35,987 research outputs found
Information of Structures in Galaxy Distribution
We introduce an information-theoretic measure, the Renyi information, to
describe the galaxy distribution in space. We discuss properties of the
information measure, and demonstrate its relationship with the probability
distribution function and multifractal descriptions. Using the First Look
Survey galaxy samples observed by the Infrared Array Camera onboard Spitzer
Space Telescope, we present measurements of the Renyi information, as well as
the counts-in-cells distribution and multifractal properties of galaxies in
mid-infrared wavelengths. Guided by multiplicative cascade simulation based on
a binomial model, we verify our measurements, and discuss the spatial selection
effects on measuring information of the spatial structures. We derive structure
scan functions at scales where selection effects are small for the Spitzer
samples. We discuss the results, and the potential of applying the Renyi
information to measuring other spatial structures.Comment: 25 pages, 8 figures, submitted to ApJ; To appear in The Astrophysical
Journal 2006, 644, 678 (June 20th
Simulations of thermally broadened HI Lya absorption arising in the warm-hot intergalactic medium
Recent far-ultraviolet (FUV) absorption line measurements of low-redshift
quasars have unveiled a population of intervening broad HI Lya absorbers (BLAs)
with large Doppler parameters (b> 40 km/s). If the large width of these lines
is dominated by thermal line broadening, the BLAs may trace highly-ionized gas
in the warm-hot intergalactic medium (WHIM) in the temperature range T ~
10^5-10^6 K, a gas phase that is expected to contain a large fraction of the
baryons at low redshift. In this paper we use a hydrodynamical simulation to
study frequency, distribution, physical conditions, and baryon content of the
BLAs at z=0. From our simulated spectra we derive a number of BLAs per unit
redshift of (dN/dz)_BLA ~ 38 for HI absorbers with log (N(cm^-2)/b(km/s))>10.7,
b>40 km/s, and log N(HII)<20.5. The baryon content of these systems is
Omega_b(BLA)=0.0121/h_65, which represents ~25 percent of the total baryon
budget in our simulation. Our results thus support the idea that BLAs represent
a significant baryon reservoir at low redshift. BLAs predominantly trace
shock-heated collisionally ionized WHIM gas at temperatures log T~4.4-6.2.
About 27 percent of the BLAs in our simulation originate in the photoionized
Lya forest (log T<4.3) and their large line widths are determined by
non-thermal broadening effects such as unresolved velocity structure and
macroscopic turbulence. Our simulation implies that for a large-enough sample
of BLAs in FUV spectra it is possible to obtain a reasonable approximation of
the baryon content of these systems solely from the measured HI column
densities and b values.Comment: 11 pages, 8 figures; minor modifications; accepted for publication in
A&
Determination of the strong coupling from semi-leptonic decay
According to heavy-meson chiral perturbation theory, the vector form factor
of exclusive semi-leptonic decay is closely
related, at least in the soft-pion region (i.e., ),
to the strong coupling or the normalized coupling .
Combining the precisely measured spectrum of decay by
the BaBar and Belle collaborations with several parametrizations of the form
factor , we can extract these couplings from the residue of the form
factor at the pole, which relies on an extrapolation of the form factor
from the semi-leptonic region to the unphysical point .
Comparing the extracted values with the other experimental and theoretical
estimates, we can test these various form-factor parametrizations, which differ
from each other by the amount of physical information embedded in. It is found
that the extracted values based on the BK, BZ and BCL parametrizations are
consistent with each other and roughly in agreement with the other theoretical
and lattice estimates, while the BGL ansatz, featured by a spurious, unwanted
pole at the threshold of the cut, gives a neatly larger value.Comment: 19 pages, no figure. Revise
Universal bifurcation property of two- or higher-dimensional dissipative systems in parameter space: Why does 1D symbolic dynamics work so well?
The universal bifurcation property of the H\'enon map in parameter space is
studied with symbolic dynamics. The universal- region is defined to
characterize the bifurcation universality. It is found that the universal-
region for relative small is not restricted to very small values. These
results show that it is also a universal phenomenon that universal sequences
with short period can be found in many nonlinear dissipative systems.Comment: 10 pages, figures can be obtained from the author, will appeared in
J. Phys.
H-Alpha and Hard X-Ray Observations of a Two-Ribbon Flare Associated with a Filament Eruption
We perform a multi-wavelength study of a two-ribbon flare on 2002 September
29 and its associated filament eruption, observed simultaneously in the H-alpha
line by a ground-based imaging spectrograph and in hard X-rays by RHESSI. The
flare ribbons contain several H-alpha bright kernels that show different
evolutional behaviors. In particular, we find two kernels that may be the
footpoints of a loop. A single hard X-ray source appears to cover these two
kernels and to move across the magnetic neutral line. We explain this as a
result of the merging of two footpoint sources that show gradually asymmetric
emission owing to an asymmetric magnetic topology of the newly reconnected
loops. In one of the H-alpha kernels, we detect a continuum enhancement at the
visible wavelength. By checking its spatial and temporal relationship with the
hard X-ray emission, we ascribe it as being caused by electron beam
precipitation. In addition, we derive the line-of-sight velocity of the
filament plasma based on the Doppler shift of the filament-caused absorption in
the H-alpha blue wing. The filament shows rapid acceleration during the
impulsive phase. These observational features are in principal consistent with
the general scenario of the canonical two-ribbon flare model.Comment: 15 pages, 5 figures, accepted for publication in Ap
Cosmology in Nonlinear Born-Infeld Scalar Field Theory With Negative Potentials
The cosmological evolution in Nonlinear Born-Infeld(hereafter NLBI) scalar
field theory with negative potentials was investigated. The cosmological
solutions in some important evolutive epoches were obtained. The different
evolutional behaviors between NLBI and linear(canonical) scalar field theory
have been presented. A notable characteristic is that NLBI scalar field behaves
as ordinary matter nearly the singularity while the linear scalar field behaves
as "stiff" matter. We find that in order to accommodate current observational
accelerating expanding universe the value of potential parameters and
must have an {\it upper bound}. We compare different cosmological
evolutions for different potential parameters .Comment: 18 pages, 18 figures, some references added, revised version for
Int.J.Mod.Phys.A, appeared in Int.J.Mod.Phys.
The Evolution of Universe with th B-I Type Phantom Scalar Field
We considered the phantom cosmology with a lagrangian ,
which is original from the nonlinear Born-Infeld type scalar field with the
lagrangian . This cosmological model can explain the
accelerated expansion of the universe with the equation of state parameter
. We get a sufficient condition for a arbitrary potential to admit a
late time attractor solution: the value of potential at the critical
point should be maximum and large than zero. We study a specific
potential with the form of
via phase plane
analysis and compute the cosmological evolution by numerical analysis in
detail. The result shows that the phantom field survive till today (to account
for the observed late time accelerated expansion) without interfering with the
nucleosynthesis of the standard model(the density parameter
at the equipartition epoch), and also avoid the
future collapse of the universe.Comment: 17 pages, 10 figures,typos corrected, references added,figures added
and enriched, title changed, main result remaine
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