Full text
The Big Start: Cosmogenesis from a Finite Planck-Phase Boundary Ridwan Sakidja Department of Physics, Astronomy and Materials Science Missouri State University Abstract The standard Big Bang picture assumes that spacetime already exists at the moment of origin and is driven to a singular state of infinite curvature and infinite density. The Curvature Transport Correspondence (CTC) offers a different beginning in which the vacuum is a physical medium with stiffness that controls whether curvature or fields can exist at all. This leads to the Big Start, a finite radius Planck phase vacuum state where gravitational transport is saturated and no geometric degrees of freedom are present. This state is a pre geometric and zero entropy vacuum, directly realizing the insight of Sir Roger Penrose that the Universe must begin in an exceptionally ordered condition. As expansion relaxes vacuum stiffness, the layers of physics appear in sequence: curvature mobility at rG, transverse and quantum modes at rT, Higgs condensation and the appearance of mass at rH, and finally a classical FRW spacetime at rS. Cosmogenesis and gravitational collapse follow the same divergence law in opposite directions, and the Big Start replaces the classical singularity with a natural vacuum phase transition in which spacetime, gravity, quantum behavior, and mass appear only when the vacuum becomes soft enough to support them 1. Introduction Classical general relativity allows the Universe to begin from zero volume and infinite curvature, but such a continuation contradicts the physical limits of the vacuum. In a transport-based formulation of curvature, introduced in the first paper on CTC [1], the curvature of any field ๐is generated by the divergence of an associated transport flux ๐น๐๐: ๐ถ[๐]=โ๐๐น๐๐.(1) When applied to gravity, this general relation yields the effective curvature source ๐eff=โ๐๐น๐บ๐,(2) identifying gravitational curvature as the vacuumโs response to transport imbalance rather than the product of intrinsic material density. In the second paper of CTC[2], we showed that the vacuum possesses a finite, phase-dependent stiffness that limits how much curvature it can support. This leads to the saturation principle โฃโ๐๐น๐บ๐โฃโค๐ทPl,(3) which imposes a maximum admissible flux divergence. This bound prevents curvature from diverging and therefore forbids singularities. Instead of collapsing to a point, the vacuum reaches a saturation radius, a finite region in which curvature attains its upper limit and cannot increase further. The same saturation mechanism also produces dark-matterโlike phenomena, resolves the hierarchy problem, and eliminates singularities inside black holes.
In this third paper of CTC, we apply this framework to the origin of the Universe. We demonstrate that the Big Bang singularity is replaced by a finite-radius Planck-phase bubble, a saturated region in which curvature reaches its allowable maximum. Cosmogenesis therefore begins not from a point of infinite curvature, but from the boundary of this finite Planck-phase domain. We will also examine the ontology of black-hole interiors and show how the same saturation principle links the structure of a black-hole core to the origin of the Universe. For clarity, we note that the CTC cosmogenesis mechanism differs fundamentally from the standard Big Bang with inflation [3], [4], [5], [6], [7] as well as from other nonsingular proposals[8], [9], [10], [11], [12], [13], [14] [15], [16]. Among the many ideas proposed to address the origin of the Universe, two frameworks are especially relevant for comparison because they touch on similar questions of initial simplicity and the replacement of the singularity. The first is Penroseโs Conformal Cyclic Cosmology[17], [18], which seeks to achieve a low entropy beginning through conformal identification between successive aeons. CTC shares the motivation for an initially simple state but obtains it through a physical mechanism: the early vacuum is a perfectly rigid phase with no degrees of freedom (DOF), and cosmogenesis begins when its stiffness relaxes, with no role for conformal matching. The second is the class of finite radius black hole core cosmogenesis models[19], [20], in which the singularity is replaced by a finite domain that births a new cosmological region. Although both approaches replace the singularity with a finite radius structure, the underlying physics is entirely different. In CTC, the finite radius arises from saturation of curvature transport in a degree of freedom free vacuum, not from black hole interior dynamics or quantum gravitational effects. 2. The Divergence Law and Vacuum Saturation CTC reinterprets gravitational curvature not as a direct response to โmass,โ but as the vacuumโs transport reaction to flux loading. In this formulation, curvature is present only to the extent that the effective density ๐eff=โ๐๐น๐บ๐ is nonzero. However, the vacuum cannot transmit arbitrarily large curvature. Just as real materials cannot sustain unlimited stress or strain, the vacuum possesses a finite curvature-carrying capacity characterized by a universal bound: โฃโ๐๐น๐บ๐โฃโค๐ทPl. When the divergence of the gravitational flux approaches this limit, the vacuum enters a saturated regime in which its normal dynamical degrees of freedom (DOF) cannot operate. In this Planck phase: โข curvature cannot increase beyond the saturated value, โข gravitational propagation shuts down, โข transverse gauge modes cannot exist, โข the Higgs condensate cannot form, โข mass and gauge interactions lose meaning, and โข quantum fluctuations are suppressed, since oscillatory modes require finite vacuum stiffness. From this perspective, there are potentially two extreme gravitational situations which drive the vacuum into this saturated state: 1. Black-hole collapse, where the inward flux loading yields
โ๐๐น๐บ๐โโ๐ทPl, 2. Cosmogenesis, where the primordial vacuum begins fully outward-loaded at โ๐๐น๐บ๐=+๐ทPl. The same divergence law governs both phenomena, differing only in the direction of flux loading. Let us examine these two cases in the following section. 3. Saturation in Black Holes and Cosmogenesis Although black holes and the birth of the Universe appear to represent opposite gravitational extremes, CTC reveals that they are controlled by a single underlying mechanism: vacuum saturation under flux divergence, with opposite signs of loading determining the physical outcome. Black holes reach saturation through inward compression; cosmogenesis begins from a fully outwardloaded saturated state. 3.1. Back Holes: Inward Loading to Saturation During gravitational collapse, the inward gravitational transport flux intensifies and the divergence โ๐๐น๐บ๐becomes increasingly negative. In the CTC framework, curvature cannot grow without bound. As shown in the second CTC paper[2], the transport field reaches a universal saturation limit ๐พmax, defined by ๐พ(๐๐ )=๐พmax, with the interior curvature profile ๐พ(๐)=48๐บ2 ๐(๐)2 ๐4๐6. Solving (3โ23) yields ๐๐ 3โผโ48๐บ2๐(๐๐ )2 ๐4๐พmax โน๐๐ โ๐1/3. This is the general result from the second CTC paper[2]: once the saturation limit is reached, the curvature no longer increases and additional mass enlarges the volume of the saturated region rather than deepening the collapse. Planck Phase Interpretation In the present work, we further identify the saturation value ๐พmax with the Planck curvature scale, ๐พmax=๐พPlโผ1 โPl 4, so that the saturated region corresponds to a Planck-phase vacuum. Because ๐พPl is extraordinarily large, the radius ๐๐ obtained by substituting ๐พPl into the ๐๐ 3 formula is extremely small. For stellar-mass black holes this yields radii on the order of
๐๐ โผ10โ23โ10โ25 m, many orders of magnitude smaller than both the Schwarzschild radius and any physical length scale relevant to astrophysical collapse. Thus, even though the scaling ๐๐ โ๐1/3 remains valid, the absolute size of the saturated region is microscopic whenever ๐พmax is identified with the Planck scale. Physical Implications Because the corresponding radius is so small, ordinary stellar or supermassive black holes do not come close to reaching the saturation boundary. Their interior curvature remains many tens of orders of magnitude below ๐พPl. Therefore, a Planck-phase core forms only if collapse drives the transport divergence so far inward that it reaches the theoretical limit ๐พ๐๐. In realistic astrophysical environments this never occurs. That said, if saturation were actually reached, the interior would enter a rigidity-dominated Planck phase in which: โข curvature is fixed at ๐พPl, โข gravitational transport ceases, โข the Higgs mechanism and the concept of mass are undefined, โข gauge fields cannot propagate, and โข quantum oscillatory modes are suppressed. General relativity remains valid only outside this microscopic, saturated region meaning that in realistic astrophysical collapse, the transport field never approaches this saturation limit, so the Planck-phase boundary is never reached. The interior vacuum therefore remains in the ordinary, dynamical phase, and gravity remains fully active throughout the black-hole interior except at the classical singularity predicted by general relativity. 3.2 Cosmogenesis: Outward Loading at Saturation In contrast to black holes, where inward transport loading must climb toward saturation, the early Universe begins already at the saturation boundary. The primordial vacuum is fully outward-loaded, such that โ๐๐น๐บ๐=+๐ทPl, is the positive extremum of the divergence law. In this regime the vacuum occupies its rigiditydominated Planck phase from the outset. Unlike gravitational collapse, which never attains this limit in practice, cosmogenesis starts precisely where the transport field is saturated. Because the total effective flux load of the Universe is enormous, ๐๐โผ1053 kg, a value consistent with standard cosmological estimates [7], [21], [22], the corresponding saturated radius is not microscopic but macroscopic. Substituting this mass into the saturation relation [2]: ๐birth 3 โผโ48 ๐บ2 ๐๐ 2 ๐4 ๐พmax ,โ๐birth โ๐๐ 1/3
and identifying the saturation curvature with the Planck value ๐พmax=๐พPl, yields ๐ birthโผ10โ6โ10โ4 m=1ฮผmโ100 ฮผm, a finite physical scale at which the early vacuum can support the total outward flux load while remaining at the saturation curvature ๐พmax. This radius is neither zero nor arbitrarily small: it is exactly the size required for a fully saturated Planck-phase vacuum containing the entire cosmic flux content for a given mass. This leads to a contrasting structural picture: โข Black holes attempt to reach saturation through inward collapse but never attain it in practice; if they did, their saturated radii would be microscopic. โข The Universe, by contrast, begins already at saturation, with a macroscopic radius ๐birth determined directly by its total flux load. As expansion proceeds and the vacuum softens, the Planck-phase boundary recedes, the transport field becomes unsaturated, and familiar field-theoretic degrees of freedom, including mass, gauge fields, and quantum fluctuations gradually emerge. Cosmogenesis is therefore the outward evolution of an initially saturated Planck-phase core into a progressively softer vacuum capable of supporting the physics we observe today. 3.3. The Big Start: A Finite-Radius Planck-Phase Beginning In the CTC picture, the Universe does not begin at a singularity. It begins as a finite spherical region of fully saturated, Planck-phase vacuum. In this state: โข gravity cannot propagate, โข electromagnetism does not exist, โข quantum fluctuations are absent, โข the Higgs field is uncondensed, โข matter and radiation cannot form. Physics, as we know it, has not yet begun. Cosmogenesis starts only when the saturated vacuum softens and the divergence of the transport flux drops below the bound, โฃโ๐๐น๐บ๐โฃ<๐ทPl. This transition is not explosive. It is a transport-driven unjamming of an extremely stiff, or vacuum relaxation that gradually restores propagating degrees of freedom (DOF) and allows the Universe to enter the dynamical phase described by physics. 4. Phase-Ordered Cosmogenesis: The Sequence of Emergence As the Universe expands from its saturated beginning, the vacuum softens in distinct steps. Each softness threshold corresponds to a characteristic radius at which a new class of physical degrees of freedom becomes possible: ๐birth<๐๐บ<๐๐<๐๐ป<๐๐. These radii reflect the order in which the vacuum becomes capable of supporting curvature, waves, quantum behavior, mass, and finally causal cosmological evolution.
4.1. ๐๐๐ข๐ซ๐ญ๐ก โ End of Saturation (No Modes Exist) For radii smaller than ๐birth, the vacuum remains in its Planck phase. This phase is defined by complete saturation of the transport flux, expressed by โฃโโ
๐น๐บโฃ=๐ท๐๐. This condition forces the curvature transport field ๐น๐บto maintain its maximal divergence everywhere within the region. A saturated flux cannot support spatial variation. As a result, no curvature degrees of freedom are available. The vacuum in this regime behaves as an ideal medium of infinite rigidity, unable to deform in any direction. The stiffness tensor in this phase is effectively ๐พ๐๐(๐<๐๐๐)=โ ๐ฟ๐๐, and any attempt to introduce a displacement field ๐ข๐leads to an unbounded energetic penalty. The Lagrangian density ๐ฟ๐๐=1 2๐(โ๐ก๐ข๐)2โ1 2๐พ๐๐(โ๐ข๐)(โ๐ข๐), becomes ill defined in the limit ๐พ๐๐โโ. The medium can neither support gradients nor allow finite strain. In this saturated phase: โข no displacements can occur, โข no gradients can form, โข no oscillations are possible, โข no waves can propagate, โข no dynamical fields exist. The Planck phase therefore represents a state in which spacetime has no internal degrees of freedom and no capacity to host physical modes of any kind. 4.2 ๐๐ฎ: Emergence of Gravity Through Longitudinal Mobility After the radius grows beyond ๐๐๐ฅ, the vacuum leaves the fully saturated Planck phase. The divergence bound remains in force, โฃโโ
๐น๐บโฃโค๐ท๐๐, but saturation no longer holds. The stiffness tensor begins to relax from its infinite value, ๐พ๐๐(๐>๐๐๐)<โ, giving the vacuum a small, nonzero capacity for deformation. This relaxation is anisotropic: the radial direction softens first while the angular directions remain locked. This directional asymmetry sets the stage for the first dynamical mode. The radius ๐๐บ thus marks the moment when this partial relaxation becomes strong enough to permit radial motion. Only the longitudinal component of the displacement field ๐ข๐=(๐ข๐,๐ข๐,๐ข๐) is released, while the tangential components remain fixed. The vacuum therefore acquires exactly one mechanical degree of freedom (DOF). The stiffness tensor in this interval takes the form
๐พ๐๐(๐๐บ<๐<๐๐)=diag(๐พ๐ฟ, 0, 0), with a finite longitudinal modulus ๐พ๐ฟ>0 and vanishing angular terms. The corresponding Lagrangian density is thus: โ<๐๐=1 2๐(โ๐ก๐ข๐)2โ1 2๐พ๐ฟ(โ๐ข๐)2, and contains no terms involving ๐ข๐ or ๐ข๐. Because the vacuum has no transverse restoring force, the angular components cannot support oscillatory behavior. The only propagating distortion is longitudinal compression of the radial field, corresponding to curvature transport but not to a wave-supporting medium. This regime is therefore characterized by: โข a single dynamical direction, โข no transverse modes, โข no harmonic oscillators, โข no possibility of quantization. The field supports curvature response but cannot sustain electromagnetic or quantum-mechanical phenomena. Gravity in this domain is strictly longitudinal: curvature can be redistributed, but not in a form that admits a spectral decomposition or wave propagation. 4.3. ๐๐ป: Emergence of Electromagnetism and the Onset of Quantum Fluctuations At the radius ๐๐the vacuum undergoes a key change: it develops transverse stiffness. This means the vacuum can now support shear-like motion in the two angular directions. The stiffness tensor becomes ๐พ๐๐(๐>๐๐)=diag(๐พ๐ฟ,๐พ๐,๐พ๐),๐พ๐>0. Once ๐พ๐appears, the transverse components of the displacement field ๐ขโฅ=(๐ข๐,๐ข๐) become dynamical. Their Lagrangian has a kinetic term and an elastic term: ๐ฟโฅ=1 2๐ (โ๐ก๐ขโฅ)2โ1 2๐พ๐(โ๐2๐ขโฅ)2, where โ๐2is the covariant gradient on the sphere. The first term describes time-varying motion; the second describes angular shear. Varying this action gives the transverse wave equation: ๐ โ๐ก2๐ขโฅโ๐พ๐ ฮ๐2๐ขโฅ=0. Because ๐ขโฅhas two components, it cannot be expanded using scalar spherical harmonics alone. The correct basis is the set of vector spherical harmonics, which provide a complete basis for any vector field on a sphere (see Jackson Classical Electrodynamics[23]; Arfken & Weber[24]; or HobsonโEfstathiouโ Lasenby[25]).
We write: ๐ขโฅ(๐,๐,๐ก)=โ๐๐๐ (๐) ๐,๐,๐ (๐ก) ๐๐๐ (๐)(๐,๐),๐=1,2, where โข ๐=1gives the divergence-free (toroidal) family, โข ๐=2gives the curl-free (poloidal) family. Each vector spherical harmonic satisfies ฮ๐2๐๐๐ (๐)=โ๐(๐+1)๐๐๐ (๐). Substituting into the wave equation shows that every coefficient obeys an independent harmonicoscillator equation: ๐๓ฐ๐๐ (๐)+๐๐2 ๐๐๐ (๐)=0,๐๐2=๐พ๐ ๐ ๐(๐+1). Thus the vacuum at ๐๐supports an entire spectrum of transverse oscillatory modes. These are the mechanical precursors of electromagnetic waves and the first genuine quantum fluctuations. For each mode, the reduced Lagrangian is simply ๐ฟ๐๐ (๐)=1 2[๐๓ฐ๐๐ (๐) 2โ๐๐2๐๐๐ (๐) 2], with canonical momentum ๐๐๐ (๐)=๐๓ฐ๐๐ (๐). Quantization follows in the usual way: [๐๐๐ (๐),๐๐โฒ๐โฒ (๐โฒ)]=๐โ ๐ฟ๐๐โฒ๐ฟ๐๐โฒ๐ฟ๐๐โฒ. Defining creation and annihilation operators gives the standard oscillator Hamiltonian: ๐ป=โโ ๐,๐,๐ ๐๐(๐๐๐ (๐)โ ๐๐๐ (๐)+1 2). This is the first radius at which photons, zero-point motion, and vacuum fluctuations exist. Quantization is therefore not added by handโit appears automatically when the vacuum becomes mechanically able to support transverse oscillatory modes. With these degrees of freedom now present (Figure 1), the Higgs field becomes a well-defined quantum field, even though the vacuum is still in the symmetric electroweak phase and โจ๐ปโฉ=0.
Universe at r= rG Universe at r= rT Figure 1 Transition from the ๐๐บto the ๐๐threshold in the CTC emergence sequence. At radius ๐๐บ, the vacuum possesses longitudinal stiffness only, permitting scalar curvature transport but no transverse or oscillatory modes. At radius ๐๐, the vacuum acquires transverse stiffness, enabling the first quantum fluctuations and the emergence of electromagnetic degrees of freedom. The structured pattern on the right sphere represents one of the allowed transverse spherical modes. 4.4 ๐๐ป: Birth of Mass (Higgs Condensation) The radius ๐๐ปmarks the transition from the electroweak-symmetric phase to the broken phase in which the Higgs field acquires a nonzero vacuum expectation value. For all ๐๐<๐<๐๐ป, the Higgs exists as a quantum scalar with a symmetric potential and โจ๐ปโฉ=0. At ๐=๐๐ป, the Higgs condenses and โจ๐ปโฉ=๐ฃโ 0, giving mass to fermions and gauge bosons through the usual Standard Model mechanism. This marks the first radius at which massive degrees of freedom can exist. Before ๐๐ป, all excitations are massless despite the presence of photons and quantum fluctuations introduced at ๐๐. 4.5 ๐๐: Classical Causality and the Start of FRW Cosmology The radius ๐๐is reached only when gravity, quantum fields, and mass are all active simultaneously. Only beyond this point does the vacuum support a classical spacetime with meaningful light cones, timelike worldlines, and a well-defined stressโenergy tensor. Thus ๐๐ marks the beginning of the FRW causal regime. For ๐>๐๐, spacetime is described by the standard EinsteinโFRW equations and the Universe enters its familiar radiation-, matter-, and dark-energyโdominated eras. For ๐<๐๐, the necessary degrees of freedom for classical cosmology do not yet exist, and the FRW picture cannot be applied. 4.6. r_ฮ: Residual Flux and the Emergence of Dark Energy After the Universe has passed the sequence ๐Pl<๐๐บ<๐๐<๐๐ป<๐๐, Electromagnetism Quantum Fluctuation Gravity
[3] A. H. Guth, โThe Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems,โ Phys. Rev. D, vol. 23, pp. 347โ356, 1981, doi: 10.1103/PhysRevD.23.347. [4] A. D. Linde, โChaotic inflation,โ Physics Letters B, vol. 129, no. 3, pp. 177โ181, Sept. 1983, doi: 10.1016/0370-2693(83)90837-7. [5] V. Mukhanov, Physical Foundations of Cosmology. Oxford: Cambridge University Press, 2005. doi: 10.1017/CBO9780511790553. [6] A. Albrecht and P. J. Steinhardt, โCosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking,โ Phys. Rev. Lett., vol. 48, no. 17, pp. 1220โ1223, Apr. 1982, doi: 10.1103/PhysRevLett.48.1220. [7] Planck Collaboration et al., โPlanck 2018 results,โ A&A, vol. 641, 2020, doi: 10.1051/00046361/201833910. [8] A. Vilenkin, โCreation of universes from nothing,โ Physics Letters B, vol. 117, no. 1, pp. 25โ28, Nov. 1982, doi: 10.1016/0370-2693(82)90866-8. [9] J. B. Hartle and S. W. Hawking, โWave function of the Universe,โ Phys. Rev. D, vol. 28, no. 12, pp. 2960โ2975, Dec. 1983, doi: 10.1103/PhysRevD.28.2960. [10] A. Linde, โQuantum creation of an open inflationary universe,โ Phys. Rev. D, vol. 58, no. 8, p. 083514, Sept. 1998, doi: 10.1103/PhysRevD.58.083514. [11] A. Ashtekar, T. Pawlowski, and P. Singh, โQuantum Nature of the Big Bang,โ Phys. Rev. Lett., vol. 96, no. 14, p. 141301, Apr. 2006, doi: 10.1103/PhysRevLett.96.141301. [12] A. Ashtekar and P. Singh, โLoop quantum cosmology: a status report,โ Classical and Quantum Gravity, vol. 28, no. 21, p. 213001, Sept. 2011, doi: 10.1088/0264-9381/28/21/213001. [13] J. Khoury, B. A. Ovrut, P. J. Steinhardt, and N. Turok, โEkpyrotic universe: Colliding branes and the origin of the hot big bang,โ Phys. Rev. D, vol. 64, no. 12, p. 123522, Nov. 2001, doi: 10.1103/PhysRevD.64.123522. [14] P. J. Steinhardt and N. Turok, โCosmic evolution in a cyclic universe,โ Phys. Rev. D, vol. 65, no. 12, p. 126003, May 2002, doi: 10.1103/PhysRevD.65.126003. [15] M. Reuter and F. Saueressig, โQuantum Einstein gravity,โ New Journal of Physics, vol. 14, no. 5, p. 055022, May 2012, doi: 10.1088/1367-2630/14/5/055022. [16] A. Bonanno and M. Reuter, โCosmology with self-adjusting vacuum energy density from a renormalization group fixed point,โ Physics Letters B, vol. 527, no. 1, pp. 9โ17, Feb. 2002, doi: 10.1016/S0370-2693(01)01522-2. [17] R. Penrose, Cycles of Time: An Extraordinary New View of the Universe. Knopf Doubleday Publishing Group, 2011. [Online]. Available: https://books.google.com/books?id=gv8o1XydoCQC [18] M. Eckstein, โConformal Cyclic Cosmology, gravitational entropy and quantum information,โ General Relativity and Gravitation, vol. 55, no. 2, p. 26, Jan. 2023, doi: 10.1007/s10714-023-03070-2. [19] N. Popลawski, โUniverse in a Black Hole in Einstein-Cartan Gravity,โ \apj, vol. 832, no. 2, p. 96, Dec. 2016, doi: 10.3847/0004-637X/832/2/96. [20] V. P. Frolov, M. A. Markov, and V. F. Mukhanov, โBlack holes as possible sources of closed and semiclosed worlds,โ Phys. Rev. D, vol. 41, no. 2, pp. 383โ394, Jan. 1990, doi: 10.1103/PhysRevD.41.383. [21] Valev, โEstimations of Total Mass and Energy of the Observable Universe,โ Physics International, vol. 5, no. 1, pp. 15โ20, Jan. 2014, doi: 10.3844/pisp.2014.15.20. [22] D. W. Hogg, โDistance measures in cosmology,โ May 1999. [23] J. D. Jackson, Classical Electrodynamics. Wiley, 2021. [Online]. Available: https://books.google.com/books?id=6VV-EAAAQBAJ [24] G. B. Arfken, G. B. Arfken, H. J. Weber, and F. E. Harris, Mathematical Methods for Physicists: A Comprehensive Guide. Elsevier Science, 2013. [Online]. Available: https://books.google.com/books?id=qLFo_Z-PoGIC
[25] M. P. Hobson, G. P. Efstathiou, and A. N. Lasenby, General Relativity. 2006. doi: 10.2277/0521829518. [26] Planck Collaboration et al., โPlanck 2015 results,โ A&A, vol. 594, 2016, doi: 10.1051/00046361/201526681. [27] P. A. R. Ade et al., โImproved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season,โ Phys. Rev. Lett., vol. 127, no. 15, p. 151301, Oct. 2021, doi: 10.1103/PhysRevLett.127.151301.
Supplement Materials: Three Fundamental CTC Results and Their Planck Signatures The CurvatureโTransport Correspondence links the mechanical response of the vacuum to the structure of primordial perturbations. The divergence law governing curvature transport determines which modes can exist, how they evolve, and which components of curvature become active as the vacuum crosses the thresholds ๐Pl<๐๐บ<๐๐<๐๐ป<๐๐. From this structure follow three mathematical results that shape the primordial spectrum. Planck observations reveal the corresponding empirical signatures, without any additional assumptions or parameter tuning. The data simply reflect the emergence properties of the vacuum. S.1 Result 1: ModeโExistence Condition Before the vacuum reaches ๐๐, transverse stiffness is zero, ๐บ๐(๐ก<๐ก๐)=0, and no oscillatory solutions exist. This implies the primordial cutoff ๐โฅ๐min=1/๐๐. Planck signature Planck observes: โข disappearance of temperature correlations for angles ๐โณ60โ, โข suppression of power at low multipoles โโฒ20, and โข absence of long-wavelength modes. These results come from Planck 2015 XVI (Isotropy and Statistics of the CMB, A&A 594, A16, 2016)[26], which documents the large-angle anomaly and the vanishing correlation function beyond about sixty degrees. The same cutoff forbids any trans-Planckian oscillations in ๐(๐), consistent with Planck 2018 X (Constraints on Inflation, A&A 641, A10, 2020)[7], which finds no evidence of periodic modulation or logarithmic features. S.2 Result 2: StiffnessโTilt Relation Between ๐๐บand ๐๐ the stiffness softens, generating a tilted scalar spectrum, ๐(๐)โ๐๐๐ โ1,๐๐ <1, with monotonic negative running, ๐ผ๐ <0. Planck signature Planck 2018 VI (Cosmological Parameters, A&A 641, A6, 2020)[7] reports ๐๐ =0.9649ยฑ0.0042,๐ผ๐ โฒโ0.004, in agreement with the CTC prediction. In ฮCDM these values depend on slow-roll conditions; in CTC they follow directly from stiffness gradients in the vacuum.
S.3 Result 3: Tensor-Suppression Condition Before ๐๐บ, the vacuum supports only longitudinal curvature. Transverse gravitational modes do not exist, ๐บ๐(๐บ)(๐ก<๐ก๐บ)=0, and therefore the primordial tensor spectrum vanishes, ๐๐(๐)=0. Planck signature Joint BICEP/Keck + Planck results give ๐<0.036. This consolidated bound comes from the BICEP/Keck 2018 analysis (PRL 127, 151301, 2021)[27], which combines WMAP, Planck, and ground-based data to rule out detectable primordial gravitational waves. Inflation must finely tune its potential to achieve such small ๐. In CTC, tensor suppression is a structural consequence of the vacuumโs stiffness ordering. S.4 Combined Interpretation Taken together, the three CTC results provide a unified explanation of the full pattern of Planck observations. The mode-existence cutoff determines which perturbations can ever appear, removing all wavelengths longer than ๐๐and all sub ๐๐modes. The stiffnessโtilt relation fixes the shape of the scalar spectrum, generating both the observed tilt and the small but persistent negative running. The tensorsuppression condition eliminates primordial gravitational waves at their origin. When these three consequences are viewed as parts of a single emergence sequence ๐Pl<๐๐บ<๐๐<๐๐ป<๐๐, the signatures measured by Planck follow naturally. The low power on large angular scales, the smooth scalar spectrum with tilt and negative running, the absence of trans Planckian features, the lack of primordial tensors, and the slightly enhanced lensing amplitude all arise from the same underlying structure of the vacuum. No additional parameters or model adjustments are required. By contrast, the ฮCDM framework must introduce extra assumptions or extensions to account for these features individually. In CTC, they emerge automatically from the mechanical response of the vacuum as it evolves through the stiffness thresholds that mark the beginning of spacetime structure.