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相关论文: Kinetic Field Theory: Higher-Order Perturbation Th…

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Kinetic Field Theory (KFT) is a statistical field theory for an ensemble of point-like classical particles in or out of equilibrium. We review its application to cosmological structure formation. Beginning with the construction of the…

In earlier work, we have developed a nonequilibrium statistical field theory description of cosmic structure formation, dubbed Kinetic Field Theory (KFT), which is based on the Hamiltonian phase-space dynamics of classical particles and…

宇宙学与河外天体物理 · 物理学 2019-04-03 Robert Lilow , Felix Fabis , Elena Kozlikin , Celia Viermann , Matthias Bartelmann

We present recent improvements in the perturbative treatment of particle interactions in Kinetic Field Theory (KFT) for inertial Zel'dovich trajectories. KFT has been developed for the systematic analytical calculation of non-linear cosmic…

宇宙学与河外天体物理 · 物理学 2022-12-28 Christophe Pixius , Safak Celik , Matthias Bartelmann

In earlier work, we have developed a Kinetic Field Theory (KFT) for cosmological structure formation and showed that the non-linear density-fluctuation power spectrum known from numerical simulations can be reproduced quite well even if…

宇宙学与河外天体物理 · 物理学 2017-09-13 Matthias Bartelmann , Felix Fabis , Elena Kozlikin , Robert Lilow , Johannes Dombrowski , Julius Mildenberger

Non-linear cosmic structures contain valuable information on the expansion history of the background space-time, the nature of dark matter, and the gravitational interaction. The recently developed kinetic field theory of cosmic structure…

宇宙学与河外天体物理 · 物理学 2023-07-18 Alexander Oestreicher , Lodovico Capuano , Sabino Matarrese , Lavinia Heisenberg , Matthias Bartelmann

Building upon the recently developed formalism of Kinetic Field Theory (KFT) for cosmic structure formation by Bartelmann et al., we investigate a kinematic relationship between diffusion and gravitational interactions in cosmic structure…

宇宙学与河外天体物理 · 物理学 2018-02-26 Johannes Dombrowski , Felix Fabis , Matthias Bartelmann

We use the recently developed Kinetic Field Theory (KFT) for cosmic structure formation to show how non-linear power spectra for cosmic density fluctuations can be calculated in a mean-field approximation to the particle interactions. Our…

宇宙学与河外天体物理 · 物理学 2021-06-23 Matthias Bartelmann , Johannes Dombrowski , Sara Konrad , Elena Kozlikin , Robert Lilow , Carsten Littek , Christophe Pixius , Felix Fabis

Recently, Bartelmann et al. presented a 'Kinetic Field Theory' (KFT) formalism to tackle the difficulties of large scale structure formation. In this approach, the dynamics of a non-equilibrium ensemble of classical particles are examined…

宇宙学与河外天体物理 · 物理学 2019-05-20 Daniel Geiss , Robert Lilow , Felix Fabis , Matthias Bartelmann

We show how kinetic theory, the statistics of classical particles obeying Newtonian dynamics, can be formulated as a field theory. The field theory can be organized to produce a self-consistent perturbation theory expansion in an effective…

统计力学 · 物理学 2015-06-03 Shankar P. Das , Gene F. Mazenko

The kinetic field theory is developed without assumptions of statistical homogeneity and isotropy. In a solvable toy model with short-ranged interactions, we compare first-order perturbation theory to an iterated mean-field approximation…

宇宙学与河外天体物理 · 物理学 2025-09-03 Matthias Bartelmann , James Stokes

The dynamics of correlated systems is relevant in many fields ranging from cosmology to plasma physics. However, they are challenging to predict and understand even for classical systems due to the typically large numbers of particles…

A closed set of equations for the evolution of linear perturbations of homogeneous, isotropic cosmological models can be obtained in various ways. The simplest approach is to assume a macroscopic equation of state, e.g.\ that of a perfect…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Anton K. Rebhan , Dominik J. Schwarz

Quantum Field Theory (QFT) makes predictions by combining two sets of assumptions: (1) quantum dynamics, such as a Schrodinger or Liouville equation; (2) quantum measurement, such as stochastic collapse to an eigenfunction of a measurement…

量子物理 · 物理学 2007-05-23 Paul J. Werbos , Ludmila Dolmatova Werbos

We apply kinetic field theory to non-linear cosmic structure formation. Kinetic field theory decomposes the cosmic density field into particles and follows their trajectories through phase space. We assume that initial particle momenta are…

宇宙学与河外天体物理 · 物理学 2022-08-24 Sara Konrad , Matthias Bartelmann

We investigate cosmic structure formation in the framework of a path-integral formulation of an $N$-particle ensemble in phase space, dubbed Resummed Kinetic Field Theory (RKFT), up to one-loop perturbative order. In particular, we compute…

宇宙学与河外天体物理 · 物理学 2026-02-11 Marvin Sipp , Hannes Heisler , Matthias Bartelmann

We present a detailed comparison of the newly developed particle-based Kinetic Field Theory framework for cosmic large-scale structure formation with the established formalism of Eulerian Standard Perturbation Theory. We highlight the…

宇宙学与河外天体物理 · 物理学 2021-07-14 Elena Kozlikin , Robert Lilow , Felix Fabis , Matthias Bartelmann

For classical field theories with probabilistic initial conditions the classical field observables are an idealization. Their arbitrarily precise values poorly reflect the characteristic uncertainty in the presence of substantial…

量子物理 · 物理学 2026-03-06 Christof Wetterich

Noncommutative field theory (NCFT) is an extension of quantum field theory (QFT) that redefines spacetime, replacing commuting coordinates with a noncommutative structure. This shift fundamentally alters the way fields, interactions, and…

高能物理 - 理论 · 物理学 2026-01-14 Badis Ydri

Quantum field theory (QFT) based on the principles of special relativity (SR) and it is in fact the \emph{kinematic theory of fields}. The root assumption is that there is "relativistic description" of \emph{any} isolated quantum system in…

综合物理 · 物理学 2018-08-02 Peter Leifer

A fundamental problem with attempting to quantize general relativity is its perturbative non-renormalizability. However, this fact does not rule out the possibility that non-perturbative effects can be computed, at least in some…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Viqar Husain , Sebastian Jaimungal
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