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Recently the formation of an expanding universe from the (1+3+6)-dimensional space-times has been proposed on the basis of super-string theory. The serious entropy problem must be solved for it to be realistic from the cosmological…

广义相对论与量子宇宙学 · 物理学 2014-02-14 Kenji Tomita

The entropy growth in a cosmological process of pair production is completely determined by the associated squeezing parameter, and is insensitive to the number of particles in the initial state. The total produced entropy may represent a…

广义相对论与量子宇宙学 · 物理学 2010-04-06 M. Gasperini , M. Giovannini

Cosmological perturbations in the (1+3+6)-dimensional space-times including photon gas without viscous processes are studied on the basis of Abbott et al.'s formalism. Space-times consist of the outer space (the 3-dimensional expanding…

广义相对论与量子宇宙学 · 物理学 2014-12-23 Kenji Tomita

We consider the generation of entropy when particle pairs are created at a cosmological level. Making a reduction via the particle number basis, we compute the classical limit for the entropy generation due to the evolution of the matter…

广义相对论与量子宇宙学 · 物理学 2010-04-06 M. Kruczenski , L. E. Oxman , M. Zaldarriaga

We estimate the entropy associated to a background of squeezed cosmic gravitons, and we argue that the process of cosmological pair production from the vacuum may explain the large amount of entropy of our present universe.

广义相对论与量子宇宙学 · 物理学 2009-10-22 M. Gasperini , M. Giovannini

In the context of higher-dimensional cosmologies with isotropic visible and internal space and multi-perfect fluid matter, we study the conditions under which adiabatic expansion of the visoble external space is possible, when a…

广义相对论与量子宇宙学 · 物理学 2015-06-25 K. Kleidis , D. B. Papadopoulos

Cosmological adiabatic particle creation results in the generation of irreversible entropy. The evolution of this entropy is examined in a flat Friedmann--Robertson--Walker universe at late times, using a dissipative model with a power-law…

广义相对论与量子宇宙学 · 物理学 2020-09-16 Nobuyoshi Komatsu

Different cooling rates of interacting fluid components of the expanding cosmic medium give rise to entropy producing bulk stresses. With the help of effective bulk pressures, on the other hand, one may phenomenologically take into account…

天体物理学 · 物理学 2011-04-15 Winfried Zimdahl , Diego Pavon , Josep Triginer

The stochastic entropy generated during the evolution of a system interacting with an environment may be separated into three components, but only two of these have a non-negative mean. The third component of entropy production is…

统计力学 · 物理学 2013-05-30 Ian J. Ford , Richard E. Spinney

The thermodynamic behavior of a decaying vacuum cosmology describing the entire cosmological history evolving between two extreme (early and late time) de Sitter eras is investigated. The thermal evolution from the early de Sitter to the…

广义相对论与量子宇宙学 · 物理学 2015-06-23 J. A. S. Lima , S. Basilakos , Joan Solà

This thesis investigates cosmological particle production within Quantum Field Theory in Curved Spacetimes, both as a dark matter mechanism and through analog simulations using Bose-Einstein condensates. While a full theory of Quantum…

广义相对论与量子宇宙学 · 物理学 2026-02-12 Álvaro Parra-López

According to the second law of thermodynamics, the arrow of time points to an ever increasing entropy of the Universe. However, exactly how the entropy evolves with time and what drives the growth remain largely unknown. Here, for the first…

宇宙学与河外天体物理 · 物理学 2012-11-09 Xinghai Zhao , Yuexing Li , Qirong Zhu , Derek Fox

We study particle production and the corresponding entropy increase in the context of cosmology with dynamical vacuum. We focus on the particular form that has been called "running vacuum model" (RVM), which is known to furnish a successful…

广义相对论与量子宇宙学 · 物理学 2020-02-14 Joan Sola , Hao Yu

We study the dynamics of a strongly-coupled quantum field theory in a cosmological spacetime using the holographic AdS/CFT correspondence. Specifically we consider a confining gauge theory in an expanding FRW universe and track the…

高能物理 - 理论 · 物理学 2015-09-30 Mukund Rangamani , Moshe Rozali , Mark Van Raamsdonk

A new definition of entropy is introduced using a model that simulates an expanding space-time compatible with the fundamental principle of cosmology. The entropy is obtained by mean of a state function that measures the variation of the…

综合物理 · 物理学 2024-05-01 Faycal Ben Adda

An accelerated universe should naturally have a vacuum energy density determined by its dynamical curvature. The cosmological constant is most likely a temporary description of a dynamical variable that has been drastically evolving from…

广义相对论与量子宇宙学 · 物理学 2015-10-28 Joan Sola

The bulk viscosity of cosmological fluid and the creation of cold dark matter both result in the generation of irreversible entropy (related to dissipative processes) in a homogeneous and isotropic universe. To consider such effects, the…

宇宙学与河外天体物理 · 物理学 2014-12-16 Nobuyoshi Komatsu , Shigeo Kimura

Cosmology is investigated within a new, scalar theory of gravitation, which is a preferred-frame bimetric theory with flat background metric. Before coming to cosmology, the motivation for an " ether theory " is exposed at length; the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Mayeul Arminjon

For several independent reasons, the idea that notorious sources of entropy could exist in the Universe has been recently revived. Taking advantage of a new framework accounting for non-equilibrium processes in cosmology, we explicitly…

广义相对论与量子宇宙学 · 物理学 2025-05-27 Jamy-Jayme Thézier , Aurélien Barrau , Killian Martineau

Introducing an effective refraction index of an isotropic cosmic medium, we investigate the cosmological fluid dynamics which is consistent with a conformal, timelike symmetry of a corresponding ``optical'' metric. We demonstrate that this…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Winfried Zimdahl , Alexander B. Balakin
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