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Christian Rembe

Publications and source records attributed to Christian Rembe.

2 recordsLinked to original sources

Self-Gravitation of Mode Quanta in a Causal Resonator: One-Loop Finiteness in Linearized Quantum Gravity and the Emergence of the Dark-Energy Scale

Perturbative quantum gravity is ultraviolet divergent and, as shown by 't Hooft and Veltman, non-renormalizable. A recent object-relative, Lorentz-invariant weighting of internal electromagnetic modes renders selected one-loop contributions of quantum electrodynamics finite without counterterms. Here that weighting is derived rather than postulated: causality defines a mode resonator bounded by the Hubble radius and re-defined in every inertial frame, and the self-gravitation of each mode quantum deforms its spectrum. Applied to linearized gravity, the graviton self-coupling reaches order unity at the Planck wave number, so that the mode content available to a loop is suppressed beyond it. Any suppression exceeding a threshold fixed by the diagram renders the one-loop integrals finite; no cutoff is imposed and no mode structure above the Planck scale need be derived. For pure gravity the same power counting extends to every loop order, and the leading suppression already meets the resulting condition for every topology with more than one vertex; a single class of single-vertex insertions is excluded. The Bianchi identity takes the role of the Ward identity at one loop, and the transformation between the resonators of two inertial frames is unitary. The same finite mode content yields a vacuum energy density of order H^2/G, of the observed sign and magnitude, from the Planck and causal infrared wave numbers alone. A contribution tracking the instantaneous expansion rate is an exact rescaling of the gravitational constant and is excluded by primordial nucleosynthesis, so the mode basis must be frozen in any inertial system; referring it to the stationary de Sitter horizon fixes the remaining coefficient to the geometric value 6/pi and makes a value for the energy density of gravitational vacuum fluctuations possible which can be interpreted as origin of the dark-energy effect.

gr-qc

Object-relative ultraviolet weighting of electromagnetic modes and one-loop ultraviolet finiteness in quantum electrodynamics

This work explores whether localized electromagnetic interactions can be modeled in terms of an effective object-relative ultraviolet weighting of internal modes. The proposal is motivated heuristically by two considerations: a weak-field self-backreaction estimate for sufficiently localized energy-carrying modes and a three-dimensional overlap argument for localized interactions. In the resulting ansatz, the infrared sector remains unchanged up to a characteristic scale the at angular wavenumber $k_c$, while ultraviolet contributions are suppressed asymptotically by a factor of order $k_c^3/k^3$ with the angular wavenumber $k$. Because a crossover based solely on $k^μk_μ$ is not well suited to the intended mode-based interpretation, the weighting is formulated in terms of the object-relative covariant mode variable $u_μ k^μ$ with the four-velocity $u^μ$, i.e. the mode frequency measured in the rest frame of the localized interaction object. Within this restricted framework, selected one-loop QED contributions considered here become ultraviolet finite, and a restricted one-loop Ward-consistency check is preserved when the same scalar weighting is assigned consistently to the same internal photon mode in self-energy and vertex corrections. Four initial test cases are discussed: the anomalous magnetic moment, a Bethe-type low-energy Lamb-shift estimate, the Casimir effect, and a compact ultraviolet one-loop test. In the first three cases, the weighting leads to physically sensible characteristic scales associated with the electron Compton scale, an atomic bound-state scale, and plate distance, respectively. The results suggest that different observables may probe different effective localization scales. Action-level derivation, spectral consistency, and extension beyond one loop remain open problems.

quant-ph