1 A ( geometrical ) Hilbert space based quantum gravity model (original) (raw)

A Form of Quantum Gravity Unification with the General Theory of Relativity

A form of Quantum gravity unification with the General theory of Relativity, 2024

The problem still remains (in theoretical physics) of how gravity can be unified with quantum mechanics, in as much as it would be possible to explain a consistent theory of quantum gravity. Which, this unification theory should (to a sufficient extent) adhere to the Friedmann-Lemaitre-Robertson-Walker metric. In the preceding work, a universal model is formulated, considering the results of the theory of quantum gravity, as well as the General theory of relativity. The space-time continuum is modelled to arise from the gravity quanta. This is by allowing the universe to retain its homogeneous nature at scales near the plank scale in (relativistic) difference from the time of the Big Bang and treating the gravity particle as behaving, both as a wave and as a particle (as of the theory of wave-particle duality). Once space-time is modelled, the field equations of general relativity are considered, and briefly mentioned, in the modelling of repulsive gravity as being the cause of the expansion of the universe. The space-time metric is considered, as possibly moving at faster than the speed of light. This is considered as suggesting, an event (as of the Special theory of relativity) of which its occasion supersedes the symmetry of which the Special theory of relativity was modelled, this is considered with no changes to the frame of reference of the Special theory of relativity.

Gravity, Geometry, and the Quantum

Springer Handbook of Spacetime, 2014

After a brief introduction, basic ideas of the quantum Riemannian geometry underlying loop quantum gravity are summarized. To illustrate physical ramifications of quantum geometry, the framework is then applied to homogeneous isotropic cosmology. Quantum geometry effects are shown to replace the big bang by a big bounce. Thus, quantum physics does not stop at the big-bang singularity. Rather there is a pre-big-bang branch joined to the current post-big-bang branch by a 'quantum bridge'. Furthermore, thanks to the background independence of loop quantum gravity, evolution is deterministic across the bridge.

Spacetime and the Philosophical Challenge of Quantum Gravity

1999

We survey some philosophical aspects of the search for a quantum theory of gravity, emphasising how quantum gravity throws into doubt the treatment of spacetime common to the two `ingredient theories' (quantum theory and general relativity), as a 4-dimensional manifold equipped with a Lorentzian metric. After an introduction, we briefly review the conceptual problems of the ingredient theories and introduce the enterprise of quantum gravity We then describe how three main research programmes in quantum gravity treat four topics of particular importance: the scope of standard quantum theory; the nature of spacetime; spacetime diffeomorphisms, and the so-called problem of time. By and large, these programmes accept most of the ingredient theories' treatment of spacetime, albeit with a metric with some type of quantum nature; but they also suggest that the treatment has fundamental limitations. This prompts the idea of going further: either by quantizing structures other than t...

Connections between Abstract Quantum Theory and Space-Time-Structure. III. Vacuum Structure and Black Holes

Quantum-theoretic considerations for the ground state of a black hole result in a change of its interior solution. lt is shown hat the interior of a Schwarzschild black hole can be modelled by an ur-theoretically described Robertson-Walker space-time. Thereby the Schwarzschild singularity is changed into a Friedman singularity. 1. INTRODUCTON One expects that an appropriate unification of quantum theory and gravitation theory should lead to an explanation of the observed smallness of the cosmological constant and to a better understanding of the space-time singularities of classical general relativity. We do not think that one should try to avoid or even remove space-time singularities in quantized gravity; we rather take singularities as precious hints to look for a new type of unification. The usual attempts to construct a union of quantum theory and gravity are applications of quantization procedures to gravitation theory retaining the space-time continuum even at very small distances. In this paper we do not presuppose a space-time continuum first but start with abstract quantum theory, i.e., the quantum theory of binary alternatives (Drieschner et al., 1987; Görnitz, 1988 a, b). Space-time is introduced via the invariance group of the "ur," the quantized binary alternative. This invariance group turns out to be U(2).

Quantum Gravity:the axiomatic approach, a possible interpretation

Twenty years ago, by extending the Wightman axiom framework, it has been found possible to quantize only a conformal factor of the gravitational field. Gravitons being excluded from this quantum scalar field theory, numerous attempts were done to give a valuable description of what could be quantum gravity. In this talk we present a familly of Lorentz manifolds which can be foliated by isotropic hypersurfaces and pose severe restrictions on the form of the energy-momentum tensor in Einstein's equations. They can be associated to gravitational waves "without gravitons" in a vacuum described by two cosmological functions, but not to a massless particle flow. From this cross-checking with the previous remark, a "very" primordial quantum cosmological scenario is proposed.

Against the disappearance of spacetime in quantum gravity

Synthese, 2019

This paper argues against the proposal to draw from current research into a physical theory of quantum gravity the ontological conclusion that spacetime or spatiotemporal relations are not fundamental. As things stand, the status of this proposal is like the one of all the other claims about radical changes in ontology that were made during the development of quantum mechanics and quantum field theory. However, none of these claims held up to scrutiny as a consequence of the physics once the theory was established and a serious discussion about its ontology had begun. Furthermore, the paper argues that if spacetime is to be recovered through a functionalist procedure in a theory that admits no fundamental spacetime, standard functionalism cannot serve as a model: all the known functional definitions are definitions in terms of a causal role for the motion of physical objects and hence presuppose spatiotemporal relations.

A model of quantum spacetime

AVS quantum science, 2022

We consider a global quantum system (the "Universe") satisfying a double constraint, both on total energy and total momentum. Generalizing the Page and Wootters quantum clock formalism, we provide a model of 3+1 dimensional, non-relativistic, quantum spacetime emerging from entanglement among different subsystems in a globally "timeless" and "positionless" Universe.

A Quantum-Physical Theory of Gravitation

A Quantum-Physical Theory of Gravitation, 2024

Of the General Theory of Relativity it has been said that it is one of the most beautiful theories invented by man, in fact personally also at the time it impressed me a lot, which led me to study Tensor Analysis and to try to understand Riemannian Geometry, but the truth is that all that world seemed to me very complicated and therefore not very beautiful, and I understood why, when it was launched, it is said that only 12 people understood it. Enrique Loedel in his excellent book writes... “arriving at the same results obtained from the exact Schwarzchild solution... whose extremely simple structure does not agree with the extreme complication of the field equations, make us think of the possibility of obtaining such a solution in a simpler and more direct way”(7,pg318). It was this that motivated me, among others, to the present solution of the gravitational fields, after having applied the concept of Basic Systemic Unit in the derivation of the Pendulum Formula, of the Schrödinger wave equation and those of Special Relativity.

Abstract quantum theory and space-time structure. I. Ur theory and Bekenstein-Hawking entropy

International Journal of Theoretical Physics, 1988

We discuss the close connection between a quantum theory of binary alternatives and the local Lorentzian structure of space-time, and outline v. WeizsS.cker's concept of the "ur"-the quantized binary alternative. Then space-time is introduced mathematically as a symmetric space of the invariance group of the ur. It is physically interpreted as "the" cosmological space-time, the universe. In our model spacelike structures rest on the concept of "hypermembranes"-dynamical manifolds of codimension 1 in space-time. For a given number of urs a smallest length is introduced in this cosmic model by group-theoretic arguments. Already before introducing a dynamics the concept of isolated noncomposite objects can be given. They can be understood as simple models either for elementary particles or for black holes. Identifying the maximal localized states of many urs with a localized state of a particle, we get a good description of the large cosmological numbers and also a lower bound for a neutrino mass. A simple counting of the particle states given from the ur-theoretic ansatz allows an easy explanation of th e Bekenstein-Hawking entropy. One can give good reasons why reality cannot at all be represented by a continuous field. From the quantum phenomena it appears to follow with certainty that a finite system of finite energy can be completely described by a finite set of numbers (quantum numbers). This does not seen to be in accordance with a continuum theory and must lead to an attempt to find a purely algebraic theory for the description of reality. But nobody knows how to obtain the basis of such a theory.-Albert Einstein, The Meaning of Relativity, 6th ed., Appendix liD.

Aspects of quantum gravity phenomenology

2015

Quantum gravity effects modify the Heisenberg's uncertainty principle to the generalized uncertainty principle (GUP). Earlier work showed that the GUP-induced corrections to the Schrödinger equation, when applied to a non-relativistic particle in a one-dimensional box, led to the quantization of length. Similarly, corrections to the Klein-Gordon and the Dirac equations, gave rise to length, area and volume quantizations. These results suggest a fundamental granular structure of space. This thesis investigates how spacetime curvature and gravity might influence this discreteness of space. In particular, by adding a weak background gravitational field to the above three quantum equations, it is shown that quantization of lengths, areas and volumes continue to hold. Although the nature of this new quantization is quite complex, under proper limits, it reduces to cases without gravity. These results indicate the universality of quantum gravity effects. I am thankful to my supervisor Dr. Saurya Das for his inspiring guidance, constructive criticism, friendly advice and academic as well as non-academic support throughout the research project. I would like to express my gratitude to my committee members Dr. Mark Walton and Dr. Kent Peacock for all the valuable suggestions and comments they provided. I would also like to thank my family and friends for their help and encouragement. v Contents List of Figures viii vi 3.6.1 Case 1 : Length quantization along x axis .