797 research outputs found
Determining the Equation of State of the Expanding Universe Using a New Independent Variable
To determine the equation of state of the universe, we propose to use a new
independent variable , where and
are the present Hubble parameter and the luminosity distance, respectively. For
the flat universe suggested from the observation of the anisotropy of cosmic
microwave background, the density and the pressure are expressed as
and where
is the present density and . In plane the sign
as well as the strength of the pressure is in proportion to the curvature of
the curve . We propose to adopt a Pade-like expression of
with . For flat
model the expansion up to N=7 has at most an error for and any value of . We also propose a general method to determine
the equation of state of the universe which has free parameters. If the
number of parameters are smaller than , there is a consistency check of
the equation of state so that we may confirm or refute each model.Comment: 12 pages, to be published in the Astrophysical Journa
A Null Test of the Cosmological Constant
We provide a consistency relation between cosmological observables in general
relativity with the cosmological constant. Breaking of this relation at any
redshift would imply the breakdown of the hypothesis of the cosmological
constant as an explanation of the current acceleration of the universe.Comment: 5 pages, 1 figure, references added, to be published in
Prog.Theor.Phy
The Luminosity Distance, the Equation of State, and the Geometry of the Universe
The second derivative of the luminosity distance with respect to the redshift
is written in terms of the deceleration parameter . We point out that the
third derivative contains the information regarding the sound speed of cosmic
matter as well as the curvature of the universe. We restrict physically
possible parameter ranges of the coefficients. It is found that there is a
relation between the coefficients in a flat universe model with matter such
that ( is the total sound speed of the matter
component and =).Comment: 5 pages + 1 figure, one reference added, Prog.Theor.Phys. in pres
Cosmology with x-matter
Motivated by the possibility of where and are the
Hubble parameter and the age of the universe, respectively, we investigate the
cosmology including x-matter. x-matter is expressed by the equation of state
, where , and
are the pressure, the density of x-matter and the density at
present, respectively. and are functions of in general.
x-matter has the most general form of the equation of state which is
characterized by 1)violation of strong energy condition at present for ; 2) locally stable (i.e. ); 3)causality is guaranteed
(). Considering the case that and are constants, we
find that there is a large parameter space of in
which the model universe is consistent with the age of the universe and the
observations of distant Type I supernovae.Comment: minor changes, 4 pages, 6 figures, accepted for publication as a
Letter in MNRA
Microwave Background Anisotropies in Primeval Isocurvature Baryon Models: Constraints on the Cosmological Parameters
We have performed the most comprehensive predictions of the temperature
fluctuations \dtt in the primeval isocurvature baryon models to see whether or
not the models are consistent with the recent data on the cosmic microwave
background anisotropies. More specifically, we computed the \dtt corresponding
to the experimental set-up by the South-Pole and the Owens Valley experiments
as well as the COBE satellite. The amplitudes of the predicted \dtt are
normalized by means of the COBE 10 data. The resulting constraints on
the models are presented on plane in the case of
(flat models) and (open models), where
is the primordial spectral index of entropy fluctuations and is the
present baryon density parameter.
Our results imply that the PIB models cannot be reconciled with the current
observations for any reasonable set of cosmological parameters.Comment: 10pages and 4figures compressed uuencoded postscript (with figures),
UTAP-93-16
Observational tests of x-matter models
We study gravitational lensing statistics, matter power spectra and the
angular power spectra of the cosmic microwave background (CMB) radiation in
x-matter models. We adopt an equation-of-state of x-matter which can express a
wide range of matter from the pressureless dust to the cosmological constant. A
new ingredient in this model is the sound speed of the x-component in addition
to the equation-of-state . Except for the cosmological
constant case, the perturbations of x-matter itself are considered. Our primary
interest is in the effect of non-zero sound speed on the structure formation
and the CMB spectra. It is found that there exist parameter ranges where
x-matter models are consistent with all current observations. The x-matter
generally leaves imprints in the CMB anisotropy and the matter power spectrum,
which should be detectable in future observations.Comment: minor changes, 10 pages+14 figures, MNRAS in pres
Determining the Equation of State of the Expanding Universe: Inverse Problem in Cosmology
Even if the luminosity distance as a function of redshift is obtained
accurately using, for example, Type Ia supernovae, the equation of state of the
Universe cannot be determined uniquely but depends on one free parameter
, where and are the present scale
factor and the Hubble parameter, respectively. This degeneracy might be
resolved if, for example, the time variations of the redshift of quasars are
measured as proposed recently by Loeb. Therefore the equation of state of the
Universe (or the metric of the universe) might be determined without any
theoretical assumption on the matter content of the Universe in future.Comment: 5 pages, accepted for publication in MNRA
Numerical analysis of voltage-controlled magnetization switching operation in magnetic-topological-insulator-based devices
We theoretically investigate influences of electronic circuit delay, noise
and temperature on write-error-rate (WER) in voltage-controlled magnetization
switching operation of a magnetic-topological-insulator-based (MTI) device by
means of the micromagnetic simulation. This device realizes magnetization
switching via spin-orbit torque(SOT) and voltage-controlled magnetic anisotropy
(VCMA) which originate from 2D-Dirac electronic structure. We reveal that the
device operation is extremely robust against circuit delay and signal-to-noise
ratio. We demonstrate that the WER on the order of approximately or
below is achieved around room temperature due to steep change in VCMA. Also, we
show that the larger SOT improves thermal stability factor. This study provides
a next perspective for developing voltage-driven spintronic devices with
ultra-low power consumption.Comment: 6 pages, 5 figure
Tibial condylar valgus osteotomy (TCVO) for osteoarthritis of the knee: 5-year clinical and radiological results
According to one line of thought only propositions can be part of one’s evidence, since only propositions can serve the central functions of our ordinary concept of evidence. Ram Neta has challenged this argument. In this paper I respond to Neta’s challenge
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