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相关论文: The Mirror Universes

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Theoretical and observational arguments are listed in favor of a new principle of relativity of units of measurements as the basis of a conformal-invariant unification of General Relativity and Standard Model by replacement of all masses…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. Pervushin , V. Zinchuk , A. Zorin

The aim of this review article is to give a comprehensive description of the scaling properties detected for the distribution of cosmic structures. Due to the great variety of statistical methods to describe the large-scale structure of the…

天体物理学 · 物理学 2008-11-26 Stefano Borgani

Parity and time reversal are obvious and plausible candidates for fundamental symmetries of nature. Hypothesising that these symmetries exist implies the existence of a new form of matter, called mirror matter. The mirror matter theory (or…

天体物理学 · 物理学 2008-11-26 R. Foot

Mirror matter is a stable self-collisional dark matter candidate. If parity is a conserved unbroken symmetry of nature, there could exist a parallel hidden (mirror) sector of the Universe composed of particles with the same masses and…

宇宙学与河外天体物理 · 物理学 2011-03-31 Paolo Ciarcelluti

Up-to-date estimates of the cosmological parameters are presented as a result of numerical simulations of cosmic microwave background and large scale structure, considering a flat Universe in which the dark matter is made entirely or partly…

宇宙学与河外天体物理 · 物理学 2014-01-21 Paolo Ciarcelluti , Quentin Wallemacq

The early Universe after inflation may have oscillations, kinations (nonoscillatory evolution of a field), topological defects, relativistic and non-relativistic particles at the same time. The Universe whose energy density is a sum of…

高能物理 - 唯象学 · 物理学 2015-06-12 Seishi Enomoto , Kazunori Kohri , Tomohiro Matsuda

B and L violating interactions of ordinary particles with their twin particles from hypothetical mirror world can co-generate baryon asymmetries in both worlds in comparable amounts, $\Omega'_B/\Omega_B \sim 5$ or so. On the other hand, the…

宇宙学与河外天体物理 · 物理学 2016-03-01 Zurab Berezhiani

We study the effect of a finite topology on the temperature correlations of the cosmic microwave background in a flat universe. Analytic expressions for the angular power spectrum are given for all possible finite flat models. We examine…

天体物理学 · 物理学 2009-10-31 Evan Scannapieco , Janna Levin , Joseph Silk

We comment on a recently discussed possibility of oscillations between neutrons and degenerate mirror neutrons in the context of mirror models for particles and forces. It has been noted by Bento and Berezhiani that if these oscillations…

高能物理 - 唯象学 · 物理学 2014-11-18 R. N. Mohapatra , S. Nasri , S. Nussinov

A lagrangian for the $k-$ essence field is constructed for a constant scalar potential and its form determined when the scale factor was very small compared to the present epoch but very large compared to the inflationary epoch. This means…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Debashis Gangopadhyay

Temperature and polarization power spectra of the cosmic microwave background can provide essentially incontrovertible evidence for coherent acoustic oscillations in the early universe. A simple model calculation demonstrates explicitly how…

天体物理学 · 物理学 2007-05-23 Arthur Kosowsky

Recent observations show that our universe is accelerating by dark energy, so it is important to investigate the thermodynamical properties of it. The Undulant Universe is a model with equation of state $\omega(a)=-\cos(b\ln a)$ for dark…

天体物理学 · 物理学 2010-06-18 Tian Lan , Tong-Jie Zhang , Bao-Quan Wang

Mirror world, a parallel hidden sector with microphysics identical to ordinary particle physics, can have several interesting phenomenological and astrophysical implications and mirror matter can be a natural candidate for dark matter in…

高能物理 - 唯象学 · 物理学 2008-10-01 Angela Lepidi

I survey physics theories involving parallel universes, which form a natural four-level hierarchy of multiverses allowing progressively greater diversity. Level I: A generic prediction of inflation is an infinite ergodic universe, which…

天体物理学 · 物理学 2007-05-23 Max Tegmark

The physical processes that define the spine of the galaxy cluster X-ray luminosity -- temperature (L-T) relation are investigated using a large hydrodynamical simulation of the Universe. This simulation models the same volume and phases as…

天体物理学 · 物理学 2009-11-13 W. G. Hartley , L. Gazzola , F. R. Pearce , S. T. Kay , P. A. Thomas

The role of turbulence and turbulent mixing in the formation and evolution of the early universe is examined. A new quantum-gravitational-dynamics model suggests that the mechanism of the hot big bang is functionally equivalent to the…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

The models of cyclic universes and cyclic multiverses based on the alternative gravity theories of varying constants are considered.

广义相对论与量子宇宙学 · 物理学 2017-08-18 Mariusz P. Dabrowski

We propose a novel model in which the Universe is created as a pair of coordinate-reversed counterparts, forming a globally CPT-symmetric system that permits local CPT violations within each sector. This framework naturally introduces a…

高能物理 - 唯象学 · 物理学 2026-04-30 M. M. Chaichian , M. Gogberashvili , M. N. Mnatsakanova , T. Tsiskaridze

We study the cosmological inflation and reheating in a teleparallel model of gravity. Reheating is assumed to be due to the decay of a scalar field to radiation during its rapid oscillation. By using cosmological perturbations during…

综合物理 · 物理学 2019-07-26 P. Goodarzi , H. Mohseni Sadjadi

Two extensions of ideas lying in the basis of the inflationary scenario of the early Universe and their effect on the large scale structure of the present-day Universe are discussed. The first of them is the possibility of fast phase…

天体物理学 · 物理学 2007-05-23 A. A. Starobinsky