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Multidimensional cosmological model describing the evolution of n+1 Einstein spaces in the theory with several scalar fields and forms is considered. When a (electro-magnetic composite) p-brane Ansatz is adopted the field equations are…

高能物理 - 理论 · 物理学 2009-10-30 V. D. Ivashchuk , V. N. Melnikov

A new cosmological scenario driven by a slow rolling homogeneous scalar field whose exponential potential $V(\Phi)$ has a quadratic dependence on the field $\Phi$ in addition to the standard linear term is discussed. The derived equation of…

天体物理学 · 物理学 2009-11-11 F. C. Carvalho , J. S. Alcaniz , J. A. S. Lima , R. Silva

The conventional phase space of classical physics treats space and time differently, and this difference carries over to field theories and quantum mechanics (QM). In this paper, the phase space is enhanced through two main extensions.…

量子物理 · 物理学 2024-05-15 N. L. Diaz , J. M. Matera , R. Rossignoli

We consider the dynamics of a charged particle in a space whose coordinates are $N\times N$ hermitian matrices. Putting things in the framework of D0-branes of String Theory, we mention that the transformations of the matrix coordinates…

高能物理 - 理论 · 物理学 2009-01-07 Amir H. Fatollahi

Classical field theory is considered as a theory of unparametrized surfaces embedded in a configuration space, which accommodates, in a symmetric way, spacetime positions and field values. Dynamics is defined by a (Hamiltonian) constraint…

数学物理 · 物理学 2016-06-20 Vaclav Zatloukal

It is an accepted practice in cosmology to invoke a scalar field with potential $V(\phi)$ when observed evolution of the universe cannot be reconciled with theoretical prejudices. Since one function-degree-of-freedom in the expansion factor…

高能物理 - 理论 · 物理学 2008-11-26 T. Padmanabhan

Understanding the late-time acceleration of the Universe is one of the major challenges in cosmology today. In this paper, we present a new scalar field model corresponding to a generalised axion-like potential. In fact, this model can be…

宇宙学与河外天体物理 · 物理学 2025-07-09 Carlos G. Boiza , Mariam Bouhmadi-López

Using tachyon or quintessence fields along with a barotropic fluid on the brane we examine the different cosmological stages in a Friedmann-Robertson-Walker(FRW) universe, from the first radiation scenario to the later era dominated by…

广义相对论与量子宇宙学 · 物理学 2011-08-11 Luis P. Chimento , Monica Forte , Gilberto M. Kremer , Martin G. Richarte

I propose a new and direct connection between classical mechanics and quantum mechanics where I derive the quantum mechanical propagator from a variational principle. This variational principle is Hamilton's modified principle generalized…

量子物理 · 物理学 2009-12-15 John Hegseth

A general class of nonlocal cosmological models is considered. A new method for solving nonlocal Friedmann equations is proposed, and solutions of the Friedmann equations with nonlocal operator are presented. The cosmological properties of…

高能物理 - 理论 · 物理学 2008-11-26 Liudmila Joukovskaya

The pressureless tachyonic matter recently found in superstring field theory has an over-abundance problem in cosmology. We argue that this problem is naturally solved in the brane inflationary scenario if almost all of the tachyon energy…

高能物理 - 理论 · 物理学 2009-11-07 Gary Shiu , S. -H. Henry Tye , Ira Wasserman

Loop quantum cosmology (LQC) predicts a nonsingular evolution of the universe through a bounce in the high energy region. But LQC has an ambiguity about the quantization scheme. Recently, the authors in [Phys. Rev. D 77, 124008 (2008)]…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Li-Fang Li , Jian-Yang Zhu

We introduce a classical field theory based on a concept of extended causality that mimics the causality of a point-particle Classical Mechanics by imposing constraints that are equivalent to a particle initial position and velocity. It…

高能物理 - 理论 · 物理学 2007-05-23 Manoelito M. de Souza

We investigate the classical limit of non-Hermitian quantum dynamics arising from a coherent state approximation, and show that the resulting classical phase space dynamics can be described by generalised "canonical" equations of motion,…

量子物理 · 物理学 2010-02-08 Eva-Maria Graefe , Michael Hoening , Hans Juergen Korsch

The Quantum Cosmology can be understand as the theory of an one object that is the Universe described in terms of fundamental mass groundstate of the free boson string, that is a tachyon - a hypothetical particle with negative mass square,…

广义相对论与量子宇宙学 · 物理学 2012-03-05 L. A. Glinka

We derive an action for scalar quantum field theory with cubic interaction in the context of relative locality. Beginning with the generating functional for standard $\varphi^3$--theory and the corresponding Feynman rules we modify them to…

高能物理 - 理论 · 物理学 2013-12-16 Laurent Freidel , Trevor Rempel

Quantum field theory of space-like particles is investigated in the framework of absolute causality scheme preserving Lorentz symmetry. It is related to an appropriate choice of the synchronization procedure (definition of time). In this…

高能物理 - 理论 · 物理学 2009-10-30 Jakub Rembielinski

In this work, we present an overview of uniqueness results derived in recent years for the quantization of Gowdy cosmological models and for (test) Klein-Gordon fields minimally coupled to Friedmann-Lema\^{\i}tre-Robertson-Walker, de…

广义相对论与量子宇宙学 · 物理学 2019-12-10 Jerónimo Cortez , Guillermo A. Mena Marugán , José Velhinho

We investigate in detail the asymptotic properties of tachyon cosmology for a broad class of self-interaction potentials. The present approach relies in an appropriate re-definition of the tachyon field, which, in conjunction with a method…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Israel Quiros , Tame Gonzalez , Dania Gonzalez , Yunelsy Napoles , Ricardo Garcia-Salcedo , Claudia Moreno

All measurable predictions of classical mechanics can be reproduced from a quantum-like interpretation of a nonlinear Schrodinger equation. The key observation leading to classical physics is the fact that a wave function that satisfies a…

量子物理 · 物理学 2014-11-18 H. Nikolic