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相关论文: Counting surface states in the loop quantum gravit…

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Equilibrium states of black holes can be modelled by isolated horizons. If the intrinsic geometry is spherical, they are called type I while if it is axi-symmetric, they are called type II. The detailed theory of geometry of \emph{quantum}…

广义相对论与量子宇宙学 · 物理学 2010-11-05 Abhay Ashtekar , Jonathan Engle , Chris Van Den Broeck

Subdominant contributions to the entanglement entropy of quantum fields include logarithmic corrections to the area law characterized by universal coefficients that are independent of the ultraviolet regulator and capture detailed…

高能物理 - 理论 · 物理学 2021-12-28 Rodolfo Soldati , L. S. Menicucci , N. Yokomizo

A general geometrical structure of the entanglement entropy for spatial partition of a relativistic QFT system is established by using methods of the effective gravity action and the spectral geometry. A special attention is payed to the…

高能物理 - 理论 · 物理学 2008-11-26 Dmitri V. Fursaev

A key test of any quantum theory of gravity is its ability to reproduce the known thermodynamic properties of black holes. A statistical mechanical description of the Bekenstein-Hawking entropy once seemed remote, but today we suffer an…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Steven Carlip

The area law obeyed by the thermodynamic entropy of black holes is one of the fundamental results relating gravity to statistical mechanics. In this work we provide a derivation of the area law for the quantum relative entropy of the…

广义相对论与量子宇宙学 · 物理学 2025-05-08 Ginestra Bianconi

We present a way of understanding the curvature of space-time, the basic philosophy being that the (linear) geometry of any space is determined by the (linear) functionals on the algebra(s) of any fields defined on the space. It is known…

数学物理 · 物理学 2009-09-15 E. Akofor

This thesis, explores the quantum entanglement and evolution through both a geometric and dynamical perspective. The first part focuses on classical phase space and its central role in Hamiltonian mechanics, emphasizing the importance of…

量子物理 · 物理学 2026-05-04 Jamal Elfakir

We study the euclidean covariant loop-quantum-gravity vertex numerically, using a cylindrically symmetric boundary state and a convenient value of the Barbero-Immirzi parameter. We show that a classical geometry emerges already at low spin.…

广义相对论与量子宇宙学 · 物理学 2016-03-28 Vincent Bayle , François Collet , Carlo Rovelli

Geometric quantization is an attempt at using the differential-geometric ingredients of classical phase spaces regarded as symplectic manifolds in order to define a corresponding quantum theory. Generally, the process of geometric…

数学物理 · 物理学 2018-01-09 Andrea Carosso

We review applications of noncommutative geometry in canonical quantum gravity. First, we show that the framework of loop quantum gravity includes natural noncommutative structures which have, hitherto, not been explored. Next, we present…

广义相对论与量子宇宙学 · 物理学 2012-03-29 Johannes Aastrup , Jesper M. Grimstrup

General relativity successfully describes space-times at scales that we can observe and probe today, but it cannot be complete as a consequence of singularity theorems. For a long time there have been indications that quantum gravity will…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Martin Bojowald

Earlier calculations of black hole entropy in loop quantum gravity have given a term proportional to the area with a correction involving the logarithm of the area when the area eigenvalue is close to the classical area. However the…

广义相对论与量子宇宙学 · 物理学 2014-06-25 P. Mitra

The degree to which a pure quantum state is entangled can be characterized by the distance or angle to the nearest unentangled state. This geometric measure of entanglement is explored for bi-partite and multi-partite pure and mixed states.…

量子物理 · 物理学 2009-05-18 Tzu-Chieh Wei

Counting of microscopic states of black holes is discussed within the framework of loop quantum gravity. There are two different ways, one allowing for all spin states and the other involving only pure horizon states. The number of states…

高能物理 - 理论 · 物理学 2009-06-26 P. Mitra

Einstein Equivalence Principle (EEP) requires all matter components to universally couple to gravity via a single common geometry: that of spacetime. This relates quantum theory with geometry as soon as interactions with gravity are…

广义相对论与量子宇宙学 · 物理学 2022-09-13 Ashkan Alibabaei

The surface Hamiltonian corresponding to the surface part of a gravitational action has $xp$ structure where $p$ is conjugate momentum of $x$. Moreover, it leads to $TS$ on the horizon of a black hole. Here $T$ and $S$ are temperature and…

广义相对论与量子宇宙学 · 物理学 2016-12-30 Ashish Bakshi , Bibhas Ranjan Majhi , Saurav Samanta

In a wide range of quantum gravity theories, quasiclassical geometries, which are solutions to the Einstein field equations approximately, are described by "coherent states." Here we propose a Hamiltonian formalism for gravitational…

广义相对论与量子宇宙学 · 物理学 2025-12-01 Sijia Wang , Achintya Sajeendran , Dong-han Yeom , Robert B. Mann , Joshua Foo

Building on parallels between geometric quantum mechanics and classical mechanics, we explore an alternative basis for quantum thermodynamics that exploits the differential geometry of the underlying state space. We develop both…

量子物理 · 物理学 2024-03-13 Fabio Anza , James P. Crutchfield

The entropy of a black hole can be obtained by counting states in loop quantum gravity. The dominant term depends on the Immirzi parameter involved in the quantization and is proportional to the area of the horizon, while there is a…

广义相对论与量子宇宙学 · 物理学 2007-05-23 A. Ghosh , P. Mitra

We revisit the topic of two-state quantum systems using Geometric Algebra (GA) in three dimensions $\mathcal G_3$. In this description, both the quantum states and Hermitian operators are written as elements of $\mathcal G_3$. By writing…

数学物理 · 物理学 2021-03-10 Pedro Amao , Hernán Castillo
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