55 research outputs found
Observational physics of mirror world
The existence of the whole world of shadow particles, interacting with each other and having no mutual interactions with ordinary particles except gravity is a specific feature of modern superstring models, being considered as models of the theory of everything. The presence of shadow particles is the necessary condition in the superstring models, providing compensation of the asymmetry of left and right chirality states of ordinary particles. If compactification of additional dimensions retains the symmetry of left and right states, shadow world turns to be the mirror one, with particles and fields having properties strictly symmetrical to the ones of corresponding ordinary particles and fields. Owing to the strict symmetry of physical laws for ordinary and mirror particles, the analysis of cosmological evolution of mirror matter provides rather definite conclusions on possible effects of mirror particles in the universe. A general qualitative discussion of possible astronomical impact of mirror matter is given, in order to make as wide as possible astronomical observational searches for the effects of mirror world, being the unique way to test the existence of mirror partners of ordinary particles in the Nature
Orbifold Family Unification
We study the possibility of complete family unification in higher-dimensional
space-time. Three families of matters in SU(5) grand unified theory are derived
from a single bulk multiplet of SU(N) gauge group (N >= 9) in the framework of
S^1/Z_2 orbifold models. In the case of the direct orbifold breaking down to
the standard model gauge group, there are models in which bulk fields from a
single multiplet and a few brane fields compose three families of quarks and
leptons.Comment: Comments added, version to appear in Physical Review D (v3);
References added (v2); 19 pages (v1
Signature of relic heavy stable neutrinos in underground experiments
Considering heavy stable neutrinos of 4th generation we calculate the relic
density of such neutrinos in the Universe. Taking into account the condensation
of heavy neutrinos in the Galaxy and applying the results of calculations to
experimental data from underground experiments on search for WIMPs in elastic
neutral current scattering on nuclei we found an exclusion region of neutrino
mass 60 GeV < m < 290 GeV. The bounds obtained from present underground
experiments while confirming the previous bounds derived from analysis of
cosmic ray spectra are more relible ones. We discuss also the first indication
of elastic scattering induced by WIMP in DAMA experiment finding a very narrow
window of neutrino mass 45 GeV < m < 50 GeV compatible with the possible signal
rate in the detector.Comment: 12 pages, 3 figure
The Formation of Primary Galactic Nuclei during Phase Transitions in the Early Universe
A new mechanism describing the formation of protogalaxies is proposed, which
is based on the second- order phase transition in the inflation stage and the
domain wall formation upon the end of inflation. The presence of closed domain
walls with the size markedly exceeding the cosmological horizon at the instant
of their formation and the wall collapse in the postinflation epoch (when the
wall size becomes comparable with the cosmological horizon), which leads to the
formation of massive black hole clusters that can serve as nuclei for the
future galaxies. The black hole mass distributions obtained do not contradict
the available experimental data. The number of black holes with M ~ 100 solar
masses () and above is comparable with the number of Galaxies in the
visible Universe. Development of the proposed approach gives ground for a
principally new scenario of the galaxy formation in the model of hot Universe.Comment: 9 page
Gravitino production by primordial black hole evaporation and constraints on the inhomogeneity of the early Universe
In supergravity models, the evaporation of light Primordial Black Holes
(PBHs) should be a source of gravitinos. By considering this process, new
stringent limits are derived on the abundance of small black holes with initial
masses less than 10^9 g. In minimal supergravity, the subsequent decay of
evaporated gravitinos into cascades of non-equilibrium particles leads to the
formation of elements whose abundance is constrained by observations. In gauge
mediated supersymmetry breaking models, their density is required not to
overclose the Universe. As a result, cosmological models with substantial
inhomogeneities on small scales are excluded.Comment: Published version. Minor changes, references adde
Testing Primordial Abundances With Sterile Neutrinos
The mixing between sterile and active neutrinos is taken into account in the
calculation of Big Bang Nucleosynthesis. The abundances of primordial elements,
like D, 3He, 4He and 7Li, are calculated by including sterile neutrinos, and by
using finite chemical potentials. It is found that the resulting theoretical
abundances are consistent with WMAP data on baryonic densities, and with limits
of LSND on mixing angles, only if 7Li is excluded from the statistical analysis
of theoretical and experimental results.Comment: 7 pages, 3 figures, 1 table, 34 reference
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