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We contrast the two approaches to ``classical" signature change used by Hayward with the one used by us (Hellaby and Dray). There is (as yet) no rigorous derivation of appropriate distributional field equations. Hayward's distributional…

General Relativity and Quantum Cosmology · Physics 2009-10-28 Charles Hellaby , Tevian dray

The change of signature of a metric is explained using simple examples and methods. The Klein-Gordon field on a signature-changing background is discussed, and it is shown how the approach of Dray et al.\ can be corrected to ensure that the…

General Relativity and Quantum Cosmology · Physics 2008-02-03 Sean A. Hayward

For a contravariant 4-metric which changes signature from Lorentzian to Riemannian across a spatial hypersurface, the mixed Einstein tensor is manifestly non-singular. In Gaussian normal coordinates, the metric contains a step function and…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Sean A. Hayward

Fundamental errors exist in the above-mentioned article, which attempts to justify previous erroneous claims concerning signature change. In the simplest example, the authors' proposed ``solutions'' do not satisfy the relevant equation, as…

General Relativity and Quantum Cosmology · Physics 2016-08-31 Sean A. Hayward

Kossowski and Kriele derived boundary conditions on the metric at a surface of signature change. We point out that their derivation is based not only on certain smoothness assumptions but also on a postulated form of the Einstein field…

General Relativity and Quantum Cosmology · Physics 2009-10-28 Tevian Dray , Charles Hellaby

Exact solutions of Einstein equations with null Riemman-Christoffel curvature tensor everywhere, except on a hypersurface, are studied using quantum particles obeying the Klein-Gordon equation. We consider the particular cases when the…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Paulo M. Pitelli , Patricio S. Letelier

We make a rigorous study of classical field equations on a 2-dimensional signature changing spacetime using the techniques of operator theory. Boundary conditions at the surface of signature change are determined by forming self-adjoint…

General Relativity and Quantum Cosmology · Physics 2008-11-26 L. J. Alty , C. J. Fewster

By means of a brief review of the derivation of the causal modified Lorentz-Abraham-Dirac classical equation of motion from the renormalization of the mass in the modified equation of motion of an extended charged sphere as its radius…

Classical Physics · Physics 2026-04-15 Arthur D. Yaghjian

A conventional wisdom often perpetuated in the literature states that: (i) a 3+1 decomposition of space-time into space and time is synonymous with the canonical treatment and this decomposition is essential for any Hamiltonian formulation…

General Relativity and Quantum Cosmology · Physics 2011-07-13 N. Kiriushcheva , S. V. Kuzmin

This paper is a serious attempt at reconciling quantum and classical mechanics through the concept of dynamic space and the acceptance of non-zero Ricci tensor for vacuum. Starting with scalar particles, the paper shows that with those two…

General Physics · Physics 2007-05-23 Jose B. Almeida

In Hamiltonian GR, change has seemed to be missing, defined only asymptotically, or otherwise obscured at best. By construing change as essential time dependence, can one find change locally in Hamiltonian GR with spinors? This paper is…

General Relativity and Quantum Cosmology · Physics 2021-11-24 J. Brian Pitts

We show in this article how the usual hamiltonian formalism of General Relativity should be modified in order to allow the inclusion of the Euclidean classical solutions of Einstein's equations. We study the effect that the dynamical change…

General Relativity and Quantum Cosmology · Physics 2010-11-01 Jerome Martin

We investigate a simple $f(R, T_\phi)$ gravity model coupled to a scalar field and demonstrate that the theory admits classical degenerate metric solutions, analogous to those known in general relativity. In particular, we identify a class…

General Relativity and Quantum Cosmology · Physics 2026-03-10 Serkan Doruk Hazinedar , Yaghoub Heydarzade

A longstanding issue is the classical equivalence between the Jordan and the Einstein frames, which is considered just a field redefinition of the metric tensor and the scalar field. In this work, based on the previous result that the…

General Relativity and Quantum Cosmology · Physics 2024-02-27 Gabriele Gionti S. J. , Matteo Galaverni

Standard formulation is unable to distinguish between the (+++-) and (---+) spacetime metric signatures. However, the Clifford algebras associated with each are inequivalent, R(4) in the first case (real 4 by 4 matrices), H(2) in the latter…

General Relativity and Quantum Cosmology · Physics 2007-05-23 William M. Pezzaglia , John J. Adams

We formulate the Einstein-Cartan-Dirac equations in the Newman-Penrose (NP) formalism, thereby presenting a more accurate and explicit analysis of previous such studies. The equations show in a transparent way how the Einstein-Dirac…

General Relativity and Quantum Cosmology · Physics 2018-10-03 Swanand Khanapurkar , Abhinav Varma , Nehal Mittal , Navya Gupta , Tejinder P. Singh

The behavior of spin-1/2 particle in a weak static gravitational field is considered. The Dirac Hamiltonian is diagonalized by the Foldy-Wouthuysen transformation providing also the simple form for the momentum and spin polarization…

General Relativity and Quantum Cosmology · Physics 2009-11-10 A. J. Silenko , O. V. Teryaev

We study the interplay of general relativity, the equivalence principle, and high-precision experiments involving atomic transitions and g factor measurements. In particular, we derive a generalized Dirac Hamiltonian, which describes both…

High Energy Physics - Phenomenology · Physics 2019-04-26 Ulrich D. Jentschura

This is a contribution on the controversy about junction conditions for classical signature change. The central issue in this debate is whether the extrinsic curvature on slices near the hypersurface of signature change has to be continuous…

General Relativity and Quantum Cosmology · Physics 2016-08-31 Franz Embacher

We analyse a classical model of gravitation coupled to a self interacting scalar field. We show that, within the context of this model for Robertson-Walker cosmologies, there exist solutions in the spatially non-flat cases exhibiting…

General Relativity and Quantum Cosmology · Physics 2014-11-17 K. Ghafoori-Tabrizi , S. S. Gousheh , H. R. Sepangi
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