-trivial bracket [v3,v3] = v6; it is the rational Whitehead algebra of the 4-sphere. Because these duality-symmetric Bianchi identities are equivalently closure conditions for L∞-valued differential forms, the paper turns them into global field data: a choice of classifying sp","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Higher Superspace Supergravity and its IR-Completions","paper_submitted_at":"2026-07-22T15:58:12+00:00"},{"claim_id":905969,"arxiv_id":"2607.19958","paper_version":1,"claim_text":"The Wheeler-DeWitt equation is presented not as a law of nature but as an artifact of applying constrained Hamiltonian quantization to gravity while discarding gauge degrees of freedom and assuming asymptotic boundary conditions in the path integral. Refusing those assumptions, the paper derives a mathematical Schrödinger equation for the extended phase-space wave function, then, using the gauge condition as a quantum constraint, a physical Schrödinger equation whose Hamiltonian depends explicitly on the chosen gauge condition. The wave function gives the probability amplitude for the geometry of the Universe as it appears to an observer in the reference frame fixed by that gauge condition.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"What may come beyond the Wheeler-DeWitt approach?","paper_submitted_at":"2026-07-22T09:34:11+00:00"},{"claim_id":910148,"arxiv_id":"2607.19602","paper_version":1,"claim_text":"The central claim is that a first-quantised wavefunction on a 2^L-point lattice carries a built-in generalised uncertainty principle. The low-energy version reduces to the Heisenberg principle as ΔL/ℏ→0, but for finite ΔL yields three momentum-dependent regions; a wavepacket can reach zero position uncertainty at a finite momentum spread. The high-energy version begins from p^H_x = Σ κ_{n-1} p_x^n. Setting the κ to the special-relativistic series p/√(1−p²/m²c²) and assuming point-momentum behaviour (δp^(n)_x = 0) gives δx δp^H ≥ (ℏ/2)[1 + τ_2 (δp^H)² + ...], with τ_2 = 3/(2m²c²) − (ΔL)²/(2ℏ²). In the continuous limit ΔL→0 this is a quadratic GUP with β_m = 3ℏc/(2Gm²), so (δx)_min = (√3/√2)ℏ/","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Quantum Gravity Simulation: Quantum simulation with a minimum length based on the generalised uncertainty principle","paper_submitted_at":"2026-07-21T22:05:21+00:00"},{"claim_id":912050,"arxiv_id":"2607.19221","paper_version":1,"claim_text":"The paper's load-bearing claim is that the GKNS quadrangular ensemble forms a universality class absent from dynamical triangulations: its percolation critical exponents are ν=1.588(17), γ=2.83(2) at p0=0.4851(13), deviating from ordinary percolation (ν=4/3, γ=43/18), and its asymptotic Hausdorff dimension is ΔH≈2, while DQ and GQ have ΔH≈4. The abstract concludes: 'GKNS and GQ define distinct classes of random geometry, implying a different underlying measure in the space of random surfaces and a possible geometric framework for a new class of noncritical string theories.' If correct, these ensembles genuinely extend the taxonomy of two-dimensional random geometry.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Statistical properties of quadrangular surfaces","paper_submitted_at":"2026-07-21T15:51:14+00:00"},{"claim_id":914253,"arxiv_id":"2607.19141","paper_version":1,"claim_text":"The paper establishes a direct link between gravity-induced entanglement (GIE) of two quantum clocks and the quantum formulation of local position invariance. For two identical clocks trapped at a fixed separation, the effective Hamiltonian places the rest Hamiltonian and the gravitational Hamiltonian as operator-valued masses. The central theorem states: entanglement is generated from an eigenstate of the rest Hamiltonian if and only if the rest and gravitational Hamiltonians do not commute—i.e., if and only if there is a genuinely quantum violation of LPI. In the complementary scheme with an equal superposition initial state, the entanglement oscillates at a frequency ω̃e = G ΔẼ²/(2ℏc⁴ℓ₀)","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Gravity-Induced Entanglement of Quantum Clocks as a Signature of Genuinely Quantum Local Position Invariance","paper_submitted_at":"2026-07-21T14:34:40+00:00"},{"claim_id":922311,"arxiv_id":"2607.18398","paper_version":1,"claim_text":"The paper's central claim is that the pattern of SMEFT coefficients at an asymptotically safe gravity-matter fixed point is dictated by the maximal global symmetry of the free kinetic terms. For the fermion sector, that is a U(N_W) symmetry rotating all Weyl fermions into each other. The single four-fermion interaction compatible with this symmetry - the axial current interaction - has a nonzero, irrelevant fixed point (the shifted Gaussian fixed point), and six of the seven studied couplings inherit nonzero values through this symmetry. The mixed-chirality coupling c+_quqd, which is incompatible with U(N_W), vanishes at the fixed point. The paper shows that this coupling can be promoted to","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"The fermion sector of the SMEFT from asymptotically safe gravity","paper_submitted_at":"2026-07-20T18:00:12+00:00"},{"claim_id":930415,"arxiv_id":"2607.17520","paper_version":1,"claim_text":"For the time-radial covariant quantum black hole metric, the Hawking temperature remains exactly T = 1/(8πM), identical to Schwarzschild. The quantum corrections act only on the effective potential barrier that emitted particles must cross. In the low-mass regime, the greybody factors for scalar, spin-half neutrino, and graviton modes deviate from their Schwarzschild counterparts, while photon greybody factors remain essentially unchanged. Consequently the mass-loss rate is suppressed for scalar and graviton emission, enhanced for neutrino emission, and nearly equal to Schwarzschild for photons. For larger black hole masses, the quantum corrections become negligible and all results converge","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Evaporation and fate of covariant quantum black holes","paper_submitted_at":"2026-07-20T03:54:59+00:00"},{"claim_id":948802,"arxiv_id":"2607.15551","paper_version":1,"claim_text":"The paper's central claim is that the decay of quantum coherence of an inertial two-level detector coupled to a Lorentz-violating vacuum is controlled by the detector's rapidity β. For a Lorentz-invariant field the transition rates are β-independent, giving coherence C = |sinθ| e^{−γ0τ/2}. With a modified dispersion ω_|k| = |k| f(|k|/M*), the rates γ± acquire a step-function threshold that depends on β, and coherence becomes C = |sinθ| e^{−(c+ + c−) γ0 τ/2}, with c± functions of β. For a polymer-quantized scalar field, f(g) dips below unity and the excitation channel switches on abruptly when the resonance condition on β is met, producing a pronounced drop in coherence at βc ≈ 1.3675. This t","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Probing Lorentz-invariance-violation with quantum coherence of Unruh-DeWitt detector","paper_submitted_at":"2026-07-17T01:51:09+00:00"},{"claim_id":954674,"arxiv_id":"2607.15007","paper_version":1,"claim_text":"Central claim: the homology of a simplicial complex built from an observer's local measurements reproduces the topology of the accessible spacetime region even when quantum fluctuations make geometric regions ill-defined. Vertices are time intervals during which some detector is active; a k-simplex is a set of k+1 measurement events that share a common active detector and span a time window no larger than Λ. Shared detector activity stands in for overlapping open sets, so the complex plays the role of a nerve construction. The paper checks the construction on a 2+1 spacetime with and without a hole, getting the expected Betti numbers, and uses persistent homology over the threshold θ and the","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Observers, local measurements, and topology","paper_submitted_at":"2026-07-16T13:53:06+00:00"},{"claim_id":956170,"arxiv_id":"2607.15324","paper_version":1,"claim_text":"On the paper's own terms, the central discovery is that the quasinormal spectrum of the rotating LQG black hole separates into opposite trends: quantum deformation (P and, weakly, a0) lowers the real part of the frequency and broadens the effective potential barrier, whereas rotation a raises the frequency and at high spin reverses the spin-dependence of the damping rate. This is obtained by reducing the scalar Klein–Gordon equation, under the slow-rotation approximation, to a Schrödinger-like radial equation with effective potential Vℓ(r) = Δ(r)/(r²+a²)² [ℓ(ℓ+1) + 2M(r)r/(r²+a²)], where Δ(r) = r²F_LQG(r;P)+a² encodes the quantum-deformed radial sector. The authors compute complex frequencie","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Quasinormal Modes of Self-Dual Loop Quantum Gravity Corrected Kerr Black Holes","paper_submitted_at":"2026-07-16T09:48:22+00:00"},{"claim_id":957721,"arxiv_id":"2607.14746","paper_version":1,"claim_text":"The paper's central claim is that the strong-field imprints of self-dual loop quantum gravity do not stay hidden in the near-horizon region: they feed into the orbital phase and therefore into the gravitational-wave signal over the long EMRI inspiral. Using geodesic evolution and leading-order quadrupole radiation reaction, the authors generate waveforms for both the static and the rotating LQG-corrected geometry and find phase deviations that grow with time. Quantitatively, their Fisher matrix analysis on a geometrically defined observable vector yields fiducial constraints a = 0.902^(+0.0042)_(-0.0041), P = 0.030 ± 0.00015, and a0 = 21.4^(+23)_(-15), leading them to conclude that EMRI obse","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Orbital Dynamics and Gravitational-Wave Signatures of EMRIs in Self-Dual Loop Quantum Gravity Black Holes","paper_submitted_at":"2026-07-16T09:29:44+00:00"},{"claim_id":962380,"arxiv_id":"2607.14213","paper_version":1,"claim_text":"The central discovery is the exact formula (3.12): U_QG = ∫ dβ_obs μ(β_obs,u1,m) e^{-β_obs H}, where the measure μ is obtained by integrating out the fluctuating JT boundary, the massive worldline, and the einbein modulus. The measure is assembled from the AdS heat kernel for the worldline and from Wheeler-de Witt wavefunctions of JT gravity in the chordal-distance basis, and is therefore an ordinary one-dimensional integral. At large mass or small β the integral is dominated by a saddle point at which β_obs equals the geodesic distance between the anchor points; the variance around this saddle separates into a Brownian term ~ β*/m and a quantum-gravity term that scales as β/φ_r (weak backre","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:22.060918+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"JT gravity on the worldline","paper_submitted_at":"2026-07-15T18:00:02+00:00"},{"claim_id":792804,"arxiv_id":"2607.13012","paper_version":1,"claim_text":"The central claim is that in a canonically quantized flat FLRW universe with dust as internal time, the back-reaction of each electromagnetic mode on the quantum geometry produces a mode-dependent dispersion relation whose photon group velocity is always less than one. Concretely, the modified dispersion is determined by a factor F(k,T) = [⟨V^{-1}⟩_k ⟨V^{1/3}⟩_k / (⟨V^{-1}⟩_o ⟨V^{1/3}⟩_o)]^{1/2} multiplying the standard frequency, and the measured 3-velocity is V = F (1 - E d/dE log F). The authors show analytically and numerically that for LQC, F < 1 and V < 1 for all accessible times and momenta, with V → 1 - 2ε as k → 0 (ε ∝ ℏ k / p_T), and ∂V/∂k < 0, meaning bluer modes travel slower. In","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Prism Effect in Quantum Gravity","paper_submitted_at":"2026-07-14T17:53:07+00:00"},{"claim_id":801771,"arxiv_id":"2607.12022","paper_version":1,"claim_text":"Strong-to-weak spontaneous symmetry breaking occurs for the BTZ black hole and is dual to wormhole geometries that join the two thermofield-double copies; equivalently, SWSSB is the emergence of global symmetries under ensemble averaging, which in turn suggests a new swampland conjecture for ensemble-averaged quantum gravity.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:22.060918+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Strong-to-Weak Spontaneous Symmetry Breaking from Wormholes in Holography","paper_submitted_at":"2026-07-13T18:00:01+00:00"},{"claim_id":770947,"arxiv_id":"2607.10663","paper_version":1,"claim_text":"Among seven explicitly defined deformations of a four-qubit product-EPR holographic code, only the matter-controlled bond-moving generator produces a leading quadratic logical-state dependence of the boundary entropy. After a state-independent physical recovery is fixed by coherent-information optimization, a nonzero variational proto-area survives, and a certified quadratic boundary witness—obtained by projecting the stabilizer-Rényi form away from all pairwise Pauli tangents—is strictly positive solely for that generator and zero for the six comparisons.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Certified boundary-magic witness for state-dependent proto-area in a holographic code","paper_submitted_at":"2026-07-12T09:16:46+00:00"},{"claim_id":663711,"arxiv_id":"2607.08134","paper_version":1,"claim_text":"Functional renormalization-group constructions of gravity and loop quantum gravity can remain distinct quantum theories, the former best suited to scale-dependent continuum phenomenology and the latter to ultraviolet completion of classically singular regimes; matching Bekenstein–Hawking entropy and the continuum limit then identifies the undetermined LQG parameters as G_LQG = g_* G and γ = γ_0 / g_*.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Field Theoretic Aspects of Gravity From Direct Action to Quantum Fields","paper_submitted_at":"2026-07-09T06:10:22+00:00"},{"claim_id":669994,"arxiv_id":"2607.06657","paper_version":1,"claim_text":"Once redundant off-shell contributions are absorbed by field redefinitions in an essential scheme, the proper-time beta function for Newton's constant becomes independent of both gauge parameters of the general linear gauge (to third order in the coupling in the four-derivative truncation, and to all orders in the coupling and the Ricci scalar on a sphere), and the resulting essential flow still exhibits a gauge-independent non-Gaussian fixed point.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Towards gauge independence in asymptotically safe quantum gravity","paper_submitted_at":"2026-07-07T18:00:00+00:00"},{"claim_id":687827,"arxiv_id":"2607.03969","paper_version":1,"claim_text":"The critical anomalous dimension γ_c, fixed by requiring that the holographically shifted bulk mass sit exactly at the Breitenlohner-Freedman bound, is the threshold that forces dual scaling dimensions into the complex principal series Δ_dS = d/2 ± iμ after Wick rotation to de Sitter space; the resulting log-periodic spacing Δ ln f = 2π/μ in the stochastic gravitational-wave background is therefore a direct imprint of OPE associativity.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.85,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"From OPE Associativity to Gravitational Wave Signatures: Critical Dimensions and AdS/dS Transition","paper_submitted_at":"2026-07-04T18:01:56+00:00"},{"claim_id":695172,"arxiv_id":"2607.03272","paper_version":1,"claim_text":"In unimodular cosmology, energy exchange between a scalar field and a bath of harmonic oscillators (quantum-gravity defects) produces an Ohmic diffusion equation that drives an initially vanishing cosmological constant to a positive asymptotic value Λ∞ = (γ mp Hd)/2, thereby generating the observed dark energy from primordial dissipation alone.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:22.060918+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Dark energy genesis: modeling dissipative effects in primordial cosmology","paper_submitted_at":"2026-07-03T12:40:38+00:00"},{"claim_id":696227,"arxiv_id":"2607.03199","paper_version":1,"claim_text":"CRT is not a gauge symmetry of quantum gravity in general. It is an asymptotic gauge symmetry in asymptotically flat and AdS space, acting on the boundary Hilbert space exactly as continuous isometries and scalar charges do. In eternal de Sitter it can be viewed as spontaneously broken only if an Alice d-3 brane is allowed inside the thermofield-double Hilbert space and the underlying quantum mechanics is time-independent; in realistic Big Bang cosmologies the symmetry is simply absent because initial conditions force small uncorrelated causal diamonds.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Singularities, Entropy and the Arrow of Time, {\\it or} Is CRT a Gauge Symmetry in Quantum Gravity?","paper_submitted_at":"2026-07-03T11:08:01+00:00"},{"claim_id":10679,"arxiv_id":"2607.01930","paper_version":1,"claim_text":"We show analytically that, in the large N limit, the quantum magic of pure Kourkoulou-Maldacena (KM) states, dual to a quantum black hole with an end-of-world particle behind the horizon, is linear in N with a slope, depending on the black hole temperature, that can be tuned between zero and 1/2.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Tuning quantum magic of pure quantum chaotic states with a gravity dual","paper_submitted_at":"2026-07-02T09:25:32+00:00"},{"claim_id":10667,"arxiv_id":"2607.01873","paper_version":1,"claim_text":"We prove that Lubkin-Page typicality bounds, which demonstrate vanishing mutual information for generic states in Type I algebras, survive for all Type II von Neumann factors. In the hyperfinite Type II₁ case with R ≅ A ⊗ B ⊗ E, the mutual information I(A:B) vanishes as O((d_A d_B / d_E)^2) when d_A d_B ≤ d_E in finite-dimensional approximations. For Type II_∞ factors including crossed-product gravitational algebras, the bound includes additional exponential suppression governed by the Bekenstein-Hawking entropy.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Lubkin-Page typicality bounds for Type~II von~Neumann factors","paper_submitted_at":"2026-07-02T08:27:45+00:00"},{"claim_id":10583,"arxiv_id":"2607.01653","paper_version":1,"claim_text":"The central claim is that the hybrid ITE-TR-FALQON protocol, formed by merging the imaginary-time evolution of ITE-FALQON with the time-rescaling mechanism of TR-FALQON, is both necessary and sufficient to prepare the thermofield double ground state of the Maldacena-Qi model from simple initial states, yielding fidelities near unity and reproducing the exact entropy spectra of the target state.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Preparing a Thermofield Double State with Feedback Quantum Algorithms","paper_submitted_at":"2026-07-02T03:25:37+00:00"},{"claim_id":8115,"arxiv_id":"2607.01393","paper_version":1,"claim_text":"The canonical equivalence among their standard characterizations - as eigenstates of the annihilation operator, displaced vacuum states and minimum-uncertainty wave packets - is generically lost in the presence of a minimal length. Minimal-length effects induce nontrivial deformations of phase-space trajectories and give rise to an intrinsic squeezing mechanism with no counterpart in ordinary quantum mechanics.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"signals","confidence":0.8,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Coherent states in minimal-length Quantum Mechanics: inequivalent characterizations and emergent squeezing","paper_submitted_at":"2026-07-01T18:52:30+00:00"},{"claim_id":8303,"arxiv_id":"2607.01385","paper_version":1,"claim_text":"The dynamics of canonically quantized JT gravity with finite Dirichlet boundaries is exactly equivalent to the scattering problem of a nonrelativistic particle in a repulsive Pöschl-Teller potential, yielding exact wavefunctions of the universe and a disk partition function interpreted as a transition matrix element between vanishing bare-length states; at finite cutoff the spectral measure exhibits genuinely nonperturbative corrections absent in T Tbar treatments.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:22.060918+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Quantum JT Gravity in a box as a P\\\"oschl-Teller Scattering Problem","paper_submitted_at":"2026-07-01T18:45:39+00:00"},{"claim_id":7995,"arxiv_id":"2607.01292","paper_version":1,"claim_text":"In models obeying the Covariant Entropy Bound, the favored initial states are those without localized excitations or consisting of one large black hole. To obtain a long radiation-dominated era, most horizon volumes must contain tiny black holes that decay into radiation, while a random population of horizon-sized black holes supplies dark matter. A suitable distribution of these primordial black holes accounts for all dark matter and seeds the early galaxies seen by the James Webb Space Telescope, with possible additional dark matter in Planck-scale remnants. The construction uses both approximate solutions to general relativity and a speculative quantum-gravity model whose hydrodynamics re","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:38.751576+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound?","paper_submitted_at":"2026-07-01T12:55:37+00:00"},{"claim_id":627138,"arxiv_id":"2606.31678","paper_version":1,"claim_text":"Both the Schrödinger evolution under the quantized Lense-Thirring Hamiltonian and the on-shell action of linearized quantum gravity in the stationary-phase approximation yield identical entanglement phases for the rotational degrees of freedom of the source and the paths of the test particle; this common phase equals the proper-time difference between the arms and is modified by gravitational retardation, thereby furnishing an explicit, relativistically causal description within linearized gravity.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:37.272541+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Relativistic Gravity-Induced Entanglement via Frame Dragging","paper_submitted_at":"2026-06-30T13:55:26+00:00"},{"claim_id":624126,"arxiv_id":"2606.31559","paper_version":1,"claim_text":"The analysis of how spacetime emerges from quantum gravity is incomplete because it fails to interpret the dynamical and quantum aspects of these theories, which differ from standard quantum theory; without showing how these aspects can fulfill spacetime roles, spacetime functionalism provides no help and the emergentist position remains unsupported by any successful reduction example.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:37.272541+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"The Dynamics of Quantum Gravity: the Missing Piece in the Spacetime Emergentist Account","paper_submitted_at":"2026-06-30T12:16:28+00:00"},{"claim_id":623030,"arxiv_id":"2606.30853","paper_version":1,"claim_text":"This paper presents a curated selection of research questions at the intersection of quantum gravity and quantum information, chosen to highlight issues that we regard as particularly important for researchers in both fields. We organize the discussion into four main themes: the operational characterization of observables, the role of observers, quantum error correction, and the infinite-dimensionality of Hilbert spaces. We hope that addressing these questions will engage researchers across both communities and further strengthen the profound interplay between the two disciplines.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:37.272541+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Rethinking quantum information in gravity and fields","paper_submitted_at":"2026-06-29T19:34:06+00:00"},{"claim_id":599758,"arxiv_id":"2606.29318","paper_version":1,"claim_text":"We provide a field-theoretic construction of Padmanabhan's duality-invariant Feynman propagator for a massive point particle in Euclidean space R^D. Padmanabhan's propagator includes quantum-gravity effects due to the existence of a quantum of length ℓ. Including O(ℓ²) corrections, the corresponding field-theory model turns out to be a free, massive scalar defined in R^{D+2}. The two additional dimensions with respect to the original R^D provide the necessary room for quantum-gravity fluctuations.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:37.272541+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"On Padmanabhan's duality invariance and the quantum of length","paper_submitted_at":"2026-06-28T10:24:15+00:00"},{"claim_id":599822,"arxiv_id":"2606.29307","paper_version":1,"claim_text":"We adapt the extended Anderson-Candelas-Christensen-DeWitt approach to compute the scalar vacuum polarization ⟨φ²⟩ exterior to the quantum-corrected LQG black hole geometry. The quantum-gravity exponent ε enhances the near-horizon polarization and induces, farther out, a small negative tail that we identify through a parameter-free DeWitt-Schwinger comparison with the field's response to the nonzero curvature of the background. The correction scales linearly with ε.","claim_key":"core","tier":"stated","source":"verdict_pith","method":"phrase","confidence":0.9,"assigned_at":"2026-08-11T03:35:37.272541+00:00","lean_module":null,"lean_decl":null,"lean_status":null,"reality_plus_commit":null,"paper_title":"Scalar Vacuum Polarization in Loop Quantum Gravity Black Holes","paper_submitted_at":"2026-06-28T10:03:54+00:00"}]}