A classification of admissible energy density profiles with bounded Kretschmann scalar yields a unified framework for regular static spherically symmetric spacetimes satisfying the weak energy condition, recovering known models and producing new families with hypergeometric and other closed forms.
Wald,General Relativity, Chicago Univ
6 Pith papers cite this work. Polarity classification is still indexing.
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2026 6representative citing papers
Hausdorff dimensions and multifractal spectra for power means of Schneider map coefficients on pZ_p are computed explicitly with polylogarithm formulas using thermodynamic formalism.
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.
Apparent instability of metric perturbations in Newtonian gauge for quadratic gravity inflation is a gauge artefact; gauge-invariant variables and other gauges show stable perturbative behaviour.
Generalized entanglement wedges rephrase the connected wedge theorem in bulk entropy terms, yielding mutual information bounds and a scattering-to-connected-wedge implication that extends to flat spacetimes.
Determining if the Higgs is composite would invalidate much of heterotic string model building and favor other quantum gravity approaches, best tested at a 50-60 TeV hadron collider.
citing papers explorer
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Families of regular spacetimes and energy conditions
A classification of admissible energy density profiles with bounded Kretschmann scalar yields a unified framework for regular static spherically symmetric spacetimes satisfying the weak energy condition, recovering known models and producing new families with hypergeometric and other closed forms.
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Multifractal analysis of power means for the Schneider map on $p\mathbb{Z}_p$
Hausdorff dimensions and multifractal spectra for power means of Schneider map coefficients on pZ_p are computed explicitly with polylogarithm formulas using thermodynamic formalism.
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The Thermodynamics of Cosmological Horizons and Their Holographic Description in de Sitter Space
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.
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Gauge-independent approach to inflation in quadratic gravity
Apparent instability of metric perturbations in Newtonian gauge for quadratic gravity inflation is a gauge artefact; gauge-invariant variables and other gauges show stable perturbative behaviour.
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Generalized Entanglement Wedges and the Connected Wedge Theorem
Generalized entanglement wedges rephrase the connected wedge theorem in bulk entropy terms, yielding mutual information bounds and a scattering-to-connected-wedge implication that extends to flat spacetimes.
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Fundamental or Composite? The Higgs Enigma
Determining if the Higgs is composite would invalidate much of heterotic string model building and favor other quantum gravity approaches, best tested at a 50-60 TeV hadron collider.