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$f(Q)$ symmetric-teleparallel gravity is considered in view of Quantum Cosmology. Specifically, we derive cosmological equations for $f(Q)$ models and then investigate the related energy conditions. In the minisuperspace formalism, the…

广义相对论与量子宇宙学 · 物理学 2023-07-04 Francesco Bajardi , Salvatore Capozziello

Bringing gravity into a quantum-mechanical framework is likely the most profound remaining problem in fundamental physics. The "unitarity crisis" for black hole evolution appears to be a key facet of this problem, whose resolution will…

广义相对论与量子宇宙学 · 物理学 2021-02-22 Steven B. Giddings

I describe a possible perspective on the current state of loop quantum gravity, at the light of the developments of the last years. I point out that a theory is now available, having a well-defined background-independent kinematics and a…

广义相对论与量子宇宙学 · 物理学 2011-05-25 Carlo Rovelli

We derive the black hole solutions with horizons of non-trivial topology and investigate their properties in the framework of an approach to quantum gravity being an extension of Bohm's formulation of quantum mechanics. The solutions we…

广义相对论与量子宇宙学 · 物理学 2009-10-31 J. Kowalski-Glikman , D. Nowak-Szczepaniak

Quantum gravity is likely the deepest problem facing current physics. While traditionally associated with short distance nonrenormalizability, it is evident that the long distance problem of unitarity, arising at high energies with black…

高能物理 - 理论 · 物理学 2022-04-01 Steven B. Giddings

In seeking to arrive at a theory of ``quantum gravity'', one faces several choices among alternative approaches. I list some of these ``forks in the road'' and offer reasons for taking one alternative over the other. In particular, I…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Rafael D. Sorkin

Loop quantum cosmology is an application of recent developments for a non-perturbative and background independent quantization of gravity to a cosmological setting. Characteristic properties of the quantization such as discreteness of…

天体物理学 · 物理学 2009-11-13 Martin Bojowald

We propose a new phenomenological model for quantum gravity. This is based on a new interpretation in which quantum gravity is not an interaction, rather it is just responsible for generation of space-time-matter. Then we show this model is…

高能物理 - 唯象学 · 物理学 2008-09-16 F. Darabi

The probability of there being sufficient inflation to solve the fine-tuning associated with the horizon and flatness problems has recently been shown to be exponentially small, within the context of classical general relativity. Here this…

广义相对论与量子宇宙学 · 物理学 2007-08-27 William Nelson

Recent progress in table-top experiments offers the opportunity to show for the first time that gravity is not compatible with a classical description. In all current experimental proposals, such as the generation of gravitationally induced…

量子物理 · 物理学 2024-08-05 Lin-Qing Chen , Flaminia Giacomini

Investigating quantum gravity requires a comprehension of both, general relativity and quantum field theory. Therefore this thesis starts, after a general introduction to the treated topics, with a brief review of the field theoretical…

高能物理 - 理论 · 物理学 2018-10-09 Natalia Alkofer

We use the idea of the symmetry between the spacetime coordinates x^\mu and the energy-momentum p^\mu in quantum theory to construct a momentum space quantum gravity geometry with a metric s_{\mu\nu} and a curvature P^\lambda_{\mu\nu\rho}.…

广义相对论与量子宇宙学 · 物理学 2016-03-08 J. W. Moffat

In a quantum theory of cosmology spacetime behaves classically only in limited patches of the configuration space on which the wave function of the universe is defined. Quantum transitions can connect classical evolution in different…

高能物理 - 理论 · 物理学 2017-07-19 Sebastian F. Bramberger , Thomas Hertog , Jean-Luc Lehners , Yannick Vreys

We study a family of physical observable quantities in quantum gravity. We denote them W functions, or n-net functions. They represent transition amplitudes between quantum states of the geometry, are analogous to the n-point functions in…

广义相对论与量子宇宙学 · 物理学 2011-04-19 Alejandro Perez , Carlo Rovelli

Wormhole spacetimes may be responsible for the possible loss of quantum coherence and the introduction of additional fundamental quantum indeterminancy of the values of constants of nature. As a system which is known to admit such classical…

高能物理 - 理论 · 物理学 2009-10-30 Hongsu Kim

We consider changes of the topological charge of vortices in quantum mechanics by investigating analytical examples where the creation or annihilation of vortices occurs. In classical hydrodynamics of non-viscous fluids the Helmholtz-Kelvin…

量子物理 · 物理学 2009-11-07 Bogdan Damski , Krzysztof Sacha

We propose an operator constraint equation for the wavefunction of the Universe that admits genuine evolution. While the corresponding classical theory is equivalent to the canonical decomposition of General Relativity, the quantum theory…

广义相对论与量子宇宙学 · 物理学 2014-04-03 Sean Gryb , Karim Thebault

This study introduces the quantum force wave equation (QFWE) as a general theory of quantum forces, a novel framework that redefines quantum forces as emergent phenomena arising from the interaction between quantum particles and curved…

综合物理 · 物理学 2025-07-11 Raheem Adom

Wave functions specifying a quantum state of the universe must satisfy the constraints of general relativity, in particular the Wheeler-DeWitt equation (WDWE). We show for a wide class of models with non-zero cosmological constant that…

高能物理 - 理论 · 物理学 2012-08-01 James B. Hartle , S. W. Hawking , Thomas Hertog

An oscillating universe cycles through a series of expansions and contractions. We propose a model in which ``phantom'' energy with $p < -\rho$ grows rapidly and dominates the late-time expanding phase. The universe's energy density is so…

天体物理学 · 物理学 2014-10-13 Matthew G. Brown , Katherine Freese , William H. Kinney